DCTAPivo://purx/datacentral-tapData CentralDeshpande, M. S.Miszalski, B.Tocknell, J.O'Toole S. J.Data Centralhelp@datacentral.org.auspectroscopystellar-astronomygalaxiesredshift-surveysgalactic-archaeologyTAP service for surveys hosted by Data Centralhttps://docs.datacentral.org.au/reference/services/tap-service/IsServiceForGAVORegTAP Service (Potsdam mirror)GloTS, theGlobal TAP SchemaAIP DaCHS Obscore Tablehttps://datacentral.org.au:443/vo/tapADQL2.0ADQL 2.0application/x-votable+xml;serialization=TABLEDATAvotableapplication/fitsfitstext/csvcsvtext/tab-separated-valuestsvtext/plaintexttext/htmlhtmlapplication/jsonjson003600360001000000010000000https://datacentral.org.au:443/vo/tap/tableshttps://datacentral.org.au:443/vo/tap/capabilitieshttps://datacentral.org.au:443/vo/tap/availabilityTAP_SCHEMASet of tables listing and describing the schemas, tables and columns published in this TAP service.TAP_SCHEMA.schemasList of schemas published in this TAP service.schema_nameschema name, possibly qualifiedVARCHARindexedprincipaldescriptionbrief description of schemaVARCHARprincipalutypeUTYPE if schema corresponds to a data modelVARCHARTAP_SCHEMA.tablesList of tables published in this TAP service.table_indexthis index is used to recommend table ordering for clientsINTEGERschema_namethe schema name from TAP_SCHEMA.schemasVARCHARprincipaltable_nametable name as it should be used in queriesVARCHARindexedprincipaltable_typeone of: table, viewVARCHARdescriptionbrief description of tableVARCHARprincipalutypeUTYPE if table corresponds to a data modelVARCHARTAP_SCHEMA.columnsList of columns of all tables listed in TAP_SCHEMA.TABLES and published in this TAP service.column_indexthis index is used to recommend column ordering for clientsINTEGERtable_nametable name from TAP_SCHEMA.tablesVARCHARindexedprincipalcolumn_namecolumn nameVARCHARindexedprincipaldatatypean XType or a TAPTypeVARCHARprincipalarraysizelength of variable length datatypesINTEGER"size"same as "arraysize" but kept for backward compatibility onlyINTEGERdescriptionbrief description of columnVARCHARprincipalutypeUTYPE of column if anyVARCHARunitunit in VO standard formatVARCHARprincipalucdUCD of column if anyVARCHARprincipalindexedan indexed column; 1 means true, 0 means falseSMALLINTprincipala principal column; 1 means true, 0 means falseSMALLINTstda standard column; 1 means true, 0 means falseSMALLINTTAP_SCHEMA.keysList all foreign keys but provides just the tables linked by the foreign key. To know which columns of these tables are linked, see in TAP_SCHEMA.key_columns using the key_id.key_idunique key identifierVARCHARindexedprincipalfrom_tablefully qualified table nameVARCHARprincipaltarget_tablefully qualified table nameVARCHARprincipaldescriptiondescription of this keyVARCHARprincipalutypeutype of this keyVARCHARTAP_SCHEMA.key_columnsList all foreign keys but provides just the columns linked by the foreign key. To know the table of these columns, see in TAP_SCHEMA.keys using the key_id.key_idunique key identifierVARCHARindexedprincipalfrom_columnkey column name in the from_tableVARCHARindexedprincipaltarget_columnkey column name in the target_tableVARCHARindexedprincipalnoirlab_test2test tables from noirlab for EMU crossmatchingnoirlab_test2.1_des_dr2The noirlab des_dr2.main table pre-joined with des_dr2.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalalphawin_j2000right ascension for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalawin_image_gg-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_ii-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_rr-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_yy-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_zz-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipala_imagemajor axis size based on an isophotal model [pixel]pixelREALprincipalbackground_gg-band background level, by ccd-amplifier [mag]magREALprincipalbackground_ii-band background level, by ccd-amplifier [mag]magREALprincipalbackground_rr-band background level, by ccd-amplifier [mag]magREALprincipalbackground_yy-band background level, by ccd-amplifier [mag]magREALprincipalbackground_zz-band background level, by ccd-amplifier [mag]magREALprincipalbwin_image_gg-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_ii-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_rr-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_yy-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_zz-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalb_imageminor axis size based on an isophotal model [pixel]pixelREALprincipalclass_star_gg-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_ii-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_rr-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_yy-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_zz-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalcoadd_object_idunique identifier for the coadded objectsmeta.id;meta.mainBIGINTindexedprincipaldecdeclination, with quantized precision for indexing (deltawin_j2000 has full precision but not indexed) [degrees]degpos.eq.dec;meta.mainDOUBLEindexedprincipaldeltawin_j2000declination for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalebv_sfd98e(b-v) reddening coefficient from schlegel, finkbeiner & davis, 1998 [mag]magDOUBLEprincipalerrawin_image_gg-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_ii-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_rr-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_yy-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_zz-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerra_imageuncertainty in major axis size, from isophotal model [pixel]pixelREALprincipalerrbwin_image_gg-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_ii-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_rr-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_yy-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_zz-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrb_imageuncertainty in minor axis size, from isophotal model [pixel]pixelREALprincipalerrthetawin_image_gg-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_ii-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_rr-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_yy-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_zz-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrtheta_imageuncertainty in source position, from isophotal model [degrees]degREALprincipalerrx2win_image_gg-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_ii-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_rr-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_yy-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_zz-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_gg-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_ii-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_rr-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_yy-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_zz-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_gg-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_ii-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_rr-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_yy-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_zz-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalextended_class_coadd0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using sextractor photometrySMALLINTprincipalextended_class_wavg0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using wavg photometrySMALLINTprincipalflags_gg-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_ii-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_rr-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_yy-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_zz-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalfluxerr_auto_gg-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_ii-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_rr-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_yy-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_zz-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_gg-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_ii-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_rr-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_yy-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_zz-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_radius_gg-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_ii-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_rr-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_yy-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_zz-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_gg-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_ii-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_rr-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_yy-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_zz-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalgalactic_lgalactic longitude [degrees]degpos.galactic.lonREALprincipalhpix_1024healpix identifier for nside=1024 grid size, in a nested schemaBIGINTprincipalhpix_16384healpix identifier for nside=16384 grid size, in a nested schemaBIGINTprincipalhpix_32healpix identifier for nside=32 grid size, in a nested schemaBIGINTprincipalhpix_4096healpix identifier for nside=4096 grid size, in a nested schemaBIGINTprincipalhpix_64healpix identifier for nside=64 grid size, in a nested schemaBIGINTprincipalimaflags_iso_gg-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_ii-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_rr-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_yy-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_zz-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalisoarea_image_gg-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_ii-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_rr-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_yy-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_zz-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalkron_radiuskron radius measured from detection image [pixel]pixelREALprincipalkron_radius_gg-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_ii-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_rr-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_yy-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_zz-band kron radius measured from coadded image [pixel]pixelREALprincipalmagerr_auto_gg-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_ii-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_rr-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_yy-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_zz-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_gg-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_g_deredg-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_ii-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_i_deredi-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_rr-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_r_deredr-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_yy-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_y_deredy-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_zz-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_z_deredz-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalnepochs_gg-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_ii-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_yy-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_zz-band number of epochs the source is detected in single epoch imagesINTEGERprincipalniter_model_gg-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_ii-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_rr-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_yy-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_zz-band number of iterations in model fitting photometric measurementsINTEGERprincipalraright ascension, with quantized precision for indexing (alphawin_j2000 has full precision but not indexed) [degrees]degpos.eq.ra;meta.mainDOUBLEindexedprincipalspreaderr_model_gg-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_ii-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_rr-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_yy-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_zz-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspread_model_gg-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_ii-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_rr-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_yy-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_zz-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalthetawin_image_gg-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_ii-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_rr-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_yy-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_zz-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipaltheta_j2000position angle of source in j2000 coordinates, from non-windowed measurement [degrees]degREALprincipaltilenameidentifier of each one of the tiles on which the survey is griddedVARCHARprincipalwavg_fluxerr_psf_gg-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_ii-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_rr-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_yy-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_zz-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_gg-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_ii-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_rr-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_yy-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_zz-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_magerr_psf_gg-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_ii-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_rr-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_yy-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_zz-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_gg-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_g_deredg-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_ii-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_i_deredi-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_rr-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_r_deredr-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_yy-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_y_deredy-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_zz-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_z_deredz-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_spreaderr_model_gg-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_ii-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_rr-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_yy-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_zz-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_gg-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_ii-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_rr-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_yy-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_zz-band spread model using the weighted averaged values from single epoch detectionsREALprincipalx2win_image_gg-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_ii-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_rr-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_yy-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_zz-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxwin_imagex-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalxwin_image_gg-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_ii-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_rr-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_yy-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_zz-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxywin_image_gg-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_ii-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_rr-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_yy-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_zz-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_gg-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalgalactic_bgalactic latitude [degrees]degpos.galactic.latREALprincipalnepochs_rr-band number of epochs the source is detected in single epoch imagesINTEGERprincipaly2win_image_ii-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_rr-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_yy-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_zz-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalywin_imagey-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalywin_image_gg-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_ii-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_rr-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_yy-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_zz-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalhtm9Ninth level (~10 arcmin resolution) Hierarchical Triangular Mesh index (Szalay et al. 2007)meta.codeINTEGERprincipalnest4096Nested-scheme HEALPix (Gorski et al. 2005) index with NSIDE=4096 (~1 arcmin resolution)meta.codeINTEGERprincipalring256Ring-scheme HEALPix (Gorski et al. 2005) index with NSIDE=256 (~14 arcmin resolution)meta.codeINTEGERprincipalg_rG-R colormagphot.colorREALprincipalr_iR-I colormagphot.colorREALprincipali_zI-Z colormagphot.colorREALprincipalz_yZ-Y colormagphot.colorREALprincipalsnr_gS/N in g-bandmagstat.snrREALprincipalsnr_rS/N in r-bandmagstat.snrREALprincipalsnr_iS/N in i-bandmagstat.snrREALprincipalsnr_yS/N in Y-bandmagstat.snrREALprincipalsnr_zS/N in z-bandmagstat.snrREALprincipalecliptic_latEcliptic Latitudedegpos.ecliptic.latDOUBLEprincipalecliptic_lonEcliptic Longitudedegpos.ecliptic.lonDOUBLEprincipalnoirlab_test2.36_ls_dr8The noirlab ls_dr8.tractor table pre-joined with ls_dr8.x1p5__tractor__allwise__source, ls_dr8.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.g_rComputed (g-r) colorREALprincipalfracdevFraction of model in deVauc [0,1]REALprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudedegDOUBLEprincipalelonEcliptic LongitudedegDOUBLEprincipalglatGalactic LatitudedegDOUBLEprincipalglonGalactic LongitudedegDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalbrickidBrick ID [1,662174]INTEGERprincipalbrightblobbitwise mask indicating that an object is near a bright foreground source, as cataloged on the DR8 bitmasks page (http://legacysurvey.org/dr8/bitmasksDR8 bitmasks)SMALLINTprincipalbxX position (0-indexed) of coordinates in brick image stackpixREALprincipalbyY position (0-indexed) of coordinates in brick image stackpixREALprincipaldchisq_1Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_2Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_3Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_4Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_5Difference in X^2 between successfully more-complex model fitsREALprincipalls_idUnique LS object ID from RELEASE, BRICKID, OBJIDBIGINTprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errors1/deg^2REALprincipaldered_flux_gDereddened G-band fluxnanomaggiesREALprincipaldered_flux_rDereddened R-band fluxnanomaggiesREALprincipaldered_flux_w1Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w2Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w3Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w4Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_zDereddened Z-band fluxnanomaggiesREALprincipaldered_mag_gDereddened G-band magnitudemagREALprincipaldered_mag_rDereddened R-band magnitudemagREALprincipaldered_mag_w1Dereddened W1 magnitudemagREALprincipaldered_mag_w2Dereddened W2 magnitudemagREALprincipaldered_mag_w3Dereddened W3 magnitudemagREALprincipaldered_mag_w4Dereddened W4 magnitudemagREALprincipaldered_mag_zDereddened Z-band magnitudemagREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsmagREALprincipalfiberflux_gPredicted g-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_rPredicted r-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_zPredicted z-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_gPredicted g-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_rPredicted r-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_zPredicted z-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)1/nanomaggies^2REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB)1/nanomaggies^2REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB)1/nanomaggies^2REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB)1/nanomaggies^2REALprincipalflux_w1WISE model flux in W1 (AB system)nanomaggiesREALprincipalflux_w2WISE model flux in W2 (AB)nanomaggiesREALprincipalflux_w3WISE model flux in W3 (AB)nanomaggiesREALprincipalflux_w4WISE model flux in W4 (AB)nanomaggiesREALprincipalfracdev_ivarInverse variance of fracdevREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a source flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a source flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a source flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in r, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in z, strictly between [0,1]REALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magmagREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magmagREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magmagREALprincipalgaldepth_gAs for PSFDEPTH_G but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_rAs for PSFDEPTH_R but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_zAs for PSFDEPTH_Z but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalhtm9HTM index (order 9 => ~10 arcmin size)meta.codeINTEGERprincipalmag_gConverted G magnitudemagREALprincipalmag_rConverted R magnitudemagREALprincipalmag_w1W1 magnitudemagREALprincipalmag_w2W2 magnitudemagREALprincipalmag_w3W3 magnitudemagREALprincipalmag_w4W4 magnitudemagREALprincipalmag_zConverted Z magnitudemagREALprincipalmaskbitsbitwise mask indicating that an object touches a pixel in the coadd maskbits maps, as cataloged on the DR8 bitmasks pageSMALLINTprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in W1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in W2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in W3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in W4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each blobINTEGERprincipalparallaxReference catalog parallaxmasREALprincipalparallax_ivarReference catalog inverse-variance on parallax1/(mas)^2REALprincipalpmdecReference catalog proper motion in the Dec directionmas / yrREALprincipalpmdec_ivarReference catalog inverse-variance on pmdec1/(mas/yr)^2REALprincipalpmraReference catalog proper motion in the RA directionmas / yrREALprincipalpmra_ivarReference catalog inverse-variance on pmra1/(mas/yr)^2REALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_g) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_g)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_rFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_r) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_r)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_z) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_z)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfsize_gWeighted average PSF FWHM in the g bandarcsecREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandarcsecREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandarcsecREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errors1/deg^2REALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)yrREALprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia-DR2 and LSLGABIGINTprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalshapedev_e1Ellipticity component 1REALprincipalshapedev_e1_ivarInverse variance of shapedev_e1REALprincipalshapedev_e2Ellipticity component 2REALprincipalshapedev_e2_ivarInverse variance of shapedev_e2REALprincipalshapedev_rHalf-light radius of deVaucouleurs model (>0)arcsecREALprincipalshapedev_r_ivarInverse variance of shapedev_r1/arcsec^2REALprincipalshapeexp_e1Ellipticity component 1REALprincipalshapeexp_e1_ivarInverse variance of shapeexp_e1REALprincipalshapeexp_e2Ellipticity component 2REALprincipalshapeexp_e2_ivarInverse variance of shapeexp_e2REALprincipalshapeexp_rHalf-light radius of exponential model (>0)arcsecREALprincipalshapeexp_r_ivarInverse variance of shapeexp_r1/arcsec^2REALprincipalsnr_gSignal-to-Noise ratio in Gstat.ratioREALprincipalsnr_rSignal-to-Noise ratio in Rstat.ratioREALprincipalsnr_w1Signal-to-Noise ratio in W1stat.ratioREALprincipalsnr_w2Signal-to-Noise ratio in W2stat.ratioREALprincipalsnr_w3Signal-to-Noise ratio in W3stat.ratioREALprincipalsnr_w4Signal-to-Noise ratio in W4stat.ratioREALprincipalsnr_zSignal-to-Noise ratio in Zstat.ratioREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-d4) colorREALprincipalz_w1Computed (z-w1 colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarySMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia G band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalgaia_pointsourceThis Gaia DR2 source is believed to be a star, not a galaxySMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 forTycho-2, G2 for Gaia DR2, L2 for the LSLGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, COMP=composite, DUP=Gaia source fit by different model. Note that in some FITS readers, a trailing space may be appended for PSF , DEV and EXP since the column data type is a 4-character stringVARCHARprincipalwise_coadd_idunWISE coadd file name for the center of each objectVARCHARprincipalflux_gmodel flux in gREALprincipalflux_rmodel flux in rREALprincipalflux_zmodel flux in zREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_zInverse variance of flux_zREALprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_median(recommended) photo-z derived from the median of the photo-z PDFREALprincipalz_phot_stdstandard deviation of the photo-z derived from the photo-z PDFREALprincipalz_phot_l68lower 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_u68upper 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_l95lower 95% confidence limit derived from the photo-z PDFREALprincipalz_phot_u95upper 95% confidence limit derived from the photo-z PDFREALprincipalz_specspectroscopic redshift, if availableREALprincipalsurveysource of the spectroscopic redshiftVARCHARprincipaltrainingwhether or not the spectroscopic redshift is used for the photo-z trainingVARCHARprincipalnoirlab_test2.34_ls_dr9The noirlab ls_dr9.tractor table pre-joined with ls_dr9.x1p5__tractor__allwise__source, ls_dr9.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalls_idUnique LS object IDBIGINTprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudeDOUBLEprincipalelonEcliptic LongitudeDOUBLEprincipalglatGalactic LatitudeDOUBLEprincipalglonGalactic LongitudeDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia DR2 and SGABIGINTprincipalbrickidBrick ID [1,662174]INTEGERprincipalblob_nea_gBlob-masked noise equivalent area in g.REALprincipalblob_nea_rBlob-masked noise equivalent area in r.REALprincipalblob_nea_zBlob-masked noise equivalent area in z.REALprincipalbxX position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipalbyY position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipaldchisq_1Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_2Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_3Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_4Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_5Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errorsREALprincipaldered_flux_gDereddened g band fluxREALprincipaldered_flux_rDereddened r band fluxREALprincipaldered_flux_w1Dereddened w1 band fluxREALprincipaldered_flux_w2Dereddened w2 band fluxREALprincipaldered_flux_w3Dereddened w3 band fluxREALprincipaldered_flux_w4Dereddened w4 band fluxREALprincipaldered_flux_zDereddened z band fluxREALprincipaldered_mag_gDereddened g-band magnitudeREALprincipaldered_mag_rDereddened r-band magnitudeREALprincipaldered_mag_w1Dereddened w1-band magnitudeREALprincipaldered_mag_w2Dereddened w2-band magnitudeREALprincipaldered_mag_w3Dereddened w3-band magnitudeREALprincipaldered_mag_w4Dereddened w4-band magnitudeREALprincipaldered_mag_zDereddened z-band magnitudeREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsREALprincipalfiberflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_rPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_zPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_rPredicted r-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_zPredicted z-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalflux_gModel flux in gREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB system)REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB system)REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB system)REALprincipalflux_ivar_zInverse variance of flux_zREALprincipalflux_rModel flux in rREALprincipalflux_w1WISE model flux in W1 (AB system)REALprincipalflux_w2WISE model flux in W2 (AB system)REALprincipalflux_w3WISE model flux in W3 (AB system)REALprincipalflux_w4WISE model flux in W4 (AB system)REALprincipalflux_zModel flux in zREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a sources flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a sources flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a sources flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalgaia_a_g_valGaia line-of-sight extinction in the G bandREALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_sigma5d_maxGaia longest semi-major axis of the 5-d error ellipsoidREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_e_bp_min_rp_valGaia line-of-sight reddening E(BP-RP)REALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magREALprincipalgaia_phot_bp_rp_excess_factorGaia BP/RP excess factorREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP band signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magREALprincipalgaldepth_gAs for psfdepth_g but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_rAs for psfdepth_r but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_zAs for psfdepth_z but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalg_rComputed (g-r) colorREALprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalmag_gConverted g magnitudeREALprincipalmag_rConverted r magnitudeREALprincipalmag_w1Converted W1 magnitudeREALprincipalmag_w2Converted W2 magnitudeREALprincipalmag_w3Converted W3 magnitudeREALprincipalmag_w4Converted W4 magnitudeREALprincipalmag_zConverted z magnitudeREALprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in w1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in w2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in w3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in w4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnea_gNoise equivalent area in gREALprincipalnea_rNoise equivalent area in rREALprincipalnea_zNoise equivalent area in zREALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each brickINTEGERprincipalparallax_ivarReference catalog inverse-variance on parallaxREALprincipalparallaxReference catalog parallaxREALprincipalpmdec_ivarReference catalog inverse-variance on pmdecREALprincipalpmdecReference catalog proper motion in the Dec directionREALprincipalpmra_ivarReference catalog inverse-variance on pmraREALprincipalpmraReference catalog proper motion in the RA directionREALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/(sqrt psfdepth_g) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_g))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_rFor a 5 sigma point source detection limit in r, 5/(sqrt psfdepth_r) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_r))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in z, 5/(sqrt psfdepth_z) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_z))-9]) gives corresponding AB magnitudeREALprincipalpsfsize_gWeighted average PSF FWHM in the g bandREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errorsREALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)REALprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalsersic_ivarInverse variance of sersicREALprincipalsersicPower-law index for the Sersic profile model (type=SER)REALprincipalshape_e1_ivarInverse variance of shape_e1REALprincipalshape_e1Ellipticity component 1 of galaxy model for galaxy type typeREALprincipalshape_e2_ivarInverse variance of shape_e2REALprincipalshape_e2Ellipticity component 2 of galaxy model for galaxy type typeREALprincipalshape_r_ivarInverse variance of shape_rREALprincipalshape_rHalf-light radius of galaxy model for galaxy type type (>0)arcsecREALprincipalsnr_gSignal-to-Noise ratio in gREALprincipalsnr_rSignal-to-Noise ratio in rREALprincipalsnr_w1Signal-to-Noise ratio in W1REALprincipalsnr_w2Signal-to-Noise ratio in W2REALprincipalsnr_w3Signal-to-Noise ratio in W3REALprincipalsnr_w4Signal-to-Noise ratio in W4REALprincipalsnr_zSignal-to-Noise ratio in zREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-w4) colorREALprincipalwise_xX position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_x and bx)REALprincipalwise_yY position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_y and by)REALprincipalz_w1Computed (z-w1) colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarSMALLINTprincipalfitbitsBitwise mask detailing pecularities of how an object was fit, as cataloged on the DR9 bitmasks pageSMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_params_solvedWhich astrometric parameters were estimated for a Gaia sourceSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia g band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP band number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalmaskbitsBitwise mask indicating that an object touches a pixel in the coadd/*/*/*maskbits* maps, as cataloged on the DR9 bitmasks pageSMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 for Tycho-2, G2 for Gaia DR2, L3 for the SGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, SER=Sersic, DUP=Gaia source fit by different model.VARCHARprincipalwise_coadd_idunWISE coadd brick name (corresponding to the, e.g., legacysurvey-<brick>-image-W1.fits.fz coadd file) for the center of each objectVARCHARprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_medianphoto-z derived from the median of the photo-z PDFREALprincipalz_phot_stdStandard deviation of the photo-zs derived from the photo-z PDFREALprincipalz_phot_l68Lower bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_u68Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_l95Lower bound of the 95% confidence region, derived from the photo-z PDFREALprincipalz_phot_u95Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_specSpectroscopic redshift, if availableREALprincipaltrainingWhether or not the spectroscopic redshift is used in photometric redshift trainingVARCHARprincipalsurveySource of the spectroscopic redshiftVARCHARprincipalnoirlab_test2.36_ls_dr9The noirlab ls_dr9.tractor table pre-joined with ls_dr9.x1p5__tractor__allwise__source, ls_dr9.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.pmdecReference catalog proper motion in the Dec directionREALprincipalpmra_ivarReference catalog inverse-variance on pmraREALprincipalpmraReference catalog proper motion in the RA directionREALprincipalbrick_primaryTrue if the object is within the brick boundarSMALLINTprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalls_idUnique LS object IDBIGINTprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudeDOUBLEprincipalelonEcliptic LongitudeDOUBLEprincipalglatGalactic LatitudeDOUBLEprincipalglonGalactic LongitudeDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia DR2 and SGABIGINTprincipalbrickidBrick ID [1,662174]INTEGERprincipalblob_nea_gBlob-masked noise equivalent area in g.REALprincipalblob_nea_rBlob-masked noise equivalent area in r.REALprincipalblob_nea_zBlob-masked noise equivalent area in z.REALprincipalbxX position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipalbyY position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipaldchisq_1Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_2Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_3Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_4Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_5Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errorsREALprincipaldered_flux_gDereddened g band fluxREALprincipaldered_flux_rDereddened r band fluxREALprincipaldered_flux_w1Dereddened w1 band fluxREALprincipaldered_flux_w2Dereddened w2 band fluxREALprincipaldered_flux_w3Dereddened w3 band fluxREALprincipaldered_flux_w4Dereddened w4 band fluxREALprincipaldered_flux_zDereddened z band fluxREALprincipaldered_mag_gDereddened g-band magnitudeREALprincipaldered_mag_rDereddened r-band magnitudeREALprincipaldered_mag_w1Dereddened w1-band magnitudeREALprincipaldered_mag_w2Dereddened w2-band magnitudeREALprincipaldered_mag_w3Dereddened w3-band magnitudeREALprincipaldered_mag_w4Dereddened w4-band magnitudeREALprincipaldered_mag_zDereddened z-band magnitudeREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsREALprincipalfiberflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_rPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_zPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_rPredicted r-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_zPredicted z-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalflux_gModel flux in gREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB system)REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB system)REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB system)REALprincipalflux_ivar_zInverse variance of flux_zREALprincipalflux_rModel flux in rREALprincipalflux_w1WISE model flux in W1 (AB system)REALprincipalflux_w2WISE model flux in W2 (AB system)REALprincipalflux_w3WISE model flux in W3 (AB system)REALprincipalflux_w4WISE model flux in W4 (AB system)REALprincipalflux_zModel flux in zREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a sources flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a sources flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a sources flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalgaia_a_g_valGaia line-of-sight extinction in the G bandREALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_sigma5d_maxGaia longest semi-major axis of the 5-d error ellipsoidREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_e_bp_min_rp_valGaia line-of-sight reddening E(BP-RP)REALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magREALprincipalgaia_phot_bp_rp_excess_factorGaia BP/RP excess factorREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP band signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magREALprincipalgaldepth_gAs for psfdepth_g but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_rAs for psfdepth_r but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_zAs for psfdepth_z but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalg_rComputed (g-r) colorREALprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalmag_gConverted g magnitudeREALprincipalmag_rConverted r magnitudeREALprincipalmag_w1Converted W1 magnitudeREALprincipalmag_w2Converted W2 magnitudeREALprincipalmag_w3Converted W3 magnitudeREALprincipalmag_w4Converted W4 magnitudeREALprincipalmag_zConverted z magnitudeREALprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in w1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in w2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in w3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in w4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnea_gNoise equivalent area in gREALprincipalnea_rNoise equivalent area in rREALprincipalnea_zNoise equivalent area in zREALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each brickINTEGERprincipalparallax_ivarReference catalog inverse-variance on parallaxREALprincipalparallaxReference catalog parallaxREALprincipalpmdec_ivarReference catalog inverse-variance on pmdecREALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/(sqrt psfdepth_g) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_g))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_rFor a 5 sigma point source detection limit in r, 5/(sqrt psfdepth_r) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_r))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in z, 5/(sqrt psfdepth_z) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_z))-9]) gives corresponding AB magnitudeREALprincipalpsfsize_gWeighted average PSF FWHM in the g bandREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errorsREALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)REALprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalsersic_ivarInverse variance of sersicREALprincipalsersicPower-law index for the Sersic profile model (type=SER)REALprincipalshape_e1_ivarInverse variance of shape_e1REALprincipalshape_e1Ellipticity component 1 of galaxy model for galaxy type typeREALprincipalshape_e2_ivarInverse variance of shape_e2REALprincipalshape_e2Ellipticity component 2 of galaxy model for galaxy type typeREALprincipalshape_r_ivarInverse variance of shape_rREALprincipalshape_rHalf-light radius of galaxy model for galaxy type type (>0)arcsecREALprincipalsnr_gSignal-to-Noise ratio in gREALprincipalsnr_rSignal-to-Noise ratio in rREALprincipalsnr_w1Signal-to-Noise ratio in W1REALprincipalsnr_w2Signal-to-Noise ratio in W2REALprincipalsnr_w3Signal-to-Noise ratio in W3REALprincipalsnr_w4Signal-to-Noise ratio in W4REALprincipalsnr_zSignal-to-Noise ratio in zREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-w4) colorREALprincipalwise_xX position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_x and bx)REALprincipalwise_yY position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_y and by)REALprincipalz_w1Computed (z-w1) colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalfitbitsBitwise mask detailing pecularities of how an object was fit, as cataloged on the DR9 bitmasks pageSMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_params_solvedWhich astrometric parameters were estimated for a Gaia sourceSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia g band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP band number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalmaskbitsBitwise mask indicating that an object touches a pixel in the coadd/*/*/*maskbits* maps, as cataloged on the DR9 bitmasks pageSMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 for Tycho-2, G2 for Gaia DR2, L3 for the SGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, SER=Sersic, DUP=Gaia source fit by different model.VARCHARprincipalwise_coadd_idunWISE coadd brick name (corresponding to the, e.g., legacysurvey-<brick>-image-W1.fits.fz coadd file) for the center of each objectVARCHARprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_medianphoto-z derived from the median of the photo-z PDFREALprincipalz_phot_stdStandard deviation of the photo-zs derived from the photo-z PDFREALprincipalz_phot_l68Lower bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_u68Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_l95Lower bound of the 95% confidence region, derived from the photo-z PDFREALprincipalz_phot_u95Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_specSpectroscopic redshift, if availableREALprincipaltrainingWhether or not the spectroscopic redshift is used in photometric redshift trainingVARCHARprincipalsurveySource of the spectroscopic redshiftVARCHARprincipalnoirlab_test2.35_ls_dr9The noirlab ls_dr9.tractor table pre-joined with ls_dr9.x1p5__tractor__allwise__source, ls_dr9.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.glatGalactic LatitudeDOUBLEprincipalglonGalactic LongitudeDOUBLEprincipalpmdec_ivarReference catalog inverse-variance on pmdecREALprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalls_idUnique LS object IDBIGINTprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudeDOUBLEprincipalelonEcliptic LongitudeDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia DR2 and SGABIGINTprincipalbrickidBrick ID [1,662174]INTEGERprincipalblob_nea_gBlob-masked noise equivalent area in g.REALprincipalblob_nea_rBlob-masked noise equivalent area in r.REALprincipalblob_nea_zBlob-masked noise equivalent area in z.REALprincipalbxX position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipalbyY position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipaldchisq_1Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_2Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_3Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_4Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_5Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errorsREALprincipaldered_flux_gDereddened g band fluxREALprincipaldered_flux_rDereddened r band fluxREALprincipaldered_flux_w1Dereddened w1 band fluxREALprincipaldered_flux_w2Dereddened w2 band fluxREALprincipaldered_flux_w3Dereddened w3 band fluxREALprincipaldered_flux_w4Dereddened w4 band fluxREALprincipaldered_flux_zDereddened z band fluxREALprincipaldered_mag_gDereddened g-band magnitudeREALprincipaldered_mag_rDereddened r-band magnitudeREALprincipaldered_mag_w1Dereddened w1-band magnitudeREALprincipaldered_mag_w2Dereddened w2-band magnitudeREALprincipaldered_mag_w3Dereddened w3-band magnitudeREALprincipaldered_mag_w4Dereddened w4-band magnitudeREALprincipaldered_mag_zDereddened z-band magnitudeREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsREALprincipalfiberflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_rPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_zPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_rPredicted r-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_zPredicted z-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalflux_gModel flux in gREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB system)REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB system)REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB system)REALprincipalflux_ivar_zInverse variance of flux_zREALprincipalflux_rModel flux in rREALprincipalflux_w1WISE model flux in W1 (AB system)REALprincipalflux_w2WISE model flux in W2 (AB system)REALprincipalflux_w3WISE model flux in W3 (AB system)REALprincipalflux_w4WISE model flux in W4 (AB system)REALprincipalflux_zModel flux in zREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a sources flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a sources flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a sources flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalgaia_a_g_valGaia line-of-sight extinction in the G bandREALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_sigma5d_maxGaia longest semi-major axis of the 5-d error ellipsoidREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_e_bp_min_rp_valGaia line-of-sight reddening E(BP-RP)REALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magREALprincipalgaia_phot_bp_rp_excess_factorGaia BP/RP excess factorREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP band signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magREALprincipalgaldepth_gAs for psfdepth_g but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_rAs for psfdepth_r but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_zAs for psfdepth_z but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalg_rComputed (g-r) colorREALprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalmag_gConverted g magnitudeREALprincipalmag_rConverted r magnitudeREALprincipalmag_w1Converted W1 magnitudeREALprincipalmag_w2Converted W2 magnitudeREALprincipalmag_w3Converted W3 magnitudeREALprincipalmag_w4Converted W4 magnitudeREALprincipalmag_zConverted z magnitudeREALprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in w1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in w2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in w3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in w4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnea_gNoise equivalent area in gREALprincipalnea_rNoise equivalent area in rREALprincipalnea_zNoise equivalent area in zREALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each brickINTEGERprincipalparallax_ivarReference catalog inverse-variance on parallaxREALprincipalparallaxReference catalog parallaxREALprincipalpmdecReference catalog proper motion in the Dec directionREALprincipalpmra_ivarReference catalog inverse-variance on pmraREALprincipalpmraReference catalog proper motion in the RA directionREALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/(sqrt psfdepth_g) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_g))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_rFor a 5 sigma point source detection limit in r, 5/(sqrt psfdepth_r) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_r))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in z, 5/(sqrt psfdepth_z) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_z))-9]) gives corresponding AB magnitudeREALprincipalpsfsize_gWeighted average PSF FWHM in the g bandREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errorsREALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)REALprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalsersic_ivarInverse variance of sersicREALprincipalsersicPower-law index for the Sersic profile model (type=SER)REALprincipalshape_e1_ivarInverse variance of shape_e1REALprincipalshape_e1Ellipticity component 1 of galaxy model for galaxy type typeREALprincipalshape_e2_ivarInverse variance of shape_e2REALprincipalshape_e2Ellipticity component 2 of galaxy model for galaxy type typeREALprincipalshape_r_ivarInverse variance of shape_rREALprincipalshape_rHalf-light radius of galaxy model for galaxy type type (>0)arcsecREALprincipalsnr_gSignal-to-Noise ratio in gREALprincipalsnr_rSignal-to-Noise ratio in rREALprincipalsnr_w1Signal-to-Noise ratio in W1REALprincipalsnr_w2Signal-to-Noise ratio in W2REALprincipalsnr_w3Signal-to-Noise ratio in W3REALprincipalsnr_w4Signal-to-Noise ratio in W4REALprincipalsnr_zSignal-to-Noise ratio in zREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-w4) colorREALprincipalwise_xX position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_x and bx)REALprincipalwise_yY position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_y and by)REALprincipalz_w1Computed (z-w1) colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarSMALLINTprincipalfitbitsBitwise mask detailing pecularities of how an object was fit, as cataloged on the DR9 bitmasks pageSMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_params_solvedWhich astrometric parameters were estimated for a Gaia sourceSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia g band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP band number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalmaskbitsBitwise mask indicating that an object touches a pixel in the coadd/*/*/*maskbits* maps, as cataloged on the DR9 bitmasks pageSMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 for Tycho-2, G2 for Gaia DR2, L3 for the SGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, SER=Sersic, DUP=Gaia source fit by different model.VARCHARprincipalwise_coadd_idunWISE coadd brick name (corresponding to the, e.g., legacysurvey-<brick>-image-W1.fits.fz coadd file) for the center of each objectVARCHARprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_medianphoto-z derived from the median of the photo-z PDFREALprincipalz_phot_stdStandard deviation of the photo-zs derived from the photo-z PDFREALprincipalz_phot_l68Lower bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_u68Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_l95Lower bound of the 95% confidence region, derived from the photo-z PDFREALprincipalz_phot_u95Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_specSpectroscopic redshift, if availableREALprincipaltrainingWhether or not the spectroscopic redshift is used in photometric redshift trainingVARCHARprincipalsurveySource of the spectroscopic redshiftVARCHARprincipalnoirlab_test2.1_ls_dr9The noirlab ls_dr9.tractor table pre-joined with ls_dr9.x1p5__tractor__allwise__source, ls_dr9.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.flux_w2WISE model flux in W2 (AB system)REALprincipalflux_w3WISE model flux in W3 (AB system)REALprincipalflux_w4WISE model flux in W4 (AB system)REALprincipalflux_zModel flux in zREALprincipalparallaxReference catalog parallaxREALprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalls_idUnique LS object IDBIGINTprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudeDOUBLEprincipalelonEcliptic LongitudeDOUBLEprincipalglatGalactic LatitudeDOUBLEprincipalglonGalactic LongitudeDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectDOUBLEprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia DR2 and SGABIGINTprincipalbrickidBrick ID [1,662174]INTEGERprincipalblob_nea_gBlob-masked noise equivalent area in g.REALprincipalblob_nea_rBlob-masked noise equivalent area in r.REALprincipalblob_nea_zBlob-masked noise equivalent area in z.REALprincipalbxX position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipalbyY position (0-indexed) of coordinates in the brick image stack (i.e. in the e.g. legacysurvey-<brick>-image-g.fits.fz coadd file)REALprincipaldchisq_1Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_2Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_3Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_4Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldchisq_5Difference in chi^2 between successively more-complex model fits: PSF, REX, DEV, EXP, SER. The difference is versus no source.REALprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errorsREALprincipaldered_flux_gDereddened g band fluxREALprincipaldered_flux_rDereddened r band fluxREALprincipaldered_flux_w1Dereddened w1 band fluxREALprincipaldered_flux_w2Dereddened w2 band fluxREALprincipaldered_flux_w3Dereddened w3 band fluxREALprincipaldered_flux_w4Dereddened w4 band fluxREALprincipaldered_flux_zDereddened z band fluxREALprincipaldered_mag_gDereddened g-band magnitudeREALprincipaldered_mag_rDereddened r-band magnitudeREALprincipaldered_mag_w1Dereddened w1-band magnitudeREALprincipaldered_mag_w2Dereddened w2-band magnitudeREALprincipaldered_mag_w3Dereddened w3-band magnitudeREALprincipaldered_mag_w4Dereddened w4-band magnitudeREALprincipaldered_mag_zDereddened z-band magnitudeREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsREALprincipalfiberflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_rPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfiberflux_zPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_gPredicted g-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_rPredicted r-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalfibertotflux_zPredicted z-band flux within a fiber of diameter 1.5 arcsec from this object in 1 arcsec Gaussian seeingREALprincipalflux_gModel flux in gREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB system)REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB system)REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB system)REALprincipalflux_ivar_zInverse variance of flux_zREALprincipalflux_rModel flux in rREALprincipalflux_w1WISE model flux in W1 (AB system)REALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a sources flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a sources flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a sources flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalgaia_a_g_valGaia line-of-sight extinction in the G bandREALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_sigma5d_maxGaia longest semi-major axis of the 5-d error ellipsoidREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_e_bp_min_rp_valGaia line-of-sight reddening E(BP-RP)REALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magREALprincipalgaia_phot_bp_rp_excess_factorGaia BP/RP excess factorREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP band signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magREALprincipalgaldepth_gAs for psfdepth_g but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_rAs for psfdepth_r but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalgaldepth_zAs for psfdepth_z but for a galaxy (0.45 arcsec exp, round) detection sensitivityREALprincipalg_rComputed (g-r) colorREALprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalmag_gConverted g magnitudeREALprincipalmag_rConverted r magnitudeREALprincipalmag_w1Converted W1 magnitudeREALprincipalmag_w2Converted W2 magnitudeREALprincipalmag_w3Converted W3 magnitudeREALprincipalmag_w4Converted W4 magnitudeREALprincipalmag_zConverted z magnitudeREALprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in w1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in w2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in w3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in w4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnea_gNoise equivalent area in gREALprincipalnea_rNoise equivalent area in rREALprincipalnea_zNoise equivalent area in zREALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each brickINTEGERprincipalparallax_ivarReference catalog inverse-variance on parallaxREALprincipalpmdec_ivarReference catalog inverse-variance on pmdecREALprincipalpmdecReference catalog proper motion in the Dec directionREALprincipalpmra_ivarReference catalog inverse-variance on pmraREALprincipalpmraReference catalog proper motion in the RA directionREALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/(sqrt psfdepth_g) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_g))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_rFor a 5 sigma point source detection limit in r, 5/(sqrt psfdepth_r) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_r))-9]) gives corresponding AB magnitudeREALprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in z, 5/(sqrt psfdepth_z) gives flux in nanomaggies and (-2.5[log10(5/(sqrt psfdepth_z))-9]) gives corresponding AB magnitudeREALprincipalpsfsize_gWeighted average PSF FWHM in the g bandREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errorsREALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)REALprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalsersic_ivarInverse variance of sersicREALprincipalsersicPower-law index for the Sersic profile model (type=SER)REALprincipalshape_e1_ivarInverse variance of shape_e1REALprincipalshape_e1Ellipticity component 1 of galaxy model for galaxy type typeREALprincipalshape_e2_ivarInverse variance of shape_e2REALprincipalshape_e2Ellipticity component 2 of galaxy model for galaxy type typeREALprincipalshape_r_ivarInverse variance of shape_rREALprincipalshape_rHalf-light radius of galaxy model for galaxy type type (>0)arcsecREALprincipalsnr_gSignal-to-Noise ratio in gREALprincipalsnr_rSignal-to-Noise ratio in rREALprincipalsnr_w1Signal-to-Noise ratio in W1REALprincipalsnr_w2Signal-to-Noise ratio in W2REALprincipalsnr_w3Signal-to-Noise ratio in W3REALprincipalsnr_w4Signal-to-Noise ratio in W4REALprincipalsnr_zSignal-to-Noise ratio in zREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-w4) colorREALprincipalwise_xX position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_x and bx)REALprincipalwise_yY position of coordinates in the brick image stack that corresponds to wise_coadd_id (see the DR9 updates page for transformations between wise_y and by)REALprincipalz_w1Computed (z-w1) colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR9 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR9 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarSMALLINTprincipalfitbitsBitwise mask detailing pecularities of how an object was fit, as cataloged on the DR9 bitmasks pageSMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_params_solvedWhich astrometric parameters were estimated for a Gaia sourceSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia g band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP band number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalmaskbitsBitwise mask indicating that an object touches a pixel in the coadd/*/*/*maskbits* maps, as cataloged on the DR9 bitmasks pageSMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR9 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 for Tycho-2, G2 for Gaia DR2, L3 for the SGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, SER=Sersic, DUP=Gaia source fit by different model.VARCHARprincipalwise_coadd_idunWISE coadd brick name (corresponding to the, e.g., legacysurvey-<brick>-image-W1.fits.fz coadd file) for the center of each objectVARCHARprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_medianphoto-z derived from the median of the photo-z PDFREALprincipalz_phot_stdStandard deviation of the photo-zs derived from the photo-z PDFREALprincipalz_phot_l68Lower bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_u68Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_phot_l95Lower bound of the 95% confidence region, derived from the photo-z PDFREALprincipalz_phot_u95Upper bound of the 68% confidence region, derived from the photo-z PDFREALprincipalz_specSpectroscopic redshift, if availableREALprincipaltrainingWhether or not the spectroscopic redshift is used in photometric redshift trainingVARCHARprincipalsurveySource of the spectroscopic redshiftVARCHARprincipalnoirlab_test2.36_des_dr2The noirlab des_dr2.main table pre-joined with des_dr2.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalalphawin_j2000right ascension for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalawin_image_gg-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_ii-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_rr-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_yy-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_zz-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipala_imagemajor axis size based on an isophotal model [pixel]pixelREALprincipalbackground_gg-band background level, by ccd-amplifier [mag]magREALprincipalbackground_ii-band background level, by ccd-amplifier [mag]magREALprincipalbackground_rr-band background level, by ccd-amplifier [mag]magREALprincipalbackground_yy-band background level, by ccd-amplifier [mag]magREALprincipalbackground_zz-band background level, by ccd-amplifier [mag]magREALprincipalbwin_image_gg-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_ii-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_rr-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_yy-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_zz-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalb_imageminor axis size based on an isophotal model [pixel]pixelREALprincipalclass_star_gg-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_ii-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_rr-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_yy-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_zz-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalcoadd_object_idunique identifier for the coadded objectsmeta.id;meta.mainBIGINTindexedprincipaldecdeclination, with quantized precision for indexing (deltawin_j2000 has full precision but not indexed) [degrees]degpos.eq.dec;meta.mainDOUBLEindexedprincipaldeltawin_j2000declination for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalebv_sfd98e(b-v) reddening coefficient from schlegel, finkbeiner & davis, 1998 [mag]magDOUBLEprincipalerrawin_image_gg-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_ii-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_rr-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_yy-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_zz-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerra_imageuncertainty in major axis size, from isophotal model [pixel]pixelREALprincipalerrbwin_image_gg-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_ii-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_rr-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_yy-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_zz-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrb_imageuncertainty in minor axis size, from isophotal model [pixel]pixelREALprincipalerrthetawin_image_gg-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_ii-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_rr-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_yy-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_zz-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrtheta_imageuncertainty in source position, from isophotal model [degrees]degREALprincipalerrx2win_image_gg-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_ii-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_rr-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_yy-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_zz-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_gg-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_ii-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_rr-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_yy-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_zz-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_gg-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_ii-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_rr-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_yy-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_zz-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalextended_class_coadd0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using sextractor photometrySMALLINTprincipalextended_class_wavg0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using wavg photometrySMALLINTprincipalflags_gg-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_ii-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_rr-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_yy-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_zz-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalfluxerr_auto_gg-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_ii-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_rr-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_yy-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_zz-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_gg-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_ii-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_rr-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_yy-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_zz-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_radius_gg-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_ii-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_rr-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_yy-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_zz-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_gg-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_ii-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_rr-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_yy-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_zz-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalgalactic_bgalactic latitude [degrees]degpos.galactic.latREALprincipalgalactic_lgalactic longitude [degrees]degpos.galactic.lonREALprincipalhpix_1024healpix identifier for nside=1024 grid size, in a nested schemaBIGINTprincipalhpix_16384healpix identifier for nside=16384 grid size, in a nested schemaBIGINTprincipalhpix_32healpix identifier for nside=32 grid size, in a nested schemaBIGINTprincipalhpix_4096healpix identifier for nside=4096 grid size, in a nested schemaBIGINTprincipalhpix_64healpix identifier for nside=64 grid size, in a nested schemaBIGINTprincipalimaflags_iso_gg-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_ii-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_rr-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_yy-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_zz-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalisoarea_image_gg-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_ii-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_rr-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_yy-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_zz-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalkron_radiuskron radius measured from detection image [pixel]pixelREALprincipalkron_radius_gg-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_ii-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_rr-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_yy-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_zz-band kron radius measured from coadded image [pixel]pixelREALprincipalmagerr_auto_gg-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_ii-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_rr-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_yy-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_zz-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_gg-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_g_deredg-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_ii-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_i_deredi-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_rr-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_r_deredr-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_yy-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_y_deredy-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_zz-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_z_deredz-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalnepochs_gg-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_ii-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_rr-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_yy-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_zz-band number of epochs the source is detected in single epoch imagesINTEGERprincipalniter_model_gg-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_ii-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_rr-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_yy-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_zz-band number of iterations in model fitting photometric measurementsINTEGERprincipalraright ascension, with quantized precision for indexing (alphawin_j2000 has full precision but not indexed) [degrees]degpos.eq.ra;meta.mainDOUBLEindexedprincipalspreaderr_model_gg-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_ii-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_rr-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_yy-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_zz-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspread_model_gg-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_ii-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_rr-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_yy-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_zz-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalthetawin_image_gg-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_ii-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_rr-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_yy-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_zz-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipaltheta_j2000position angle of source in j2000 coordinates, from non-windowed measurement [degrees]degREALprincipaltilenameidentifier of each one of the tiles on which the survey is griddedVARCHARprincipalwavg_fluxerr_psf_gg-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_ii-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_rr-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_yy-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_zz-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_gg-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_ii-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_rr-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_yy-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_zz-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_magerr_psf_gg-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_ii-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_rr-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_yy-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_zz-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_gg-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_g_deredg-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_ii-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_i_deredi-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_rr-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_r_deredr-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_yy-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_y_deredy-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_zz-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_z_deredz-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_spreaderr_model_gg-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_ii-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_rr-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_yy-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_zz-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_gg-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_ii-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_rr-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_yy-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_zz-band spread model using the weighted averaged values from single epoch detectionsREALprincipalx2win_image_gg-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_ii-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_rr-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_yy-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_zz-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxwin_imagex-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalxwin_image_gg-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_ii-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_rr-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_yy-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_zz-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxywin_image_gg-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_ii-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_rr-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_yy-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_zz-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_gg-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_ii-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_rr-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_yy-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_zz-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalywin_imagey-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalywin_image_gg-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_ii-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_rr-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_yy-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_zz-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalhtm9Ninth level (~10 arcmin resolution) Hierarchical Triangular Mesh index (Szalay et al. 2007)meta.codeINTEGERprincipalnest4096Nested-scheme HEALPix (Gorski et al. 2005) index with NSIDE=4096 (~1 arcmin resolution)meta.codeINTEGERprincipalring256Ring-scheme HEALPix (Gorski et al. 2005) index with NSIDE=256 (~14 arcmin resolution)meta.codeINTEGERprincipalg_rG-R colormagphot.colorREALprincipalr_iR-I colormagphot.colorREALprincipali_zI-Z colormagphot.colorREALprincipalz_yZ-Y colormagphot.colorREALprincipalsnr_gS/N in g-bandmagstat.snrREALprincipalsnr_rS/N in r-bandmagstat.snrREALprincipalsnr_iS/N in i-bandmagstat.snrREALprincipalsnr_yS/N in Y-bandmagstat.snrREALprincipalsnr_zS/N in z-bandmagstat.snrREALprincipalecliptic_latEcliptic Latitudedegpos.ecliptic.latDOUBLEprincipalecliptic_lonEcliptic Longitudedegpos.ecliptic.lonDOUBLEprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalnoirlab_test2.36_des_dr1The noirlab des_dr1.main table pre-joined with des_dr1.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.ywin_image_iY-centroid from windowed measurements on coadded imageVARCHARprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalcoadd_object_idUnique identifier for the coadded objectsVARCHARprincipalhpix_32Healpix ID for nside=32, nested schemaVARCHARprincipalhpix_64Healpix ID for nside=64, nested schemaVARCHARprincipalhpix_1024Healpix ID for nside=1024, nested schemaVARCHARprincipalhpix_4096Healpix ID for nside=4096, nested schemaVARCHARprincipalhpix_16384Healpix ID for nside=16384, nested schemaVARCHARprincipalraRight ascension, with quantized precision for indexing (ALPHAWIN_J2000 has full precision but not indexed)degpos.eq.raVARCHARprincipaldecDeclination, with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed)degpos.eq.decVARCHARprincipalalphawin_j2000Right ascension for the object, J2000 in ICRS system (full precision but not indexed)degVARCHARprincipaldeltawin_j2000Declination for the object, J2000 in ICRS (full precision but not indexed)degVARCHARprincipalgalactic_lGalactic LongitudedegVARCHARprincipalgalactic_bGalactic LatitudedegVARCHARprincipalecliptic_lonEcliptic LongitudedegVARCHARprincipalecliptic_latEcliptic LatitudedegVARCHARprincipalxwin_imageX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_imageY-centroid from windowed measurements on coadded imagepixelVARCHARprincipalerrx2win_image_gUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_rUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_iUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_zUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_yUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_gUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_rUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_iUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_zUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_yUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_gUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_rUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_iUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_zUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_yUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalx2win_image_gSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_rSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_iSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_zSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_ySecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_gSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_rSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_iSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_zSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_ySecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_gSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_rSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_iSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_zSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_ySecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxwin_image_gX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_rX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_iX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_zX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_yX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_image_gY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_rY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_zY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_yY-centroid from windowed measurements on coadded imageVARCHARprincipala_imageMajor axis size based on an isophotal modelpixelVARCHARprincipalerra_imageUncertainty in major axis size, from isophotal modelpixelVARCHARprincipalb_imageMinor axis size based on an isophotal modelpixelVARCHARprincipalerrb_imageUncertainty in minor axis size, from isophotal modelpixelVARCHARprincipaltheta_j2000Position angle of source in J2000 coordinates, from non-windowed measurementdegVARCHARprincipalerrtheta_imageUncertainty in source position, from isophotal modeldegVARCHARprincipalkron_radiusKron radiuspixelVARCHARprincipalebv_sfd98E(B-V) reddening oefficient from Schelgel, Finkbeiner & Davis (1998)magVARCHARprincipalmag_auto_g_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_r_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_i_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_z_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_y_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_aper_8_g_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_r_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_i_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_z_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_y_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalwavg_mag_psf_g_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_r_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_i_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_z_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_y_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalawin_image_gMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_rMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_iMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_zMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_yMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_gMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_rMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_iMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_zMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_yMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalthetawin_image_gPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_rPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_iPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_zPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_yPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalerrawin_image_gUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_rUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_iUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_zUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_yUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_gUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_rUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_iUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_zUncertainty in Minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_yUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrthetawin_image_gUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_rUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_iUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_zUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_yUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalflux_radius_gHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_rHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_iHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_zHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_yHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_gFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_rFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_iFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_zFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_yFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalbackground_gBackground level, by CCD-amplifiermagVARCHARprincipalbackground_rBackground level, by CCD-amplifiermagVARCHARprincipalbackground_iBackground level, by CCD-amplifiermagVARCHARprincipalbackground_zBackground level, by CCD-amplifiermagVARCHARprincipalbackground_yBackground level, by CCD-amplifiermagVARCHARprincipalkron_radius_gKron radius measured from detection imagepixelVARCHARprincipalkron_radius_rKron radius measured from detection imagepixelVARCHARprincipalkron_radius_iKron radius measured from detection imagepixelVARCHARprincipalkron_radius_zKron radius measured from detection imagepixelVARCHARprincipalkron_radius_yKron radius measured from detection imagepixelVARCHARprincipalmag_auto_gMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_rMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_iMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_zMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_yMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_gUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_rUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_iUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_zUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_yUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmag_aper_8_gMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_rMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_iMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_zMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_yMagnitude estimation for circular aperturesmagVARCHARprincipalmagerr_aper_8_gUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_rUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_iUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_zUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_yUncertainty in magnitude estimation for circular aperturesVARCHARprincipalwavg_mag_psf_gWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_rWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_iWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_zWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_yWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_gUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_rUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_iUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_zUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_yUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalflux_auto_gFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_rFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_iFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_zFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_yFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_guncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_runcertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_iuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_zuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_yuncertainty in flux measurement, for an elliptical model based on Kron radiusVARCHARprincipalflux_aper_8_gFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_rFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_iFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_zFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_yFlux measurement for circular aperturesADUVARCHARprincipalfluxerr_aper_8_gUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_rUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_iUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_zUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_yUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalwavg_flux_psf_gWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_rWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_iWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_zWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_yWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_gUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_rUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_iUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_zUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_yUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalclass_star_gSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_rSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_iSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_zSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_ySimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalspread_model_gMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_rMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_iMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_zMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_yMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalwavg_spread_model_gSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_rSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_iSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_zSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_ySPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalspreaderr_model_gUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_rUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_iUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_zUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_yUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalwavg_spreaderr_model_gUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_rUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_iUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_zUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_yUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalg_rG-R colorVARCHARprincipalr_iR-I colorVARCHARprincipali_zI-Z colorVARCHARprincipalz_yZ-Y colorVARCHARprincipalsnr_gS/NVARCHARprincipalsnr_rS/NVARCHARprincipalsnr_iS/NVARCHARprincipalsnr_zS/NVARCHARprincipalsnr_yS/NVARCHARprincipalimaflags_iso_gFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_gNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_rFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_rNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_iFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_iNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_zFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_zNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_yFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_yNumber of epochs the source in detected in single epoch imagesVARCHARprincipalhtm9HTM Level-9 indexVARCHARprincipalring256Healpix ID with nside=256, ring schemaVARCHARprincipalnest4096Healpix ID with nside=4096, nested schemaVARCHARprincipalisoarea_image_gIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_rIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_iIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_zIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_yIsophotal area of the coadded sourcepixel^2VARCHARprincipalniter_model_gNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_rNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_iNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_zNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_yNumber of iterations in model fitting photometric measurementsVARCHARprincipalflags_gAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_rAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_iAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_zAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_yAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipaltilenameTile nameVARCHARprincipalnoirlab_test2.35_des_dr2The noirlab des_dr2.main table pre-joined with des_dr2.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.hpix_16384healpix identifier for nside=16384 grid size, in a nested schemaBIGINTprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalalphawin_j2000right ascension for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalawin_image_gg-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_ii-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_rr-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_yy-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_zz-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipala_imagemajor axis size based on an isophotal model [pixel]pixelREALprincipalbackground_gg-band background level, by ccd-amplifier [mag]magREALprincipalbackground_ii-band background level, by ccd-amplifier [mag]magREALprincipalbackground_rr-band background level, by ccd-amplifier [mag]magREALprincipalbackground_yy-band background level, by ccd-amplifier [mag]magREALprincipalbackground_zz-band background level, by ccd-amplifier [mag]magREALprincipalbwin_image_gg-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_ii-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_rr-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_yy-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_zz-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalb_imageminor axis size based on an isophotal model [pixel]pixelREALprincipalclass_star_gg-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_ii-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_rr-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_yy-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_zz-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalcoadd_object_idunique identifier for the coadded objectsmeta.id;meta.mainBIGINTindexedprincipaldecdeclination, with quantized precision for indexing (deltawin_j2000 has full precision but not indexed) [degrees]degpos.eq.dec;meta.mainDOUBLEindexedprincipaldeltawin_j2000declination for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalebv_sfd98e(b-v) reddening coefficient from schlegel, finkbeiner & davis, 1998 [mag]magDOUBLEprincipalerrawin_image_gg-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_ii-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_rr-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_yy-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_zz-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerra_imageuncertainty in major axis size, from isophotal model [pixel]pixelREALprincipalerrbwin_image_gg-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_ii-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_rr-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_yy-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_zz-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrb_imageuncertainty in minor axis size, from isophotal model [pixel]pixelREALprincipalerrthetawin_image_gg-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_ii-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_rr-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_yy-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_zz-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrtheta_imageuncertainty in source position, from isophotal model [degrees]degREALprincipalerrx2win_image_gg-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_ii-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_rr-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_yy-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_zz-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_gg-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_ii-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalhpix_32healpix identifier for nside=32 grid size, in a nested schemaBIGINTprincipalerrxywin_image_rr-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_yy-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_zz-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_gg-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_ii-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_rr-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_yy-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_zz-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalextended_class_coadd0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using sextractor photometrySMALLINTprincipalextended_class_wavg0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using wavg photometrySMALLINTprincipalflags_gg-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_ii-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_rr-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_yy-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_zz-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalfluxerr_auto_gg-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_ii-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_rr-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_yy-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_zz-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_gg-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_ii-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_rr-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_yy-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_zz-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_radius_gg-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_ii-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_rr-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_yy-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_zz-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_gg-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_ii-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_rr-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_yy-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_zz-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalgalactic_bgalactic latitude [degrees]degpos.galactic.latREALprincipalgalactic_lgalactic longitude [degrees]degpos.galactic.lonREALprincipalhpix_1024healpix identifier for nside=1024 grid size, in a nested schemaBIGINTprincipalhpix_4096healpix identifier for nside=4096 grid size, in a nested schemaBIGINTprincipalhpix_64healpix identifier for nside=64 grid size, in a nested schemaBIGINTprincipalimaflags_iso_gg-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_ii-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_rr-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_yy-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_zz-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalisoarea_image_gg-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_ii-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_rr-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_yy-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_zz-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalkron_radiuskron radius measured from detection image [pixel]pixelREALprincipalkron_radius_gg-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_ii-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_rr-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_yy-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_zz-band kron radius measured from coadded image [pixel]pixelREALprincipalmagerr_auto_gg-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_ii-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_rr-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_yy-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_zz-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_gg-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_g_deredg-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_ii-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_i_deredi-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_rr-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_r_deredr-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_yy-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_y_deredy-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_zz-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_z_deredz-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalnepochs_gg-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_ii-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_rr-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_yy-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_zz-band number of epochs the source is detected in single epoch imagesINTEGERprincipalniter_model_gg-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_ii-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_rr-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_yy-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_zz-band number of iterations in model fitting photometric measurementsINTEGERprincipalraright ascension, with quantized precision for indexing (alphawin_j2000 has full precision but not indexed) [degrees]degpos.eq.ra;meta.mainDOUBLEindexedprincipalspreaderr_model_gg-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_ii-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_rr-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_yy-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_zz-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspread_model_gg-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_ii-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_rr-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_yy-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_zz-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalthetawin_image_gg-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_ii-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_rr-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_yy-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_zz-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipaltheta_j2000position angle of source in j2000 coordinates, from non-windowed measurement [degrees]degREALprincipaltilenameidentifier of each one of the tiles on which the survey is griddedVARCHARprincipalwavg_fluxerr_psf_gg-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_ii-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_rr-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_yy-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_zz-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_gg-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_ii-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_rr-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_yy-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_zz-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_magerr_psf_gg-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_ii-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_rr-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_yy-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_zz-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_gg-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_g_deredg-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_ii-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_i_deredi-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_rr-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_r_deredr-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_yy-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_y_deredy-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_zz-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_z_deredz-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_spreaderr_model_gg-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_ii-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_rr-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_yy-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_zz-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_gg-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_ii-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_rr-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_yy-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_zz-band spread model using the weighted averaged values from single epoch detectionsREALprincipalx2win_image_gg-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_ii-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_rr-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_yy-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_zz-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxwin_imagex-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalxwin_image_gg-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_ii-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_rr-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_yy-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_zz-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxywin_image_gg-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_ii-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_rr-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_yy-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_zz-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_gg-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_ii-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_rr-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_yy-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_zz-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalywin_imagey-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalywin_image_gg-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_ii-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_rr-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_yy-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_zz-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalhtm9Ninth level (~10 arcmin resolution) Hierarchical Triangular Mesh index (Szalay et al. 2007)meta.codeINTEGERprincipalnest4096Nested-scheme HEALPix (Gorski et al. 2005) index with NSIDE=4096 (~1 arcmin resolution)meta.codeINTEGERprincipalring256Ring-scheme HEALPix (Gorski et al. 2005) index with NSIDE=256 (~14 arcmin resolution)meta.codeINTEGERprincipalg_rG-R colormagphot.colorREALprincipalr_iR-I colormagphot.colorREALprincipali_zI-Z colormagphot.colorREALprincipalz_yZ-Y colormagphot.colorREALprincipalsnr_gS/N in g-bandmagstat.snrREALprincipalsnr_rS/N in r-bandmagstat.snrREALprincipalsnr_iS/N in i-bandmagstat.snrREALprincipalsnr_yS/N in Y-bandmagstat.snrREALprincipalsnr_zS/N in z-bandmagstat.snrREALprincipalecliptic_latEcliptic Latitudedegpos.ecliptic.latDOUBLEprincipalecliptic_lonEcliptic Longitudedegpos.ecliptic.lonDOUBLEprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalnoirlab_test2.34_ls_dr8The noirlab ls_dr8.tractor table pre-joined with ls_dr8.x1p5__tractor__allwise__source, ls_dr8.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.dered_flux_w4Dereddened W1 fluxnanomaggiesREALprincipalflux_rmodel flux in rREALprincipalflux_zmodel flux in zREALprincipaldered_flux_w2Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w3Dereddened W1 fluxnanomaggiesREALprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudedegDOUBLEprincipalelonEcliptic LongitudedegDOUBLEprincipalglatGalactic LatitudedegDOUBLEprincipalglonGalactic LongitudedegDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalbrickidBrick ID [1,662174]INTEGERprincipalbrightblobbitwise mask indicating that an object is near a bright foreground source, as cataloged on the DR8 bitmasks page (http://legacysurvey.org/dr8/bitmasksDR8 bitmasks)SMALLINTprincipalbxX position (0-indexed) of coordinates in brick image stackpixREALprincipalbyY position (0-indexed) of coordinates in brick image stackpixREALprincipaldchisq_1Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_2Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_3Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_4Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_5Difference in X^2 between successfully more-complex model fitsREALprincipalls_idUnique LS object ID from RELEASE, BRICKID, OBJIDBIGINTprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errors1/deg^2REALprincipaldered_flux_gDereddened G-band fluxnanomaggiesREALprincipaldered_flux_rDereddened R-band fluxnanomaggiesREALprincipaldered_flux_w1Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_zDereddened Z-band fluxnanomaggiesREALprincipaldered_mag_gDereddened G-band magnitudemagREALprincipaldered_mag_rDereddened R-band magnitudemagREALprincipaldered_mag_w1Dereddened W1 magnitudemagREALprincipaldered_mag_w2Dereddened W2 magnitudemagREALprincipaldered_mag_w3Dereddened W3 magnitudemagREALprincipaldered_mag_w4Dereddened W4 magnitudemagREALprincipaldered_mag_zDereddened Z-band magnitudemagREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsmagREALprincipalfiberflux_gPredicted g-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_rPredicted r-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_zPredicted z-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_gPredicted g-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_rPredicted r-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_zPredicted z-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)1/nanomaggies^2REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB)1/nanomaggies^2REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB)1/nanomaggies^2REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB)1/nanomaggies^2REALprincipalflux_w1WISE model flux in W1 (AB system)nanomaggiesREALprincipalflux_w2WISE model flux in W2 (AB)nanomaggiesREALprincipalflux_w3WISE model flux in W3 (AB)nanomaggiesREALprincipalflux_w4WISE model flux in W4 (AB)nanomaggiesREALprincipalfracdevFraction of model in deVauc [0,1]REALprincipalfracdev_ivarInverse variance of fracdevREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a source flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a source flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a source flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in r, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in z, strictly between [0,1]REALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magmagREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magmagREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magmagREALprincipalgaldepth_gAs for PSFDEPTH_G but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalshapedev_rHalf-light radius of deVaucouleurs model (>0)arcsecREALprincipalgaldepth_rAs for PSFDEPTH_R but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_zAs for PSFDEPTH_Z but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalg_rComputed (g-r) colorREALprincipalhtm9HTM index (order 9 => ~10 arcmin size)meta.codeINTEGERprincipalmag_gConverted G magnitudemagREALprincipalmag_rConverted R magnitudemagREALprincipalmag_w1W1 magnitudemagREALprincipalmag_w2W2 magnitudemagREALprincipalmag_w3W3 magnitudemagREALprincipalmag_w4W4 magnitudemagREALprincipalmag_zConverted Z magnitudemagREALprincipalmaskbitsbitwise mask indicating that an object touches a pixel in the coadd maskbits maps, as cataloged on the DR8 bitmasks pageSMALLINTprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in W1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in W2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in W3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in W4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each blobINTEGERprincipalparallaxReference catalog parallaxmasREALprincipalparallax_ivarReference catalog inverse-variance on parallax1/(mas)^2REALprincipalpmdecReference catalog proper motion in the Dec directionmas / yrREALprincipalpmdec_ivarReference catalog inverse-variance on pmdec1/(mas/yr)^2REALprincipalpmraReference catalog proper motion in the RA directionmas / yrREALprincipalpmra_ivarReference catalog inverse-variance on pmra1/(mas/yr)^2REALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_g) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_g)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_rFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_r) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_r)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_z) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_z)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfsize_gWeighted average PSF FWHM in the g bandarcsecREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandarcsecREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandarcsecREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errors1/deg^2REALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)yrREALprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia-DR2 and LSLGABIGINTprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalshapedev_e1Ellipticity component 1REALprincipalshapedev_e1_ivarInverse variance of shapedev_e1REALprincipalshapedev_e2Ellipticity component 2REALprincipalshapedev_e2_ivarInverse variance of shapedev_e2REALprincipalshapedev_r_ivarInverse variance of shapedev_r1/arcsec^2REALprincipalshapeexp_e1Ellipticity component 1REALprincipalshapeexp_e1_ivarInverse variance of shapeexp_e1REALprincipalshapeexp_e2Ellipticity component 2REALprincipalshapeexp_e2_ivarInverse variance of shapeexp_e2REALprincipalshapeexp_rHalf-light radius of exponential model (>0)arcsecREALprincipalshapeexp_r_ivarInverse variance of shapeexp_r1/arcsec^2REALprincipalsnr_gSignal-to-Noise ratio in Gstat.ratioREALprincipalsnr_rSignal-to-Noise ratio in Rstat.ratioREALprincipalsnr_w1Signal-to-Noise ratio in W1stat.ratioREALprincipalsnr_w2Signal-to-Noise ratio in W2stat.ratioREALprincipalsnr_w3Signal-to-Noise ratio in W3stat.ratioREALprincipalsnr_w4Signal-to-Noise ratio in W4stat.ratioREALprincipalsnr_zSignal-to-Noise ratio in Zstat.ratioREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-d4) colorREALprincipalz_w1Computed (z-w1 colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarySMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia G band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalgaia_pointsourceThis Gaia DR2 source is believed to be a star, not a galaxySMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 forTycho-2, G2 for Gaia DR2, L2 for the LSLGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, COMP=composite, DUP=Gaia source fit by different model. Note that in some FITS readers, a trailing space may be appended for PSF , DEV and EXP since the column data type is a 4-character stringVARCHARprincipalwise_coadd_idunWISE coadd file name for the center of each objectVARCHARprincipalflux_gmodel flux in gREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_zInverse variance of flux_zREALprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_median(recommended) photo-z derived from the median of the photo-z PDFREALprincipalz_phot_stdstandard deviation of the photo-z derived from the photo-z PDFREALprincipalz_phot_l68lower 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_u68upper 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_l95lower 95% confidence limit derived from the photo-z PDFREALprincipalz_phot_u95upper 95% confidence limit derived from the photo-z PDFREALprincipalz_specspectroscopic redshift, if availableREALprincipalsurveysource of the spectroscopic redshiftVARCHARprincipaltrainingwhether or not the spectroscopic redshift is used for the photo-z trainingVARCHARprincipalnoirlab_test2.34_des_dr1The noirlab des_dr1.main table pre-joined with des_dr1.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalcoadd_object_idUnique identifier for the coadded objectsVARCHARprincipalhpix_32Healpix ID for nside=32, nested schemaVARCHARprincipalhpix_64Healpix ID for nside=64, nested schemaVARCHARprincipalhpix_1024Healpix ID for nside=1024, nested schemaVARCHARprincipalhpix_4096Healpix ID for nside=4096, nested schemaVARCHARprincipalhpix_16384Healpix ID for nside=16384, nested schemaVARCHARprincipalraRight ascension, with quantized precision for indexing (ALPHAWIN_J2000 has full precision but not indexed)degpos.eq.raVARCHARprincipaldecDeclination, with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed)degpos.eq.decVARCHARprincipalalphawin_j2000Right ascension for the object, J2000 in ICRS system (full precision but not indexed)degVARCHARprincipaldeltawin_j2000Declination for the object, J2000 in ICRS (full precision but not indexed)degVARCHARprincipalgalactic_lGalactic LongitudedegVARCHARprincipalgalactic_bGalactic LatitudedegVARCHARprincipalecliptic_lonEcliptic LongitudedegVARCHARprincipalecliptic_latEcliptic LatitudedegVARCHARprincipalxwin_imageX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_imageY-centroid from windowed measurements on coadded imagepixelVARCHARprincipalerrx2win_image_gUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_rUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_iUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_zUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_yUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_gUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_rUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_iUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_zUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_yUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_gUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_rUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_iUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_zUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_yUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalx2win_image_gSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_rSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_iSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_zSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_ySecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_gSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_rSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_iSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_zSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_ySecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_gSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_rSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_iSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_zSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_ySecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxwin_image_gX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_rX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_iX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_zX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_yX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_image_gY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_rY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_iY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_zY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_yY-centroid from windowed measurements on coadded imageVARCHARprincipala_imageMajor axis size based on an isophotal modelpixelVARCHARprincipalerra_imageUncertainty in major axis size, from isophotal modelpixelVARCHARprincipalb_imageMinor axis size based on an isophotal modelpixelVARCHARprincipalerrb_imageUncertainty in minor axis size, from isophotal modelpixelVARCHARprincipaltheta_j2000Position angle of source in J2000 coordinates, from non-windowed measurementdegVARCHARprincipalerrtheta_imageUncertainty in source position, from isophotal modeldegVARCHARprincipalkron_radiusKron radiuspixelVARCHARprincipalebv_sfd98E(B-V) reddening oefficient from Schelgel, Finkbeiner & Davis (1998)magVARCHARprincipalmag_auto_g_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_r_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_i_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_z_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_y_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_aper_8_g_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_r_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_i_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_z_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_y_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalwavg_mag_psf_g_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_r_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_i_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_z_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_y_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalawin_image_gMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_rMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_iMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_zMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_yMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_gMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_rMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_iMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_zMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_yMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalthetawin_image_gPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_rPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_iPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_zPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_yPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalerrawin_image_gUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_rUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_iUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_zUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_yUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_gUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_rUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_iUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_zUncertainty in Minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_yUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrthetawin_image_gUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_rUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_iUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_zUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_yUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalflux_radius_gHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_rHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_iHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_zHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_yHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_gFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_rFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_iFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_zFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_yFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalbackground_gBackground level, by CCD-amplifiermagVARCHARprincipalbackground_rBackground level, by CCD-amplifiermagVARCHARprincipalbackground_iBackground level, by CCD-amplifiermagVARCHARprincipalbackground_zBackground level, by CCD-amplifiermagVARCHARprincipalbackground_yBackground level, by CCD-amplifiermagVARCHARprincipalkron_radius_gKron radius measured from detection imagepixelVARCHARprincipalkron_radius_rKron radius measured from detection imagepixelVARCHARprincipalkron_radius_iKron radius measured from detection imagepixelVARCHARprincipalkron_radius_zKron radius measured from detection imagepixelVARCHARprincipalkron_radius_yKron radius measured from detection imagepixelVARCHARprincipalmag_auto_gMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_rMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_iMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_zMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_yMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_gUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_rUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_iUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_zUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_yUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmag_aper_8_gMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_rMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_iMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_zMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_yMagnitude estimation for circular aperturesmagVARCHARprincipalmagerr_aper_8_gUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_rUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_iUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_zUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_yUncertainty in magnitude estimation for circular aperturesVARCHARprincipalwavg_mag_psf_gWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_rWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_iWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_zWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_yWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_gUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_rUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_iUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_zUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_yUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalflux_auto_gFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_rFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_iFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_zFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_yFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_guncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_runcertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_iuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_zuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_yuncertainty in flux measurement, for an elliptical model based on Kron radiusVARCHARprincipalflux_aper_8_gFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_rFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_iFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_zFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_yFlux measurement for circular aperturesADUVARCHARprincipalfluxerr_aper_8_gUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_rUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_iUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_zUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_yUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalwavg_flux_psf_gWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_rWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_iWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_zWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_yWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_gUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_rUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_iUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_zUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_yUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalclass_star_gSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_rSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_iSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_zSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_ySimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalspread_model_gMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_rMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_iMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_zMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_yMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalwavg_spread_model_gSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_rSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_iSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_zSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_ySPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalspreaderr_model_gUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_rUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_iUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_zUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_yUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalwavg_spreaderr_model_gUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_rUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_iUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_zUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_yUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalg_rG-R colorVARCHARprincipalr_iR-I colorVARCHARprincipali_zI-Z colorVARCHARprincipalz_yZ-Y colorVARCHARprincipalsnr_gS/NVARCHARprincipalsnr_rS/NVARCHARprincipalsnr_iS/NVARCHARprincipalsnr_zS/NVARCHARprincipalsnr_yS/NVARCHARprincipalimaflags_iso_gFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_gNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_rFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_rNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_iFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_iNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_zFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_zNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_yFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_yNumber of epochs the source in detected in single epoch imagesVARCHARprincipalhtm9HTM Level-9 indexVARCHARprincipalring256Healpix ID with nside=256, ring schemaVARCHARprincipalnest4096Healpix ID with nside=4096, nested schemaVARCHARprincipalisoarea_image_gIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_rIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_iIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_zIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_yIsophotal area of the coadded sourcepixel^2VARCHARprincipalniter_model_gNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_rNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_iNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_zNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_yNumber of iterations in model fitting photometric measurementsVARCHARprincipalflags_gAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_rAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_iAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_zAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_yAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipaltilenameTile nameVARCHARprincipalnoirlab_test2.34_allwiseThe noirlab allwise.source table for the respective EMU regiondesignationUnique source IDmeta.idVARCHARindexedprincipalraRight Ascension (ICRS)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination (ICRS)degpos.eq.dec;meta.mainDOUBLEindexedprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalsigraOne-sigma uncertaintly in RA from non-moving source extractionarcsecREALprincipalsigdecOne-sigma uncertaintly in Dec from non-moving source extractionarcsecREALprincipalsigradecThe co-sigma of equatorial position uncertainties sigra/sigdecarcsecREALprincipalglonGalactic Longitudedegpos.gal.lonDOUBLEprincipalglatGalactic Latitudedegpos.gal.latDOUBLEprincipalelonEcliptic Longitudedegpos.ecl.lonDOUBLEprincipalelatEcliptic Latitudedegpos.ecl.latDOUBLEprincipalwxX-pixel coord of source in Atlas imagepixREALprincipalwyY-pixel coord of source in Atlas imagepixREALprincipalcntrUnique ID number for this object in the AllWISE Catalog/Reject table.BIGINTprincipalsource_idUnique source IDVARCHARprincipalcoadd_idAtlas Tile identifier from which source was extractedVARCHARprincipalsrcSequential number of the source extraction in the Atlas TileINTEGERprincipalw1mproW1 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.3-4umREALprincipalw1sigmproW1 measurement uncertainty in mag unitsmagREALprincipalw1snrW1 S/N ratioREALprincipalw1rchi2Reduced chi^2 of the W1 measurementREALprincipalw2mproW2 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.4-8umREALprincipalw2sigmproW2 measurement uncertainty in mag unitsmagREALprincipalw2snrW2 S/N ratioREALprincipalw2rchi2Reduced chi^2 of the W2 measurementREALprincipalw3mproW3 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.8-15umREALprincipalw3sigmproW3 measurement uncertainty in mag unitsmagREALprincipalw3snrW3 S/N ratioREALprincipalw3rchi2Reduced chi^2 of the W3 measurementREALprincipalw4mproW4 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.15-30umREALprincipalw4sigmproW4 measurement uncertainty in mag unitsmagREALprincipalw4snrW4 S/N ratioREALprincipalw4rchi2Reduced chi^2 of the W4 measurementREALprincipalrchi2Combined reduced chi^w in all bandsREALprincipalnbNumber of PSF components used simultaneously in profile-fitting for this sourcemeta.numberINTEGERprincipalnaActive deblending flag (0 = source not actively deblended, 1 = source actively deblended)meta.numberINTEGERprincipalw1satSaturated pixel fraction, W1instr.saturationREALprincipalw2satSaturated pixel fraction, W2instr.saturationREALprincipalw3satSaturated pixel fraction, W3instr.saturationREALprincipalw4satSaturated pixel fraction, W4instr.saturationREALprincipalsatnumMinimum sample at which saturation occurs in each bandinstr.saturationVARCHARprincipalra_pmRA at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipaldec_pmDeclination at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipalsigra_pmOne-sigma uncertaintly in ra_pmarcsecREALprincipalsigdec_pmOne-sigma uncertaintly in dec_pmarcsecREALprincipalsigradec_pmThe co-sigma of the equatorial position uncertainties from the profile-fitting measurement model that includes motion, sigra_pm, sigdec_pmarcsecREALprincipalpmraApparent motion in RA for this sourcemas / yrINTEGERprincipalsigpmraUncertainty in RA motion estimationmas / yrINTEGERprincipalpmdecApparent motion in Dec for this sourcemas / yrINTEGERprincipalsigpmdecUncertainty in Dec motion estimationmas / yrINTEGERprincipalw1rchi2_pmReduced chi^2 of W1 including motion estimationREALprincipalw2rchi2_pmReduced chi^2 of W2 including motion estimationREALprincipalw3rchi2_pmReduced chi^2 of W3 including motion estimationREALprincipalw4rchi2_pmReduced chi^2 of W4 including motion estimationREALprincipalrchi2_pmCombined reduced chi^2 in all bands including motion estimationREALprincipalpmcodeThis is a five character string that encodes information about factors that impact the accuracy of the motion estimation.VARCHARprincipalcc_flagsContamination and confusion flagVARCHARprincipalrelSmall separation, same-Tile detection flagVARCHARprincipalext_flgExtended source flagINTEGERprincipalvar_flgVariability flagVARCHARprincipalph_qualPhotometric quality flagVARCHARprincipaldet_bitBit-encoded integer indicating bands in which a source has a w?snr>2 detectionINTEGERprincipalmoon_levScattered moonlight contamination flagVARCHARprincipalw1nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement.INTEGERprincipalw1mInteger frame coverage -- no. of individual 7.2s W1 exposures on which measurement was possibleINTEGERprincipalw2nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement.INTEGERprincipalw2mInteger frame coverage -- no. of individual 7.2s W2 exposures on which measurement was possibleINTEGERprincipalw3nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement.INTEGERprincipalw3mInteger frame coverage -- no. of individual 7.2s W3 exposures on which measurement was possibleINTEGERprincipalw4nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement.INTEGERprincipalw4mInteger frame coverage -- no. of individual 7.2s W4 exposures on which measurement was possibleINTEGERprincipalw1covMean pixel coverage in W1REALprincipalw2covMean pixel coverage in W2REALprincipalw3covMean pixel coverage in W3REALprincipalw4covMean pixel coverage in W4REALprincipalw1cc_mapContamination and confusion map for this source in W1INTEGERprincipalw1cc_map_strContamination and confusion stringVARCHARprincipalw2cc_mapContamination and confusion map for this source in W2INTEGERprincipalw2cc_map_strContamination and confusion stringVARCHARprincipalw3cc_mapContamination and confusion map for this source in W3INTEGERprincipalw3cc_map_strContamination and confusion stringVARCHARprincipalw4cc_mapContamination and confusion map for this source in W4INTEGERprincipalw4cc_map_strContamination and confusion stringVARCHARprincipalbest_use_cntrCntr identification value of the source extraction that was selected as a candidate Catalog source in the duplicate resolution process for the group of associated sources that included this extraction.BIGINTprincipalngrpExcess number of positionally associated duplicate resolution groups in which this extractions was includedSMALLINTprincipaltmass_key2MASS PSC association. Unique identifier of the closest source in the 2MASS Point Source Catalog (PSC) that falls within 3arcsec of the non-motion fit position of this WISE source.INTEGERprincipalr_2massDistance separating the positions of the WISE source and associated 2MASS PSC sourceREALprincipalpa_2massPosition angle (degrees E of N) of the vector from the WISE source to the associated 2MASS PSC sourceREALprincipaln_2massThe number of 2MASS PSC entries found within a 3arcsec radius of the WISE source positionINTEGERprincipalj_m_2mass2MASS J-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalj_msig_2mass2MASS J-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalh_m_2mass2MASS H-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalh_msig_2mass2MASS H-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalk_m_2mass2MASS K-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalk_msig_2mass2MASS K-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalspt_indLevel 7 HTM spatial index keyINTEGERprincipalhtm20Level 20 HTM spatial index keyBIGINTprincipalnoirlab_test2.1_ls_dr8The noirlab ls_dr8.tractor table pre-joined with ls_dr8.x1p5__tractor__allwise__source, ls_dr8.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.g_rComputed (g-r) colorREALprincipalsnr_w3Signal-to-Noise ratio in W3stat.ratioREALprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudedegDOUBLEprincipalelonEcliptic LongitudedegDOUBLEprincipalglatGalactic LatitudedegDOUBLEprincipalglonGalactic LongitudedegDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalbrickidBrick ID [1,662174]INTEGERprincipalbrightblobbitwise mask indicating that an object is near a bright foreground source, as cataloged on the DR8 bitmasks page (http://legacysurvey.org/dr8/bitmasksDR8 bitmasks)SMALLINTprincipalbxX position (0-indexed) of coordinates in brick image stackpixREALprincipalbyY position (0-indexed) of coordinates in brick image stackpixREALprincipaldchisq_1Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_2Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_3Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_4Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_5Difference in X^2 between successfully more-complex model fitsREALprincipalls_idUnique LS object ID from RELEASE, BRICKID, OBJIDBIGINTprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errors1/deg^2REALprincipaldered_flux_gDereddened G-band fluxnanomaggiesREALprincipaldered_flux_rDereddened R-band fluxnanomaggiesREALprincipaldered_flux_w1Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w2Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w3Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w4Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_zDereddened Z-band fluxnanomaggiesREALprincipaldered_mag_gDereddened G-band magnitudemagREALprincipaldered_mag_rDereddened R-band magnitudemagREALprincipaldered_mag_w1Dereddened W1 magnitudemagREALprincipaldered_mag_w2Dereddened W2 magnitudemagREALprincipaldered_mag_w3Dereddened W3 magnitudemagREALprincipaldered_mag_w4Dereddened W4 magnitudemagREALprincipaldered_mag_zDereddened Z-band magnitudemagREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsmagREALprincipalfiberflux_gPredicted g-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalsnr_w4Signal-to-Noise ratio in W4stat.ratioREALprincipalfiberflux_rPredicted r-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_zPredicted z-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_gPredicted g-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_rPredicted r-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_zPredicted z-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)1/nanomaggies^2REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB)1/nanomaggies^2REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB)1/nanomaggies^2REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB)1/nanomaggies^2REALprincipalflux_w1WISE model flux in W1 (AB system)nanomaggiesREALprincipalflux_w2WISE model flux in W2 (AB)nanomaggiesREALprincipalflux_w3WISE model flux in W3 (AB)nanomaggiesREALprincipalflux_w4WISE model flux in W4 (AB)nanomaggiesREALprincipalfracdevFraction of model in deVauc [0,1]REALprincipalfracdev_ivarInverse variance of fracdevREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a source flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a source flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a source flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in r, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in z, strictly between [0,1]REALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magmagREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magmagREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magmagREALprincipalgaldepth_gAs for PSFDEPTH_G but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_rAs for PSFDEPTH_R but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_zAs for PSFDEPTH_Z but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalhtm9HTM index (order 9 => ~10 arcmin size)meta.codeINTEGERprincipalmag_gConverted G magnitudemagREALprincipalmag_rConverted R magnitudemagREALprincipalmag_w1W1 magnitudemagREALprincipalmag_w2W2 magnitudemagREALprincipalmag_w3W3 magnitudemagREALprincipalmag_w4W4 magnitudemagREALprincipalmag_zConverted Z magnitudemagREALprincipalmaskbitsbitwise mask indicating that an object touches a pixel in the coadd maskbits maps, as cataloged on the DR8 bitmasks pageSMALLINTprincipalsnr_zSignal-to-Noise ratio in Zstat.ratioREALprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in W1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in W2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in W3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in W4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each blobINTEGERprincipalparallaxReference catalog parallaxmasREALprincipalparallax_ivarReference catalog inverse-variance on parallax1/(mas)^2REALprincipalpmdecReference catalog proper motion in the Dec directionmas / yrREALprincipalpmdec_ivarReference catalog inverse-variance on pmdec1/(mas/yr)^2REALprincipalpmraReference catalog proper motion in the RA directionmas / yrREALprincipalpmra_ivarReference catalog inverse-variance on pmra1/(mas/yr)^2REALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_g) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_g)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_rFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_r) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_r)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_z) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_z)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfsize_gWeighted average PSF FWHM in the g bandarcsecREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandarcsecREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandarcsecREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errors1/deg^2REALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)yrREALprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia-DR2 and LSLGABIGINTprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalshapedev_e1Ellipticity component 1REALprincipalshapedev_e1_ivarInverse variance of shapedev_e1REALprincipalshapedev_e2Ellipticity component 2REALprincipalshapedev_e2_ivarInverse variance of shapedev_e2REALprincipalshapedev_rHalf-light radius of deVaucouleurs model (>0)arcsecREALprincipalshapedev_r_ivarInverse variance of shapedev_r1/arcsec^2REALprincipalshapeexp_e1Ellipticity component 1REALprincipalshapeexp_e1_ivarInverse variance of shapeexp_e1REALprincipalshapeexp_e2Ellipticity component 2REALprincipalshapeexp_e2_ivarInverse variance of shapeexp_e2REALprincipalshapeexp_rHalf-light radius of exponential model (>0)arcsecREALprincipalshapeexp_r_ivarInverse variance of shapeexp_r1/arcsec^2REALprincipalsnr_gSignal-to-Noise ratio in Gstat.ratioREALprincipalsnr_rSignal-to-Noise ratio in Rstat.ratioREALprincipalsnr_w1Signal-to-Noise ratio in W1stat.ratioREALprincipalsnr_w2Signal-to-Noise ratio in W2stat.ratioREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-d4) colorREALprincipalz_w1Computed (z-w1 colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarySMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia G band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalgaia_pointsourceThis Gaia DR2 source is believed to be a star, not a galaxySMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 forTycho-2, G2 for Gaia DR2, L2 for the LSLGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, COMP=composite, DUP=Gaia source fit by different model. Note that in some FITS readers, a trailing space may be appended for PSF , DEV and EXP since the column data type is a 4-character stringVARCHARprincipalwise_coadd_idunWISE coadd file name for the center of each objectVARCHARprincipalflux_gmodel flux in gREALprincipalflux_rmodel flux in rREALprincipalflux_zmodel flux in zREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_zInverse variance of flux_zREALprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_median(recommended) photo-z derived from the median of the photo-z PDFREALprincipalz_phot_stdstandard deviation of the photo-z derived from the photo-z PDFREALprincipalz_phot_l68lower 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_u68upper 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_l95lower 95% confidence limit derived from the photo-z PDFREALprincipalz_phot_u95upper 95% confidence limit derived from the photo-z PDFREALprincipalz_specspectroscopic redshift, if availableREALprincipalsurveysource of the spectroscopic redshiftVARCHARprincipaltrainingwhether or not the spectroscopic redshift is used for the photo-z trainingVARCHARprincipalnoirlab_test2.1_des_dr1The noirlab des_dr1.main table pre-joined with des_dr1.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalcoadd_object_idUnique identifier for the coadded objectsVARCHARprincipalhpix_32Healpix ID for nside=32, nested schemaVARCHARprincipalhpix_64Healpix ID for nside=64, nested schemaVARCHARprincipalhpix_1024Healpix ID for nside=1024, nested schemaVARCHARprincipalhpix_4096Healpix ID for nside=4096, nested schemaVARCHARprincipalhpix_16384Healpix ID for nside=16384, nested schemaVARCHARprincipalraRight ascension, with quantized precision for indexing (ALPHAWIN_J2000 has full precision but not indexed)degpos.eq.raVARCHARprincipaldecDeclination, with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed)degpos.eq.decVARCHARprincipalalphawin_j2000Right ascension for the object, J2000 in ICRS system (full precision but not indexed)degVARCHARprincipaldeltawin_j2000Declination for the object, J2000 in ICRS (full precision but not indexed)degVARCHARprincipalgalactic_lGalactic LongitudedegVARCHARprincipalgalactic_bGalactic LatitudedegVARCHARprincipalecliptic_lonEcliptic LongitudedegVARCHARprincipalecliptic_latEcliptic LatitudedegVARCHARprincipalxwin_imageX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_imageY-centroid from windowed measurements on coadded imagepixelVARCHARprincipalerrx2win_image_gUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_rUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_iUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_zUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_yUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_gUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_rUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_iUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_zUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_yUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_gUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_rUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_iUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_zUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_yUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalx2win_image_gSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_rSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_iSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_zSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_ySecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalkron_radius_gKron radius measured from detection imagepixelVARCHARprincipaly2win_image_gSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_rSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_iSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_zSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_ySecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_gSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_rSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_iSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_zSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_ySecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxwin_image_gX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_rX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_iX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_zX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_yX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_image_gY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_rY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_iY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_zY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_yY-centroid from windowed measurements on coadded imageVARCHARprincipala_imageMajor axis size based on an isophotal modelpixelVARCHARprincipalerra_imageUncertainty in major axis size, from isophotal modelpixelVARCHARprincipalb_imageMinor axis size based on an isophotal modelpixelVARCHARprincipalerrb_imageUncertainty in minor axis size, from isophotal modelpixelVARCHARprincipaltheta_j2000Position angle of source in J2000 coordinates, from non-windowed measurementdegVARCHARprincipalerrtheta_imageUncertainty in source position, from isophotal modeldegVARCHARprincipalkron_radiusKron radiuspixelVARCHARprincipalebv_sfd98E(B-V) reddening oefficient from Schelgel, Finkbeiner & Davis (1998)magVARCHARprincipalmag_auto_g_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_r_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_i_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_z_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_y_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_aper_8_g_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_r_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_i_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_z_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_y_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalwavg_mag_psf_g_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_r_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_i_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_z_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_y_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalawin_image_gMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_rMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_iMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_zMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_yMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_gMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_rMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_iMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_zMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_yMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalthetawin_image_gPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_rPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_iPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_zPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_yPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalerrawin_image_gUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_rUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_iUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_zUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_yUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_gUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_rUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_iUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_zUncertainty in Minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_yUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrthetawin_image_gUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_rUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_iUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_zUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_yUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalflux_radius_gHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_rHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_iHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_zHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_yHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_gFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_rFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_iFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_zFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_yFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalbackground_gBackground level, by CCD-amplifiermagVARCHARprincipalbackground_rBackground level, by CCD-amplifiermagVARCHARprincipalbackground_iBackground level, by CCD-amplifiermagVARCHARprincipalbackground_zBackground level, by CCD-amplifiermagVARCHARprincipalbackground_yBackground level, by CCD-amplifiermagVARCHARprincipalkron_radius_rKron radius measured from detection imagepixelVARCHARprincipalkron_radius_iKron radius measured from detection imagepixelVARCHARprincipalkron_radius_zKron radius measured from detection imagepixelVARCHARprincipalkron_radius_yKron radius measured from detection imagepixelVARCHARprincipalmag_auto_gMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_rMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_iMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_zMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_yMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_gUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_rUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_iUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_zUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_yUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmag_aper_8_gMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_rMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_iMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_zMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_yMagnitude estimation for circular aperturesmagVARCHARprincipalmagerr_aper_8_gUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_rUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_iUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_zUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_yUncertainty in magnitude estimation for circular aperturesVARCHARprincipalwavg_mag_psf_gWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_rWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_iWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_zWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_yWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_gUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_rUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_iUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_zUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_yUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalflux_auto_gFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_rFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_iFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_zFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_yFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_guncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_runcertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_iuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_zuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_yuncertainty in flux measurement, for an elliptical model based on Kron radiusVARCHARprincipalflux_aper_8_gFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_rFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_iFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_zFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_yFlux measurement for circular aperturesADUVARCHARprincipalfluxerr_aper_8_gUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_rUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_iUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_zUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_yUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalwavg_flux_psf_gWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_rWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_iWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_zWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_yWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_gUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_rUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_iUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_zUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_yUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalclass_star_gSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_rSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_iSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_zSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_ySimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalspread_model_gMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_rMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_iMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_zMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_yMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalwavg_spread_model_gSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_rSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_iSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_zSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_ySPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalspreaderr_model_gUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_rUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_iUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_zUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_yUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalwavg_spreaderr_model_gUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_rUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_iUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_zUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_yUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalg_rG-R colorVARCHARprincipalr_iR-I colorVARCHARprincipali_zI-Z colorVARCHARprincipalz_yZ-Y colorVARCHARprincipalsnr_gS/NVARCHARprincipalsnr_rS/NVARCHARprincipalsnr_iS/NVARCHARprincipalsnr_zS/NVARCHARprincipalsnr_yS/NVARCHARprincipalimaflags_iso_gFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_gNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_rFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_rNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_iFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_iNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_zFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_zNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_yFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_yNumber of epochs the source in detected in single epoch imagesVARCHARprincipalhtm9HTM Level-9 indexVARCHARprincipalring256Healpix ID with nside=256, ring schemaVARCHARprincipalnest4096Healpix ID with nside=4096, nested schemaVARCHARprincipalisoarea_image_gIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_rIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_iIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_zIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_yIsophotal area of the coadded sourcepixel^2VARCHARprincipalniter_model_gNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_rNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_iNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_zNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_yNumber of iterations in model fitting photometric measurementsVARCHARprincipalflags_gAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_rAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_iAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_zAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_yAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipaltilenameTile nameVARCHARprincipalnoirlab_test2.1_allwiseThe noirlab allwise.source table for the respective EMU regionext_flgExtended source flagINTEGERprincipalvar_flgVariability flagVARCHARprincipalph_qualPhotometric quality flagVARCHARprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalraRight Ascension (ICRS)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination (ICRS)degpos.eq.dec;meta.mainDOUBLEindexedprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalsigraOne-sigma uncertaintly in RA from non-moving source extractionarcsecREALprincipalsigdecOne-sigma uncertaintly in Dec from non-moving source extractionarcsecREALprincipalsigradecThe co-sigma of equatorial position uncertainties sigra/sigdecarcsecREALprincipalglonGalactic Longitudedegpos.gal.lonDOUBLEprincipalglatGalactic Latitudedegpos.gal.latDOUBLEprincipalelonEcliptic Longitudedegpos.ecl.lonDOUBLEprincipalelatEcliptic Latitudedegpos.ecl.latDOUBLEprincipalwxX-pixel coord of source in Atlas imagepixREALprincipalwyY-pixel coord of source in Atlas imagepixREALprincipalcntrUnique ID number for this object in the AllWISE Catalog/Reject table.BIGINTprincipalsource_idUnique source IDVARCHARprincipalcoadd_idAtlas Tile identifier from which source was extractedVARCHARprincipalsrcSequential number of the source extraction in the Atlas TileINTEGERprincipalw1mproW1 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.3-4umREALprincipalw1sigmproW1 measurement uncertainty in mag unitsmagREALprincipalw1snrW1 S/N ratioREALprincipalw1rchi2Reduced chi^2 of the W1 measurementREALprincipalw2mproW2 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.4-8umREALprincipalw2sigmproW2 measurement uncertainty in mag unitsmagREALprincipalw2snrW2 S/N ratioREALprincipalw2rchi2Reduced chi^2 of the W2 measurementREALprincipalw3mproW3 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.8-15umREALprincipalw3sigmproW3 measurement uncertainty in mag unitsmagREALprincipalw3snrW3 S/N ratioREALprincipalw3rchi2Reduced chi^2 of the W3 measurementREALprincipalw4mproW4 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.15-30umREALprincipalw4sigmproW4 measurement uncertainty in mag unitsmagREALprincipalw4snrW4 S/N ratioREALprincipalw4rchi2Reduced chi^2 of the W4 measurementREALprincipalrchi2Combined reduced chi^w in all bandsREALprincipalnbNumber of PSF components used simultaneously in profile-fitting for this sourcemeta.numberINTEGERprincipalnaActive deblending flag (0 = source not actively deblended, 1 = source actively deblended)meta.numberINTEGERprincipalw1satSaturated pixel fraction, W1instr.saturationREALprincipalw2satSaturated pixel fraction, W2instr.saturationREALprincipalw3satSaturated pixel fraction, W3instr.saturationREALprincipalw4satSaturated pixel fraction, W4instr.saturationREALprincipalsatnumMinimum sample at which saturation occurs in each bandinstr.saturationVARCHARprincipalra_pmRA at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipaldec_pmDeclination at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipalsigra_pmOne-sigma uncertaintly in ra_pmarcsecREALprincipalsigdec_pmOne-sigma uncertaintly in dec_pmarcsecREALprincipalsigradec_pmThe co-sigma of the equatorial position uncertainties from the profile-fitting measurement model that includes motion, sigra_pm, sigdec_pmarcsecREALprincipalpmraApparent motion in RA for this sourcemas / yrINTEGERprincipalsigpmraUncertainty in RA motion estimationmas / yrINTEGERprincipalpmdecApparent motion in Dec for this sourcemas / yrINTEGERprincipalsigpmdecUncertainty in Dec motion estimationmas / yrINTEGERprincipalw1rchi2_pmReduced chi^2 of W1 including motion estimationREALprincipalw2rchi2_pmReduced chi^2 of W2 including motion estimationREALprincipalw3rchi2_pmReduced chi^2 of W3 including motion estimationREALprincipalw4rchi2_pmReduced chi^2 of W4 including motion estimationREALprincipalrchi2_pmCombined reduced chi^2 in all bands including motion estimationREALprincipalpmcodeThis is a five character string that encodes information about factors that impact the accuracy of the motion estimation.VARCHARprincipalcc_flagsContamination and confusion flagVARCHARprincipalrelSmall separation, same-Tile detection flagVARCHARprincipaldet_bitBit-encoded integer indicating bands in which a source has a w?snr>2 detectionINTEGERprincipalmoon_levScattered moonlight contamination flagVARCHARprincipalw1nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement.INTEGERprincipalw1mInteger frame coverage -- no. of individual 7.2s W1 exposures on which measurement was possibleINTEGERprincipalw2nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement.INTEGERprincipalw2mInteger frame coverage -- no. of individual 7.2s W2 exposures on which measurement was possibleINTEGERprincipalw3nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement.INTEGERprincipalw3mInteger frame coverage -- no. of individual 7.2s W3 exposures on which measurement was possibleINTEGERprincipalw4nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement.INTEGERprincipalw4mInteger frame coverage -- no. of individual 7.2s W4 exposures on which measurement was possibleINTEGERprincipalw1covMean pixel coverage in W1REALprincipalw2covMean pixel coverage in W2REALprincipalw3covMean pixel coverage in W3REALprincipalw4covMean pixel coverage in W4REALprincipalw1cc_mapContamination and confusion map for this source in W1INTEGERprincipalw1cc_map_strContamination and confusion stringVARCHARprincipalw2cc_mapContamination and confusion map for this source in W2INTEGERprincipalw2cc_map_strContamination and confusion stringVARCHARprincipalw3cc_mapContamination and confusion map for this source in W3INTEGERprincipalw3cc_map_strContamination and confusion stringVARCHARprincipalw4cc_mapContamination and confusion map for this source in W4INTEGERprincipalw4cc_map_strContamination and confusion stringVARCHARprincipalbest_use_cntrCntr identification value of the source extraction that was selected as a candidate Catalog source in the duplicate resolution process for the group of associated sources that included this extraction.BIGINTprincipalngrpExcess number of positionally associated duplicate resolution groups in which this extractions was includedSMALLINTprincipaltmass_key2MASS PSC association. Unique identifier of the closest source in the 2MASS Point Source Catalog (PSC) that falls within 3arcsec of the non-motion fit position of this WISE source.INTEGERprincipalr_2massDistance separating the positions of the WISE source and associated 2MASS PSC sourceREALprincipalpa_2massPosition angle (degrees E of N) of the vector from the WISE source to the associated 2MASS PSC sourceREALprincipaln_2massThe number of 2MASS PSC entries found within a 3arcsec radius of the WISE source positionINTEGERprincipalj_m_2mass2MASS J-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalj_msig_2mass2MASS J-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalh_m_2mass2MASS H-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalh_msig_2mass2MASS H-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalk_m_2mass2MASS K-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalk_msig_2mass2MASS K-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalspt_indLevel 7 HTM spatial index keyINTEGERprincipalhtm20Level 20 HTM spatial index keyBIGINTprincipalnoirlab_test2.36_allwiseThe noirlab allwise.source table for the respective EMU regionw1snrW1 S/N ratioREALprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalraRight Ascension (ICRS)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination (ICRS)degpos.eq.dec;meta.mainDOUBLEindexedprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalsigraOne-sigma uncertaintly in RA from non-moving source extractionarcsecREALprincipalsigdecOne-sigma uncertaintly in Dec from non-moving source extractionarcsecREALprincipalsigradecThe co-sigma of equatorial position uncertainties sigra/sigdecarcsecREALprincipalglonGalactic Longitudedegpos.gal.lonDOUBLEprincipalglatGalactic Latitudedegpos.gal.latDOUBLEprincipalelonEcliptic Longitudedegpos.ecl.lonDOUBLEprincipalelatEcliptic Latitudedegpos.ecl.latDOUBLEprincipalwxX-pixel coord of source in Atlas imagepixREALprincipalwyY-pixel coord of source in Atlas imagepixREALprincipalcntrUnique ID number for this object in the AllWISE Catalog/Reject table.BIGINTprincipalsource_idUnique source IDVARCHARprincipalcoadd_idAtlas Tile identifier from which source was extractedVARCHARprincipalsrcSequential number of the source extraction in the Atlas TileINTEGERprincipalw1mproW1 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.3-4umREALprincipalw1sigmproW1 measurement uncertainty in mag unitsmagREALprincipalw1rchi2Reduced chi^2 of the W1 measurementREALprincipalw2mproW2 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.4-8umREALprincipalw2sigmproW2 measurement uncertainty in mag unitsmagREALprincipalw2snrW2 S/N ratioREALprincipalw2rchi2Reduced chi^2 of the W2 measurementREALprincipalw3mproW3 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.8-15umREALprincipalw3sigmproW3 measurement uncertainty in mag unitsmagREALprincipalw3snrW3 S/N ratioREALprincipalw3rchi2Reduced chi^2 of the W3 measurementREALprincipalw4mproW4 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.15-30umREALprincipalw4sigmproW4 measurement uncertainty in mag unitsmagREALprincipalw4snrW4 S/N ratioREALprincipalw4rchi2Reduced chi^2 of the W4 measurementREALprincipalrchi2Combined reduced chi^w in all bandsREALprincipalnbNumber of PSF components used simultaneously in profile-fitting for this sourcemeta.numberINTEGERprincipalnaActive deblending flag (0 = source not actively deblended, 1 = source actively deblended)meta.numberINTEGERprincipalw1satSaturated pixel fraction, W1instr.saturationREALprincipalw2satSaturated pixel fraction, W2instr.saturationREALprincipalw3satSaturated pixel fraction, W3instr.saturationREALprincipalw4satSaturated pixel fraction, W4instr.saturationREALprincipalsatnumMinimum sample at which saturation occurs in each bandinstr.saturationVARCHARprincipalra_pmRA at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipaldec_pmDeclination at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipalsigra_pmOne-sigma uncertaintly in ra_pmarcsecREALprincipalsigdec_pmOne-sigma uncertaintly in dec_pmarcsecREALprincipalsigradec_pmThe co-sigma of the equatorial position uncertainties from the profile-fitting measurement model that includes motion, sigra_pm, sigdec_pmarcsecREALprincipalpmraApparent motion in RA for this sourcemas / yrINTEGERprincipalsigpmraUncertainty in RA motion estimationmas / yrINTEGERprincipalpmdecApparent motion in Dec for this sourcemas / yrINTEGERprincipalsigpmdecUncertainty in Dec motion estimationmas / yrINTEGERprincipalw1rchi2_pmReduced chi^2 of W1 including motion estimationREALprincipalw2rchi2_pmReduced chi^2 of W2 including motion estimationREALprincipalw3rchi2_pmReduced chi^2 of W3 including motion estimationREALprincipalw4rchi2_pmReduced chi^2 of W4 including motion estimationREALprincipalrchi2_pmCombined reduced chi^2 in all bands including motion estimationREALprincipalpmcodeThis is a five character string that encodes information about factors that impact the accuracy of the motion estimation.VARCHARprincipalcc_flagsContamination and confusion flagVARCHARprincipalrelSmall separation, same-Tile detection flagVARCHARprincipalext_flgExtended source flagINTEGERprincipalvar_flgVariability flagVARCHARprincipalph_qualPhotometric quality flagVARCHARprincipaldet_bitBit-encoded integer indicating bands in which a source has a w?snr>2 detectionINTEGERprincipalmoon_levScattered moonlight contamination flagVARCHARprincipalw1nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement.INTEGERprincipalw1mInteger frame coverage -- no. of individual 7.2s W1 exposures on which measurement was possibleINTEGERprincipalw2nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement.INTEGERprincipalw2mInteger frame coverage -- no. of individual 7.2s W2 exposures on which measurement was possibleINTEGERprincipalw3nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement.INTEGERprincipalw3mInteger frame coverage -- no. of individual 7.2s W3 exposures on which measurement was possibleINTEGERprincipalw4nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement.INTEGERprincipalw4mInteger frame coverage -- no. of individual 7.2s W4 exposures on which measurement was possibleINTEGERprincipalw1covMean pixel coverage in W1REALprincipalw2covMean pixel coverage in W2REALprincipalw3covMean pixel coverage in W3REALprincipalw4covMean pixel coverage in W4REALprincipalw1cc_mapContamination and confusion map for this source in W1INTEGERprincipalw1cc_map_strContamination and confusion stringVARCHARprincipalw2cc_mapContamination and confusion map for this source in W2INTEGERprincipalw2cc_map_strContamination and confusion stringVARCHARprincipalw3cc_mapContamination and confusion map for this source in W3INTEGERprincipalw3cc_map_strContamination and confusion stringVARCHARprincipalw4cc_mapContamination and confusion map for this source in W4INTEGERprincipalw4cc_map_strContamination and confusion stringVARCHARprincipalbest_use_cntrCntr identification value of the source extraction that was selected as a candidate Catalog source in the duplicate resolution process for the group of associated sources that included this extraction.BIGINTprincipalngrpExcess number of positionally associated duplicate resolution groups in which this extractions was includedSMALLINTprincipaltmass_key2MASS PSC association. Unique identifier of the closest source in the 2MASS Point Source Catalog (PSC) that falls within 3arcsec of the non-motion fit position of this WISE source.INTEGERprincipalr_2massDistance separating the positions of the WISE source and associated 2MASS PSC sourceREALprincipalpa_2massPosition angle (degrees E of N) of the vector from the WISE source to the associated 2MASS PSC sourceREALprincipaln_2massThe number of 2MASS PSC entries found within a 3arcsec radius of the WISE source positionINTEGERprincipalj_m_2mass2MASS J-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalj_msig_2mass2MASS J-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalh_m_2mass2MASS H-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalh_msig_2mass2MASS H-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalk_m_2mass2MASS K-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalk_msig_2mass2MASS K-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalspt_indLevel 7 HTM spatial index keyINTEGERprincipalhtm20Level 20 HTM spatial index keyBIGINTprincipalnoirlab_test2.35_ls_dr8The noirlab ls_dr8.tractor table pre-joined with ls_dr8.x1p5__tractor__allwise__source, ls_dr8.photo_z and allwise.source tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (ls_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalpsfdepth_w1As for psfdepth_g (and also on the AB system) but for WISE W1REALprincipalpsfdepth_w2As for psfdepth_g (and also on the AB system) but for WISE W2REALprincipalpsfdepth_w3As for psfdepth_g (and also on the AB system) but for WISE W3REALprincipalpsfdepth_w4As for psfdepth_g (and also on the AB system) but for WISE W4REALprincipaldecDeclination at equinox J2000degpos.eq.dec;meta.mainDOUBLEindexedprincipalelatEcliptic LatitudedegDOUBLEprincipalelonEcliptic LongitudedegDOUBLEprincipalglatGalactic LatitudedegDOUBLEprincipalglonGalactic LongitudedegDOUBLEprincipalmjd_maxMaximum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalmjd_minMinimum Modified Julian Date of observations used to construct the model of this objectdaysDOUBLEprincipalraRight ascension at equinox J2000degpos.eq.ra;meta.mainDOUBLEindexedprincipalbrickidBrick ID [1,662174]INTEGERprincipalbrightblobbitwise mask indicating that an object is near a bright foreground source, as cataloged on the DR8 bitmasks page (http://legacysurvey.org/dr8/bitmasksDR8 bitmasks)SMALLINTprincipalbxX position (0-indexed) of coordinates in brick image stackpixREALprincipalbyY position (0-indexed) of coordinates in brick image stackpixREALprincipaldchisq_1Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_2Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_3Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_4Difference in X^2 between successfully more-complex model fitsREALprincipaldchisq_5Difference in X^2 between successfully more-complex model fitsREALprincipalls_idUnique LS object ID from RELEASE, BRICKID, OBJIDBIGINTprincipaldec_ivarInverse variance of DEC, excluding astrometric calibration errors1/deg^2REALprincipaldered_flux_gDereddened G-band fluxnanomaggiesREALprincipaldered_flux_rDereddened R-band fluxnanomaggiesREALprincipaldered_flux_w1Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w2Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w3Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_w4Dereddened W1 fluxnanomaggiesREALprincipaldered_flux_zDereddened Z-band fluxnanomaggiesREALprincipaldered_mag_gDereddened G-band magnitudemagREALprincipaldered_mag_rDereddened R-band magnitudemagREALprincipaldered_mag_w1Dereddened W1 magnitudemagREALprincipaldered_mag_w2Dereddened W2 magnitudemagREALprincipaldered_mag_w3Dereddened W3 magnitudemagREALprincipaldered_mag_w4Dereddened W4 magnitudemagREALprincipaldered_mag_zDereddened Z-band magnitudemagREALprincipalebvGalactic extinction E(B-V) reddening from SFD98, used to compute the mw_transmission_ columnsmagREALprincipalfiberflux_gPredicted g-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_rPredicted r-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfiberflux_zPredicted z-band flux within a fiber from this object in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_gPredicted g-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_rPredicted r-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalfibertotflux_zPredicted z-band flux within a fiber from all sources at this location in 1 arcsec Gaussian seeingnanomaggiesREALprincipalflux_ivar_w1Inverse variance of flux_w1 (AB system)1/nanomaggies^2REALprincipalflux_ivar_w2Inverse variance of flux_w2 (AB)1/nanomaggies^2REALprincipalflux_ivar_w3Inverse variance of flux_w3 (AB)1/nanomaggies^2REALprincipalflux_ivar_w4Inverse variance of flux_w4 (AB)1/nanomaggies^2REALprincipalflux_w1WISE model flux in W1 (AB system)nanomaggiesREALprincipalflux_w2WISE model flux in W2 (AB)nanomaggiesREALprincipalflux_w3WISE model flux in W3 (AB)nanomaggiesREALprincipalflux_w4WISE model flux in W4 (AB)nanomaggiesREALprincipalfracdevFraction of model in deVauc [0,1]REALprincipalfracdev_ivarInverse variance of fracdevREALprincipalfracflux_gProfile-weighted fraction of the flux from other sources divided by the total flux in g (typically [0,1])REALprincipalfracflux_rProfile-weighted fraction of the flux from other sources divided by the total flux in r (typically [0,1])REALprincipalfracflux_w1Profile-weighted fraction of the flux from other sources divided by the total flux in W1 (typically [0,1])REALprincipalfracflux_w2Profile-weighted fraction of the flux from other sources divided by the total flux in W2 (typically [0,1])REALprincipalfracflux_w3Profile-weighted fraction of the flux from other sources divided by the total flux in W3 (typically [0,1])REALprincipalfracflux_w4Profile-weighted fraction of the flux from other sources divided by the total flux in W4 (typically [0,1])REALprincipalfracflux_zProfile-weighted fraction of the flux from other sources divided by the total flux in z (typically [0,1])REALprincipalfracin_gFraction of a source flux within the blob in g, near unity for real sourcesREALprincipalfracin_rFraction of a source flux within the blob in r, near unity for real sourcesREALprincipalfracin_zFraction of a source flux within the blob in z, near unity for real sourcesREALprincipalfracmasked_gProfile-weighted fraction of pixels masked from all observations of this object in g, strictly between [0,1]REALprincipalfracmasked_rProfile-weighted fraction of pixels masked from all observations of this object in r, strictly between [0,1]REALprincipalfracmasked_zProfile-weighted fraction of pixels masked from all observations of this object in z, strictly between [0,1]REALprincipalgaia_astrometric_excess_noiseGaia astrometric excess noiseREALprincipalgaia_astrometric_excess_noise_sigGaia astrometric excess noise uncertaintyREALprincipalgaia_astrometric_weight_alGaia astrometric weight along scan directionREALprincipalgaia_phot_bp_mean_flux_over_errorGaia BP signal-to-noiseREALprincipalgaia_phot_bp_mean_magGaia BP magmagREALprincipalgaia_phot_g_mean_flux_over_errorGaia G band signal-to-noiseREALprincipalgaia_phot_g_mean_magGaia G band magmagREALprincipalgaia_phot_rp_mean_flux_over_errorGaia RP signal-to-noiseREALprincipalgaia_phot_rp_mean_magGaia RP magmagREALprincipalgaldepth_gAs for PSFDEPTH_G but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_rAs for PSFDEPTH_R but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalgaldepth_zAs for PSFDEPTH_Z but for a galaxy (0.45 arcsec exp, round) detection sensitivity1/nanomaggies^2REALprincipalg_rComputed (g-r) colorREALprincipalhtm9HTM index (order 9 => ~10 arcmin size)meta.codeINTEGERprincipalmag_gConverted G magnitudemagREALprincipalmag_rConverted R magnitudemagREALprincipalmag_w1W1 magnitudemagREALprincipalmag_w2W2 magnitudemagREALprincipalmag_w3W3 magnitudemagREALprincipalmag_w4W4 magnitudemagREALprincipalmag_zConverted Z magnitudemagREALprincipalmaskbitsbitwise mask indicating that an object touches a pixel in the coadd maskbits maps, as cataloged on the DR8 bitmasks pageSMALLINTprincipalmw_transmission_gGalactic transmission in g filter in linear units [0, 1]REALprincipalmw_transmission_rGalactic transmission in r filter in linear units [0, 1]REALprincipalmw_transmission_w1Galactic transmission in W1 filter in linear units [0, 1]REALprincipalmw_transmission_w2Galactic transmission in W2 filter in linear units [0, 1]REALprincipalmw_transmission_w3Galactic transmission in W3 filter in linear units [0, 1]REALprincipalmw_transmission_w4Galactic transmission in W4 filter in linear units [0, 1]REALprincipalmw_transmission_zGalactic transmission in z filter in linear units [0, 1]REALprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalobjidCatalog object number within this brick; a unique identifier hash is release,brickid,objid; objid spans [0,N-1] and is contiguously enumerated within each blobINTEGERprincipalparallaxReference catalog parallaxmasREALprincipalparallax_ivarReference catalog inverse-variance on parallax1/(mas)^2REALprincipalpmdecReference catalog proper motion in the Dec directionmas / yrREALprincipalpmdec_ivarReference catalog inverse-variance on pmdec1/(mas/yr)^2REALprincipalpmraReference catalog proper motion in the RA directionmas / yrREALprincipalpmra_ivarReference catalog inverse-variance on pmra1/(mas/yr)^2REALprincipalpsfdepth_gFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_g) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_g)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_rFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_r) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_r)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfdepth_zFor a 5 sigma point source detection limit in g, 5/sqrt(psfdepth_z) gives flux in nanomaggies and -2.5[log_10(5 / sqrt(psfdepth_z)) - 9] gives corresponding AB magnitude1/nanomaggies^2REALprincipalpsfsize_gWeighted average PSF FWHM in the g bandarcsecREALprincipalpsfsize_rWeighted average PSF FWHM in the r bandarcsecREALprincipalpsfsize_zWeighted average PSF FWHM in the z bandarcsecREALprincipalra_ivarInverse variance of RA (no cosine term!), excluding astrometric calibration errors1/deg^2REALprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalrchisq_gProfile-weighted chi^2 of model fit normalized by the number of pixels in gREALprincipalrchisq_rProfile-weighted chi^2 of model fit normalized by the number of pixels in rREALprincipalrchisq_w1Profile-weighted chi^2 of model fit normalized by the number of pixels in W1REALprincipalrchisq_w2Profile-weighted chi^2 of model fit normalized by the number of pixels in W2REALprincipalrchisq_w3Profile-weighted chi^2 of model fit normalized by the number of pixels in W3REALprincipalrchisq_w4Profile-weighted chi^2 of model fit normalized by the number of pixels in W4REALprincipalrchisq_zProfile-weighted chi^2 of model fit normalized by the number of pixels in zREALprincipalref_epochReference catalog reference epoch (eg, 2015.5 for Gaia DR2)yrREALprincipalref_idReference catalog identifier for this star; Tyc1*1,000,000+Tyc2*10+Tyc3 for Tycho2; sourceid for Gaia-DR2 and LSLGABIGINTprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalr_zComputed (r-z) colorREALprincipalshapedev_e1Ellipticity component 1REALprincipalshapedev_e1_ivarInverse variance of shapedev_e1REALprincipalshapedev_e2Ellipticity component 2REALprincipalshapedev_e2_ivarInverse variance of shapedev_e2REALprincipalshapedev_rHalf-light radius of deVaucouleurs model (>0)arcsecREALprincipalshapedev_r_ivarInverse variance of shapedev_r1/arcsec^2REALprincipalshapeexp_e1Ellipticity component 1REALprincipalshapeexp_e1_ivarInverse variance of shapeexp_e1REALprincipalshapeexp_e2Ellipticity component 2REALprincipalshapeexp_e2_ivarInverse variance of shapeexp_e2REALprincipalshapeexp_rHalf-light radius of exponential model (>0)arcsecREALprincipalshapeexp_r_ivarInverse variance of shapeexp_r1/arcsec^2REALprincipalsnr_gSignal-to-Noise ratio in Gstat.ratioREALprincipalsnr_rSignal-to-Noise ratio in Rstat.ratioREALprincipalsnr_w1Signal-to-Noise ratio in W1stat.ratioREALprincipalsnr_w2Signal-to-Noise ratio in W2stat.ratioREALprincipalsnr_w3Signal-to-Noise ratio in W3stat.ratioREALprincipalsnr_w4Signal-to-Noise ratio in W4stat.ratioREALprincipalsnr_zSignal-to-Noise ratio in Zstat.ratioREALprincipalw1_w2Computed (w1-w2) colorREALprincipalw2_w3Computed (w2-w3) colorREALprincipalw3_w4Computed (w3-d4) colorREALprincipalz_w1Computed (z-w1 colorREALprincipalallmask_gBitwise mask set if the central pixel from all images satisfy each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_rBitwise mask set if the central pixel from all images satisfy each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalallmask_zBitwise mask set if the central pixel from all images satisfy each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_gBitwise mask set if the central pixel from any image satisfies each condition in g as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_rBitwise mask set if the central pixel from any image satisfies each condition in r as cataloged on the DR8 bitmasks pageSMALLINTprincipalanymask_zBitwise mask set if the central pixel from any image satisfies each condition in z as cataloged on the DR8 bitmasks pageSMALLINTprincipalbrick_primaryTrue if the object is within the brick boundarySMALLINTprincipalgaia_astrometric_n_good_obs_alGaia number of good astrometric observations along scan directionSMALLINTprincipalgaia_astrometric_n_obs_alGaia number of astrometric observations along scan directionSMALLINTprincipalgaia_duplicated_sourceGaia duplicated source flagSMALLINTprincipalgaia_phot_bp_n_obsGaia BP number of observationsSMALLINTprincipalgaia_phot_g_n_obsGaia G band number of observationsSMALLINTprincipalgaia_phot_rp_n_obsGaia RP number of observationsSMALLINTprincipalgaia_phot_variable_flagGaia photometric variable flagSMALLINTprincipalgaia_pointsourceThis Gaia DR2 source is believed to be a star, not a galaxySMALLINTprincipalnobs_gNumber of images that contribute to the central pixel in g: filter for this object (not profile-weighted)SMALLINTprincipalnobs_rNumber of images that contribute to the central pixel in r: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w1Number of images that contribute to the central pixel in W1: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w2Number of images that contribute to the central pixel in W2: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w3Number of images that contribute to the central pixel in W3: filter for this object (not profile-weighted)SMALLINTprincipalnobs_w4Number of images that contribute to the central pixel in W4: filter for this object (not profile-weighted)SMALLINTprincipalnobs_zNumber of images that contribute to the central pixel in z: filter for this object (not profile-weighted)SMALLINTprincipalreleaseUnique integer denoting the camera and filter set usedSMALLINTprincipalwisemask_w1W1 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalwisemask_w2W2 bitmask as cataloged on the DR8 bitmasks pageSMALLINTprincipalbricknameName of brick, encoding the brick sky position, eg 1126p222 near RA=112.6, Dec=+22.2VARCHARprincipalref_catReference catalog source for this star: T2 forTycho-2, G2 for Gaia DR2, L2 for the LSLGA, empty otherwiseVARCHARprincipaltypeMorphological model: PSF=stellar, REX=round exponential galaxy, DEV=deVauc, EXP=exponential, COMP=composite, DUP=Gaia source fit by different model. Note that in some FITS readers, a trailing space may be appended for PSF , DEV and EXP since the column data type is a 4-character stringVARCHARprincipalwise_coadd_idunWISE coadd file name for the center of each objectVARCHARprincipalflux_gmodel flux in gREALprincipalflux_rmodel flux in rREALprincipalflux_zmodel flux in zREALprincipalflux_ivar_gInverse variance of flux_gREALprincipalflux_ivar_rInverse variance of flux_rREALprincipalflux_ivar_zInverse variance of flux_zREALprincipalz_phot_meanphoto-z derived from the mean of the photo-z PDFREALprincipalz_phot_median(recommended) photo-z derived from the median of the photo-z PDFREALprincipalz_phot_stdstandard deviation of the photo-z derived from the photo-z PDFREALprincipalz_phot_l68lower 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_u68upper 68% confidence limit derived from the photo-z PDFREALprincipalz_phot_l95lower 95% confidence limit derived from the photo-z PDFREALprincipalz_phot_u95upper 95% confidence limit derived from the photo-z PDFREALprincipalz_specspectroscopic redshift, if availableREALprincipalsurveysource of the spectroscopic redshiftVARCHARprincipaltrainingwhether or not the spectroscopic redshift is used for the photo-z trainingVARCHARprincipalnoirlab_test2.35_des_dr1The noirlab des_dr1.main table pre-joined with des_dr1.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.snr_yS/NVARCHARprincipaldesignationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalcoadd_object_idUnique identifier for the coadded objectsVARCHARprincipalhpix_32Healpix ID for nside=32, nested schemaVARCHARprincipalhpix_64Healpix ID for nside=64, nested schemaVARCHARprincipalhpix_1024Healpix ID for nside=1024, nested schemaVARCHARprincipalhpix_4096Healpix ID for nside=4096, nested schemaVARCHARprincipalhpix_16384Healpix ID for nside=16384, nested schemaVARCHARprincipalraRight ascension, with quantized precision for indexing (ALPHAWIN_J2000 has full precision but not indexed)degpos.eq.raVARCHARprincipaldecDeclination, with quantized precision for indexing (DELTAWIN_J2000 has full precision but not indexed)degpos.eq.decVARCHARprincipalalphawin_j2000Right ascension for the object, J2000 in ICRS system (full precision but not indexed)degVARCHARprincipaldeltawin_j2000Declination for the object, J2000 in ICRS (full precision but not indexed)degVARCHARprincipalgalactic_lGalactic LongitudedegVARCHARprincipalgalactic_bGalactic LatitudedegVARCHARprincipalecliptic_lonEcliptic LongitudedegVARCHARprincipalecliptic_latEcliptic LatitudedegVARCHARprincipalxwin_imageX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_imageY-centroid from windowed measurements on coadded imagepixelVARCHARprincipalerrx2win_image_gUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_rUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_iUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_zUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrx2win_image_yUncertainty in second moment of x-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_gUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_rUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_iUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_zUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerry2win_image_yUncertainty in second moment of y-distribution centroid, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_gUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_rUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_iUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_zUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalerrxywin_image_yUncertainty in second moment of xy-distribution, from converged windowed measurementspixel2VARCHARprincipalx2win_image_gSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_rSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_iSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_zSecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipalx2win_image_ySecond moment in x-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_gSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_rSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_iSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_zSecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipaly2win_image_ySecond moment in y-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_gSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_rSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_iSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_zSecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxywin_image_ySecond moment in xy-direction, from converged windowed measurementspixel2VARCHARprincipalxwin_image_gX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_rX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_iX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_zX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalxwin_image_yX-centroid from windowed measurements on coadded imagepixelVARCHARprincipalywin_image_gY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_rY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_iY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_zY-centroid from windowed measurements on coadded imageVARCHARprincipalywin_image_yY-centroid from windowed measurements on coadded imageVARCHARprincipala_imageMajor axis size based on an isophotal modelpixelVARCHARprincipalerra_imageUncertainty in major axis size, from isophotal modelpixelVARCHARprincipalb_imageMinor axis size based on an isophotal modelpixelVARCHARprincipalerrb_imageUncertainty in minor axis size, from isophotal modelpixelVARCHARprincipaltheta_j2000Position angle of source in J2000 coordinates, from non-windowed measurementdegVARCHARprincipalerrtheta_imageUncertainty in source position, from isophotal modeldegVARCHARprincipalkron_radiusKron radiuspixelVARCHARprincipalebv_sfd98E(B-V) reddening oefficient from Schelgel, Finkbeiner & Davis (1998)magVARCHARprincipalmag_auto_g_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_r_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_i_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_z_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_y_deredDereddened magnitude estimation (using SFD98), for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_aper_8_g_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_r_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_i_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_z_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalmag_aper_8_y_deredDereddened magnitude estimation (using SFD98) for circular aperturesmagVARCHARprincipalwavg_mag_psf_g_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_r_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_i_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_z_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_y_deredDereddened weighted average magnitude (using SFD98) from PSF fit single epoch detectionsmagVARCHARprincipalawin_image_gMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_rMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_iMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_zMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalawin_image_yMajor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_gMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_rMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_iMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_zMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalbwin_image_yMinor axis size, from 2nd order windowed moment measurementspixelsVARCHARprincipalthetawin_image_gPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_rPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_iPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_zPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalthetawin_image_yPosition angle of source, for converged windowed measurement grow from x to ydegVARCHARprincipalerrawin_image_gUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_rUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_iUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_zUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrawin_image_yUncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_gUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_rUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_iUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_zUncertainty in Minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrbwin_image_yUncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noisepixelVARCHARprincipalerrthetawin_image_gUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_rUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_iUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_zUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalerrthetawin_image_yUncertainty in source position angle, from converged windowed measurementdegVARCHARprincipalflux_radius_gHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_rHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_iHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_zHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalflux_radius_yHalf-light radius for the object, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_gFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_rFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_iFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_zFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalfwhm_image_yFWHM measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensionspixelVARCHARprincipalbackground_gBackground level, by CCD-amplifiermagVARCHARprincipalbackground_rBackground level, by CCD-amplifiermagVARCHARprincipalbackground_iBackground level, by CCD-amplifiermagVARCHARprincipalbackground_zBackground level, by CCD-amplifiermagVARCHARprincipalbackground_yBackground level, by CCD-amplifiermagVARCHARprincipalkron_radius_gKron radius measured from detection imagepixelVARCHARprincipalkron_radius_rKron radius measured from detection imagepixelVARCHARprincipalkron_radius_iKron radius measured from detection imagepixelVARCHARprincipalkron_radius_zKron radius measured from detection imagepixelVARCHARprincipalkron_radius_yKron radius measured from detection imagepixelVARCHARprincipalmag_auto_gMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_rMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_iMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_zMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmag_auto_yMagnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_gUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_rUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusmagVARCHARprincipalmagerr_auto_iUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_zUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmagerr_auto_yUncertainty in magnitude estimation, for an elliptical model based on the Kron radiusVARCHARprincipalmag_aper_8_gMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_rMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_iMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_zMagnitude estimation for circular aperturesmagVARCHARprincipalmag_aper_8_yMagnitude estimation for circular aperturesmagVARCHARprincipalmagerr_aper_8_gUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_rUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_iUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_zUncertainty in magnitude estimation for circular aperturesVARCHARprincipalmagerr_aper_8_yUncertainty in magnitude estimation for circular aperturesVARCHARprincipalwavg_mag_psf_gWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_rWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_iWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_zWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_mag_psf_yWeighted average magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_gUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_rUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_iUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_zUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalwavg_magerr_psf_yUncertainty of weighted averaged magnitude, of PSF fit single epoch detectionsmagVARCHARprincipalflux_auto_gFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_rFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_iFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_zFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalflux_auto_yFlux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_guncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_runcertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_iuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_zuncertainty in flux measurement, for an elliptical model based on Kron radiusADUVARCHARprincipalfluxerr_auto_yuncertainty in flux measurement, for an elliptical model based on Kron radiusVARCHARprincipalflux_aper_8_gFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_rFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_iFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_zFlux measurement for circular aperturesADUVARCHARprincipalflux_aper_8_yFlux measurement for circular aperturesADUVARCHARprincipalfluxerr_aper_8_gUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_rUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_iUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_zUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalfluxerr_aper_8_yUncertainty in aperture-flux measurement, elliptical model based on the Kron radiusADUVARCHARprincipalwavg_flux_psf_gWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_rWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_iWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_zWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_flux_psf_yWeighted average flux measurement of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_gUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_rUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_iUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_zUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalwavg_fluxerr_psf_yUncertainty of weighted average flux, of PSF fit single epoch detectionsADUVARCHARprincipalclass_star_gSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_rSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_iSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_zSimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalclass_star_ySimple morphological extended source classifier. Values between 0 (galaxies) and 1 (stars). SPREAD_MODEL exhibits better performance for morphological classification.VARCHARprincipalspread_model_gMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_rMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_iMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_zMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalspread_model_yMorphology based classifier based on comparison between a PSF versus exponential-PSF model. Values closer to 0 correspond to stars, larger values correspond to galaxies.VARCHARprincipalwavg_spread_model_gSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_rSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_iSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_zSPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spread_model_ySPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalspreaderr_model_gUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_rUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_iUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_zUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalspreaderr_model_yUncertainty in morphology based classifier based on comparison between PSF versus exponential-PSF model.VARCHARprincipalwavg_spreaderr_model_gUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_rUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_iUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_zUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalwavg_spreaderr_model_yUncertainty in SPREAD MODEL using the weighted averaged values from single epoch detectionsVARCHARprincipalg_rG-R colorVARCHARprincipalr_iR-I colorVARCHARprincipali_zI-Z colorVARCHARprincipalz_yZ-Y colorVARCHARprincipalsnr_gS/NVARCHARprincipalsnr_rS/NVARCHARprincipalsnr_iS/NVARCHARprincipalsnr_zS/NVARCHARprincipalimaflags_iso_gFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_gNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_rFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_rNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_iFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_iNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_zFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_zNumber of epochs the source in detected in single epoch imagesVARCHARprincipalimaflags_iso_yFlag identifying sources with missing/flagged pixels, considering all single epoch imagesVARCHARprincipalnepochs_yNumber of epochs the source in detected in single epoch imagesVARCHARprincipalhtm9HTM Level-9 indexVARCHARprincipalring256Healpix ID with nside=256, ring schemaVARCHARprincipalnest4096Healpix ID with nside=4096, nested schemaVARCHARprincipalisoarea_image_gIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_rIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_iIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_zIsophotal area of the coadded sourcepixel^2VARCHARprincipalisoarea_image_yIsophotal area of the coadded sourcepixel^2VARCHARprincipalniter_model_gNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_rNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_iNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_zNumber of iterations in model fitting photometric measurementsVARCHARprincipalniter_model_yNumber of iterations in model fitting photometric measurementsVARCHARprincipalflags_gAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_rAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_iAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_zAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipalflags_yAdditive flag describing cautionary advice about source extraction process. Use less than 4 for well behaved objectsVARCHARprincipaltilenameTile nameVARCHARprincipalnoirlab_test2.35_allwiseThe noirlab allwise.source table for the respective EMU regiondesignationUnique source IDmeta.idVARCHARindexedprincipalraRight Ascension (ICRS)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination (ICRS)degpos.eq.dec;meta.mainDOUBLEindexedprincipalhtm9HTM index (order 9 => ~10 arcmin size)INTEGERprincipalring256HEALPIX index (Nsides 256, Ring scheme => ~14 arcmin size)INTEGERprincipalnest4096HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec sizeINTEGERprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalsigraOne-sigma uncertaintly in RA from non-moving source extractionarcsecREALprincipalsigdecOne-sigma uncertaintly in Dec from non-moving source extractionarcsecREALprincipalsigradecThe co-sigma of equatorial position uncertainties sigra/sigdecarcsecREALprincipalglonGalactic Longitudedegpos.gal.lonDOUBLEprincipalglatGalactic Latitudedegpos.gal.latDOUBLEprincipalelonEcliptic Longitudedegpos.ecl.lonDOUBLEprincipalelatEcliptic Latitudedegpos.ecl.latDOUBLEprincipalwxX-pixel coord of source in Atlas imagepixREALprincipalwyY-pixel coord of source in Atlas imagepixREALprincipalcntrUnique ID number for this object in the AllWISE Catalog/Reject table.BIGINTprincipalsource_idUnique source IDVARCHARprincipalcoadd_idAtlas Tile identifier from which source was extractedVARCHARprincipalsrcSequential number of the source extraction in the Atlas TileINTEGERprincipalw1mproW1 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.3-4umREALprincipalw1sigmproW1 measurement uncertainty in mag unitsmagREALprincipalw1snrW1 S/N ratioREALprincipalw1rchi2Reduced chi^2 of the W1 measurementREALprincipalw2mproW2 magnitude measured with profile-fitting photometrymagphot.mag;em.IR.4-8umREALprincipalw2sigmproW2 measurement uncertainty in mag unitsmagREALprincipalw2snrW2 S/N ratioREALprincipalw2rchi2Reduced chi^2 of the W2 measurementREALprincipalw3mproW3 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.8-15umREALprincipalw3sigmproW3 measurement uncertainty in mag unitsmagREALprincipalw3snrW3 S/N ratioREALprincipalw3rchi2Reduced chi^2 of the W3 measurementREALprincipalw4mproW4 magnitude measured with profile-fitting photometrymagphot.flux.density;em.IR.15-30umREALprincipalw4sigmproW4 measurement uncertainty in mag unitsmagREALprincipalw4snrW4 S/N ratioREALprincipalw4rchi2Reduced chi^2 of the W4 measurementREALprincipalrchi2Combined reduced chi^w in all bandsREALprincipalnbNumber of PSF components used simultaneously in profile-fitting for this sourcemeta.numberINTEGERprincipalnaActive deblending flag (0 = source not actively deblended, 1 = source actively deblended)meta.numberINTEGERprincipalw1satSaturated pixel fraction, W1instr.saturationREALprincipalw2satSaturated pixel fraction, W2instr.saturationREALprincipalw3satSaturated pixel fraction, W3instr.saturationREALprincipalw4satSaturated pixel fraction, W4instr.saturationREALprincipalsatnumMinimum sample at which saturation occurs in each bandinstr.saturationVARCHARprincipalra_pmRA at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipaldec_pmDeclination at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted.degDOUBLEprincipalsigra_pmOne-sigma uncertaintly in ra_pmarcsecREALprincipalsigdec_pmOne-sigma uncertaintly in dec_pmarcsecREALprincipalsigradec_pmThe co-sigma of the equatorial position uncertainties from the profile-fitting measurement model that includes motion, sigra_pm, sigdec_pmarcsecREALprincipalpmraApparent motion in RA for this sourcemas / yrINTEGERprincipalsigpmraUncertainty in RA motion estimationmas / yrINTEGERprincipalpmdecApparent motion in Dec for this sourcemas / yrINTEGERprincipalsigpmdecUncertainty in Dec motion estimationmas / yrINTEGERprincipalw1rchi2_pmReduced chi^2 of W1 including motion estimationREALprincipalw2rchi2_pmReduced chi^2 of W2 including motion estimationREALprincipalw3rchi2_pmReduced chi^2 of W3 including motion estimationREALprincipalw4rchi2_pmReduced chi^2 of W4 including motion estimationREALprincipalrchi2_pmCombined reduced chi^2 in all bands including motion estimationREALprincipalpmcodeThis is a five character string that encodes information about factors that impact the accuracy of the motion estimation.VARCHARprincipalcc_flagsContamination and confusion flagVARCHARprincipalrelSmall separation, same-Tile detection flagVARCHARprincipalext_flgExtended source flagINTEGERprincipalvar_flgVariability flagVARCHARprincipalph_qualPhotometric quality flagVARCHARprincipaldet_bitBit-encoded integer indicating bands in which a source has a w?snr>2 detectionINTEGERprincipalmoon_levScattered moonlight contamination flagVARCHARprincipalw1nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement.INTEGERprincipalw1mInteger frame coverage -- no. of individual 7.2s W1 exposures on which measurement was possibleINTEGERprincipalw2nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement.INTEGERprincipalw2mInteger frame coverage -- no. of individual 7.2s W2 exposures on which measurement was possibleINTEGERprincipalw3nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement.INTEGERprincipalw3mInteger frame coverage -- no. of individual 7.2s W3 exposures on which measurement was possibleINTEGERprincipalw4nmInteger frame detection count -- no. of individual 7.7s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement.INTEGERprincipalw4mInteger frame coverage -- no. of individual 7.2s W4 exposures on which measurement was possibleINTEGERprincipalw1covMean pixel coverage in W1REALprincipalw2covMean pixel coverage in W2REALprincipalw3covMean pixel coverage in W3REALprincipalw4covMean pixel coverage in W4REALprincipalw1cc_mapContamination and confusion map for this source in W1INTEGERprincipalw1cc_map_strContamination and confusion stringVARCHARprincipalw2cc_mapContamination and confusion map for this source in W2INTEGERprincipalw2cc_map_strContamination and confusion stringVARCHARprincipalw3cc_mapContamination and confusion map for this source in W3INTEGERprincipalw3cc_map_strContamination and confusion stringVARCHARprincipalw4cc_mapContamination and confusion map for this source in W4INTEGERprincipalw4cc_map_strContamination and confusion stringVARCHARprincipalbest_use_cntrCntr identification value of the source extraction that was selected as a candidate Catalog source in the duplicate resolution process for the group of associated sources that included this extraction.BIGINTprincipalngrpExcess number of positionally associated duplicate resolution groups in which this extractions was includedSMALLINTprincipaltmass_key2MASS PSC association. Unique identifier of the closest source in the 2MASS Point Source Catalog (PSC) that falls within 3arcsec of the non-motion fit position of this WISE source.INTEGERprincipalr_2massDistance separating the positions of the WISE source and associated 2MASS PSC sourceREALprincipalpa_2massPosition angle (degrees E of N) of the vector from the WISE source to the associated 2MASS PSC sourceREALprincipaln_2massThe number of 2MASS PSC entries found within a 3arcsec radius of the WISE source positionINTEGERprincipalj_m_2mass2MASS J-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalj_msig_2mass2MASS J-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalh_m_2mass2MASS H-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalh_msig_2mass2MASS H-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalk_m_2mass2MASS K-band magnitude or magnitude upper limit of the associated 2MASS PSC sourceREALprincipalk_msig_2mass2MASS K-band corrected photometric uncertainty of the associated 2MASS PSC sourceREALprincipalspt_indLevel 7 HTM spatial index keyINTEGERprincipalhtm20Level 20 HTM spatial index keyBIGINTprincipalnoirlab_test2.34_des_dr2The noirlab des_dr2.main table pre-joined with des_dr2.x1p5__main__allwise__source and allwise.source noirlab tables for the respective EMU region. Join with the allwise table for all the allwise columns.designationUnique source IDmeta.idVARCHARindexedprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalalphawin_j2000right ascension for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalawin_image_gg-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_ii-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_rr-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_yy-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalawin_image_zz-band major axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipala_imagemajor axis size based on an isophotal model [pixel]pixelREALprincipalbackground_gg-band background level, by ccd-amplifier [mag]magREALprincipalbackground_ii-band background level, by ccd-amplifier [mag]magREALprincipalbackground_rr-band background level, by ccd-amplifier [mag]magREALprincipalbackground_yy-band background level, by ccd-amplifier [mag]magREALprincipalbackground_zz-band background level, by ccd-amplifier [mag]magREALprincipalbwin_image_gg-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_ii-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_rr-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_yy-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalbwin_image_zz-band minor axis size, from 2nd order windowed moment measurements [pixels]pixelsREALprincipalb_imageminor axis size based on an isophotal model [pixel]pixelREALprincipalclass_star_gg-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_ii-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_rr-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_yy-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalclass_star_zz-band simple morphological extended source classifier. values between 0 (galaxies) and 1 (stars). spread_model exhibits better performance for morphological classification.src.classREALprincipalcoadd_object_idunique identifier for the coadded objectsmeta.id;meta.mainBIGINTindexedprincipaldecdeclination, with quantized precision for indexing (deltawin_j2000 has full precision but not indexed) [degrees]degpos.eq.dec;meta.mainDOUBLEindexedprincipaldeltawin_j2000declination for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalebv_sfd98e(b-v) reddening coefficient from schlegel, finkbeiner & davis, 1998 [mag]magDOUBLEprincipalerrawin_image_gg-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_ii-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_rr-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_yy-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrawin_image_zz-band uncertainty in major axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerra_imageuncertainty in major axis size, from isophotal model [pixel]pixelREALprincipalerrbwin_image_gg-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_ii-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_rr-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_yy-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrbwin_image_zz-band uncertainty in minor axis size, from converged windowed measurement, assuming uncorrelated noise [pixel]pixelREALprincipalerrb_imageuncertainty in minor axis size, from isophotal model [pixel]pixelREALprincipalerrthetawin_image_gg-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_ii-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_rr-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_yy-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrthetawin_image_zz-band uncertainty in source position angle, from converged windowed measurement [degrees]degREALprincipalerrtheta_imageuncertainty in source position, from isophotal model [degrees]degREALprincipalerrx2win_image_gg-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalnepochs_ii-band number of epochs the source is detected in single epoch imagesINTEGERprincipalerrx2win_image_ii-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_rr-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_yy-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrx2win_image_zz-band uncertainty in second moment of x-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_gg-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_ii-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_rr-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_yy-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerrxywin_image_zz-band uncertainty in second moment of xy-distribution, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_gg-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_ii-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_rr-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_yy-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalerry2win_image_zz-band uncertainty in second moment of y-distribution centroid, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalextended_class_coadd0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using sextractor photometrySMALLINTprincipalextended_class_wavg0: high confidence stars; 1: candidate stars; 2: mostly galaxies; 3: high confidence galaxies; -9: no data; using wavg photometrySMALLINTprincipalflags_gg-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_ii-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_rr-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_yy-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_zz-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalfluxerr_auto_gg-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_ii-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_rr-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_yy-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_zz-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_gg-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_ii-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_rr-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_yy-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_zz-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_radius_gg-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_ii-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_rr-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_yy-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalflux_radius_zz-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_gg-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_ii-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_rr-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_yy-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalfwhm_image_zz-band fwhm measured from the isophotal area, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixelREALprincipalgalactic_bgalactic latitude [degrees]degpos.galactic.latREALprincipalgalactic_lgalactic longitude [degrees]degpos.galactic.lonREALprincipalhpix_1024healpix identifier for nside=1024 grid size, in a nested schemaBIGINTprincipalhpix_16384healpix identifier for nside=16384 grid size, in a nested schemaBIGINTprincipalhpix_32healpix identifier for nside=32 grid size, in a nested schemaBIGINTprincipalhpix_4096healpix identifier for nside=4096 grid size, in a nested schemaBIGINTprincipalhpix_64healpix identifier for nside=64 grid size, in a nested schemaBIGINTprincipalimaflags_iso_gg-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_ii-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_rr-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_yy-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalimaflags_iso_zz-band flag identifying sources with missing/flagged pixels, considering all single epoch imagesINTEGERprincipalisoarea_image_gg-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_ii-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_rr-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_yy-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalisoarea_image_zz-band isophotal area of the coadded source [pixel2]pixel2INTEGERprincipalkron_radiuskron radius measured from detection image [pixel]pixelREALprincipalkron_radius_gg-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_ii-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_rr-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_yy-band kron radius measured from coadded image [pixel]pixelREALprincipalkron_radius_zz-band kron radius measured from coadded image [pixel]pixelREALprincipalmagerr_auto_gg-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_ii-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_rr-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_yy-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmagerr_auto_zz-band uncertainty in magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_gg-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_g_deredg-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_ii-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_i_deredi-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_rr-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_r_deredr-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_yy-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_y_deredy-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_zz-band magnitude estimation, for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_z_deredz-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalnepochs_gg-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_rr-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_yy-band number of epochs the source is detected in single epoch imagesINTEGERprincipalnepochs_zz-band number of epochs the source is detected in single epoch imagesINTEGERprincipalniter_model_gg-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_ii-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_rr-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_yy-band number of iterations in model fitting photometric measurementsINTEGERprincipalniter_model_zz-band number of iterations in model fitting photometric measurementsINTEGERprincipalraright ascension, with quantized precision for indexing (alphawin_j2000 has full precision but not indexed) [degrees]degpos.eq.ra;meta.mainDOUBLEindexedprincipalspreaderr_model_gg-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_ii-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_rr-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_yy-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspreaderr_model_zz-band uncertainty in morphology based classifier based on comparison between psf versus exponential-psf model.REALprincipalspread_model_gg-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_ii-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_rr-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_yy-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalspread_model_zz-band morphology based classifier based on comparison between a psf versus exponential-psf model. values closer to 0 correspond to stars, larger values correspond to galaxiessrc.classREALprincipalthetawin_image_gg-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_ii-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_rr-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_yy-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipalthetawin_image_zz-band position angle of source, for converged windowed measurement grow from x to y [degrees]degREALprincipaltheta_j2000position angle of source in j2000 coordinates, from non-windowed measurement [degrees]degREALprincipaltilenameidentifier of each one of the tiles on which the survey is griddedVARCHARprincipalwavg_fluxerr_psf_gg-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_ii-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_rr-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_yy-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_zz-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_gg-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_ii-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_rr-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_yy-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_zz-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_magerr_psf_gg-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_ii-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_rr-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_yy-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_magerr_psf_zz-band uncertainty of weighted averaged magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_gg-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_g_deredg-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_ii-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_i_deredi-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_rr-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_r_deredr-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_yy-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_y_deredy-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_zz-band weighted average magnitude, of psf fit single epoch detections [mag]magREALprincipalwavg_mag_psf_z_deredz-band dereddened weighted average magnitude (using sfd98) from psf fit single epoch detections [mag]magREALprincipalwavg_spreaderr_model_gg-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_ii-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_rr-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_yy-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spreaderr_model_zz-band uncertainty in spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_gg-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_ii-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_rr-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_yy-band spread model using the weighted averaged values from single epoch detectionsREALprincipalwavg_spread_model_zz-band spread model using the weighted averaged values from single epoch detectionsREALprincipalx2win_image_gg-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_ii-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_rr-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_yy-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalx2win_image_zz-band second moment in x-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxwin_imagex-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalxwin_image_gg-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_ii-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_rr-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_yy-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxwin_image_zz-band x-centroid from windowed measurements on coadded band image [pixel]pixelDOUBLEprincipalxywin_image_gg-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_ii-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_rr-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_yy-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalxywin_image_zz-band second moment in xy-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_gg-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_ii-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_rr-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_yy-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipaly2win_image_zz-band second moment in y-direction, from converged windowed measurements [pixel2]pixel2DOUBLEprincipalywin_imagey-centroid from windowed measurements on coadded image [pixel]pixelDOUBLEprincipalywin_image_gg-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_ii-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_rr-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_yy-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalywin_image_zz-band y-centroid from windowed measurements on coadded band images [pixel]pixelDOUBLEprincipalhtm9Ninth level (~10 arcmin resolution) Hierarchical Triangular Mesh index (Szalay et al. 2007)meta.codeINTEGERprincipalnest4096Nested-scheme HEALPix (Gorski et al. 2005) index with NSIDE=4096 (~1 arcmin resolution)meta.codeINTEGERprincipalring256Ring-scheme HEALPix (Gorski et al. 2005) index with NSIDE=256 (~14 arcmin resolution)meta.codeINTEGERprincipalg_rG-R colormagphot.colorREALprincipalr_iR-I colormagphot.colorREALprincipali_zI-Z colormagphot.colorREALprincipalz_yZ-Y colormagphot.colorREALprincipalsnr_gS/N in g-bandmagstat.snrREALprincipalsnr_rS/N in r-bandmagstat.snrREALprincipalsnr_iS/N in i-bandmagstat.snrREALprincipalsnr_yS/N in Y-bandmagstat.snrREALprincipalsnr_zS/N in z-bandmagstat.snrREALprincipalecliptic_latEcliptic Latitudedegpos.ecliptic.latDOUBLEprincipalecliptic_lonEcliptic Longitudedegpos.ecliptic.lonDOUBLEprincipalrandom_idRandom ID in the range 0.0 => 100.0REALprincipalsami_dr3<div id="project_overview_text"><p>The SAMI Galaxy Survey is a spatially resolved spectroscopic survey of a large sample of nearby (z<0.1) galaxies, conducted with the Sydney – Australian Astronomical Observatory Multi-Object Integral Field Spectrograph (SAMI). SAMI is mounted on the 3.9 meter Anglo-Australian Telescope at Siding Spring Observatory. Survey observations began in March 2013 and were completed in May 2018. At the completion of survey observing, just over 3000 total galaxies were observed.</p><p>The key science goals of the SAMI Survey are to answer the following questions:</p><ul><li>What is the physical role of environment in galaxy evolution?</li><li>What is the relationship between stellar mass growth and angular momentum development in galaxies?</li><li>How does gas get into and out of galaxies, and how does this drive star formation?</li></ul></div>sami_dr3.SSPAperturesDR3Single stellar population equivalent age, [Z/H] and [alpha/Fe] measured from aperture spectraCATIDSAMI galaxy IDmeta.idVARCHARprincipalCUBEIDFull internal filename of the source cube for the measurementsmeta.idVARCHARprincipalCUBEIDPUBFull filename of the public source cube for the measurementsmeta.idVARCHARprincipalAge_3KPC_ROUNDSSP Age within the 3KPC apertureGyrstime.ageDOUBLEprincipalZ_3KPC_ROUNDSSP Z within the 3KPC aperturephys.abundDOUBLEprincipalalpha_3KPC_ROUNDSSP alpha within the 3KPC aperturephys.abundDOUBLEprincipalAge_3KPC_ROUND_ERRUncertainty on SSP Age within the 3KPC apertureGyrstime.age;stat.errorDOUBLEprincipalZ_3KPC_ROUND_ERRUncertainty on SSP Z within the 3KPC aperturephys.abund;stat.errorDOUBLEprincipalalpha_3KPC_ROUND_ERRUncertainty on SSP alpha within the 3KPC aperturephys.abund;stat.errorDOUBLEprincipalAge_3_ARCSECONDSSP Age within the 3 arcsec apertureGyrstime.ageDOUBLEprincipalZ_3_ARCSECONDSSP Z within the 3 arcsec aperturephys.abundDOUBLEprincipalalpha_3_ARCSECONDSSP alpha within the 3 arcsec aperturephys.abundDOUBLEprincipalAge_3_ARCSECOND_ERRUncertainty on SSP Age within the 3 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_3_ARCSECOND_ERRUncertainty on SSP Z within the 3 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_3_ARCSECOND_ERRUncertainty on SSP alpha within the 3 arcsec aperturephys.abund;stat.errorDOUBLEprincipalAge_RESSP Age within the RE apertureGyrstime.ageDOUBLEprincipalZ_RESSP Z within the RE aperturephys.abundDOUBLEprincipalalpha_RESSP alpha within the RE aperturephys.abundDOUBLEprincipalAge_RE_ERRUncertainty on SSP Age within the RE apertureGyrstime.age;stat.errorDOUBLEprincipalZ_RE_ERRUncertainty on SSP Z within the RE aperturephys.abund;stat.errorDOUBLEprincipalalpha_RE_ERRUncertainty on SSP alpha within the RE aperturephys.abund;stat.errorDOUBLEprincipalAge_RE_MGESSP Age within the RE apertureGyrstime.ageDOUBLEprincipalZ_RE_MGESSP Z within the RE aperturephys.abundDOUBLEprincipalalpha_RE_MGESSP alpha within the RE aperturephys.abundDOUBLEprincipalAge_RE_MGE_ERRUncertainty on SSP Age within the RE apertureGyrstime.age;stat.errorDOUBLEprincipalZ_RE_MGE_ERRUncertainty on SSP Z within the RE aperturephys.abund;stat.errorDOUBLEprincipalalpha_RE_MGE_ERRUncertainty on SSP alpha within the RE aperturephys.abund;stat.errorDOUBLEprincipalAge_2_ARCSECONDSSP Age within the 2 arcsec apertureGyrstime.ageDOUBLEprincipalZ_2_ARCSECONDSSP Z within the 2 arcsec aperturephys.abundDOUBLEprincipalalpha_2_ARCSECONDSSP alpha within the 2 arcsec aperturephys.abundDOUBLEprincipalAge_2_ARCSECOND_ERRUncertainty on SSP Age within the 2 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_2_ARCSECOND_ERRUncertainty on SSP Z within the 2 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_2_ARCSECOND_ERRUncertainty on SSP alpha within the 2 arcsec aperturephys.abund;stat.errorDOUBLEprincipalAge_1_4_ARCSECONDSSP Age within the 1.4 arcsec apertureGyrstime.ageDOUBLEprincipalZ_1_4_ARCSECONDSSP Z within the 1.4 arcsec aperturephys.abundDOUBLEprincipalalpha_1_4_ARCSECONDSSP alpha within the 1.4 arcsec aperturephys.abundDOUBLEprincipalAge_1_4_ARCSECOND_ERRUncertainty on SSP Age within the 1.4 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_1_4_ARCSECOND_ERRUncertainty on SSP Z within the 1.4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_1_4_ARCSECOND_ERRUncertainty on SSP alpha within the 1.4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalAge_4_ARCSECONDSSP Age within the 4 arcsec apertureGyrstime.ageDOUBLEprincipalZ_4_ARCSECONDSSP Z within the 4 arcsec aperturephys.abundDOUBLEprincipalalpha_4_ARCSECONDSSP alpha within the 4 arcsec aperturephys.abundDOUBLEprincipalAge_4_ARCSECOND_ERRUncertainty on SSP Age within the 4 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_4_ARCSECOND_ERRUncertainty on SSP Z within the 4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_4_ARCSECOND_ERRUncertainty on SSP alpha within the 4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalsami_dr3.samiDR3gaskinPAGas Kinematic PA CatalogueCUBEIDInternal unique cube IDmeta.idVARCHARprincipalCUBEIDPUBPublic unique cube ID for data releasemeta.idVARCHARprincipalCUBENAMEInternal unique cube name for blue cubemeta.idVARCHARprincipalCATIDSAMI Galaxy IDmeta.idVARCHARprincipalPA_GASKINGas kinematic position angle. Anticlockwise, North=0 degreesdegpos.posAngREALprincipalPA_GASKIN_ERR1-sigma error on the gas kinematic position angledegpos.posAngREALprincipalsami_dr3.CubeObsSAMI cube observations, quality and flagging catalogueCUBEIDPUBPublic unique cube ID for data releasemeta.idVARCHARprincipalCUBEIDInternal unique cube IDmeta.idVARCHARprincipalCUBENAMEInternal unique cube name for blue cubemeta.idVARCHARprincipalCATIDSAMI Galaxy IDmeta.idVARCHARprincipalCUBEFWHMFWHM of PSF in cubearcsecinst.beamREALprincipalCUBETEXPTotal exposure time for cubesecobs.exposureREALprincipalMEANTRANSMean transmission for cubeobs.paramREALprincipalISBESTFlag to indicate best repeatmeta.code.qualBOOLEANprincipalCATSOURCEFlag to identify input source cataloguemeta.code.classINTEGERprincipalWARNSTARFlag to indicate that object is a calibration starmeta.code.qualINTEGERprincipalWARNFILLFlag to indicate that object is from a filler cataloguemeta.code.qualINTEGERprincipalWARNZFlag to indicate potential error in input catalogue redshiftmeta.code.qualINTEGERprincipalWARNMULTFlag to indicate multiple objects within IFU field-of-viewmeta.code.qualINTEGERprincipalWARNAKPCFlag to indicate 3kpc aperture spectra are missingmeta.code.qualINTEGERprincipalWARNAREFlag to indicate Sersic Re aperture spectra are missingmeta.code.qualINTEGERprincipalWARNAMGEFlag to indicate MGE Re aperture spectra are missingmeta.code.qualINTEGERprincipalWARNSK2MFlag to indicate 2-moment stellar kinematics are missingmeta.code.qualINTEGERprincipalWARNSK4MFlag to indicate 4-moment stellar kinematics are missingmeta.code.qualINTEGERprincipalWARNSK4MHSNFlag to indicate high-S/N binned 4-moment stellar kinematics are missingmeta.code.qualINTEGERprincipalWARNFCALFlag to indicate flux calibration issuesmeta.code.qualINTEGERprincipalWARNFCBRFlag to indicate flux calibration issues with offset between red and blue armmeta.code.qualINTEGERprincipalWARNSKYBFlag to indicate excess sky subtraction residuals in blue armmeta.code.qualINTEGERprincipalWARNSKYRFlag to indicate excess sky subtraction residuals in red armmeta.code.qualINTEGERprincipalWARNSKERFlag to indicate problem with stellar kinematicsmeta.code.qualINTEGERprincipalWARNWCSFlag to indicate target galaxy is offset from centre of cubemeta.code.qualINTEGERprincipalWARNREFlag to indicate large difference between MGE and Sersic effective radiusmeta.code.qualINTEGERprincipalWARNSKEMFlag to indicate possible impact of sky lines on emission line fittingmeta.code.qualINTEGERprincipalWARNEMFTFlag to indicate missing emission line fitsmeta.code.qualINTEGERprincipalsami_dr3.InputCatFillerSAMI input catalogue for filler objectsCATIDSAMI Galaxy IDmeta.idVARCHARindexedprincipalRA_OBJJ2000 Right Ascension of objectdegpos.eq.raDOUBLEindexedprincipalDEC_OBJJ2000 Declination of objectdegpos.eq.decDOUBLEindexedprincipalz_specSpectroscopic redshiftsrc.redshiftREALprincipalFILLFLAGFlag for different filler classesmeta.code.classINTEGERprincipalsami_dr3.VisualMorphologyDR3SDSS/VST-based Visual morphological classificationCATIDSAMI Galaxy IDnonemeta.idVARCHARprincipalTYPEMorphological Type (0=E; 0.5=E/S0; 1=S0; 1.5=S0/Early-spiral; 2=Early-spiral; 2.5=Early/Late spiral; 3=Late spiral; 5=?; -9=no agreement)nonemeta.code.classDOUBLEprincipalsami_dr3.FstarCatClustersSAMI calibration stars in cluster regionsCATIDObject identifiermeta.idVARCHARindexedprincipalRAJ2000 Right Ascension of objectdegpos.eq.raDOUBLEindexedprincipalDecJ2000 Declination of objectdegpos.eq.decDOUBLEindexedprincipalrr-band PSF magnitudemagphot.magREALprincipalpriorityPriority class for targetsmeta.code.classINTEGERprincipalsami_dr3.InputCatGAMADR3SAMI input catalogue for GAMA regionsCATIDSAMI Galaxy IDmeta.idVARCHARindexedprincipalRA_OBJJ2000 Right Ascension of objectdegpos.eq.raDOUBLEindexedprincipalDEC_OBJJ2000 Declination of objectdegpos.eq.decDOUBLEindexedprincipalRA_IFUJ2000 Right Ascension of nominal IFU centredegpos.eq.raDOUBLEprincipalDEC_IFUJ2000 Declination of nominal IFU centredegpos.eq.decDOUBLEprincipalr_petroExtinction-corrected SDSS DR7 r-band Petrosian magmagphot.magREALprincipalr_autor-band SExtractor auto magnitudemagphot.magREALprincipalz_tonryFlow-corrected redshiftsrc.redshiftREALprincipalz_specSpectroscopic redshiftsrc.redshiftREALprincipalM_rAbsolute r-band magnitudemagphot.magAbs;em.opt.RREALprincipalr_er-band major axis effective radiusarcsecphys.angSizeREALprincipalmu_within_1reMean r-band surface brightness within 1 effective radiusmag/arcsec^2phot.mag.sbREALprincipalmu_1rer-band surface brightness at 1 effective radiusmag/arcsec^2phot.mag.sbREALprincipalmu_2rer-band surface brightness at 2 effective radiimag/arcsec^2phot.mag.sbREALprincipalellipr-band ellipticitysrc.ellipticityREALprincipalPAr-band position angledegpos.posAngREALprincipalMstarLogarithm of stellar massdex solar massesphys.massREALprincipalg_i(g-i) colourmagphot.colorREALprincipalA_gg-band extinctionmagphys.absorptionREALprincipalSURV_SAMIPriority class for targetsmeta.code.classINTEGERprincipalBAD_CLASSFlag for bad or problem objectsmeta.code.qualINTEGERprincipalsami_dr3.MGEPhotomUnregDR3Results from Multi Gaussian Expansion fitting of imaging dataCATIDSAMI Galaxy ID. Galaxies with two entries have both VST and SDSS photometry.meta.idVARCHARprincipalphotometryDenotes which images were used.meta.refVARCHARprincipalReMGECircularised effective radius from MGE fit.arcsecphys.angSizeREALprincipalmMGETotal AB magnitude from the MGE fit. No corrections applied.magphot.magREALprincipalrExtinctionExtinction from Schlafly+2011.magphys.absorptionREALprincipalPAMGEPosition Angle of the MGE model, from N to E is positive.degpos.posAngREALprincipalepsMGE_ReModel isophotal ellipticity at one Re.src.ellipticityREALprincipalepsMGE_LWLight-weighted ellipticity of the model.src.ellipticityREALprincipaldist2NNeighDistance to nearest neighbour from SExtractor source extraction.arcsecpos.angDistanceREALprincipalChi2Chi^2 from MGE fit.stat.fit.chi2REALprincipalsami_dr3.InputCatClustersDR3SAMI input catalogue for cluster regionsCATIDSAMI Galaxy IDmeta.idVARCHARindexedprincipalRA_OBJJ2000 Right Ascension of objectdegpos.eq.raDOUBLEindexedprincipalDEC_OBJJ2000 Declination of objectdegpos.eq.decDOUBLEindexedprincipalr_petroExtinction-corrected r-band Petrosian magmagphot.magREALprincipalr_autor-band SExtractor auto magnitudemagphot.magREALprincipalz_specSpectroscopic redshiftsrc.redshiftREALprincipalM_rAbsolute r-band magnitudemagphot.magAbs;em.opt.RREALprincipalr_er-band major axis effective radiusarcsecphys.angSizeREALprincipalmu_within_1reMean r-band surface brightness within 1 effective radiusmag/arcsec^2phot.mag.sbREALprincipalmu_1rer-band surface brightness at 1 effective radiusmag/arcsec^2phot.mag.sbREALprincipalmu_2rer-band surface brightness at 2 effective radiimag/arcsec^2phot.mag.sbREALprincipalellipr-band ellipticitysrc.ellipticityREALprincipalPAr-band position angledegpos.posAngREALprincipalg_i(g-i) colourmagphot.colorREALprincipalMstarLogarithm of stellar massdexphys.massREALprincipalR_on_rtwoProjected distance from cluster centre normalised by R200arith.ratioREALprincipalV_on_sigmaLine-of-sight velocity relative to cluster redshift normalised by cluster velocity dispersion measured within R200arith.ratioREALprincipalis_memFlag indicating cluster membership (1=member, 0=non-member)meta.code.memberREALprincipalSURV_SAMIPriority class for targetsmeta.code.classINTEGERprincipalBAD_CLASSFlag for bad or problem objectsmeta.code.qualINTEGERprincipalsami_dr3.DensityCatDR35th nearest neighbour surface density estimatesCATIDSAMI Galaxy IDmeta.idVARCHARprincipalSurfaceDensity5th nearest neighbour surface density estimateMpc^-2src.densityREALprincipalSurfaceDensity_errSurface density uncertaintyMpc^-2stat.error;src.densityREALprincipalCompletenessCorrectionMultiplicative factor correcting SurfaceDensity for spectroscopic completenesarith.factorREALprincipalAreaCorrectionMultiplicative factor correcting SurfaceDensity for smaller area due to edge effectsarith.factorREALprincipalSurfaceDensityFlagFlag indicating problems with surface density measurementmeta.code.error;src.densitylINTEGERprincipalSurfaceDensity_m19Same as SurfaceDensity, but for Mr < -19.Mpc^-2src.densityREALprincipalSurfaceDensity_err_m19Same as SurfaceDensity_err, but for Mr < -19.Mpc^-2stat.error;src.densityREALprincipalCompletenessCorrection_m19Same as CompletenessCorrection, but for Mr < -19.arith.factorREALprincipalAreaCorrection_m19Same as AreaCorrection, but for Mr < -19.arith.factorREALprincipalSurfaceDensityFlag_m19Same as SurfaceDensityFlag, but for Mr < -19.meta.code.error;src.densitylINTEGERprincipalsami_dr3.FstarCatGAMASAMI calibration stars in GAMA regionsCATIDObject identifiermeta.idVARCHARindexedprincipalRAJ2000 Right Ascension of objectdegpos.eq.raDOUBLEindexedprincipalDecJ2000 Declination of objectdegpos.eq.decDOUBLEindexedprincipalrr-band PSF magnitudemagphot.magREALprincipalpriorityPriority class for targetsmeta.code.classINTEGERprincipalsami_dr3.samiDR3StelkinStellar kinematic measurements catalogueCUBEIDInternal ID for cubemeta.idVARCHARprincipalCUBEIDPUBPublic cube IDmeta.idVARCHARprincipalCUBENAMEName of blue cube filemeta.idVARCHARprincipalCATIDCatalog ID from Bryant et al. 2015 and Owers et al. 2017meta.idVARCHARprincipalPA_STELKINKinematic position angle. Anticlockwise, North=0 degreesdegpos.posAngREALprincipalPA_STELKIN_ERR1-sigma error on the kinematic position angledegpos.posAngREALprincipalSIGMA_REVelocity dispersion from Re Sersic aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_RE_ERR1-sigma error on sigma_rekm/sphys.veloc.dispersionREALprincipalSIGMA_3KPC_ROUNDVelocity dispersion from 3kpc aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_3KPC_ROUND_ERR1-sigma error on sigma_3kpckm/sphys.veloc.dispersionREALprincipalSIGMA_1_4_ARCSECONDVelocity dispersion from 1.4 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_1_4_ARCSECOND_ERR1-sigma error on sigma_1_4_arcseckm/sphys.veloc.dispersionREALprincipalSIGMA_2_ARCSECONDVelocity dispersion from 2 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_2_ARCSECOND_ERR1-sigma error on sigma_2_arcseckm/sphys.veloc.dispersionREALprincipalSIGMA_3_ARCSECONDVelocity dispersion from 3 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_3_ARCSECOND_ERR1-sigma error on sigma_3_arcseckm/sphys.veloc.dispersionREALprincipalSIGMA_4_ARCSECONDVelocity dispersion from 4 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_4_ARCSECOND_ERR1-sigma error on sigma_4_arcseckm/sphys.veloc.dispersionREALprincipalAPER_CORR_FLAGFlag to indicate whether lambdar_re and vsigma_re have been aperture corrected. 0 = no aperture correction applied. 1 = inside-out aperture corrected (rmax < re). 2 = from outside in (re < hwhm_psf)meta.code.errorREALprincipalRMAX_APER_CORRRadius at which the aperture corrected value was determined fromRearith.ratioREALprincipalLAMBDAR_RESpin Parameter proxy within effective ellipse as defined in van de Sande et al. 2017arith.ratioREALprincipalLAMBDAR_RE_ERR1-sigma error on lambdar_rearith.ratioREALprincipalLAMBDAR_MAXLambdar at maximum radius that is used for aperture correction (where APER_CORR_FLAG = 1)arith.ratioREALprincipalLAMBDAR_MAX_ERR1-sigma error on lambdar_Maxarith.ratioREALprincipalVSIGMA_REFlux weighted V/sigma within Re effective ellipsearith.ratioREALprincipalVSIGMA_RE_ERR1-sigma error on vsigma_earith.ratioREALprincipalVSIGMA_MAXV/sigma at maximum radius that is used for aperture correction (where APER_CORR_FLAG = 1)arith.ratioREALprincipalVSIGMA_MAX_ERR1-sigma error on VSigma_maxarith.ratioREALprincipalMEAN_K51_REkinematic asymmetry estimate from kinemetry within Rearith.ratioREALprincipalMEAN_K51_RE_ERR1-sigma error on mean_k51_rearith.ratioREALprincipalSIGMA_RE_MGEVelocity dispersion from MGE Re aperture spectrakm/sphys.veloc.dispersionREALprincipalSIGMA_RE_MGE_ERR1-sigma error on sigma_re_mgekm/sphys.veloc.dispersionREALprincipalAPER_CORR_FLAG_MGEFlag to indicate whether lambdar_re_mge and vsigma_re_mge have been aperture corrected. 0 = no aperture correction applied. 1 = inside-out aperture corrected (rmax < MGE re). 2 = from outside in (re < hwhm_psf)meta.code.errorREALprincipalRMAX_APER_CORR_MGEMGE relative Radius at which the aperture corrected value was determined fromRearith.ratioREALprincipalLAMBDAR_RE_MGESpin Parameter proxy within MGE effective ellipse as defined in van de Sande et al. 2017arith.ratioREALprincipalLAMBDAR_RE_MGE_ERR1-sigma error on lambdar_re_mgearith.ratioREALprincipalLAMBDAR_MAX_MGEMGE Lambdar at maximum radius that is used for aperture correction (where APER_CORR_FLAG_MGE = 1)arith.ratioREALprincipalLAMBDAR_MAX_MGE_ERR1-sigma error on lambdar_Max_mgearith.ratioREALprincipalVSIGMA_RE_MGEFlux weighted V/sigma within MGE Re effective ellipsearith.ratioREALprincipalVSIGMA_RE_MGE_ERR1-sigma error on vsigma_e_mgearith.ratioREALprincipalVSIGMA_MAX_MGEMGE V/sigma at maximum radius that is used for aperture correction (where APER_CORR_FLAG_MGE = 1)arith.ratioREALprincipalVSIGMA_MAX_MGE_ERR1-sigma error on VSigma_max_mgearith.ratioREALprincipalMEAN_K51_RE_MGEkinematic asymmetry estimate from kinemetry within MGE Rearith.ratioREALprincipalMEAN_K51_RE_MGE_ERR1-sigma error on mean_k51_re_mgearith.ratioREALprincipalsami_dr3.EmissionLine1compDR3Aperture 1-component emission line fluxes, ionised gas kinematics, and star formation ratesCUBEIDInternal unique cube IDmeta.idVARCHARprincipalCUBEIDPUBPublic unique cube ID for data releasemeta.idVARCHARprincipalCUBENAMEName of specific blue cubemeta.idVARCHARprincipalCATIDSAMI galaxy IDmeta.idVARCHARprincipalZ_SPECSAMI galaxy Redshiftmeta.idREALprincipalNPIX_1_4_ARCSECONDNumber of pixels in 1.4-ARCSECOND aperture_meta.valueINTEGERprincipalAREA_COV_1_4_ARCSECONDFraction of SAMI FoV covered by 1.4-ARCSECOND aperturemeta.valueREALprincipalV_GAS_1_4_ARCSECONDGas velocity in 1.4-ARCSECOND aperturekm/sphys.velocityREALprincipalV_GAS_1_4_ARCSECOND_ERRUncertainty on Gas velocity in 1.4-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_1_4_ARCSECONDGas velocity dispersion in 1.4-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_1_4_ARCSECOND_ERRUncertainty on Gas velocity dispersion in 1.4-ARCSECOND aperturekm/sphys.velocityREALprincipalOII3726_1_4_ARCSECONDTotal [OII]3726 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_1_4_ARCSECOND_ERRUncertainty on total [OII]3726 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_1_4_ARCSECONDTotal [OII]3729 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_1_4_ARCSECOND_ERRUncertainty on total [OII]3729 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_1_4_ARCSECONDTotal [NeIII]3869 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_1_4_ARCSECOND_ERRUncertainty on total [NeIII]3869 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_1_4_ARCSECONDTotal Hepsilon flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_1_4_ARCSECOND_ERRUncertainty on total Hepsilon flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_1_4_ARCSECONDTotal Hdelta flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_1_4_ARCSECOND_ERRUncertainty on total Hdelta flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_1_4_ARCSECONDTotal Hgamma flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_1_4_ARCSECOND_ERRUncertainty on total Hgamma flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_1_4_ARCSECONDTotal [OIII]4363 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_1_4_ARCSECOND_ERRUncertainty on total [OIII]4363 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_1_4_ARCSECONDTotal Hbeta flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_1_4_ARCSECOND_ERRUncertainty on total Hbeta flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_1_4_ARCSECONDTotal [OIII]5007 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_1_4_ARCSECOND_ERRUncertainty on total [OIII]5007 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_1_4_ARCSECONDTotal [OI]6300 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_1_4_ARCSECOND_ERRUncertainty on total [OI]6300 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_1_4_ARCSECONDTotal Halpha flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_1_4_ARCSECOND_ERRUncertainty on total Halpha flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_1_4_ARCSECONDTotal [NII]6583 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_1_4_ARCSECOND_ERRUncertainty on total [NII]6583 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_1_4_ARCSECONDTotal [SII]6716 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_1_4_ARCSECOND_ERRUncertainty on total [SII]6716 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_1_4_ARCSECONDTotal [SII]6731 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_1_4_ARCSECOND_ERRUncertainty on total [SII]6731 flux in 1.4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_1_4_ARCSECONDExtinction correction on total Halpha flux in 1.4-ARCSECOND aperturephys.fluxcorrREALprincipalEXT_CORR_1_4_ARCSECOND_ERRUncertainty in extinction correction on Halpha flux in 1.4-ARCSECOND aperturephys.fluxcorrREALprincipalSFR_1_4_ARCSECONDStar formation rate in 1.4-ARCSECOND apertureMsun/yrphys.sfrREALprincipalSFR_1_4_ARCSECOND_ERRUncertainty in star formation rate in 1.4-ARCSECOND apertureMsun/yrphys.sfrREALprincipalNPIX_2_ARCSECONDNumber of pixels in 2-ARCSECOND aperture_meta.valueINTEGERprincipalAREA_COV_2_ARCSECONDFraction of SAMI FoV covered by 2-ARCSECOND aperturemeta.valueREALprincipalV_GAS_2_ARCSECONDGas velocity in 2-ARCSECOND aperturekm/sphys.velocityREALprincipalV_GAS_2_ARCSECOND_ERRUncertainty on Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_2_ARCSECONDGas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_2_ARCSECOND_ERRUncertainty on Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityREALprincipalOII3726_2_ARCSECONDTotal [OII]3726 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_2_ARCSECOND_ERRUncertainty on total [OII]3726 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_2_ARCSECONDTotal [OII]3729 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_2_ARCSECOND_ERRUncertainty on total [OII]3729 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_2_ARCSECONDTotal [NeIII]3869 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_2_ARCSECOND_ERRUncertainty on total [NeIII]3869 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_2_ARCSECONDTotal Hepsilon flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_2_ARCSECOND_ERRUncertainty on total Hepsilon flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_2_ARCSECONDTotal Hdelta flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_2_ARCSECOND_ERRUncertainty on total Hdelta flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_2_ARCSECONDTotal Hgamma flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_2_ARCSECOND_ERRUncertainty on total Hgamma flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_2_ARCSECONDTotal [OIII]4363 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_2_ARCSECOND_ERRUncertainty on total [OIII]4363 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_2_ARCSECONDTotal Hbeta flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_2_ARCSECOND_ERRUncertainty on total Hbeta flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_2_ARCSECONDTotal [OIII]5007 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_2_ARCSECOND_ERRUncertainty on total [OIII]5007 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_2_ARCSECONDTotal [OI]6300 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_2_ARCSECOND_ERRUncertainty on total [OI]6300 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_2_ARCSECONDTotal Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_2_ARCSECOND_ERRUncertainty on total Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_2_ARCSECONDTotal [NII]6583 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_2_ARCSECOND_ERRUncertainty on total [NII]6583 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_2_ARCSECONDTotal [SII]6716 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_2_ARCSECOND_ERRUncertainty on total [SII]6716 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_2_ARCSECONDTotal [SII]6731 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_2_ARCSECOND_ERRUncertainty on total [SII]6731 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_2_ARCSECONDExtinction correction on total Halpha flux in 2-ARCSECOND aperturephys.fluxcorrREALprincipalEXT_CORR_2_ARCSECOND_ERRUncertainty in extinction correction on Halpha flux in 2-ARCSECOND aperturephys.fluxcorrREALprincipalSFR_2_ARCSECONDStar formation rate in 2-ARCSECOND apertureMsun/yrphys.sfrREALprincipalSFR_2_ARCSECOND_ERRUncertainty in star formation rate in 2-ARCSECOND apertureMsun/yrphys.sfrREALprincipalNPIX_3_ARCSECONDNumber of pixels in 3-ARCSECOND aperture_meta.valueINTEGERprincipalAREA_COV_3_ARCSECONDFraction of SAMI FoV covered by 3-ARCSECOND aperturemeta.valueREALprincipalV_GAS_3_ARCSECONDGas velocity in 3-ARCSECOND aperturekm/sphys.velocityREALprincipalV_GAS_3_ARCSECOND_ERRUncertainty on Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_3_ARCSECONDGas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_3_ARCSECOND_ERRUncertainty on Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityREALprincipalOII3726_3_ARCSECONDTotal [OII]3726 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_3_ARCSECOND_ERRUncertainty on total [OII]3726 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_3_ARCSECONDTotal [OII]3729 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_3_ARCSECOND_ERRUncertainty on total [OII]3729 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_3_ARCSECONDTotal [NeIII]3869 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_3_ARCSECOND_ERRUncertainty on total [NeIII]3869 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_3_ARCSECONDTotal Hepsilon flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_3_ARCSECOND_ERRUncertainty on total Hepsilon flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_3_ARCSECONDTotal Hdelta flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_3_ARCSECOND_ERRUncertainty on total Hdelta flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_3_ARCSECONDTotal Hgamma flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_3_ARCSECOND_ERRUncertainty on total Hgamma flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_3_ARCSECONDTotal [OIII]4363 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_3_ARCSECOND_ERRUncertainty on total [OIII]4363 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_3_ARCSECONDTotal Hbeta flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_3_ARCSECOND_ERRUncertainty on total Hbeta flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_3_ARCSECONDTotal [OIII]5007 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_3_ARCSECOND_ERRUncertainty on total [OIII]5007 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_3_ARCSECONDTotal [OI]6300 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_3_ARCSECOND_ERRUncertainty on total [OI]6300 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_3_ARCSECONDTotal Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_3_ARCSECOND_ERRUncertainty on total Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_3_ARCSECONDTotal [NII]6583 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_3_ARCSECOND_ERRUncertainty on total [NII]6583 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_3_ARCSECONDTotal [SII]6716 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_3_ARCSECOND_ERRUncertainty on total [SII]6716 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_3_ARCSECONDTotal [SII]6731 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_3_ARCSECOND_ERRUncertainty on total [SII]6731 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_3_ARCSECONDExtinction correction on total Halpha flux in 3-ARCSECOND aperturephys.fluxcorrREALprincipalEXT_CORR_3_ARCSECOND_ERRUncertainty in extinction correction on Halpha flux in 3-ARCSECOND aperturephys.fluxcorrREALprincipalSFR_3_ARCSECONDStar formation rate in 3-ARCSECOND apertureMsun/yrphys.sfrREALprincipalSFR_3_ARCSECOND_ERRUncertainty in star formation rate in 3-ARCSECOND apertureMsun/yrphys.sfrREALprincipalNPIX_4_ARCSECONDNumber of pixels in 4-ARCSECOND aperture_meta.valueINTEGERprincipalAREA_COV_4_ARCSECONDFraction of SAMI FoV covered by 4-ARCSECOND aperturemeta.valueREALprincipalV_GAS_4_ARCSECONDGas velocity in 4-ARCSECOND aperturekm/sphys.velocityREALprincipalV_GAS_4_ARCSECOND_ERRUncertainty on Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_4_ARCSECONDGas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityREALprincipalVDISP_GAS_4_ARCSECOND_ERRUncertainty on Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityREALprincipalOII3726_4_ARCSECONDTotal [OII]3726 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_4_ARCSECOND_ERRUncertainty on total [OII]3726 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_4_ARCSECONDTotal [OII]3729 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_4_ARCSECOND_ERRUncertainty on total [OII]3729 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_4_ARCSECONDTotal [NeIII]3869 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_4_ARCSECOND_ERRUncertainty on total [NeIII]3869 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_4_ARCSECONDTotal Hepsilon flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_4_ARCSECOND_ERRUncertainty on total Hepsilon flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_4_ARCSECONDTotal Hdelta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_4_ARCSECOND_ERRUncertainty on total Hdelta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_4_ARCSECONDTotal Hgamma flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_4_ARCSECOND_ERRUncertainty on total Hgamma flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_4_ARCSECONDTotal [OIII]4363 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_4_ARCSECOND_ERRUncertainty on total [OIII]4363 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_4_ARCSECONDTotal Hbeta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_4_ARCSECOND_ERRUncertainty on total Hbeta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_4_ARCSECONDTotal [OIII]5007 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_4_ARCSECOND_ERRUncertainty on total [OIII]5007 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_4_ARCSECONDTotal [OI]6300 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_4_ARCSECOND_ERRUncertainty on total [OI]6300 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_4_ARCSECONDTotal Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_4_ARCSECOND_ERRUncertainty on total Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_4_ARCSECONDTotal [NII]6583 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_4_ARCSECOND_ERRUncertainty on total [NII]6583 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_4_ARCSECONDTotal [SII]6716 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_4_ARCSECOND_ERRUncertainty on total [SII]6716 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_4_ARCSECONDTotal [SII]6731 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_4_ARCSECOND_ERRUncertainty on total [SII]6731 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_4_ARCSECONDExtinction correction on total Halpha flux in 4-ARCSECOND aperturephys.fluxcorrREALprincipalEXT_CORR_4_ARCSECOND_ERRUncertainty in extinction correction on Halpha flux in 4-ARCSECOND aperturephys.fluxcorrREALprincipalSFR_4_ARCSECONDStar formation rate in 4-ARCSECOND apertureMsun/yrphys.sfrREALprincipalSFR_4_ARCSECOND_ERRUncertainty in star formation rate in 4-ARCSECOND apertureMsun/yrphys.sfrREALprincipalNPIX_3KPC_ROUNDNumber of pixels in 3KPC ROUND aperture_meta.valueINTEGERprincipalAREA_COV_3KPC_ROUNDFraction of SAMI FoV covered by 3KPC ROUND aperturemeta.valueREALprincipalV_GAS_3KPC_ROUNDGas velocity in 3KPC ROUND aperturekm/sphys.velocityREALprincipalV_GAS_3KPC_ROUND_ERRUncertainty on Gas velocity in 3KPC ROUND aperturekm/sphys.velocityREALprincipalVDISP_GAS_3KPC_ROUNDGas velocity dispersion in 3KPC ROUND aperturekm/sphys.velocityREALprincipalVDISP_GAS_3KPC_ROUND_ERRUncertainty on Gas velocity dispersion in 3KPC ROUND aperturekm/sphys.velocityREALprincipalOII3726_3KPC_ROUNDTotal [OII]3726 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_3KPC_ROUND_ERRUncertainty on total [OII]3726 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_3KPC_ROUNDTotal [OII]3729 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_3KPC_ROUND_ERRUncertainty on total [OII]3729 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_3KPC_ROUNDTotal [NeIII]3869 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_3KPC_ROUND_ERRUncertainty on total [NeIII]3869 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_3KPC_ROUNDTotal Hepsilon flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_3KPC_ROUND_ERRUncertainty on total Hepsilon flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_3KPC_ROUNDTotal Hdelta flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_3KPC_ROUND_ERRUncertainty on total Hdelta flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_3KPC_ROUNDTotal Hgamma flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_3KPC_ROUND_ERRUncertainty on total Hgamma flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_3KPC_ROUNDTotal [OIII]4363 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_3KPC_ROUND_ERRUncertainty on total [OIII]4363 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_3KPC_ROUNDTotal Hbeta flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_3KPC_ROUND_ERRUncertainty on total Hbeta flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_3KPC_ROUNDTotal [OIII]5007 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_3KPC_ROUND_ERRUncertainty on total [OIII]5007 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_3KPC_ROUNDTotal [OI]6300 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_3KPC_ROUND_ERRUncertainty on total [OI]6300 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_3KPC_ROUNDTotal Halpha flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_3KPC_ROUND_ERRUncertainty on total Halpha flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_3KPC_ROUNDTotal [NII]6583 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_3KPC_ROUND_ERRUncertainty on total [NII]6583 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_3KPC_ROUNDTotal [SII]6716 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_3KPC_ROUND_ERRUncertainty on total [SII]6716 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_3KPC_ROUNDTotal [SII]6731 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_3KPC_ROUND_ERRUncertainty on total [SII]6731 flux in 3KPC ROUND aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_3KPC_ROUNDExtinction correction on total Halpha flux in 3KPC ROUND aperturephys.fluxcorrREALprincipalEXT_CORR_3KPC_ROUND_ERRUncertainty in extinction correction on Halpha flux in 3KPC ROUND aperturephys.fluxcorrREALprincipalSFR_3KPC_ROUNDStar formation rate in 3KPC ROUND apertureMsun/yrphys.sfrREALprincipalSFR_3KPC_ROUND_ERRUncertainty in star formation rate in 3KPC ROUND apertureMsun/yrphys.sfrREALprincipalNPIX_RENumber of pixels in RE aperture_meta.valueINTEGERprincipalAREA_COV_REFraction of SAMI FoV covered by RE aperturemeta.valueREALprincipalV_GAS_REGas velocity in RE aperturekm/sphys.velocityREALprincipalV_GAS_RE_ERRUncertainty on Gas velocity in RE aperturekm/sphys.velocityREALprincipalVDISP_GAS_REGas velocity dispersion in RE aperturekm/sphys.velocityREALprincipalVDISP_GAS_RE_ERRUncertainty on Gas velocity dispersion in RE aperturekm/sphys.velocityREALprincipalOII3726_RETotal [OII]3726 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_RE_ERRUncertainty on total [OII]3726 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_RETotal [OII]3729 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_RE_ERRUncertainty on total [OII]3729 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_RETotal [NeIII]3869 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_RE_ERRUncertainty on total [NeIII]3869 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_RETotal Hepsilon flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_RE_ERRUncertainty on total Hepsilon flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_RETotal Hdelta flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_RE_ERRUncertainty on total Hdelta flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_RETotal Hgamma flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_RE_ERRUncertainty on total Hgamma flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_RETotal [OIII]4363 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_RE_ERRUncertainty on total [OIII]4363 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_RETotal Hbeta flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_RE_ERRUncertainty on total Hbeta flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_RETotal [OIII]5007 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_RE_ERRUncertainty on total [OIII]5007 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_RETotal [OI]6300 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_RE_ERRUncertainty on total [OI]6300 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_RETotal Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_RE_ERRUncertainty on total Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_RETotal [NII]6583 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_RE_ERRUncertainty on total [NII]6583 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_RETotal [SII]6716 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_RE_ERRUncertainty on total [SII]6716 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_RETotal [SII]6731 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_RE_ERRUncertainty on total [SII]6731 flux in RE aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_REExtinction correction on total Halpha flux in RE aperturephys.fluxcorrREALprincipalEXT_CORR_RE_ERRUncertainty in extinction correction on Halpha flux in RE aperturephys.fluxcorrREALprincipalSFR_REStar formation rate in RE apertureMsun/yrphys.sfrREALprincipalSFR_RE_ERRUncertainty in star formation rate in RE apertureMsun/yrphys.sfrREALprincipalNPIX_RE_MGENumber of pixels in RE_MGE aperture_meta.valueINTEGERprincipalAREA_COV_RE_MGEFraction of SAMI FoV covered by RE_MGE aperturemeta.valueREALprincipalV_GAS_RE_MGEGas velocity in RE_MGE aperturekm/sphys.velocityREALprincipalV_GAS_RE_MGE_ERRUncertainty on Gas velocity in RE_MGE aperturekm/sphys.velocityREALprincipalVDISP_GAS_RE_MGEGas velocity dispersion in RE_MGE aperturekm/sphys.velocityREALprincipalVDISP_GAS_RE_MGE_ERRUncertainty on Gas velocity dispersion in RE_MGE aperturekm/sphys.velocityREALprincipalOII3726_RE_MGETotal [OII]3726 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3726_RE_MGE_ERRUncertainty on total [OII]3726 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_RE_MGETotal [OII]3729 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOII3729_RE_MGE_ERRUncertainty on total [OII]3729 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_RE_MGETotal [NeIII]3869 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNEIII3869_RE_MGE_ERRUncertainty on total [NeIII]3869 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_RE_MGETotal Hepsilon flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHEPSILON_RE_MGE_ERRUncertainty on total Hepsilon flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_RE_MGETotal Hdelta flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHDELTA_RE_MGE_ERRUncertainty on total Hdelta flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_RE_MGETotal Hgamma flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHGAMMA_RE_MGE_ERRUncertainty on total Hgamma flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_RE_MGETotal [OIII]4363 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII4363_RE_MGE_ERRUncertainty on total [OIII]4363 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_RE_MGETotal Hbeta flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHBETA_RE_MGE_ERRUncertainty on total Hbeta flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_RE_MGETotal [OIII]5007 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOIII5007_RE_MGE_ERRUncertainty on total [OIII]5007 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_RE_MGETotal [OI]6300 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalOI6300_RE_MGE_ERRUncertainty on total [OI]6300 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_RE_MGETotal Halpha flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalHALPHA_RE_MGE_ERRUncertainty on total Halpha flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_RE_MGETotal [NII]6583 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalNII6583_RE_MGE_ERRUncertainty on total [NII]6583 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_RE_MGETotal [SII]6716 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6716_RE_MGE_ERRUncertainty on total [SII]6716 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_RE_MGETotal [SII]6731 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalSII6731_RE_MGE_ERRUncertainty on total [SII]6731 flux in RE_MGE aperture1E-16 erg/s/cm2phys.fluxREALprincipalEXT_CORR_RE_MGEExtinction correction on total Halpha flux in RE_MGE aperturephys.fluxcorrREALprincipalEXT_CORR_RE_MGE_ERRUncertainty in extinction correction on Halpha flux in RE_MGE aperturephys.fluxcorrREALprincipalSFR_RE_MGEStar formation rate in RE_MGE apertureMsun/yrphys.sfrREALprincipalSFR_RE_MGE_ERRUncertainty in star formation rate in RE_MGE apertureMsun/yrphys.sfrREALprincipalsami_dr3.IndexAperturesDR3Lick index measurements from aperture spectraCATIDSAMI galaxy IDmeta.idVARCHARprincipalCUBEIDFull internal filename of the source cube for the measurementsmeta.idVARCHARprincipalCUBEIDPUBFull filename of the public source cube for the measurementsmeta.idVARCHARprincipalHdeltaA_3KPC_ROUNDHdeltaA index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_3KPC_ROUNDHdeltaF index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_3KPC_ROUNDHgammaA index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_3KPC_ROUNDHgammaF index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_3KPC_ROUNDHbeta index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_3KPC_ROUNDMgb index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_3KPC_ROUNDFe4383 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_3KPC_ROUNDFe4668 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_3KPC_ROUNDFe5015 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_3KPC_ROUNDFe5270 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_3KPC_ROUNDFe5335 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_3KPC_ROUNDCN1 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalCN2_3KPC_ROUNDCN2 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalCa4227_3KPC_ROUNDCa4227 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_3KPC_ROUNDG4300 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_3KPC_ROUNDMg1 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalMg2_3KPC_ROUNDMg2 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalFe4531_3KPC_ROUNDFe4531 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_3KPC_ROUNDFe5406 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_3KPC_ROUNDCa4455 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_3KPC_ROUND_ERRUncertainty on the HdeltaA index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_3KPC_ROUND_ERRUncertainty on the HdeltaF index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_3KPC_ROUND_ERRUncertainty on the HgammaA index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_3KPC_ROUND_ERRUncertainty on the HgammaF index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_3KPC_ROUND_ERRUncertainty on the Hbeta index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_3KPC_ROUND_ERRUncertainty on the Mgb index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_3KPC_ROUND_ERRUncertainty on the Fe4383 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_3KPC_ROUND_ERRUncertainty on the Fe4668 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_3KPC_ROUND_ERRUncertainty on the Fe5015 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_3KPC_ROUND_ERRUncertainty on the Fe5270 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_3KPC_ROUND_ERRUncertainty on the Fe5335 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_3KPC_ROUND_ERRUncertainty on the CN1 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_3KPC_ROUND_ERRUncertainty on the CN2 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_3KPC_ROUND_ERRUncertainty on the Ca4227 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_3KPC_ROUND_ERRUncertainty on the G4300 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_3KPC_ROUND_ERRUncertainty on the Mg1 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_3KPC_ROUND_ERRUncertainty on the Mg2 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_3KPC_ROUND_ERRUncertainty on the Fe4531 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_3KPC_ROUND_ERRUncertainty on the Fe5406 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_3KPC_ROUND_ERRUncertainty on the Ca4455 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_3_ARCSECONDHdeltaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_3_ARCSECONDHdeltaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_3_ARCSECONDHgammaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_3_ARCSECONDHgammaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_3_ARCSECONDHbeta index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_3_ARCSECONDMgb index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_3_ARCSECONDFe4383 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_3_ARCSECONDFe4668 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_3_ARCSECONDFe5015 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_3_ARCSECONDFe5270 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_3_ARCSECONDFe5335 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_3_ARCSECONDCN1 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_3_ARCSECONDCN2 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_3_ARCSECONDCa4227 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_3_ARCSECONDG4300 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_3_ARCSECONDMg1 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_3_ARCSECONDMg2 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_3_ARCSECONDFe4531 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_3_ARCSECONDFe5406 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_3_ARCSECONDCa4455 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_3_ARCSECOND_ERRUncertainty on the HdeltaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_3_ARCSECOND_ERRUncertainty on the HdeltaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_3_ARCSECOND_ERRUncertainty on the HgammaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_3_ARCSECOND_ERRUncertainty on the HgammaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_3_ARCSECOND_ERRUncertainty on the Hbeta index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_3_ARCSECOND_ERRUncertainty on the Mgb index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_3_ARCSECOND_ERRUncertainty on the Fe4383 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_3_ARCSECOND_ERRUncertainty on the Fe4668 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_3_ARCSECOND_ERRUncertainty on the Fe5015 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_3_ARCSECOND_ERRUncertainty on the Fe5270 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_3_ARCSECOND_ERRUncertainty on the Fe5335 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_3_ARCSECOND_ERRUncertainty on the CN1 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_3_ARCSECOND_ERRUncertainty on the CN2 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_3_ARCSECOND_ERRUncertainty on the Ca4227 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_3_ARCSECOND_ERRUncertainty on the G4300 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_3_ARCSECOND_ERRUncertainty on the Mg1 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_3_ARCSECOND_ERRUncertainty on the Mg2 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_3_ARCSECOND_ERRUncertainty on the Fe4531 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_3_ARCSECOND_ERRUncertainty on the Fe5406 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_3_ARCSECOND_ERRUncertainty on the Ca4455 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_REHdeltaA index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_REHdeltaF index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_REHgammaA index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_REHgammaF index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_REHbeta index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_REMgb index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_REFe4383 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_REFe4668 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_REFe5015 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_REFe5270 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_REFe5335 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_RECN1 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalCN2_RECN2 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalCa4227_RECa4227 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_REG4300 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_REMg1 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalMg2_REMg2 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalFe4531_REFe4531 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_REFe5406 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_RECa4455 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_RE_ERRUncertainty on the HdeltaA index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_RE_ERRUncertainty on the HdeltaF index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_RE_ERRUncertainty on the HgammaA index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_RE_ERRUncertainty on the HgammaF index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_RE_ERRUncertainty on the Hbeta index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_RE_ERRUncertainty on the Mgb index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_RE_ERRUncertainty on the Fe4383 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_RE_ERRUncertainty on the Fe4668 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_RE_ERRUncertainty on the Fe5015 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_RE_ERRUncertainty on the Fe5270 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_RE_ERRUncertainty on the Fe5335 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_RE_ERRUncertainty on the CN1 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_RE_ERRUncertainty on the CN2 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_RE_ERRUncertainty on the Ca4227 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_RE_ERRUncertainty on the G4300 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_RE_ERRUncertainty on the Mg1 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_RE_ERRUncertainty on the Mg2 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_RE_ERRUncertainty on the Fe4531 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_RE_ERRUncertainty on the Fe5406 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_RE_ERRUncertainty on the Ca4455 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_2_ARCSECONDHdeltaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_2_ARCSECONDHdeltaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_2_ARCSECONDHgammaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_2_ARCSECONDHgammaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_2_ARCSECONDHbeta index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_2_ARCSECONDMgb index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_2_ARCSECONDFe4383 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_2_ARCSECONDFe4668 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_2_ARCSECONDFe5015 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_2_ARCSECONDFe5270 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_2_ARCSECONDFe5335 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_2_ARCSECONDCN1 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_2_ARCSECONDCN2 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_2_ARCSECONDCa4227 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_2_ARCSECONDG4300 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_2_ARCSECONDMg1 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_2_ARCSECONDMg2 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_2_ARCSECONDFe4531 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_2_ARCSECONDFe5406 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_2_ARCSECONDCa4455 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_2_ARCSECOND_ERRUncertainty on the HdeltaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_2_ARCSECOND_ERRUncertainty on the HdeltaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_2_ARCSECOND_ERRUncertainty on the HgammaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_2_ARCSECOND_ERRUncertainty on the HgammaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_2_ARCSECOND_ERRUncertainty on the Hbeta index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_2_ARCSECOND_ERRUncertainty on the Mgb index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_2_ARCSECOND_ERRUncertainty on the Fe4383 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_2_ARCSECOND_ERRUncertainty on the Fe4668 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_2_ARCSECOND_ERRUncertainty on the Fe5015 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_2_ARCSECOND_ERRUncertainty on the Fe5270 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_2_ARCSECOND_ERRUncertainty on the Fe5335 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_2_ARCSECOND_ERRUncertainty on the CN1 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_2_ARCSECOND_ERRUncertainty on the CN2 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_2_ARCSECOND_ERRUncertainty on the Ca4227 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_2_ARCSECOND_ERRUncertainty on the G4300 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_2_ARCSECOND_ERRUncertainty on the Mg1 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_2_ARCSECOND_ERRUncertainty on the Mg2 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_2_ARCSECOND_ERRUncertainty on the Fe4531 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_2_ARCSECOND_ERRUncertainty on the Fe5406 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_2_ARCSECOND_ERRUncertainty on the Ca4455 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_1_4_ARCSECONDHdeltaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_1_4_ARCSECONDHdeltaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_1_4_ARCSECONDHgammaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_1_4_ARCSECONDHgammaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_1_4_ARCSECONDHbeta index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_1_4_ARCSECONDMgb index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_1_4_ARCSECONDFe4383 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_1_4_ARCSECONDFe4668 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_1_4_ARCSECONDFe5015 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_1_4_ARCSECONDFe5270 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_1_4_ARCSECONDFe5335 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_1_4_ARCSECONDCN1 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_1_4_ARCSECONDCN2 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_1_4_ARCSECONDCa4227 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_1_4_ARCSECONDG4300 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_1_4_ARCSECONDMg1 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_1_4_ARCSECONDMg2 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_1_4_ARCSECONDFe4531 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_1_4_ARCSECONDFe5406 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_1_4_ARCSECONDCa4455 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_1_4_ARCSECOND_ERRUncertainty on the HdeltaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_1_4_ARCSECOND_ERRUncertainty on the HdeltaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_1_4_ARCSECOND_ERRUncertainty on the HgammaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_1_4_ARCSECOND_ERRUncertainty on the HgammaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_1_4_ARCSECOND_ERRUncertainty on the Hbeta index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_1_4_ARCSECOND_ERRUncertainty on the Mgb index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_1_4_ARCSECOND_ERRUncertainty on the Fe4383 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_1_4_ARCSECOND_ERRUncertainty on the Fe4668 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_1_4_ARCSECOND_ERRUncertainty on the Fe5015 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_1_4_ARCSECOND_ERRUncertainty on the Fe5270 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_1_4_ARCSECOND_ERRUncertainty on the Fe5335 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_1_4_ARCSECOND_ERRUncertainty on the CN1 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_1_4_ARCSECOND_ERRUncertainty on the CN2 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_1_4_ARCSECOND_ERRUncertainty on the Ca4227 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_1_4_ARCSECOND_ERRUncertainty on the G4300 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_1_4_ARCSECOND_ERRUncertainty on the Mg1 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_1_4_ARCSECOND_ERRUncertainty on the Mg2 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_1_4_ARCSECOND_ERRUncertainty on the Fe4531 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_1_4_ARCSECOND_ERRUncertainty on the Fe5406 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_1_4_ARCSECOND_ERRUncertainty on the Ca4455 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_4_ARCSECONDHdeltaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_4_ARCSECONDHdeltaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_4_ARCSECONDHgammaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_4_ARCSECONDHgammaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_4_ARCSECONDHbeta index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_4_ARCSECONDMgb index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_4_ARCSECONDFe4383 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_4_ARCSECONDFe4668 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_4_ARCSECONDFe5015 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_4_ARCSECONDFe5270 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_4_ARCSECONDFe5335 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_4_ARCSECONDCN1 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_4_ARCSECONDCN2 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_4_ARCSECONDCa4227 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_4_ARCSECONDG4300 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_4_ARCSECONDMg1 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_4_ARCSECONDMg2 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_4_ARCSECONDFe4531 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_4_ARCSECONDFe5406 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_4_ARCSECONDCa4455 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_4_ARCSECOND_ERRUncertainty on the HdeltaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_4_ARCSECOND_ERRUncertainty on the HdeltaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_4_ARCSECOND_ERRUncertainty on the HgammaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_4_ARCSECOND_ERRUncertainty on the HgammaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_4_ARCSECOND_ERRUncertainty on the Hbeta index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_4_ARCSECOND_ERRUncertainty on the Mgb index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_4_ARCSECOND_ERRUncertainty on the Fe4383 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_4_ARCSECOND_ERRUncertainty on the Fe4668 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_4_ARCSECOND_ERRUncertainty on the Fe5015 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_4_ARCSECOND_ERRUncertainty on the Fe5270 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_4_ARCSECOND_ERRUncertainty on the Fe5335 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_4_ARCSECOND_ERRUncertainty on the CN1 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_4_ARCSECOND_ERRUncertainty on the CN2 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_4_ARCSECOND_ERRUncertainty on the Ca4227 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_4_ARCSECOND_ERRUncertainty on the G4300 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_4_ARCSECOND_ERRUncertainty on the Mg1 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_4_ARCSECOND_ERRUncertainty on the Mg2 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_4_ARCSECOND_ERRUncertainty on the Fe4531 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_4_ARCSECOND_ERRUncertainty on the Fe5406 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_4_ARCSECOND_ERRUncertainty on the Ca4455 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_RE_MGEHdeltaA index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_RE_MGEHdeltaF index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_RE_MGEHgammaA index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_RE_MGEHgammaF index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_RE_MGEHbeta index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_RE_MGEMgb index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_RE_MGEFe4383 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_RE_MGEFe4668 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_RE_MGEFe5015 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_RE_MGEFe5270 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_RE_MGEFe5335 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_RE_MGECN1 index strength within the RE_MGE aperturemagspect.line;phot.magDOUBLEprincipalCN2_RE_MGECN2 index strength within the RE_MGE aperturemagspect.line;phot.magDOUBLEprincipalCa4227_RE_MGECa4227 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_RE_MGEG4300 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_RE_MGEMg1 index strength within the RE_MGE aperturemagspect.line;phot.magDOUBLEprincipalMg2_RE_MGEMg2 index strength within the RE_MGE aperturemagspect.line;phot.magDOUBLEprincipalFe4531_RE_MGEFe4531 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_RE_MGEFe5406 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_RE_MGECa4455 index strength within the RE_MGE apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_RE_MGE_ERRUncertainty on the HdeltaA index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_RE_MGE_ERRUncertainty on the HdeltaF index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_RE_MGE_ERRUncertainty on the HgammaA index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_RE_MGE_ERRUncertainty on the HgammaF index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_RE_MGE_ERRUncertainty on the Hbeta index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_RE_MGE_ERRUncertainty on the Mgb index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_RE_MGE_ERRUncertainty on the Fe4383 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_RE_MGE_ERRUncertainty on the Fe4668 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_RE_MGE_ERRUncertainty on the Fe5015 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_RE_MGE_ERRUncertainty on the Fe5270 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_RE_MGE_ERRUncertainty on the Fe5335 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_RE_MGE_ERRUncertainty on the CN1 index strength within the RE_MGE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_RE_MGE_ERRUncertainty on the CN2 index strength within the RE_MGE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_RE_MGE_ERRUncertainty on the Ca4227 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_RE_MGE_ERRUncertainty on the G4300 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_RE_MGE_ERRUncertainty on the Mg1 index strength within the RE_MGE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_RE_MGE_ERRUncertainty on the Mg2 index strength within the RE_MGE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_RE_MGE_ERRUncertainty on the Fe4531 index strength within the RE_MGE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_RE_MGE_ERRUncertainty on the Fe5406 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_RE_MGE_ERRUncertainty on the Ca4455 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFLAG_3KPC_ROUNDPotentially unreliable index measurements in the 3KPC aperturemeta.code.qualINTEGERprincipalFLAG_3_ARCSECONDPotentially unreliable index measurements in the 3 arcsec aperturemeta.code.qualINTEGERprincipalFLAG_REPotentially unreliable index measurements in the RE aperturemeta.code.qualINTEGERprincipalFLAG_2_ARCSECONDPotentially unreliable index measurements in the 2 arcsec aperturemeta.code.qualINTEGERprincipalFLAG_1_4_ARCSECONDPotentially unreliable index measurements in the 1.4 arcsec aperturemeta.code.qualINTEGERprincipalFLAG_4_ARCSECONDPotentially unreliable index measurements in the 4 arcsec aperturemeta.code.qualINTEGERprincipalFLAG_RE_MGEPotentially unreliable index measurements in the RE aperturemeta.code.qualINTEGERprincipalgama_dr2<p>GAMA is a project to exploit the latest generation of ground-based and space-borne survey facilities to study cosmology and galaxy formation and evolution. </p> <p>At the heart of this project lies the GAMA spectroscopic survey of ~300,000 galaxies down to r&nbsp;&lt;&nbsp;19.8&nbsp;mag over ~286&nbsp;deg², carried out using the <a href="http://www.aao.gov.au/AAO/2df/aaomega/aaomega.html">AAOmega</a> multi-object spectrograph on the <a href="http://www.aao.gov.au/">Anglo-Australian Telescope (AAT)</a> by the GAMA team</a>. This project was awarded 210 nights over 7 years (2008–2014) and the observations are now completed. This survey builds on, and is augmented by, previous spectroscopic surveys such as the <a href="http://www.sdss.org/">Sloan Digital Sky Survey (SDSS)</a>, the <a href="http://www.mso.anu.edu.au/2dFGRS/">2dF Galaxy Redshift Survey(2dFGRS)</a> and the <a href="http://www.eso.org/~jliske/mgc/">Millennium Galaxy Catalogue (MGC)</a>.</p>gama_dr2.EmLinesPhysGAMAThis table provides Balmer decrements, Halpha luminosities, Halpha derived star-formation rates and emission line classifications for all spectra in SpecLines with any measured Halpha emission and z > 0.001.AB_RSDSS r band absolute magnitude: PETROMAG_R - DM_70_30_70 - A_R - K_R; AB magnitudemagphys.magAbsVARCHARprincipalA_RGalactic extinction in SDSS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalBALMERDEC_FLAGIs the Balmer decrement measured or estimated?meta.code;phot.flux;arith.ratioVARCHARprincipalBALMER_DECREMENTBalmer decrement (see notes)phot.flux;arith.ratio;spect.lineVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDM_70_30_70Distance modulus for 737 cosmologymagphot.mag.distModVARCHARprincipalEMLINE_CLASSAGN classification based on Kewley et al. (2001)meta.codeVARCHARprincipalEMLINE_METHODAGN classification method (see notes)meta.codeVARCHARprincipalF_HALPHAStellar absorption corrected Halpha flux10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalF_HBETAStellar absorption corrected Hbeta flux10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalIS_BESTSpectrum with best redshift for this object across all surveys?meta.codeVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in GAMA AAT survey?meta.codeVARCHARprincipalK_RK-correction in SDSS r bandmagphot.magVARCHARprincipalL_APCORHalpha luminosity corrected for stellar absorption and fibre aperture effectsWphys.luminosity;em.line.HalphaVARCHARprincipalL_APOBSCORHalpha luminosity corrected for stellar absorption, fibre aperture effects and dust obscurationWphys.luminosity;em.line.HalphaVARCHARprincipalNQNormalised redshift quality (use NQ>2 for science)meta.code.qual;src.redshiftVARCHARprincipalPETROMAG_RSDSS r band Petrosian magnitude (not corrected for Galactic extinction)magphot.mag;em.opt.RVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSFRHalpha derived star formation rate assuming a Salpeter IMFM_sun/yrphys.SFR;em.line.HalphaVARCHARprincipalSN_CONTContinuum signal-to-noisestat.snrVARCHARprincipalSN_EMIHalpha emission signal-to-noisestat.snrVARCHARprincipalSPECIDUnique spectrum IDmeta.id;meta.mainVARCHARindexedprincipalWARNING_FLAGHalpha or Hbeta affected by data reduction issues?meta.codeVARCHARprincipalZ_HELIOHeliocentric redshiftsrc.redshiftVARCHARprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalgama_dr2.TilingCatScience targets and information for tiling and spectroscopic observation.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalDECJ2000 coordinatedegpos.eq.decVARCHARindexedprincipalDR2_FLAGIndicates whether spectra, redshifts and ancillary data for this object are released in DR2meta.codeVARCHARprincipalFIBERMAG_R3-arcsec fiber magnitudemagphot.mag;em.opt.RVARCHARprincipalG_MODELExtinction-corrected SDSS DR6 magmagphot.mag;em.opt.BVARCHARprincipalI_MODELExtinction-corrected SDSS DR6 magmagphot.mag;em.opt.IVARCHARprincipalK_AUTOExtinction-corrected r-defined auto AB magmagphot.mag;em.IR.KVARCHARprincipalMASK_IC_10Mask value 0.0 to 1.0 around V<10 starsmeta.codeVARCHARprincipalMASK_IC_12Mask value 0.0 to 1.0 around V<12 starsmeta.codeVARCHARprincipalNEIGHBOUR_CLASSNumber of priority_class>=8 targets within 40 arcsecmeta.code.classVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra matched to objectmeta.number;spectVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalPRIORITY_CLASSPriorities for targeting, see notesmeta.code.classVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARindexedprincipalR_MODELExtinction-corrected SDSS DR6 magmagphot.mag;em.opt.RVARCHARprincipalR_PETROExtinction-corrected SDSS DR6 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalR_SBSDSS Petro half-light surface brightnessmag/arcsec^2phot.mag.sb;em.opt.RVARCHARprincipalSG_SEPr_psf - r_model star-galaxy separation parametermagsrc.class.starGalaxyVARCHARprincipalSG_SEP_JKJ - K - f_locus star-galaxy separation parametermagsrc.class.starGalaxyVARCHARprincipalSPECIDID of spectrum from SpecAll tablemeta.id.cross;spectVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CODESurvey code for redshift source, see notesmeta.code;meta.datasetVARCHARprincipalTARGET_FLAGSBitwise target criteria, see notesmeta.codeVARCHARprincipalU_MODELExtinction-corrected SDSS DR6 magmagphot.mag;em.opt.UVARCHARprincipalVIS_CLASSVisual classification, see notesmata.code.qualVARCHARprincipalVIS_CLASS_USERInitials of classifiers, xxx for nonemeta.idVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalZ_MODELExtinction-corrected SDSS DR6 magmagphot.mag;em.opt.IVARCHARprincipalgama_dr2.ExternalzAllThis table lists a few redshifts of GAMA DR2 objects taken from the literature. The spectra from which these redshifts were measured are NOT available in the GAMA DR2 database.GAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.ExternalSpecAllThis table lists all spectra of GAMA DR2 objects that are available from previous spectroscopic surveys (such as the SDSS), including duplicate observations. Every spectrum listed in this table is available in the GAMA DR2 database.CATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalIS_SBESTIs this the spectrum with the best redshift of this GAMA object within the originating survey?meta.codeVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum`s imagemeta.ref.url;meta.fileVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.ExternalSpecThis table lists those spectra from previous spectroscopic surveys (such as the SDSS) that provide the best redshifts for GAMA DR2 objects. This table is an exact subset of the table ExternalSpecAll. It lists only those entries with IS_SBEST = TRUE, meaning that it excludes intra-survey duplicate observations. However, it still includes inter-survey duplications.CATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalIS_SBESTIs this the spectrum with the best redshift of this GAMA object within the originating survey?meta.codeVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum`s imagemeta.ref.url;meta.fileVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.AATFieldsTable of all AAT 2dF/AAOmega fields observed for GAMA I.COMPLRedshift success ratearith.ratio;meta.number;spectVARCHARprincipalCONFIG_FILEName of configuration filemeta.id;meta.file;instr.setupVARCHARprincipalCRCORVERRunz version used for original redshifting runmeta.version;meta.softwareVARCHARprincipalDATE_OBSUT date of observationiso-8601time.epoch;obs.exposureVARCHARprincipalDATE_ZDate of original redshifting runiso-8601time.processingVARCHARprincipalDECDEC of field centre (J2000)degpos.eq.dec;obs.fieldVARCHARprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalGAL_COMPLRedshift success rate among galaxy targetsarith.ratio;meta.number;srcVARCHARprincipalHAENDHour angle at end of last exposuredegpos.eq.ha;time.endVARCHARprincipalHASTARTHour angle at start of first exposuredegpos.eq.ha;time.startVARCHARprincipalHEL_VCHeliocentric velocity correctionkm/sphys.velocity;pos.heliocentricVARCHARprincipalMEAN_SNMean S/N of spectrastat.snr;spectVARCHARprincipalN_EXPNumber of exposuresmeta.number;obs.exposureVARCHARprincipalN_GALNumber of galaxy targets observedmeta.number;srcVARCHARprincipalN_GAL_GOODNumber of galaxy target spectra with a good quality redshift, i.e. nQ >= 3meta.number;srcVARCHARprincipalN_GOODNumber of spectra with a good quality redshift, i.e. nQ >= 3meta.number;spectVARCHARprincipalN_NIGHTSNumber of nights over which exposures were spreadmeta.numberVARCHARprincipalN_SPECNumber of spectra observedmeta.number;spectVARCHARprincipalN_STARNumber of calibration stars observedmeta.number;src.calibVARCHARprincipalPLATE2dF plate numbermeta.id;instrVARCHARprincipalRARA of field centre (J2000)degpos.eq.ra;obs.fieldVARCHARprincipalTDFDRVERVersion of 2dfdr data reduction softwaremeta.version;meta.softwareVARCHARprincipalT_EXPTotal exposure timestime.duration;obs.exposureVARCHARprincipalUSEROriginal redshifter of this fieldmeta.idVARCHARprincipalUTENDUT of end of last exposuretime.end;obs.exposureVARCHARprincipalUTMJDMean MJD of start of exposurestime.epoch;obs.exposureVARCHARprincipalUTSTARTUT of start of first exposuretime.start;obs.exposureVARCHARprincipalZDENDZenith distance at end of last exposuredegpos.az.zd;time.rndVARCHARprincipalZDSTARTZenith distance at start of first exposuredegpos.az.zd;time.startVARCHARprincipalgama_dr2.SpecObjThis table lists each observed target included in DR2 and the spectrum that provides its best redshift (from GAMA or otherwise).CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between GAMA object and best matched spectrumarcsecpos.angDistanceVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalIC_FLAGCatalogue source(s) of GAMA objectmeta.code.memberVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalN_GAMA_SPECNumber of GAMA spectra available for this objectmeta.number;spectVARCHARprincipalN_SPECNumber of spectra available for this objectmeta.number;spectVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDID of best matched spectrummeta.id.cross;spectVARCHARprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalSURVEY_CODENumerical code for originating surveymeta.code;meta.datasetVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum`s imagemeta.ref.url;meta.fileVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.SpecAllThis table lists all spectra that are available for GAMA objects included in DR2, including GAMA spectra and those from previous spectroscopic surveys (such as the SDSS). Duplicate observations of the same object are retained in this table (but a flag is provided to mark the spectrum that provided the best available redshift of a given object). Every spectrum listed in this table is available in the GAMA DR2 database.CATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalIS_BESTIs this the best spectrum of this GAMA object?meta.codeVARCHARprincipalIS_SBESTIs this the best spectrum of this GAMA object within the originating survey?meta.codeVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalSURVEY_CODENumerical code for originating surveymeta.code;meta.datasetVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum`s imagemeta.ref.url;meta.fileVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.LTSpecAllThis table lists a small number of spectra of fibre-bright targets collected by the GAMA team at the Liverpool Telescope (LT).CATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalIS_SBESTIs this the best GAMA LT spectrum of this object?meta.codeVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDID of GAMA LT spectrummeta.id;meta.mainVARCHARindexedprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum`s imagemeta.ref.url;meta.fileVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.AATSpecAllzAllMany GAMA AAT spectra were redshifted more than once. For each spectrum included in DR2 this table contains one line summarising all of the redshifting results for this spectrum, as well as listing the results of the analysis to determine the best redshift based on the reliabilities of the redshifters.BEST_IDXIndex of best possibility in the above listVARCHARprincipalBEST_PROBProbability that the most probable possibility is correctstat.probability;src.redshiftVARCHARprincipalBEST_ZRedshift of the most probable possibilitysrc.redshiftVARCHARprincipalBEST_Z_NNumber of opinions supporting the most probable possibilitymeta.numberVARCHARprincipalBEST_Z_NQNormalised Q of the most probable possibilitymeta.code.qual;src.redshiftVARCHARprincipalBEST_Z_N_Q0Number of supporting Q=0 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q1Number of supporting Q=1 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalCOMP_PROBProbability that all offered possibilities are wrongstat.probabilityVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalN_OPNumber of opinions for this spectrummeta.numberVARCHARprincipalN_OPQBNumber of opinions with Q < 2meta.numberVARCHARprincipalN_OPQGNumber of opinions with Q >= 2meta.numberVARCHARprincipalN_ZNumber of different redshiftsmeta.numberVARCHARprincipalOP1_QOriginal QVARCHARprincipalOP1_RSOriginal redshifterVARCHARprincipalOP1_RUNZRESIDID of original runz result in AATRunzResultsVARCHARprincipalOP1_ZOriginal redshiftVARCHARprincipalOP1_ZIDXIndex of possibility in above list that is supported by this redshiftVARCHARprincipalOP2_QQVARCHARprincipalOP2_RSRedshifterVARCHARprincipalOP2_RUNZRESIDID of additional runz result in AATRunzResultsVARCHARprincipalOP2_ZRedshiftVARCHARprincipalOP2_ZIDXIndex of possibility in above list that is supported by this redshiftVARCHARprincipalOP3_QQVARCHARprincipalOP3_RSRedshifterVARCHARprincipalOP3_RUNZRESIDID of additional runz result in AATRunzResultsVARCHARprincipalOP3_ZRedshiftVARCHARprincipalOP3_ZIDXIndex of possibility in above list that is supported by this redshiftVARCHARprincipalOP4_QQVARCHARprincipalOP4_RSRedshifterVARCHARprincipalOP4_RUNZRESIDID of additional runz result in AATRunzResultsVARCHARprincipalOP4_ZRedshiftVARCHARprincipalOP4_ZIDXIndex of possibility in above list that is supported by this redshiftVARCHARprincipalOP5_QQVARCHARprincipalOP5_RSRedshifterVARCHARprincipalOP5_RUNZRESIDID of additional runz result in AATRunzResultsVARCHARprincipalOP5_ZRedshiftVARCHARprincipalOP5_ZIDXIndex of possibility in above list that is supported by this redshiftVARCHARprincipalQ1_N_Q0Number of supporting Q=0 opinionsmeta.numberVARCHARprincipalQ1_N_Q1Number of supporting Q=1 opinionsmeta.numberVARCHARprincipalQ1_PROBProbability that the possibility Q=1 is correctstat.probabilityVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalZ1_NNumber of opinions supporting ZX_ZVARCHARprincipalZ1_NQNormalised Q of ZX_ZVARCHARprincipalZ1_N_Q2Number of supporting Q=2 opinionsVARCHARprincipalZ1_N_Q3Number of supporting Q=3 opinionsVARCHARprincipalZ1_N_Q4Number of supporting Q=4 opinionsVARCHARprincipalZ1_PROBProbability that ZX_Z is correctVARCHARprincipalZ1_ZPossible redshiftVARCHARprincipalZ2_NNumber of opinions supporting ZX_ZVARCHARprincipalZ2_NQNormalised Q of ZX_ZVARCHARprincipalZ2_N_Q2Number of supporting Q=2 opinionsVARCHARprincipalZ2_N_Q3Number of supporting Q=3 opinionsVARCHARprincipalZ2_N_Q4Number of supporting Q=4 opinionsVARCHARprincipalZ2_PROBProbability that ZX_Z is correctVARCHARprincipalZ2_ZPossible redshiftVARCHARprincipalZ3_NNumber of opinions supporting ZX_ZVARCHARprincipalZ3_NQNormalised Q of ZX_ZVARCHARprincipalZ3_N_Q2Number of supporting Q=2 opinionsVARCHARprincipalZ3_N_Q3Number of supporting Q=3 opinionsVARCHARprincipalZ3_N_Q4Number of supporting Q=4 opinionsVARCHARprincipalZ3_PROBProbability that ZX_Z is correctVARCHARprincipalZ3_ZPossible redshiftVARCHARprincipalZ4_NNumber of opinions supporting ZX_ZVARCHARprincipalZ4_NQNormalised Q of ZX_ZVARCHARprincipalZ4_N_Q2Number of supporting Q=2 opinionsVARCHARprincipalZ4_N_Q3Number of supporting Q=3 opinionsVARCHARprincipalZ4_N_Q4Number of supporting Q=4 opinionsVARCHARprincipalZ4_PROBProbability that ZX_Z is correctVARCHARprincipalZ4_ZPossible redshiftVARCHARprincipalgama_dr2.AATSpecAllThis is a table of all GAMA AAT spectra included in DR2. Many targets were observed more than once by GAMA, and these duplications are retained here.CATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalDATE_OBSUT date of observationiso-8601time.epoch;obs.exposureVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalIS_SBESTIs this the best GAMA AAT spectrum of this object?meta.codeVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPLATEPlate numbermeta.id;instrVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalS_NS/N of spectrumstat.snrVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum`s imagemeta.ref.url;meta.fileVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalX_POSNFibre x position on plateVARCHARprincipalY_POSNFibre y position on plateVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalgama_dr2.AATRunzResultsThis table contains the complete output of the redshifting code for all spectra released in DR2. Note that many spectra were redshifted more than once and this catalogue contains all duplications.CATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalCCDCCD numbermeta.id;instrVARCHARprincipalCOMMENTUser commentmeta.noteVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalDATE_ZDate of runz runiso-8601time.processingVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDECDDEC degree of spectrum (J2000)degVARCHARprincipalDECMDEC minutesmVARCHARprincipalDECSDEC secondssVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFFlag indicating whether Z_FIN is different from automatic redshifts: 0 = equal to best auto redshift; 1 = not equal to best auto redshift; 2 = not equal to either auto redshiftsmeta.codeVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalFLDUnusedVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalNEBNumber of matching emission lines at best emission line redshiftVARCHARprincipalNEGTotal number of detected potential emission linesVARCHARprincipalOBJECTObject nameVARCHARprincipalPLATEPlate numbermeta.id;instrVARCHARprincipalQAAutomatic quality of final selected redshiftVARCHARprincipalQEMEmission line redshift qualityVARCHARprincipalQOPUser assigned quality of final selected redshiftmeta.code.qual;src.redshiftVARCHARprincipalQXCross-correlation redshift qualityVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalRAHRA hours of spectrum (J2000)hVARCHARprincipalRAMRA minutesmVARCHARprincipalRASRA secondssVARCHARprincipalRMAGExtinction corrected SDSS r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalRSPApproximate R-band fibre mag with zeropoint 32.3magVARCHARprincipalRUNZRESIDID of runz outputmeta.id;meta.mainVARCHARindexedprincipalSPECIDID of GAMA AAT spectrummeta.id;spectVARCHARprincipalSPMAGUnusedmagVARCHARprincipalS_NS/N of spectrumstat.snrVARCHARprincipalTEMPCross-correlation templateVARCHARprincipalUSERRedshiftermeta.idVARCHARprincipalVSPApproximate V-band fibre mag with zeropoint 32magVARCHARprincipalXCORCross-correlation peak heightVARCHARprincipalX_POSNFibre x position on plateVARCHARprincipalY_POSNFibre y position on plateVARCHARprincipalZEMEmission line redshiftVARCHARprincipalZEM_ERREmission line redshift errorVARCHARprincipalZXCross-correlation redshiftVARCHARprincipalZX_ERRCross-correlation redshift errorVARCHARprincipalZ_FINFinal selected redshiftsrc.redshiftVARCHARprincipalZ_FIN_ERRError of final selected redshiftstat.error;src.redshiftVARCHARprincipalgama_dr2.SpecLinesThis table provides emission and absorption line measurements for all GAMA DR2 AAT spectra with a redshift measurement.DECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalHAHalpha line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensity;em.line.HalphaVARCHARprincipalHAERRHalpha line flux error (Gaussian fit)10^(-17)erg/s/cm^2stat.error;spect.line.intensity;em.li...VARCHARprincipalHAEWHalpha equivalent width (see notes)Aspect.line.eqWidth;em.line.HalphaVARCHARprincipalHASIGHalpha sigmaAspect.line.width;em.line.HalphaVARCHARprincipalHASIGERRHalpha sigma errorAstat.error;spect.line.width;em.line.H...VARCHARprincipalHBHbeta line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalHBERRHbeta line flux error (Gaussian fit)10^(-17)erg/s/cm^2stat.error;spect.line.intensity;em.li...VARCHARprincipalHBEWHbeta equivalent width (see notes)Aspect.line.eqWidth;em.line.HbetaVARCHARprincipalHBSIGHbeta sigmaAspect.line.width;em.line.HbetaVARCHARprincipalHBSIGERRHbeta sigma errorAstat.error;spect.line.width;em.line.H...VARCHARprincipalIHAHalpha integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;em.line.HalphaVARCHARprincipalIHAERRHalpha integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;em.line.HalphaVARCHARprincipalIHBHbeta integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;em.line.HbetaVARCHARprincipalIHBERRHbeta integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;em.line.HbetaVARCHARprincipalIHDHdelta integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalIHDERRHdelta integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIMGMg 5174A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalIMGERRMg 5174A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalINADNaID 5892A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalINADERRNaID 5892A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalINEIII[NeIII] 3869A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalINEIIIERR[NeIII] 3869A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalINEVB[NeV] 3345A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalINEVBERR[NeV] 3345A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalINEVR[NeV] 3425A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalINEVRERR[NeV] 3425A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalINIIB[NII] 6548A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalINIIBERR[NII] 6548A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalINIIR[NII] 6584A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalINIIRERR[NII] 6584A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIOI6300[OI] 6300A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalIOI6300ERR[OI] 6300A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIOI6364[OI] 6364A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalIOI6364ERR[OI] 6364A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIOII[OII] 3727A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalIOIIERR[OII] 3727A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIOIIIB[OIII] 4959A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalIOIIIBERR[OIII] 4959A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIOIIIR[OIII] 5007A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;em.line.OIIIVARCHARprincipalIOIIIRERR[OIII] 5007A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;em.line.OIIIVARCHARprincipalISIIB[SII] 6716A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalISIIBERR[SII] 6716A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalISIIR[SII] 6731A integrated line flux (see notes)10^(-17)erg/s/cm^2phot.flux;spect.lineVARCHARprincipalISIIRERR[SII] 6731A integrated line flux error10^(-17)erg/s/cm^2stat.error;phot.flux;spect.lineVARCHARprincipalIS_BESTSpectrum with best redshift for this object across all surveys?meta.codeVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in GAMA AAT survey?meta.codeVARCHARprincipalNIIB[NII] 6548A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalNIIBERR[NII] 6548A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalNIIBEW[NII] 6548A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalNIIBSIGERR[NII] 6548A sigma errorAstat.error;spect.line.widthVARCHARprincipalNIIR[NII] 6584A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalNIIRERR[NII] 6584A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalNIIREW[NII] 6584A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalNIIRSIG[NII] 6584A sigmaAspect.line.widthVARCHARprincipalNIIRSIGERR[NII] 6584A sigma errorAstat.error;spect.line.widthVARCHARprincipalNQQuality flag (4 is reliable, 3 tentative)meta.code.qual;src.redshiftVARCHARprincipalOII[OII] 3727A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalOIIB[OII] 3727A line flux (double Gaussian fit to blue peak, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalOIIBERR[OII] 3727A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalOIIBEW[OII] 3727A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalOIIBSIG[OII] 3727A sigmaAspect.line.widthVARCHARprincipalOIIBSIGERR[OII] 3727A sigma errorAstat.error;spect.line.widthVARCHARprincipalOIIERR[OII] 3727A line flux error (Gaussian fit)10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalOIIIB[OIII] 4959A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalOIIIBERR[OIII] 4959A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalOIIIBEW[OIII] 4959A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalOIIIBSIG[OIII] 4959A sigmaAspect.line.widthVARCHARprincipalOIIIBSIGERR[OIII] 4959A sigma errorAstat.error;spect.line.widthVARCHARprincipalOIIIR[OIII] 5007A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensity;em.line.OIIIVARCHARprincipalOIIIRERR[OIII] 5007A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensity;em.li...VARCHARprincipalOIIIREW[OIII] 5007A equivalent width (see notes)Aspect.line.eqWidth;em.line.OIIIVARCHARprincipalOIIIRSIG[OIII] 5007A sigmaAspect.line.width;em.line.OIIIVARCHARprincipalOIIIRSIGERR[OIII] 5007A sigma errorAstat.error;spect.line.width;em.line.OIIIVARCHARprincipalOIIR[OII] 3727A line flux (double Gaussian fit to red peak, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalOIIRERR[OII] 3727A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalOIIREW[OII] 3727A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalOIIRSIG[OII] 3727A sigmaAspect.line.widthVARCHARprincipalOIIRSIGERR[OII] 3727A sigma errorAstat.error;spect.line.widthVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSIIB[SII] 6716A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalSIIBERR[SII] 6716A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalSIIBEW[SII] 6716A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalSIIBSIG[SII] 6716A sigmaAspect.line.widthVARCHARprincipalSIIBSIGERR[SII] 6716A sigma errorAstat.error;spect.line.widthVARCHARprincipalSIIR[SII] 6731A line flux (Gaussian fit, see notes)10^(-17)erg/s/cm^2spect.line.intensityVARCHARprincipalSIIRERR[SII] 6731A line flux error10^(-17)erg/s/cm^2stat.error;spect.line.intensityVARCHARprincipalSIIREW[SII] 6731A equivalent width (see notes)Aspect.line.eqWidthVARCHARprincipalSIIRSIG[SII] 6731A sigmaAspect.line.widthVARCHARprincipalSIIRSIGERR[SII] 6731A sigma errorAstat.error;spect.line.widthVARCHARprincipalSPECIDUnique spectrum IDmeta.id;meta.mainVARCHARindexedprincipalZ_HELIOSpectroscopic redshiftsrc.redshiftVARCHARprincipalNIIBSIG[NII] 6548A sigmaAspect.line.widthVARCHARprincipalgama_dr2.EmLinesPhysSDSSThis table provides Balmer decrements, Halpha luminosities, Halpha derived star-formation rates and emission line classifications for all SDSS spectra of GAMA DR2 objects with any measured Halpha emission and z > 0.001. The values in this table were derived from the MPA/JHU SDSS line measurements database.AB_RSDSS r band absolute magnitude: PETROMAG_R - DM_70_30_70 - A_R - K_R; AB magnitudemagphys.magAbsVARCHARprincipalA_RGalactic extinction in SDSS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalBALMERDEC_FLAGIs the Balmer decrement measured or estimated?meta.code;phot.flux;arith.ratioVARCHARprincipalBALMER_DECREMENTBalmer decrement (see notes)phot.flux;arith.ratio;spect.lineVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalDM_70_30_70Distance modulus for 737 cosmologymagphot.mag.distModVARCHARprincipalEMLINE_CLASSAGN classification based on Kewley et al. (2001)meta.codeVARCHARprincipalEMLINE_METHODAGN classification method (see notes)meta.codeVARCHARprincipalF_HALPHAStellar absorption corrected Halpha flux10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalF_HBETAStellar absorption corrected Hbeta flux10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalIS_BESTSpectrum with best redshift for this object across all surveys?meta.codeVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in SDSS?meta.codeVARCHARprincipalK_RK-correction in SDSS r bandmagphot.magVARCHARprincipalL_APCORHalpha luminosity corrected for stellar absorption and fibre aperture effectsWphys.luminosity;em.line.HalphaVARCHARprincipalL_APOBSCORHalpha luminosity corrected for stellar absorption, fibre aperture effects and dust obscurationWphys.luminosity;em.line.HalphaVARCHARprincipalMPACAT_ROWIDRow number of object in MPA/JHU cataloguemeta.idVARCHARprincipalPETROMAG_RSDSS r band Petrosian magnitude (not corrected for Galactic extinction)magphot.mag;em.opt.RVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSFRHalpha derived star formation rate assuming a Salpeter IMFM_sun/yrphys.SFR;em.line.HalphaVARCHARprincipalSN_CONTContinuum signal-to-noisestat.snrVARCHARprincipalSPECIDUnique spectrum IDmeta.id;meta.mainVARCHARindexedprincipalZ_HELIORedshift from MPA/JHU cataloguesrc.redshiftVARCHARprincipalZ_HELIO_ERRRedshift errorsrc.redshiftVARCHARprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalgama_dr2.SpStandardsStandard stars from SDSS.CATAIDGAMA IDmeta.id;meta.mainVARCHARindexedprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RDR7 magmagphot.mag;em.opt.RVARCHARprincipalOBJIDSDSS IDmeta.idVARCHARprincipalPRIORITY_CLASSSee notesmeta.code.classVARCHARprincipalPSFMAG_GDR7 magmagphot.mag;em.optVARCHARprincipalPSFMAG_IDR7 magmagphot.mag;em.opt.IVARCHARprincipalPSFMAG_RDR7 magmagphot.mag;em.opt.RVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalRUNSDSS run numberobs.paramVARCHARprincipalSECTARGET2^1 for REDDEN_STD, 2^5 for SPECTROPHOTO_STDmeta.code.classVARCHARprincipalSTATUSSDSS status flag related to primary secondarymeta.code.statusVARCHARprincipalgama_dr2.G3CMockFoFGroupThis is a catalogue of G3C mock FoF group properties.AxAngAngle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)degVARCHARprincipalAxRatAxial ratio of the group using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)VARCHARprincipalBCGDecDec of BCG (J2000)degpos.eq.decVARCHARprincipalBCGGalIDGalID of BCGmeta.idVARCHARprincipalBCGRARA of BCG (J2000)degpos.eq.raVARCHARprincipalCenDecDec of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.decVARCHARprincipalCenRARA of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.raVARCHARprincipalGroupEdgeFraction of the group within the survey volume, as estimated from IterCen and Rad100VARCHARprincipalGroupIDUnique group ID, as referred to by G3CMockGalmeta.id;meta.mainVARCHARindexedprincipalIterCenDECDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalIterCenGalIDGalID of the iterative central galaxy (prefered position of the group centre, see Robotham et al. 2011 section 4.2)meta.idVARCHARprincipalIterCenRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalIterCenZRedshift of the iterative central galaxyVARCHARprincipalLinkStrenCombLink strength combined, average of LinkStrenProj*LinkStrenZ for all the links in the group (0<=LinkStrenComb<=1)VARCHARprincipalLinkStrenProjLink strength in projection, average projected FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenProj<=1)VARCHARprincipalLinkStrenRadLink strength radially, average radial FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenZ<=1)VARCHARprincipalLinkTotTotal number of FoF links in the systemVARCHARprincipalLumBTotFluxProxy times the global B factor required to get a median unbaised halo mass estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)LsunVARCHARprincipalLumBfuncTotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)LsunVARCHARprincipalMassAMass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)MsunVARCHARprincipalMassAfuncMass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)MsunVARCHARprincipalMassProxyProxy for dynamical group mass estimated via M propto Rad50 * VelDisp^2 . Value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)MsunVARCHARprincipalModalityThe modality of the system: (1+VelSkew^2)/(3+VelKurt^2). This will be 1/3 for a normal distribution and 0.555 for a uniform.VARCHARprincipalNfofGroup multiplicityVARCHARprincipalRad100Group radius defined by the most distant group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRad1SigGroup radius defined by the 68th percentile group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRad50Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRadKurtUnbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCenVARCHARprincipalRelDenRelative galaxy space density (w.r.t. the SWML prediction) within a cylinder of radius 1.5 Mpc/h and length 18Mpc/h centred on IterCenID.VARCHARprincipalRgapApparent r-band magnitude gap between BCG and second brightest group membermagVARCHARprincipalSymKSKS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)VARCHARprincipalTotFluxProxyProxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on the total observed r-band flux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift. Value listed corresponds to B=1 in Eq. 21 of Robotham et al. (2011)LsunVARCHARprincipalTotRmagr-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its membersmagVARCHARprincipalVelDispGroup velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRaw (see eq. 17 in Robotham et al. 2011)km/sVARCHARprincipalVelDispRawRaw group velocity dispersionkm/sVARCHARprincipalVelErrTotal group velocity errorkm/sVARCHARprincipalVelKurtUnbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)VARCHARprincipalVelSkewUnbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)VARCHARprincipalVolumeThe mock volume numberVARCHARprincipalZfofMedian redshift of the groupVARCHARprincipalgama_dr2.G3CFoFGroupThis is a catalogue of G3C GAMA group properties. G15 only.AxAngAngle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)degVARCHARprincipalAxRatAxial ratio of the group using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)VARCHARprincipalBCGCATAIDGAMA ID of BCGmeta.idVARCHARprincipalBCGDecDec of BCG (J2000)degpos.eq.decVARCHARprincipalBCGRARA of BCG (J2000)degpos.eq.raVARCHARprincipalCenDecDec of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.decVARCHARprincipalCenRARA of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.raVARCHARprincipalGroupEdgeFraction of the group within the survey volume, as estimated from IterCen and Rad100VARCHARprincipalGroupIDUnique group ID, as used in G3CGalmeta.id;meta.mainVARCHARindexedprincipalIterCenCATAIDGAMA ID of the iterative central galaxy (prefered position of the group centre, see Robotham et al. 2011 section 4.2)meta.idVARCHARprincipalIterCenDECDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalIterCenRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalIterCenZRedshift of the iterative central galaxyVARCHARprincipalLinkStrenCombLink strength combined, average of LinkStrenProj*LinkStrenZ for all the links in the group (0<=LinkStrenComb<=1)VARCHARprincipalLinkStrenProjLink strength in projection, average projected FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenProj<=1)VARCHARprincipalLinkStrenRadLink strength radially, average radial FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenZ<=1)VARCHARprincipalLinkTotTotal number of FoF links in the systemVARCHARprincipalLumBTotFluxProxy times the global B factor required to get a median unbaised halo mass estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)LsunVARCHARprincipalLumBfuncTotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)LsunVARCHARprincipalMassAMass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)MsunVARCHARprincipalMassAfuncMass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)MsunVARCHARprincipalMassProxyProxy for dynamical group mass estimated via M propto Rad50 * VelDisp^2 . Value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)MsunVARCHARprincipalModalityThe modality of the system: (1+VelSkew^2)/(3+VelKurt^2). This will be 1/3 for a normal distribution and 0.555 for a uniform.VARCHARprincipalNfofGroup multiplicityVARCHARprincipalRad100Group radius defined by the most distant group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRad1SigGroup radius defined by the 68th percentile group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRad50Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRadKurtUnbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCenVARCHARprincipalRelDenRelative galaxy space density (w.r.t. the SWML prediction) within a cylinder of radius 1.5 Mpc/h and length 18Mpc/h centred on IterCenID.VARCHARprincipalRgapApparent r-band magnitude gap between BCG and second brightest group membermagVARCHARprincipalSymKSKS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)VARCHARprincipalTotFluxProxyProxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on the total observed r-band flux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift. Value listed corresponds to B=1 in Eq. 21 of Robotham et al. (2011)LsunVARCHARprincipalTotRmagr-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its membersmagVARCHARprincipalURL_IMGURL of the group`s imagemeta.ref.url;meta.fileVARCHARprincipalVelDispGroup velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRaw (see eq. 17 in Robotham et al. 2011)km/sVARCHARprincipalVelDispRawRaw group velocity dispersionkm/sVARCHARprincipalVelErrTotal group velocity errorkm/sVARCHARprincipalVelKurtUnbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)VARCHARprincipalVelSkewUnbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)VARCHARprincipalZcompAverage redshift completeness of the group: for each group member the redshift completeness within a projected 1.5 Mpc/h radius (at the position of the galaxy) is estimated and then averaged over all group members to provide ZCompVARCHARprincipalZfofMedian redshift of the groupVARCHARprincipalgama_dr2.G3CMockHaloGroupThis is a catalogue of G3C mock halo group properties. These are the intrinsic groups found in the mocks.AxAngAngle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)degVARCHARprincipalAxRatAxial ratio of the group using the Carter & Metcalfe (1984) algorithm (requires 3 or more members, so -999 otherwise)VARCHARprincipalBCGDecDec of BCG (J2000)degpos.eq.decVARCHARprincipalBCGGalIDGalID of BCGmeta.idVARCHARprincipalBCGRARA of BCG (J2000)degpos.eq.raVARCHARprincipalCenDecDec of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.decVARCHARprincipalCenRARA of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.raVARCHARprincipalGroupEdgeFraction of the group within the survey volume, as estimated from IterCen and Rad100VARCHARprincipalHaloIDUnique halo ID, as referred to by G3CMockGalmeta.id;meta.mainVARCHARindexedprincipalHaloMassThe dark matter halo mass for the group halo in the Millennium simulationMsun/hVARCHARprincipalIterCenDECDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalIterCenGalIDGalID of the iterative central galaxy (prefered position of the group centre, see Robotham et al. 2011 section 4.2)meta.idVARCHARprincipalIterCenRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalIterCenZRedshift of the iterative central galaxyVARCHARprincipalLumBTotFluxProxy times the global B factor required to get a median unbaised halo mass estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)LsunVARCHARprincipalLumBfuncTotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)LsunVARCHARprincipalMassAMass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)MsunVARCHARprincipalMassAfuncMass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)MsunVARCHARprincipalMassProxyProxy for dynamical group mass estimated via M propto Rad50 * VelDisp^2 . Value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)MsunVARCHARprincipalModalityThe modality of the system: (1+VelSkew^2)/(3+VelKurt^2). This will be 1/3 for a normal distribution and 0.555 for a uniform.VARCHARprincipalNhaloGroup multiplicityVARCHARprincipalRad100Group radius defined by the most distant group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRad1SigGroup radius defined by the 68th percentile group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRad50Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenIDMpc/hVARCHARprincipalRadKurtUnbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCenVARCHARprincipalRelDenRelative galaxy space density (w.r.t. the SWML prediction) within a cylinder of radius 1.5 Mpc/h and length 18Mpc/h centred on IterCenID.VARCHARprincipalRgapApparent r-band magnitude gap between BCG and second brightest group membermagVARCHARprincipalSymKSKS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)VARCHARprincipalTotFluxProxyProxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on TotFlux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift. Value listed corresponds to B=1 in Eq. 21 of Robotham et al. (2011)LsunVARCHARprincipalTotRmagObserved r-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its membersmagVARCHARprincipalVelDispGroup velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRaw (see eq. 17 in Robotham et al. 2011)km/sVARCHARprincipalVelDispRawRaw group velocity dispersionkm/sVARCHARprincipalVelErrTotal group velocity errorkm/sVARCHARprincipalVelKurtUnbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)VARCHARprincipalVelSkewUnbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)VARCHARprincipalVolumeThe mock volume numberVARCHARprincipalZhaloMedian redshift of the groupVARCHARprincipalgama_dr2.G3CMockLinkCatalogue that gives linking between all mock galaxies that share a common group in G3CMockFoFGroup.Gal1IDGalID of galaxy 1 in G3CMockGalmeta.idVARCHARprincipalGal2IDGalID of galaxy 2 in G3CMockGalmeta.idVARCHARprincipalLimProjCoMaximum allowed projected separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimProjCo>=SepProjCo)kpc/hVARCHARprincipalLimRadCoMaximum allowed radial separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimRadCo>=SepRadCo)kpc/hVARCHARprincipalLinkIDUnique linking ID for cataloguemeta.id;meta.mainVARCHARindexedprincipalSepProjCoProjected separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hVARCHARprincipalSepRadCoRadial separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hVARCHARprincipalVolumeThe mock volume numberVARCHARprincipalgama_dr2.G3CMockGalsInPairCatalogue of galaxies that live in pairs (thus gal1-gal2 and gal2-gal1 combinations are both listed). Galaxy pairs are required to be within 50 kpc/h in physical separation and 1000 km/s in velocity separation.Gal1GalIDGalID of galaxy 1 in G3CMockGalmeta.idVARCHARprincipalGal2GalIDGalID of galaxy 2 in G3CMockGalmeta.idVARCHARprincipalPairIDUnique pair ID for cataloguemeta.id;meta.mainVARCHARindexedprincipalSepProjAngPhysical projected separation between galaxy 1 and galaxy 2kpc/hVARCHARprincipalSepVelVelocity separation of galaxy 1 and galaxy 2km/sVARCHARprincipalVolumeThe mock volume numberVARCHARprincipalgama_dr2.G3CMockGalCatalogue of all mock galaxies used in the G3C.DECDeclination (J2000)degpos.eq.decVARCHARprincipalDM_100_25_75Distance modulusmagVARCHARprincipalGalIDMock galaxy IDmeta.id;meta.mainVARCHARindexedprincipalGroupIDGroupID of the group this galaxy belongs to as listed in G3CMockFoFGroup, 0 is un-groupedmeta.idVARCHARprincipalHaloIDHaloID of the halo group this galaxy belongs to as listed in G3CMockHaloGroupVARCHARprincipalMillSimIDA unique group/halo id used in the Millennium Simulation, see notes for detailsVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalRpetroPetrosian apparent r-band magnitude (AB, extinction corrected) [GAMA selection magnitude]magVARCHARprincipalSelIDGalaxy listed as #idsel used in the Millennium Simulation, see notes for detailsVARCHARprincipalVolumeThe mock volume numberVARCHARprincipalZspecHeliocentric redshiftVARCHARprincipalgama_dr2.G3CLinkCatalogue that gives linking between all GAMA galaxies that share a common group in G3CFoFGroup. G15 only.Gal1CATAIDGAMA ID of galaxy 1 in G3CGalmeta.idVARCHARprincipalGal2CATAIDGAMA ID of galaxy 2 in G3CGalmeta.idVARCHARprincipalLimProjCoMaximum allowed projected separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimProjCo>=SepProjCo)kpc/hVARCHARprincipalLimRadCoMaximum allowed radial separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimRadCo>=SepRadCo)kpc/hVARCHARprincipalLinkIDUnique linking ID for cataloguemeta.id;meta.mainVARCHARindexedprincipalSepProjCoProjected separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hVARCHARprincipalSepRadCoRadial separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hVARCHARprincipalgama_dr2.G3CGalsInPairCatalogue of galaxies that live in pairs (thus gal1-gal2 and gal2-gal1 combinations are both listed). Galaxy pairs are required to be within 50 kpc/h in physical separation and 1000 km/s in velocity separation. G15 only.Gal1CATAIDGAMA ID of galaxy 1 in G3CGalmeta.idVARCHARprincipalGal2CATAIDGAMA ID of galaxy 2 in G3CGalmeta.idVARCHARprincipalPairIDUnique pair ID for cataloguemeta.id;meta.mainVARCHARindexedprincipalSepProjAngPhysical projected separation between galaxy 1 and galaxy 2kpc/hVARCHARprincipalSepVelVelocity separation of galaxy 1 and galaxy 2km/sVARCHARprincipalgama_dr2.G3CGalCatalogue of all GAMA galaxies used in the G3C. G15 only.CATAIDGAMA IDmeta.id;meta.mainVARCHARindexedprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalDM_100_25_75Distance modulus using H0=100 km/s/Mpc, Omega_m=0.25 and Omega_L=0.75magVARCHARprincipalGroupIDGroupID of the group this galaxy belongs to as listed in G3CFoFGroup, 0 is un-groupedmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalRpetroPetrosian apparent r-band magnitude (AB, extinction corrected) [GAMA selection magnitude]magVARCHARprincipalSURVEY_CODESource of the redshift. See the notes of table TilingCat in the InputCat DMU for full detailsVARCHARprincipalSigErrVelocity uncertainty (on redshift): assumed to be 30 km/s for SDSS, 50 km/s for GAMA and 80 km/s for 2dFGRSkm/sVARCHARprincipalZHeliocentric redshiftVARCHARprincipalgama_dr2.EmLinesPhysThis is the main table of the SpecLineSFR DMU. It provides Balmer decrements, Halpha luminosities, Halpha derived star-formation rates and emission line classifications for all GAMA DR2 objects with z > -0.01 (where available).DECDEC of GAMA object (J2000)degpos.eq.decVARCHARprincipalAB_RSDSS r band absolute magnitude: PETROMAG_R - DM_70_30_70 - A_R - K_R; AB magnitudemagphys.magAbsVARCHARprincipalA_RGalactic extinction in SDSS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalBALMERDEC_FLAGIs the Balmer decrement measured or estimated?meta.code;phot.flux;arith.ratioVARCHARprincipalBALMER_DECREMENTBalmer decrement (see notes)phot.flux;arith.ratio;spect.lineVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.id.cross;srcVARCHARprincipalDM_70_30_70Distance modulus for 737 cosmology calculated from Z_TONRYmagphot.mag.distModVARCHARprincipalEMLINE_CLASSAGN classification based on Kewley et al. (2001)meta.codeVARCHARprincipalEMLINE_METHODAGN classification method (see notes)meta.codeVARCHARprincipalF_HALPHAStellar absorption corrected Halpha flux10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalF_HBETAStellar absorption corrected Hbeta flux10^(-17)erg/s/cm^2spect.line.intensity;em.line.HbetaVARCHARprincipalK_RK-correction in SDSS r bandmagphot.magVARCHARprincipalL_APCORHalpha luminosity corrected for stellar absorption and fibre aperture effectsWphys.luminosity;em.line.HalphaVARCHARprincipalL_APOBSCORHalpha luminosity corrected for stellar absorption, fibre aperture effects and dust obscurationWphys.luminosity;em.line.HalphaVARCHARprincipalNQNormalised redshift quality of Z_HELIOmeta.code.qual;src.redshiftVARCHARprincipalNQ_BESTNormalised redshift quality of Z_HELIO_BESTmeta.code.qual;src.redshiftVARCHARprincipalPETROMAG_RSDSS r band Petrosian magnitude (not corrected for Galactic extinction)magphot.mag;em.opt.RVARCHARprincipalRARA of GAMA object (J2000)degpos.eq.raVARCHARprincipalSFRHalpha derived star formation rate assuming a Salpeter IMFM_sun/yrphys.SFR;em.line.HalphaVARCHARprincipalSN_CONTContinuum signal-to-noisestat.snrVARCHARprincipalSN_EMIHalpha emission signal-to-noisestat.snrVARCHARprincipalSPECIDUnique ID of spectrum on which line measurements were performed (measurement spectrum)meta.id;meta.mainVARCHARindexedprincipalSPECID_BESTUnique ID of the spectrum that provides the best redshift for this object (IS_BEST spectrum)meta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey the measurement spectrum originated frommeta.codeVARCHARprincipalSURVEY_BESTSurvey the IS_BEST spectrum originated frommeta.codeVARCHARprincipalWARNING_FLAGHalpha or Hbeta affected by data reduction issues?meta.codeVARCHARprincipalZ_HELIOHeliocentric redshift of the measurement spectrumsrc.redshiftVARCHARprincipalZ_HELIO_BESTHeliocentric redshift of the IS_BEST spectrumsrc.redshiftVARCHARprincipalZ_TONRYFlow corrected redshift calculated from Z_HELIO_BEST using Tonry et al. modelsrc.redshiftVARCHARprincipalgama_dr2.StellarMassesThis table provides stellar masses, restframe photometry, and other ancillary stellar population parameters from stellar population fits to ugriz SEDs for all z < 0.65 galaxies in the GAMA DR2 sample.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalC_logM_eBVCorrelation coefficient between logmstar and extBV for covariant error matrixstat.correlationVARCHARprincipalC_logM_giCorrelation coefficient between logmstar and gminusi for covariant error matrixstat.correlationVARCHARprincipalC_logM_urCorrelation coefficient between logmstar and uminusi for covariant error matrixstat.correlationVARCHARprincipalSURVEY_CODERedshift source flag (5=GAMA; 1=SDSS)meta.code;meta.datasetVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalabsmag_gAbsolute magnitude in restframe g-band from SPS SED fitsmagphys.magAbsVARCHARprincipalabsmag_g_starsIntrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe g-bandmagphys.magAbsVARCHARprincipalabsmag_iAbsolute magnitude in restframe i-band from SPS SED fitsmagphys.magAbsVARCHARprincipalabsmag_i_starsIntrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe i-bandmagphys.magAbsVARCHARprincipalabsmag_rAbsolute magnitude in restframe r-band from SPS SED fitsmagphys.magAbsVARCHARprincipalabsmag_r_starsIntrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe r-bandmagphys.magAbsVARCHARprincipalabsmag_uAbsolute magnitude in restframe u-band from SPS SED fitsmagphys.magAbsVARCHARprincipalabsmag_u_starsIntrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe u-bandmagphys.magAbsVARCHARprincipalabsmag_zAbsolute magnitude in restframe z-band from SPS SED fitsmagphys.magAbsVARCHARprincipalabsmag_z_starsIntrinsic abs. mag. of all stellar emission (i.e. corrected for internal dust extinction) in restframe z-bandmagphys.magAbsVARCHARprincipaldelabsmag_gFormal uncertainty in absmag_gmagstat.errorVARCHARprincipaldelabsmag_iFormal uncertainty in absmag_imagstat.errorVARCHARprincipaldelabsmag_rFormal uncertainty in absmag_rmagstat.errorVARCHARprincipaldelabsmag_uFormal uncertainty in absmag_umagstat.errorVARCHARprincipaldelabsmag_zFormal uncertainty in absmag_zmagstat.errorVARCHARprincipaldelextBVFormal uncertainty on extBVmagstat.errorVARCHARprincipaldelfitphot_gFormal uncertainty in fitphot_gmagstat.errorVARCHARprincipaldelfitphot_iFormal uncertainty in fitphot_imagstat.errorVARCHARprincipaldelfitphot_rFormal uncertainty in fitphot_rmagstat.errorVARCHARprincipaldelfitphot_uFormal uncertainty in fitphot_umagstat.errorVARCHARprincipaldelfitphot_zFormal uncertainty in fitphot_zmagstat.errorVARCHARprincipaldelgminusiFormal uncertainty on gminusimagstat.errorVARCHARprincipaldellogLWageFormal uncertainty on logLWagedexstat.errorVARCHARprincipaldellogageFormal uncertainty on logagedexstat.errorVARCHARprincipaldellogmoverl_iFormal uncertainty on logmoverl_idexstat.errorVARCHARprincipaldellogmstarFormal uncertainty on logmstardexstat.errorVARCHARprincipaldellogtauFormal uncertainty on logtaudexstat.errorVARCHARprincipaldelmetalFormal uncertainty on metalstat.errorVARCHARprincipaldeluminusrFormal uncertainty on uminusrmagstat.errorVARCHARprincipalextBVSPS dust obscuration; for Calzetti et al. (2003) dust A_V = 3.1 x E(B-V)magphys.absorptionVARCHARprincipalfitphot_gBest-fit observers` frame g-band apparent magnitude from SPS SED fitsmagphot.magVARCHARprincipalfitphot_iBest-fit observers` frame i-band apparent magnitude from SPS SED fitsmagphot.magVARCHARprincipalfitphot_rBest-fit observers` frame r-band apparent magnitude from SPS SED fitsmagphot.magVARCHARprincipalfitphot_uBest-fit observers` frame u-band apparent magnitude from SPS SED fitsmagphot.magVARCHARprincipalfitphot_zBest-fit observers` frame z-band apparent magnitude from SPS SED fitsmagphot.magVARCHARprincipalfluxscaleAperture correction factor for scaling total luminosities and stellar masses (see notes)arith.factorVARCHARprincipalgminusiRestframe (g-i) colour from SED fitmagphot.colorVARCHARprincipalgminusi_starsIntrinsic, stellar (g-i) colour from SED fit, i.e. corrected for internal dust obscurationmagphot.colorVARCHARprincipallogLWageRestframe i-band luminosity weighted mean stellar age, represented as log10(t*/[yr])dextime.ageVARCHARprincipallogageSPS age T = t(z_obs) - t(z_form), represented as log10(T/[yr])dextime.ageVARCHARprincipallogmoverl_iMass-to-light ratio (restframe i-band) represented as log10( (M_*/L_i) / [M_Sol/L_Sol,i] )dexphys.composition.massLightRatioVARCHARprincipallogmstarStellar mass within the photometric aperture represented as log10(M_*/[M_Sol]) (see notes)dexphys.massVARCHARprincipallogtauSPS e-folding time for the exponentially declining SFH, represented as log10(tau/[yr])dextime.scaleVARCHARprincipalmetalSPS stellar metallicity (Z_Sol = 0.02)phys.abund.ZVARCHARprincipalnQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalnbandsNumber of bands used in SPS fits (max. is 5; NIR data have not been used)meta.numberVARCHARprincipaluminusrRestframe (u-r) colour from SED fitmagphot.colorVARCHARprincipaluminusr_starsIntrinsic, stellar (u-r) colour from SED fit, i.e. corrected for internal dust obscurationmagphot.colorVARCHARprincipalzmax_17p88Maximum redshift for which r_petro <= 17.8 (SDSS main survey selection)src.redshift;stat.maxVARCHARprincipalzmax_19p4Maximum redshift for which r_petro <= 19.4 (G09/G15 SURVEY_CLASS>=6 selection)src.redshift;stat.maxVARCHARprincipalzmax_19p8Maximum redshift for which r_petro <= 19.8 (G12 SURVEY_CLASS>=6 selection)src.redshift;stat.maxVARCHARprincipalgama_dr2.kcorr_z01This table provides k-corrections at redshift 0.1 in the GALEX FUV and NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands for all GAMA DR2 galaxies.B1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalCATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalG_MODELSDSS DR6 g-band model magnitudemagphot.mag;em.opt.BVARCHARprincipalG_MODEL_ERRSDSS DR6 g-band model magnitude errormagstat.error;phot.mag;em.opt.BVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalI_MODELSDSS DR6 i-band model magnitudemagphot.mag;em.opt.IVARCHARprincipalI_MODEL_ERRSDSS DR6 i-band model magnitude errormagstat.error;phot.mag;em.opt.IVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalPCOEFF_FUV_1Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_2Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_3Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_4Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_5Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_G_1Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_2Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_3Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_4Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_5Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_H_1Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_2Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_3Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_5Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_J_1Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_2Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_3Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_4Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_5Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_K_1Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_2Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_3Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_4Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_5Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_NUV_1Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_2Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_3Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_4Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_5Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_U_1Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_2Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_3Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_4Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_5Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_Y_1Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_2Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_3Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_4Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_5Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Z_1Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_2Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_3Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_4Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_5Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalR_MODELSDSS DR6 r-band model magnitudemagphot.mag;em.opt.RVARCHARprincipalR_MODEL_ERRSDSS DR6 r-band model magnitude errormagstat.error;phot.mag;em.opt.RVARCHARprincipalU_MODELSDSS DR6 u-band model magnitudemagphot.mag;em.opt.UVARCHARprincipalU_MODEL_ERRSDSS DR6 u-band model magnitude errormagstat.error;phot.mag;em.opt.UVARCHARprincipalZ_MODELSDSS DR6 z-band model magnitudemagphot.mag;em.opt.IVARCHARprincipalZ_MODEL_ERRSDSS DR6 z-band model magnitude errormagstat.error;phot.mag;em.opt.IVARCHARprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalPCOEFF_H_4Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalgama_dr2.kcorr_z00This table provides k-corrections at redshift 0.0 in the GALEX FUV and NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands for all GAMA DR2 galaxies.B1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalCATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalG_MODELSDSS DR6 g-band model magnitudemagphot.mag;em.opt.BVARCHARprincipalG_MODEL_ERRSDSS DR6 g-band model magnitude errormagstat.error;phot.mag;em.opt.BVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalI_MODELSDSS DR6 i-band model magnitudemagphot.mag;em.opt.IVARCHARprincipalI_MODEL_ERRSDSS DR6 i-band model magnitude errormagstat.error;phot.mag;em.opt.IVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalPCOEFF_FUV_1Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_2Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_3Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_4Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_FUV_5Coefficient of polynomial fit to K(z) in GALEX FUV bandarith.factorVARCHARprincipalPCOEFF_G_1Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_2Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_3Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_4Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_G_5Coefficient of polynomial fit to K(z) in SDSS g bandarith.factorVARCHARprincipalPCOEFF_H_1Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_2Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_3Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_4Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_H_5Coefficient of polynomial fit to K(z) in UKIDSS H bandarith.factorVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_J_1Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_2Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_3Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_4Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_J_5Coefficient of polynomial fit to K(z) in UKIDSS J bandarith.factorVARCHARprincipalPCOEFF_K_1Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_2Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_3Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_4Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_K_5Coefficient of polynomial fit to K(z) in UKIDSS K bandarith.factorVARCHARprincipalPCOEFF_NUV_1Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_2Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_3Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_4Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_NUV_5Coefficient of polynomial fit to K(z) in GALEX NUV bandarith.factorVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_U_1Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_2Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_3Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_4Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_U_5Coefficient of polynomial fit to K(z) in SDSS u bandarith.factorVARCHARprincipalPCOEFF_Y_1Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_2Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_3Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_4Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Y_5Coefficient of polynomial fit to K(z) in UKIDSS Y bandarith.factorVARCHARprincipalPCOEFF_Z_1Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_2Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_3Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_4Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalPCOEFF_Z_5Coefficient of polynomial fit to K(z) in SDSS z bandarith.factorVARCHARprincipalR_MODEL_ERRSDSS DR6 r-band model magnitude errormagstat.error;phot.mag;em.opt.RVARCHARprincipalU_MODELSDSS DR6 u-band model magnitudemagphot.mag;em.opt.UVARCHARprincipalU_MODEL_ERRSDSS DR6 u-band model magnitude errormagstat.error;phot.mag;em.opt.UVARCHARprincipalZ_MODELSDSS DR6 z-band model magnitudemagphot.mag;em.opt.IVARCHARprincipalZ_MODEL_ERRSDSS DR6 z-band model magnitude errormagstat.error;phot.mag;em.opt.IVARCHARprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalR_MODELSDSS DR6 r-band model magnitudemagphot.mag;em.opt.RVARCHARprincipalgama_dr2.ApMatchedCatThis table contains r-band aperture matched photometry and other Source Extractor outputs for all GAMA DR2 objects.ALPHA_J2000RA (r band)degpos.eq.ra;em.opt.RVARCHARprincipalA_IMAGEProfile RMS along major axis (r band)pixelphys.angSize;em.opt.RVARCHARprincipalBACKGROUND_GBackground at centroid (g band)countsinstr.background;phot.count;em.opt.GVARCHARprincipalBACKGROUND_HBackground at centroid (H band)countsinstr.background;phot.count;em.IR.HVARCHARprincipalBACKGROUND_IBackground at centroid (i band)countsinstr.background;phot.count;em.opt.IVARCHARprincipalBACKGROUND_JBackground at centroid (J band)countsinstr.background;phot.count;em.IR.JVARCHARprincipalBACKGROUND_KBackground at centroid (K band)countsinstr.background;phot.count;em.IR.KVARCHARprincipalBACKGROUND_RBackground at centroid (r band)countsinstr.background;phot.count;em.opt.RVARCHARprincipalBACKGROUND_UBackground at centroid (u band)countsinstr.background;phot.count;em.opt.UVARCHARprincipalBACKGROUND_YBackground at centroid (Y band)countsinstr.background;phot.count;em.IR.YVARCHARprincipalBACKGROUND_ZBackground at centroid (z band)countsinstr.background;phot.count;em.opt.ZVARCHARprincipalB_IMAGEProfile RMS along minor axis (r band)pixelphys.angsSize;em.opt.RVARCHARprincipalCATAIDUnique GAMA object IDmeta.idVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalDELTA_J2000DEC (r band)degpos.eq.dec;em.opt.RVARCHARprincipalERRA_IMAGEMajor axis profile RMS error (r band)pixelstat.error;phys.angSize;em.opt.RVARCHARprincipalERRB_IMAGEMinor axis profile RMS error (r band)pixelstat.error;phys.angSize;em.opt.RVARCHARprincipalERRTHETA_J2000J2000 position angle error (r band)degstat.error;pos.posAng;em.opt.RVARCHARprincipalFLAGS_GSource Extractor flags (g band)meta.code.qual;em.opt.GVARCHARprincipalFLAGS_HSource Extractor flags (H band)meta.code.qual;em.IR.HVARCHARprincipalFLAGS_ISource Extractor flags (i band)meta.code.qual;em.opt.IVARCHARprincipalFLAGS_JSource Extractor flags (J band)meta.code.qual;em.IR.JVARCHARprincipalFLAGS_KSource Extractor flags (K band)mag.code.qual;em.IR.KVARCHARprincipalFLAGS_RSource Extractor flags (r band)meta.code.qual;em.opt.RVARCHARprincipalFLAGS_USource Extractor flags (u band)meta.code.qual;em.opt.UVARCHARprincipalFLAGS_YSource Extractor flags (Y band)meta.code.qual;em.IR.YVARCHARprincipalFLAGS_ZSource Extractor flags (z band)meta.code.qual;em.opt.ZVARCHARprincipalFLUXERR_AUTO_GKron flux error (g band)countsstat.error;phot.flux;em.opt.GVARCHARprincipalFLUXERR_AUTO_HKron flux error (H band)countsstat.error;phot.flux;em.IR.HVARCHARprincipalFLUXERR_AUTO_IKron flux error (i band)countsstat.error;phot.flux;em.opt.IVARCHARprincipalFLUXERR_AUTO_JKron flux error (J band)countstat.error;phot.flux;em.IR.JVARCHARprincipalFLUXERR_AUTO_KKron flux error (K band)countsstat.error;phot.flux;em.IR.KVARCHARprincipalFLUXERR_AUTO_RKron flux error (r band)countsstat.error;phot.flux;em.opt.RVARCHARprincipalFLUXERR_AUTO_UKron flux error (u band)countsstat.error;phot.flux;em.opt.UVARCHARprincipalFLUXERR_AUTO_YKron flux error (Y band)countsstat.error;phot.flux;em.IR.YVARCHARprincipalFLUXERR_AUTO_ZKron flux error (z band)countsstat.error;phot.flux;em.opt.ZVARCHARprincipalFLUXERR_PETRO_GPetrosian flux error (g band)countsstat.error;phot.flux;em.opt.GVARCHARprincipalFLUXERR_PETRO_HPetrosian flux error (H band)countsstat.error;phot.flux;em.IR.HVARCHARprincipalFLUXERR_PETRO_IPetrosian flux error (i band)countsstat.error;phot.flux;em.opt.IVARCHARprincipalFLUXERR_PETRO_JPetrosian flux error (J band)countstat.error;phot.flux;em.IR.JVARCHARprincipalFLUXERR_PETRO_KPetrosian flux error (K band)countsstat.error;phot.flux;em.IR.KVARCHARprincipalFLUXERR_PETRO_RPetrosian flux error (r band)countsstat.error;phot.flux;em.opt.RVARCHARprincipalFLUXERR_PETRO_UPetrosian flux error (u band)countsstat.error;phot.flux;em.opt.UVARCHARprincipalFLUXERR_PETRO_YPetrosian flux error (Y band)countsstat.error;phot.flux;em.IR.YVARCHARprincipalFLUXERR_PETRO_ZPetrosian flux error (z band)countsstat.error;phot.flux;em.opt.ZVARCHARprincipalFLUX_AUTO_GKron flux (g band)countsphot.flux;em.opt.GVARCHARprincipalFLUX_AUTO_HKron flux (H band)countsphot.flux;em.IR.HVARCHARprincipalFLUX_AUTO_IKron flux (i band)countsphot.flux;em.opt.IVARCHARprincipalFLUX_AUTO_JKron flux (J band)countphot.flux;em.IR.JVARCHARprincipalFLUX_AUTO_KKron flux (K band)countsphot.flux;em.IR.KVARCHARprincipalFLUX_AUTO_RKron flux (r band)countsphot.flux;em.opt.RVARCHARprincipalFLUX_AUTO_UKron flux (u band)countsphot.flux;em.opt.UVARCHARprincipalFLUX_AUTO_YKron flux (Y band)countsphot.flux;em.IR.YVARCHARprincipalFLUX_AUTO_ZKron flux (z band)countsphot.flux;em.opt.ZVARCHARprincipalFLUX_MAX_GPeak flux (g band)countsphot.flux;stat.max;em.opt.GVARCHARprincipalFLUX_MAX_HPeak flux (H band)countsphot.flux;stat.max;em.IR.HVARCHARprincipalFLUX_MAX_IPeak flux (i band)countsphot.flux;stat.max;em.opt.IVARCHARprincipalFLUX_MAX_JPeak flux (J band)countsphot.flux;stat.max;em.IR.JVARCHARprincipalFLUX_MAX_KPeak flux (K band)countsphot.flux;stat.max;em.IR.KVARCHARprincipalFLUX_MAX_RPeak flux (r band)countsphot.flux;stat.max;em.opt.RVARCHARprincipalFLUX_MAX_UPeak flux (u band)countsphot.flux;stat.max;em.opt.UVARCHARprincipalFLUX_MAX_YPeak flux (Y band)countsphot.flux;stat.max;em.IR.YVARCHARprincipalFLUX_MAX_ZPeak flux (z band)countphot.flux;stat.max;em.opt.ZVARCHARprincipalFLUX_PETRO_GPetrosian flux (g band)countsphot.flux;em.opt.GVARCHARprincipalFLUX_PETRO_HPetrosian flux (H band)countsphot.flux;em.IR.HVARCHARprincipalFLUX_PETRO_IPetrosian flux (i band)countsphot.flux;em.opt.IVARCHARprincipalFLUX_PETRO_JPetrosian flux (J band)countphot.flux;em.IR.JVARCHARprincipalFLUX_PETRO_KPetrosian flux (K band)countsphot.flux;em.IR.KVARCHARprincipalFLUX_PETRO_RPetrosian flux (r band)countsphot.flux;em.opt.RVARCHARprincipalFLUX_PETRO_UPetrosian flux (u band)countsphot.flux;em.opt.UVARCHARprincipalFLUX_PETRO_YPetrosian flux (Y band)countsphot.flux;em.IR.YVARCHARprincipalFLUX_PETRO_ZPetrosian flux (z band)countsphot.flux;em.opt.ZVARCHARprincipalFWHM_IMAGE_GFWHM assuming a Gaussian core (g band)pixelspect.line.width;obs.image;em.opt.GVARCHARprincipalFWHM_IMAGE_HFWHM assuming a Gaussian core (H band)pixelspect.line.width;obs.image;em.IR.HVARCHARprincipalFWHM_IMAGE_IFWHM assuming a Gaussian core (i band)pixelspect.line.width;obs.image;em.opt.IVARCHARprincipalFWHM_IMAGE_JFWHM assuming a Gaussian core (J band)pixelspect.line.width;obs.image;em.IR.JVARCHARprincipalFWHM_IMAGE_KFWHM assuming a Gaussian core (K band)pixelspect.line.width;obs.image;em.IR.KVARCHARprincipalFWHM_IMAGE_RFWHM assuming a Gaussian core (r band)pixelspect.line.width;obs.image;em.opt.RVARCHARprincipalFWHM_IMAGE_UFWHM assuming a Gaussian core (u band)pixelspect.line.width;obs.image;em.opt.UVARCHARprincipalFWHM_IMAGE_YFWHM assuming a Gaussian core (Y band)pixelspect.line.width;obs.image;em.IR.YVARCHARprincipalFWHM_IMAGE_ZFWHM assuming a Gaussian core (z band)pixelspect.line.width;obs.image;em.opt.ZVARCHARprincipalISOAREAF_IMAGEIsophotal area (filtered) (r band)pixelphys.angArea;em.opt.RVARCHARprincipalISOAREA_IMAGE_GIsophotal area (g band)pixelphys.angArea;em.opt.GVARCHARprincipalISOAREA_IMAGE_HIsophotal area (H band)pixelphys.angArea;em.IR.HVARCHARprincipalISOAREA_IMAGE_IIsophotal area (i band)pixelphys.angArea;em.opt.IVARCHARprincipalISOAREA_IMAGE_JIsophotal area (J band)pixelphys.angArea;em.IR.JVARCHARprincipalISOAREA_IMAGE_KIsophotal area (K band)pixelphys.angArea;em.IR.KVARCHARprincipalISOAREA_IMAGE_RIsophotal area (r band)pixelphys.angArea;em.opt.RVARCHARprincipalISOAREA_IMAGE_UIsophotal area (u band)pixelphys.angArea;em.opt.UVARCHARprincipalISOAREA_IMAGE_YIsophotal area (Y band)pixelphys.angArea;em.IR.YVARCHARprincipalISOAREA_IMAGE_ZIsophotal area (z band)pixelphys.angArea;em.opt.ZVARCHARprincipalKRON_RADIUSKron radius (r band)pixelphys.size.radius;em.opt.RVARCHARprincipalMAGERR_AUTO_GKron magnitude error (g band)magstat.error;phot.mag;em.opt.GVARCHARprincipalMAGERR_AUTO_HKron magnitude error (H band)magstat.error;phot.mag;em.IR.HVARCHARprincipalMAGERR_AUTO_IKron magnitude error (i band)magstat.error;phot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_JKron magnitude error (J band)magstat.error;phot.mag;em.IR.JVARCHARprincipalMAGERR_AUTO_KKron magnitude error (K band)magstat.error;phot.mag;em.IR.KVARCHARprincipalMAGERR_AUTO_RKron magnitude (r band)magstat.error;phot.mag;em.opt.RVARCHARprincipalMAGERR_AUTO_UKron magnitude error (u band)magstat.error;phot.mag;em.opt.UVARCHARprincipalMAGERR_AUTO_YKron magnitude error (Y band)magstat.error;phot.mag;em.IR.YVARCHARprincipalMAGERR_AUTO_ZKron magnitude error (z band)magstat.error;phot.mag;em.opt.ZVARCHARprincipalMAGERR_PETRO_GPetrosian magnitude (g band)magstat.error;phot.mag;em.opt.GVARCHARprincipalMAGERR_PETRO_HPetrosian magnitude error (H band)magstat.error;phot.mag;em.IR.HVARCHARprincipalMAGERR_PETRO_IPetrosian magnitude error (i band)magstat.error;phot.mag;em.opt.IVARCHARprincipalMAGERR_PETRO_JPetrosian magnitude error (J band)magstat.error;phot.mag;em.IR.JVARCHARprincipalMAGERR_PETRO_KPetrosian magnitude error (K band)magstat.error;phot.mag;em.IR.KVARCHARprincipalMAGERR_PETRO_RPetrosian magnitude (r band)magstat.error;phot.mag;em.opt.RVARCHARprincipalMAGERR_PETRO_UPetrosian magnitude error (u band)magstat.error;phot.mag;em.opt.UVARCHARprincipalMAGERR_PETRO_YPetrosian magnitude error (Y band)magstat.error;phot.mag;em.IR.YVARCHARprincipalMAGERR_PETRO_ZPetrosian magnitude error (z band)magstat.error;phot.mag;em.opt.ZVARCHARprincipalMAG_AUTO_GKron magnitude (g band)magphot.mag;em.opt.GVARCHARprincipalMAG_AUTO_HKron magnitude (H band)magphot.mag;em.IR.HVARCHARprincipalMAG_AUTO_IKron magntiude (i band)magphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_JKron magnitude (J band)magphot.mag;em.IR.JVARCHARprincipalMAG_AUTO_KKron magintude (K band)magphot.mag;em.IR.KVARCHARprincipalMAG_AUTO_RKron magnitude (r band)magphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_UKron magnitude (u band)magphot.mag;em.opt.UVARCHARprincipalMAG_AUTO_YKron magnitude (Y band)magphot.mag;em.IR.YVARCHARprincipalMAG_AUTO_ZKron magnitude (z band)magphot.mag.em.opt.ZVARCHARprincipalMAG_PETRO_GPetrosian magnitude (g band)magphot.mag;em.opt.GVARCHARprincipalMAG_PETRO_HPetrosian magnitude (H band)magphot.mag;em.IR.HVARCHARprincipalMAG_PETRO_IPetrosian magnitude (i band)magphot.mag;em.opt.IVARCHARprincipalMAG_PETRO_JPetrosian magnitude (J band)magphot.mag;em.IR.JVARCHARprincipalMAG_PETRO_KPetrosian magnitude (K band)magphot.mag;em.IR.KVARCHARprincipalMAG_PETRO_RPetrosian magnitude (r band)magphot.mag;em.opt.RVARCHARprincipalMAG_PETRO_UPetrosian magnitude (u band)magphot.mag;em.opt.UVARCHARprincipalMAG_PETRO_YPetrosian magnitude (Y band)magphot.mag;em.IR.YVARCHARprincipalMAG_PETRO_ZPetrosian magnitude (z band)magphot.mag;em.opt.ZVARCHARprincipalMU_MAX_GPeak surface brightness (g band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.GVARCHARprincipalMU_MAX_HPeak surface brightness (H band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.HVARCHARprincipalMU_MAX_IPeak surface brightness (i band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.IVARCHARprincipalMU_MAX_JPeak surface brightness (J band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.JVARCHARprincipalMU_MAX_KPeak surface brightness (K band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.KVARCHARprincipalMU_MAX_RPeak surface brightness (r band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.RVARCHARprincipalMU_MAX_UPeak surface brightness (u band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.UVARCHARprincipalMU_MAX_YPeak surface brightness (Y band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.YVARCHARprincipalMU_MAX_ZPeak surface brightness (z band)mag/arcsec^2phot.mag.sb;statm.ax;em.opt.ZVARCHARprincipalMU_THRESHOLDDetection threshold above background (r band)mag/arcsec^2instr.sensitivity;phot.mag.sb;em.opt.RVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalPETRO_RADIUSPetrosian radius (r band)pixelphys.size.radius;em.opt.RVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalTHETA_IMAGEPosition angle (counterclockwise)degpos.posAng;em.opt.RVARCHARprincipalTHETA_J2000Position angle (east of north)degpos.posAng;em.opt.RVARCHARprincipalTHRESHOLDDetection threshold above background (r band)countsinstr.sensitivity;phot.count;em.opt.RVARCHARprincipalXx coordinate of aperture centre in r band cutoutpixelposVARCHARprincipalYy coordinate of aperture centre in r band cutoutpixelposVARCHARprincipalgama_dr2.GalacticExtinctionThis table provides the Galactic foreground extinction in all GALEX, SDSS and UKIDSS bands for every object in InputCatA and SpStandards.A_BGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_HGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_JGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_KGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_YGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_gGalactic extinction in SDSS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_iGalactic extinction in SDSS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_rGalactic extinction in SDSS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_uGalactic extinction in SDSS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_zGalactic extinction in SDSS z bandmagphys.absorption.gal;em.optVARCHARprincipalCATAIDUnique GAMA of objectmeta.id;meta.mainVARCHARindexedprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalgama_dr2.InputCatASDSS DR6 data of GAMA I survey regions. This is GAMA`s master input catalogue.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalEXTINCTION_Rr-band Galactic extinctionmagphys.absorption.gal;em.opt.RVARCHARprincipalFIBERMAG_R3-arcsec fiber magnitudemagphot.mag;em.opt.RVARCHARprincipalFLAGSSee SDSS photoobj tablemeta.code.qual;photVARCHARprincipalFLAGS_RSee SDSS photoobj tablemeta.code.qual;phot;em.opt.RVARCHARprincipalMODELMAG_GDR6 magmagphot.mag;em.optVARCHARprincipalMODELMAG_IDR6 magmagphot.mag;em.opt.IVARCHARprincipalMODELMAG_RDR6 magmagphot.mag;em.opt.RVARCHARprincipalMODELMAG_UDR6 magmagphot.mag;em.opt.UVARCHARprincipalMODELMAG_ZDR6 magmagphot.mag;em.optVARCHARprincipalPETROMAG_GDR6 magmagphot.mag;em.optVARCHARprincipalPETROMAG_IDR6 magmagphot.mag;em.opt.IVARCHARprincipalPETROMAG_RDR6 magmagphot.mag;em.opt.RVARCHARprincipalPETROMAG_UDR6 magmagphot.mag;em.opt.UVARCHARprincipalPETROMAG_ZDR6 magmagphot.mag;em.optVARCHARprincipalPETROR50_RRadius containing 50% of Petrosian fluxarcsecphys.angSize;em.opt.RVARCHARprincipalPETROR90_RRadius containing 90% of Petrosian fluxarcsecphys.angSize;em.opt.RVARCHARprincipalPETRORAD_RPetrosian radiusarcsecphys.angSize;em.opt.RVARCHARprincipalPRIMTARGETSee SDSS photoobj tablemeta.code.classVARCHARprincipalPSFMAG_RPSF magnitudemagphot.mag;em.opt.RVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalRUNSDSS run numberobs.paramVARCHARprincipalSTATUSSee SDSS photoobj tablemeta.code.statusVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalgama_dr2.DistancesFramesThis table provides redhifts in various reference frames, flow corrected redshifts, and distance moduli for all GAMA DR2 objects.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalDM_100_25_75distance modulus for H0=100, 0.25, 0.75magphot.mag.distModVARCHARprincipalDM_100_30_70distance modulus for H0=100, 0.30, 0.70magphot.mag.distModVARCHARprincipalDM_70_30_70distance modulus for 737 cosmologymagphot.mag.distModVARCHARprincipalNQquality of redshift (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalZ_CMBCMB frame redshiftsrc.redshiftVARCHARprincipalZ_HELIOheliocentric redshiftsrc.redshiftVARCHARprincipalZ_LGLocal Group frame redshiftsrc.redshiftVARCHARprincipalZ_TONRYflow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalZ_TONRY_HIGHrecomputed after adjusting z_helio by +180 km/ssrc.redshiftVARCHARprincipalZ_TONRY_LOWrecomputed after adjusting z_helio by -180 km/ssrc.redshiftVARCHARprincipalgama_dr2.EnvironmentMeasuresThis catalogue provides three different environment measures for all GAMA DR2 galaxies in G15 with 0.002 < z < 0.18: a surface density, the number of galaxies within a cylinder, and the density of galaxies within an adaptive Gaussian ellipsoid.AGEDensityDensity of galaxies within an adaptive Gaussian ellipsoidMpc^-3src.densityVARCHARprincipalAGEDensityFlagFlag indicating problems with AGEDensity, see notesmeta.code.error;src.densityVARCHARprincipalAGEErrPoisson error on the number of galaxies used to calculate AGEDensitysrc.density;stat.errorVARCHARprincipalAGEScaleAdaptive scaling factor for adaptive Gaussian ellipsoidarith.factorVARCHARprincipalCATAIDUnique GAMA IDmeta.idVARCHARprincipalCompletenessValue used to correct environment measures for local survey incompleteness (see notes)arith.factorVARCHARprincipalCountInCylNumber of (other) galaxies within cylinder of radius 1 co-moving Mpcsrc.densityVARCHARprincipalCountInCylErrPoisson error on number of galaxies in cylinderstat.error;src.densityVARCHARprincipalCountInCylFlagFlag indicating problems with CountInCyl (see notes)meta.code.error;src.densityVARCHARprincipalDECJ2000degpos.eq.decVARCHARprincipalDistanceTo5nnDistance to 5th nearest neighbour in co-moving unitsMpcpos.distanceVARCHARprincipalDistanceToEdgeDistance to nearest angular survey edge in co-moving unitsMpcpos.distanceVARCHARprincipalM_rExtinction and k-corrected absolute r-band magnitudemagphys.magAbsVARCHARprincipalRAJ2000degpos.eq.raVARCHARprincipalSurfaceDensitySurface density based on the distance to the 5th nearest neighbourMpc^-2src.densityVARCHARprincipalSurfaceDensityErrSurface density uncertaintyMpc^-2src.density;stat.errorVARCHARprincipalSurfaceDensityFlagFlag indicating problems with surface density measurement (see notes)meta.code.error;src.densityVARCHARprincipalZ_TONRYHeliocentric redshift corrected for the effects of peculiar velocitysrc.redshiftVARCHARprincipalnQRedshift quality flagmeta.code.qual;src.redshiftVARCHARprincipalgama_dr2.SersicCatAllThis catalogue contains the complete output of the SersicPhotometry DMU, using SIGMA v0.9-0 (Structural Investigation of Galaxies via Model Analysis) to generate a single-Sersic fit to every GAMA DR2 object.RARight Ascension (J2000)degpos.eq.raVARCHARprincipalCATAIDGAMA Object IDmeta.idVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalFILENAMEFull path to object`s data directorymeta.id;meta.fileVARCHARprincipalGAL_CHFLAG_Gcomponent history flag (see notes)meta.code;em.optVARCHARprincipalGAL_CHFLAG_Hcomponent history flag (see notes)meta.code;em.IR.HVARCHARprincipalGAL_CHFLAG_Icomponent history flag (see notes)meta.code;em.opt.IVARCHARprincipalGAL_CHFLAG_Jcomponent history flag (see notes)meta.code;em.IR.JVARCHARprincipalGAL_CHFLAG_Kcomponent history flag (see notes)meta.code;em.IR.KVARCHARprincipalGAL_CHFLAG_Rcomponent history flag (see notes)meta.code;em.opt.RVARCHARprincipalGAL_CHFLAG_Ucomponent history flag (see notes)meta.code;em.opt.UVARCHARprincipalGAL_CHFLAG_Ycomponent history flag (see notes)meta.code;em.IR.NIRVARCHARprincipalGAL_CHFLAG_Zcomponent history flag (see notes)meta.code;em.optVARCHARprincipalGAL_CHI2_Greduced Chi^2 of output modelstat.fit.goodness;em.optVARCHARprincipalGAL_CHI2_Hreduced Chi^2 of output modelstat.fit.goodness;em.IR.HVARCHARprincipalGAL_CHI2_Ireduced Chi^2 of output modelstat.fit.goodness;em.opt.IVARCHARprincipalGAL_CHI2_Jreduced Chi^2 of output modelstat.fit.goodness;em.IR.JVARCHARprincipalGAL_CHI2_Kreduced Chi^2 of output modelstat.fit.goodness;em.IR.KVARCHARprincipalGAL_CHI2_Rreduced Chi^2 of output modelstat.fit.goodness;em.opt.RVARCHARprincipalGAL_CHI2_Ureduced Chi^2 of output modelstat.fit.goodness;em.opt.UVARCHARprincipalGAL_CHI2_Yreduced Chi^2 of output modelstat.fit.goodness;em.IR.NIRVARCHARprincipalGAL_CHI2_Zreduced Chi^2 of output modelstat.fit.goodness;em.optVARCHARprincipalGAL_COMPS_Gnumber of modelled galaxy componentsmeta.number;em.optVARCHARprincipalGAL_COMPS_Hnumber of modelled galaxy componentsmeta.number;em.IR.HVARCHARprincipalGAL_COMPS_Inumber of modelled galaxy componentsmeta.number;em.opt.IVARCHARprincipalGAL_COMPS_Jnumber of modelled galaxy componentsmeta.number;em.IR.JVARCHARprincipalGAL_COMPS_Knumber of modelled galaxy componentsmeta.number;em.IR.KVARCHARprincipalGAL_COMPS_Rnumber of modelled galaxy componentsmeta.number;em.opt.RVARCHARprincipalGAL_COMPS_Unumber of modelled galaxy componentsmeta.number;em.opt.UVARCHARprincipalGAL_COMPS_Ynumber of modelled galaxy componentsmeta.number;em.IR.NIRVARCHARprincipalGAL_COMPS_Znumber of modelled galaxy componentsmeta.number;em.optVARCHARprincipalGAL_DEC_GDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.optVARCHARprincipalGAL_DEC_HDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.HVARCHARprincipalGAL_DEC_IDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.IVARCHARprincipalGAL_DEC_JDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.JVARCHARprincipalGAL_DEC_KDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.KVARCHARprincipalGAL_DEC_RDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.RVARCHARprincipalGAL_DEC_UDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.UVARCHARprincipalGAL_DEC_YDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.NIRVARCHARprincipalGAL_DEC_ZDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.optVARCHARprincipalGAL_ELLIP_ERR_GGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_HGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_IGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_JGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_KGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_RGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_UGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_YGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_ERR_ZGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.model...VARCHARprincipalGAL_ELLIP_Gellipticity (1-(b/a))src.ellipticity;meta.modelled;em.optVARCHARprincipalGAL_ELLIP_Hellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.HVARCHARprincipalGAL_ELLIP_Iellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.IVARCHARprincipalGAL_ELLIP_Jellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.JVARCHARprincipalGAL_ELLIP_Kellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.KVARCHARprincipalGAL_ELLIP_Rellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.RVARCHARprincipalGAL_ELLIP_Uellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.UVARCHARprincipalGAL_ELLIP_Yellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.NIRVARCHARprincipalGAL_ELLIP_Zellipticity (1-(b/a))src.ellipticity;meta.modelled;em.optVARCHARprincipalGAL_EXTRAS_Gnumber of additional neighbours modelledmeta.number;em.optVARCHARprincipalGAL_EXTRAS_Hnumber of additional neighbours modelledmeta.number;em.IR.HVARCHARprincipalGAL_EXTRAS_Inumber of additional neighbours modelledmeta.number;em.opt.IVARCHARprincipalGAL_EXTRAS_Jnumber of additional neighbours modelledmeta.number;em.IR.JVARCHARprincipalGAL_EXTRAS_Knumber of additional neighbours modelledmeta.number;em.IR.KVARCHARprincipalGAL_EXTRAS_Rnumber of additional neighbours modelledmeta.number;em.opt.RVARCHARprincipalGAL_EXTRAS_Unumber of additional neighbours modelledmeta.number;em.opt.UVARCHARprincipalGAL_EXTRAS_Ynumber of additional neighbours modelledmeta.number;em.IR.NIRVARCHARprincipalGAL_EXTRAS_Znumber of additional neighbours modelledmeta.number;em.optVARCHARprincipalGAL_FITWORD_Gtype of fitem.optVARCHARprincipalGAL_FITWORD_Htype of fitem.IR.HVARCHARprincipalGAL_FITWORD_Itype of fitem.opt.IVARCHARprincipalGAL_FITWORD_Jtype of fitem.IR.JVARCHARprincipalGAL_FITWORD_Ktype of fitem.IR.KVARCHARprincipalGAL_FITWORD_Rtype of fitem.opt.RVARCHARprincipalGAL_FITWORD_Utype of fitem.opt.UVARCHARprincipalGAL_FITWORD_Ytype of fitem.IR.NIRVARCHARprincipalGAL_FITWORD_Ztype of fitem.optVARCHARprincipalGAL_FIT_Gtype of fit (see notes)em.optVARCHARprincipalGAL_FIT_Htype of fit (see notes)em.IR.HVARCHARprincipalGAL_FIT_Itype of fit (see notes)em.opt.IVARCHARprincipalGAL_FIT_Jtype of fit (see notes)em.IR.JVARCHARprincipalGAL_FIT_Ktype of fit (see notes)em.IR.KVARCHARprincipalGAL_FIT_Rtype of fit (see notes)em.opt.RVARCHARprincipalGAL_FIT_Utype of fit (see notes)em.opt.UVARCHARprincipalGAL_FIT_Ytype of fit (see notes)em.IR.NIRVARCHARprincipalGAL_FIT_Ztype of fit (see notes)em.optVARCHARprincipalGAL_GHFLAG_Gglobal history flag (see notes)meta.code;em.optVARCHARprincipalGAL_GHFLAG_Hglobal history flag (see notes)meta.code;em.IR.HVARCHARprincipalGAL_GHFLAG_Iglobal history flag (see notes)meta.code;em.opt.IVARCHARprincipalGAL_GHFLAG_Jglobal history flag (see notes)meta.code;em.IR.JVARCHARprincipalGAL_GHFLAG_Kglobal history flag (see notes)meta.code;em.IR.KVARCHARprincipalGAL_GHFLAG_Rglobal history flag (see notes)meta.code;em.opt.RVARCHARprincipalGAL_GHFLAG_Uglobal history flag (see notes)meta.code;em.opt.UVARCHARprincipalGAL_GHFLAG_Yglobal history flag (see notes)meta.code;em.IR.NIRVARCHARprincipalGAL_GHFLAG_Zglobal history flag (see notes)meta.code;em.optVARCHARprincipalGAL_INDEX_ERR_GGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_HGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_IGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_JGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_KGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_RGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_UGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_YGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_ERR_ZGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modell...VARCHARprincipalGAL_INDEX_GSersic indexstat.fit.param;meta.modelled;em.optVARCHARprincipalGAL_INDEX_HSersic indexstat.fit.param;meta.modelled;em.IR.HVARCHARprincipalGAL_INDEX_ISersic indexstat.fit.param;meta.modelled;em.opt.IVARCHARprincipalGAL_INDEX_JSersic indexstat.fit.param;meta.modelled;em.IR.JVARCHARprincipalGAL_INDEX_KSersic indexstat.fit.param;meta.modelled;em.IR.KVARCHARprincipalGAL_INDEX_RSersic indexstat.fit.param;meta.modelled;em.opt.RVARCHARprincipalGAL_INDEX_USersic indexstat.fit.param;meta.modelled;em.opt.UVARCHARprincipalGAL_INDEX_YSersic indexstat.fit.param;meta.modelled;em.IR.NIRVARCHARprincipalGAL_INDEX_ZSersic indexstat.fit.param;meta.modelled;em.optVARCHARprincipalGAL_ITERATIONS_Gnumber of iterations for convergencemeta.number;em.optVARCHARprincipalGAL_ITERATIONS_Hnumber of iterations for convergencemeta.number;em.IR.HVARCHARprincipalGAL_ITERATIONS_Inumber of iterations for convergencemeta.number;em.opt.IVARCHARprincipalGAL_ITERATIONS_Jnumber of iterations for convergencemeta.number;em.IR.JVARCHARprincipalGAL_ITERATIONS_Knumber of iterations for convergencemeta.number;em.IR.KVARCHARprincipalGAL_ITERATIONS_Rnumber of iterations for convergencemeta.number;em.opt.RVARCHARprincipalGAL_ITERATIONS_Unumber of iterations for convergencemeta.number;em.opt.UVARCHARprincipalGAL_ITERATIONS_Ynumber of iterations for convergencemeta.number;em.IR.NIRVARCHARprincipalGAL_ITERATIONS_Znumber of iterations for convergencemeta.number;em.optVARCHARprincipalGAL_MAG_10RE_Gmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MAG_10RE_Hmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGAL_MAG_10RE_Imagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.IVARCHARprincipalGAL_MAG_10RE_Jmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGAL_MAG_10RE_Kmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGAL_MAG_10RE_Rmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.RVARCHARprincipalGAL_MAG_10RE_Umagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.UVARCHARprincipalGAL_MAG_10RE_Ymagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MAG_10RE_Zmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MAG_ERR_GGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.optVARCHARprincipalGAL_MAG_ERR_HGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_IGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_JGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_KGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_RGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_UGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_YGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em....VARCHARprincipalGAL_MAG_ERR_ZGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.optVARCHARprincipalGAL_MAG_Gmagnitude of Sersic modelmagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MAG_Hmagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGAL_MAG_Imagnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.IVARCHARprincipalGAL_MAG_Jmagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGAL_MAG_Kmagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGAL_MAG_Rmagnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.RVARCHARprincipalGAL_MAG_Umagnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.UVARCHARprincipalGAL_MAG_Ymagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MAG_Zmagnitude of Sersic modelmagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MU_0_Gcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_0_Hcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGAL_MU_0_Icentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.IVARCHARprincipalGAL_MU_0_Jcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGAL_MU_0_Kcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGAL_MU_0_Rcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.RVARCHARprincipalGAL_MU_0_Ucentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.UVARCHARprincipalGAL_MU_0_Ycentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MU_0_Zcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_AVG_Geffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_AVG_Heffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGAL_MU_E_AVG_Ieffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.IVARCHARprincipalGAL_MU_E_AVG_Jeffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGAL_MU_E_AVG_Keffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGAL_MU_E_AVG_Reffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.RVARCHARprincipalGAL_MU_E_AVG_Ueffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.UVARCHARprincipalGAL_MU_E_AVG_Yeffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MU_E_AVG_Zeffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_Geffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_Heffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGAL_MU_E_Ieffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.IVARCHARprincipalGAL_MU_E_Jeffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGAL_MU_E_Keffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGAL_MU_E_Reffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.RVARCHARprincipalGAL_MU_E_Ueffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.UVARCHARprincipalGAL_MU_E_Yeffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MU_E_Zeffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_PA_ERR_GGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_HGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_IGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_JGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_KGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_RGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_UGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_YGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_ERR_ZGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;e...VARCHARprincipalGAL_PA_Gposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.optVARCHARprincipalGAL_PA_Hposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.HVARCHARprincipalGAL_PA_Iposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.IVARCHARprincipalGAL_PA_Jposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.JVARCHARprincipalGAL_PA_Kposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.KVARCHARprincipalGAL_PA_Rposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.RVARCHARprincipalGAL_PA_Uposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.UVARCHARprincipalGAL_PA_Yposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.NIRVARCHARprincipalGAL_PA_Zposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.optVARCHARprincipalGAL_QFLAG_Gquality flag (see notes)meta.code.qual;em.optVARCHARprincipalGAL_QFLAG_Hquality flag (see notes)meta.code.qual;em.IR.HVARCHARprincipalGAL_QFLAG_Iquality flag (see notes)meta.code.qual;em.opt.IVARCHARprincipalGAL_QFLAG_Jquality flag (see notes)meta.code.qual;em.IR.JVARCHARprincipalGAL_QFLAG_Kquality flag (see notes)meta.code.qual;em.IR.KVARCHARprincipalGAL_QFLAG_Rquality flag (see notes)meta.code.qual;em.opt.RVARCHARprincipalGAL_QFLAG_Uquality flag (see notes)meta.code.qual;em.opt.UVARCHARprincipalGAL_QFLAG_Yquality flag (see notes)meta.code.qual;em.IR.NIRVARCHARprincipalGAL_QFLAG_Zquality flag (see notes)meta.code.qual;em.optVARCHARprincipalGAL_R90_Grad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_R90_Hrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGAL_R90_Irad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalGAL_R90_Jrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGAL_R90_Krad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGAL_R90_Rrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalGAL_R90_Urad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalGAL_R90_Yrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.NIRVARCHARprincipalGAL_R90_Zrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RA_GRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.optVARCHARprincipalGAL_RA_HRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.HVARCHARprincipalGAL_RA_IRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.IVARCHARprincipalGAL_RA_JRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.JVARCHARprincipalGAL_RA_KRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.KVARCHARprincipalGAL_RA_RRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.RVARCHARprincipalGAL_RA_URight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.UVARCHARprincipalGAL_RA_YRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.NIRVARCHARprincipalGAL_RA_ZRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.optVARCHARprincipalGAL_RESULT_GGALFIT run result (see notes)em.optVARCHARprincipalGAL_RESULT_HGALFIT run result (see notes)em.IR.HVARCHARprincipalGAL_RESULT_IGALFIT run result (see notes)em.opt.IVARCHARprincipalGAL_RESULT_JGALFIT run result (see notes)em.IR.JVARCHARprincipalGAL_RESULT_KGALFIT run result (see notes)em.IR.KVARCHARprincipalGAL_RESULT_RGALFIT run result (see notes)em.opt.RVARCHARprincipalGAL_RESULT_UGALFIT run result (see notes)em.opt.UVARCHARprincipalGAL_RESULT_YGALFIT run result (see notes)em.IR.NIRVARCHARprincipalGAL_RESULT_ZGALFIT run result (see notes)em.optVARCHARprincipalGAL_RE_C_Gcircularised effective radiusarcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RE_C_Hcircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGAL_RE_C_Icircularised effective radiusarcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalGAL_RE_C_Jcircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGAL_RE_C_Kcircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGAL_RE_C_Rcircularised effective radiusarcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalGAL_RE_C_Ucircularised effective radiusarcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalGAL_RE_C_Ycircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.NIRVARCHARprincipalGAL_RE_C_Zcircularised effective radiusarcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RE_ERR_GGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_HGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_IGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_JGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_KGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_RGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_UGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_YGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_ERR_ZGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled...VARCHARprincipalGAL_RE_Geffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RE_Heffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGAL_RE_Ieffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalGAL_RE_Jeffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGAL_RE_Keffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGAL_RE_Reffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalGAL_RE_Ueffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalGAL_RE_Yeffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.NIRVARCHARprincipalGAL_RE_Zeffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RUN_Gnumber of GALFIT runs requiredmeta.number;em.optVARCHARprincipalGAL_RUN_Hnumber of GALFIT runs requiredmeta.number;em.IR.HVARCHARprincipalGAL_RUN_Inumber of GALFIT runs requiredmeta.number;em.opt.IVARCHARprincipalGAL_RUN_Jnumber of GALFIT runs requiredmeta.number;em.IR.JVARCHARprincipalGAL_RUN_Knumber of GALFIT runs requiredmeta.number;em.IR.KVARCHARprincipalGAL_RUN_Rnumber of GALFIT runs requiredmeta.number;em.opt.RVARCHARprincipalGAL_RUN_Unumber of GALFIT runs requiredmeta.number;em.opt.UVARCHARprincipalGAL_RUN_Ynumber of GALFIT runs requiredmeta.number;em.IR.NIRVARCHARprincipalGAL_RUN_Znumber of GALFIT runs requiredmeta.number;em.optVARCHARprincipalGAL_SKY_ERR_Ginput sky errorcountsstat.error;phot.count;em.optVARCHARprincipalGAL_SKY_ERR_Hinput sky errorcountsstat.error;phot.count;em.IR.HVARCHARprincipalGAL_SKY_ERR_Iinput sky errorcountsstat.error;phot.count;em.opt.IVARCHARprincipalGAL_SKY_ERR_Jinput sky errorcountsstat.error;phot.count;em.IR.JVARCHARprincipalGAL_SKY_ERR_Kinput sky errorcountsstat.error;phot.count;em.IR.KVARCHARprincipalGAL_SKY_ERR_Rinput sky errorcountsstat.error;phot.count;em.opt.RVARCHARprincipalGAL_SKY_ERR_Uinput sky errorcountsstat.error;phot.count;em.opt.UVARCHARprincipalGAL_SKY_ERR_Yinput sky errorcountsstat.error;phot.count;em.IR.NIRVARCHARprincipalGAL_SKY_ERR_Zinput sky errorcountsstat.error;phot.count;em.optVARCHARprincipalGAL_SKY_Ginput skycountsinstr.skyLevel;phot.count;em.optVARCHARprincipalGAL_SKY_Hinput skycountsinstr.skyLevel;phot.count;em.IR.HVARCHARprincipalGAL_SKY_Iinput skycountsinstr.skyLevel;phot.count;em.opt.IVARCHARprincipalGAL_SKY_Jinput skycountsinstr.skyLevel;phot.count;em.IR.JVARCHARprincipalGAL_SKY_Kinput skycountsinstr.skyLevel;phot.count;em.IR.KVARCHARprincipalGAL_SKY_Rinput skycountsinstr.skyLevel;phot.count;em.opt.RVARCHARprincipalGAL_SKY_Uinput skycountsinstr.skyLevel;phot.count;em.opt.UVARCHARprincipalGAL_SKY_Yinput skycountsinstr.skyLevel;phot.count;em.IR.NIRVARCHARprincipalGAL_SKY_Zinput skycountsinstr.skyLevel;phot.count;em.optVARCHARprincipalGAL_TYPEWORD_Gtype of component modelledem.optVARCHARprincipalGAL_TYPEWORD_Htype of component modelledem.IR.HVARCHARprincipalGAL_TYPEWORD_Itype of component modelledem.opt.IVARCHARprincipalGAL_TYPEWORD_Jtype of component modelledem.IR.JVARCHARprincipalGAL_TYPEWORD_Ktype of component modelledem.IR.KVARCHARprincipalGAL_TYPEWORD_Rtype of component modelledem.opt.RVARCHARprincipalGAL_TYPEWORD_Utype of component modelledem.opt.UVARCHARprincipalGAL_TYPEWORD_Ytype of component modelledem.IR.NIRVARCHARprincipalGAL_TYPEWORD_Ztype of component modelledem.optVARCHARprincipalGAL_TYPE_Gtype of component modelled (see notes)em.optVARCHARprincipalGAL_TYPE_Htype of component modelled (see notes)em.IR.HVARCHARprincipalGAL_TYPE_Itype of component modelled (see notes)em.opt.IVARCHARprincipalGAL_TYPE_Jtype of component modelled (see notes)em.IR.JVARCHARprincipalGAL_TYPE_Ktype of component modelled (see notes)em.IR.KVARCHARprincipalGAL_TYPE_Rtype of component modelled (see notes)em.opt.RVARCHARprincipalGAL_TYPE_Utype of component modelled (see notes)em.opt.UVARCHARprincipalGAL_TYPE_Ytype of component modelled (see notes)em.IR.NIRVARCHARprincipalGAL_TYPE_Ztype of component modelled (see notes)em.optVARCHARprincipalGAL_XCEN_ERR_GGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_HGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_IGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_JGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_KGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_RGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_UGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_YGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_ERR_ZGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.model...VARCHARprincipalGAL_XCEN_Gpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.optVARCHARprincipalGAL_XCEN_Hpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.HVARCHARprincipalGAL_XCEN_Ipixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.IVARCHARprincipalGAL_XCEN_Jpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.JVARCHARprincipalGAL_XCEN_Kpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.KVARCHARprincipalGAL_XCEN_Rpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.RVARCHARprincipalGAL_XCEN_Upixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.UVARCHARprincipalGAL_XCEN_Ypixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.NIRVARCHARprincipalGAL_XCEN_Zpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.optVARCHARprincipalGAL_YCEN_ERR_GGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_HGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_IGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_JGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_KGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_RGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_UGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_YGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_ERR_ZGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.model...VARCHARprincipalGAL_YCEN_Gpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.optVARCHARprincipalGAL_YCEN_Hpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.HVARCHARprincipalGAL_YCEN_Ipixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.IVARCHARprincipalGAL_YCEN_Jpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.JVARCHARprincipalGAL_YCEN_Kpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.KVARCHARprincipalGAL_YCEN_Rpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.RVARCHARprincipalGAL_YCEN_Upixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.UVARCHARprincipalGAL_YCEN_Ypixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.NIRVARCHARprincipalGAL_YCEN_Zpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.optVARCHARprincipalOBJNAMESIGMA Object name (see notes)meta.idVARCHARprincipalPSF_CHI2_GPSFEx PSF reduced Chi^2stat.fit.goodness;em.optVARCHARprincipalPSF_CHI2_HPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.HVARCHARprincipalPSF_CHI2_IPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.IVARCHARprincipalPSF_CHI2_JPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.JVARCHARprincipalPSF_CHI2_KPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.KVARCHARprincipalPSF_CHI2_RPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.RVARCHARprincipalPSF_CHI2_UPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.UVARCHARprincipalPSF_CHI2_YPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.NIRVARCHARprincipalPSF_CHI2_ZPSFEx PSF reduced Chi^2stat.fit.goodness;em.optVARCHARprincipalPSF_FWHM_GPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.optVARCHARprincipalPSF_FWHM_HPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.HVARCHARprincipalPSF_FWHM_IPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.IVARCHARprincipalPSF_FWHM_JPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.JVARCHARprincipalPSF_FWHM_KPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.KVARCHARprincipalPSF_FWHM_RPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.RVARCHARprincipalPSF_FWHM_UPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.UVARCHARprincipalPSF_FWHM_YPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.NIRVARCHARprincipalPSF_FWHM_ZPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.optVARCHARprincipalPSF_NUM_GPSFEx number of stars usedmeta.number;em.optVARCHARprincipalPSF_NUM_HPSFEx number of stars usedmeta.number;em.IR.HVARCHARprincipalPSF_NUM_IPSFEx number of stars usedmeta.number;em.opt.IVARCHARprincipalPSF_NUM_JPSFEx number of stars usedmeta.number;em.IR.JVARCHARprincipalPSF_NUM_KPSFEx number of stars usedmeta.number;em.IR.KVARCHARprincipalPSF_NUM_RPSFEx number of stars usedmeta.number;em.opt.RVARCHARprincipalPSF_NUM_UPSFEx number of stars usedmeta.number;em.opt.UVARCHARprincipalPSF_NUM_YPSFEx number of stars usedmeta.number;em.IR.NIRVARCHARprincipalPSF_NUM_ZPSFEx number of stars usedmeta.number;em.optVARCHARprincipalPSF_RUN_GPSFEx runs required for satisfactory PSFmeta.number;em.optVARCHARprincipalPSF_RUN_HPSFEx runs required for satisfactory PSFmeta.number;em.IR.HVARCHARprincipalPSF_RUN_IPSFEx runs required for satisfactory PSFmeta.number;em.opt.IVARCHARprincipalPSF_RUN_JPSFEx runs required for satisfactory PSFmeta.number;em.IR.JVARCHARprincipalPSF_RUN_KPSFEx runs required for satisfactory PSFmeta.number;em.IR.KVARCHARprincipalPSF_RUN_RPSFEx runs required for satisfactory PSFmeta.number;em.opt.RVARCHARprincipalPSF_RUN_UPSFEx runs required for satisfactory PSFmeta.number;em.opt.UVARCHARprincipalPSF_RUN_YPSFEx runs required for satisfactory PSFmeta.number;em.IR.NIRVARCHARprincipalPSF_RUN_ZPSFEx runs required for satisfactory PSFmeta.number;em.optVARCHARprincipalSEX_A_GSEx semi-major axisarcsecem.optVARCHARprincipalSEX_A_HSEx semi-major axisarcsecem.IR.HVARCHARprincipalSEX_A_ISEx semi-major axisarcsecem.opt.IVARCHARprincipalSEX_A_JSEx semi-major axisarcsecem.IR.JVARCHARprincipalSEX_A_KSEx semi-major axisarcsecem.IR.KVARCHARprincipalSEX_A_RSEx semi-major axisarcsecem.opt.RVARCHARprincipalSEX_A_USEx semi-major axisarcsecem.opt.UVARCHARprincipalSEX_A_YSEx semi-major axisarcsecem.IR.NIRVARCHARprincipalSEX_A_ZSEx semi-major axisarcsecem.optVARCHARprincipalSEX_B_GSEx semi-minor axisarcsecem.optVARCHARprincipalSEX_B_HSEx semi-minor axisarcsecem.IR.HVARCHARprincipalSEX_B_ISEx semi-minor axisarcsecem.opt.IVARCHARprincipalSEX_B_JSEx semi-minor axisarcsecem.IR.JVARCHARprincipalSEX_B_KSEx semi-minor axisarcsecem.IR.KVARCHARprincipalSEX_B_RSEx semi-minor axisarcsecem.opt.RVARCHARprincipalSEX_B_USEx semi-minor axisarcsecem.opt.UVARCHARprincipalSEX_B_YSEx semi-minor axisarcsecem.IR.NIRVARCHARprincipalSEX_B_ZSEx semi-minor axisarcsecem.optVARCHARprincipalSEX_CLASS_STAR_GSEx star class (1=star-like)src.class.starGalaxy;em.optVARCHARprincipalSEX_CLASS_STAR_HSEx star class (1=star-like)src.class.starGalaxy;em.IR.HVARCHARprincipalSEX_CLASS_STAR_ISEx star class (1=star-like)src.class.starGalaxy;em.opt.IVARCHARprincipalSEX_CLASS_STAR_JSEx star class (1=star-like)src.class.starGalaxy;em.IR.JVARCHARprincipalSEX_CLASS_STAR_KSEx star class (1=star-like)src.class.starGalaxy;em.IR.KVARCHARprincipalSEX_CLASS_STAR_RSEx star class (1=star-like)src.class.starGalaxy;em.opt.RVARCHARprincipalSEX_CLASS_STAR_USEx star class (1=star-like)src.class.starGalaxy;em.opt.UVARCHARprincipalSEX_CLASS_STAR_YSEx star class (1=star-like)src.class.starGalaxy;em.IR.NIRVARCHARprincipalSEX_CLASS_STAR_ZSEx star class (1=star-like)src.class.starGalaxy;em.optVARCHARprincipalSEX_ELLIP_GSEx Ellipticity (1-(b/a))src.ellipticity;em.optVARCHARprincipalSEX_ELLIP_HSEx Ellipticity (1-(b/a))src.ellipticity;em.IR.HVARCHARprincipalSEX_ELLIP_ISEx Ellipticity (1-(b/a))src.ellipticity;em.opt.IVARCHARprincipalSEX_ELLIP_JSEx Ellipticity (1-(b/a))src.ellipticity;em.IR.JVARCHARprincipalSEX_ELLIP_KSEx Ellipticity (1-(b/a))src.ellipticity;em.IR.KVARCHARprincipalSEX_ELLIP_RSEx Ellipticity (1-(b/a))src.ellipticity;em.opt.RVARCHARprincipalSEX_ELLIP_USEx Ellipticity (1-(b/a))src.ellipticity;em.opt.UVARCHARprincipalSEX_ELLIP_YSEx Ellipticity (1-(b/a))src.ellipticity;em.IR.NIRVARCHARprincipalSEX_ELLIP_ZSEx Ellipticity (1-(b/a))src.ellipticity;em.optVARCHARprincipalSEX_FLUXRAD_GSEx half-light rad (circularised)arcsecphys.angSize;em.optVARCHARprincipalSEX_FLUXRAD_HSEx half-light rad (circularised)arcsecphys.angSize;em.IR.HVARCHARprincipalSEX_FLUXRAD_ISEx half-light rad (circularised)arcsecphys.angSize;em.opt.IVARCHARprincipalSEX_FLUXRAD_JSEx half-light rad (circularised)arcsecphys.angSize;em.IR.JVARCHARprincipalSEX_FLUXRAD_KSEx half-light rad (circularised)arcsecphys.angSize;em.IR.KVARCHARprincipalSEX_FLUXRAD_RSEx half-light rad (circularised)arcsecphys.angSize;em.opt.RVARCHARprincipalSEX_FLUXRAD_USEx half-light rad (circularised)arcsecphys.angSize;em.opt.UVARCHARprincipalSEX_FLUXRAD_YSEx half-light rad (circularised)arcsecphys.angSize;em.IR.NIRVARCHARprincipalSEX_FLUXRAD_ZSEx half-light rad (circularised)arcsecphys.angSize;em.optVARCHARprincipalSEX_INDEX_GSEx expected Sersic indexstat.fit.param;em.optVARCHARprincipalSEX_INDEX_HSEx expected Sersic indexstat.fit.param;em.IR.HVARCHARprincipalSEX_INDEX_ISEx expected Sersic indexstat.fit.param;em.opt.IVARCHARprincipalSEX_INDEX_JSEx expected Sersic indexstat.fit.param;em.IR.JVARCHARprincipalSEX_INDEX_KSEx expected Sersic indexstat.fit.param;em.IR.KVARCHARprincipalSEX_INDEX_RSEx expected Sersic indexstat.fit.param;em.opt.RVARCHARprincipalSEX_INDEX_USEx expected Sersic indexstat.fit.param;em.opt.UVARCHARprincipalSEX_INDEX_YSEx expected Sersic indexstat.fit.param;em.IR.NIRVARCHARprincipalSEX_INDEX_ZSEx expected Sersic indexstat.fit.param;em.optVARCHARprincipalSEX_KRONRAD_GSEx Kron radius (in units of A or B)AorBphys.angSize;em.optVARCHARprincipalSEX_KRONRAD_HSEx Kron radius (in units of A or B)AorBphys.angSize;em.IR.HVARCHARprincipalSEX_KRONRAD_ISEx Kron radius (in units of A or B)AorBphys.angSize;em.opt.IVARCHARprincipalSEX_KRONRAD_JSEx Kron radius (in units of A or B)AorBphys.angSize;em.IR.JVARCHARprincipalSEX_KRONRAD_KSEx Kron radius (in units of A or B)AorBphys.angSize;em.IR.KVARCHARprincipalSEX_KRONRAD_RSEx Kron radius (in units of A or B)AorBphys.angSize;em.opt.RVARCHARprincipalSEX_KRONRAD_USEx Kron radius (in units of A or B)AorBphys.angSize;em.opt.UVARCHARprincipalSEX_KRONRAD_YSEx Kron radius (in units of A or B)AorBphys.angSize;em.IR.NIRVARCHARprincipalSEX_KRONRAD_ZSEx Kron radius (in units of A or B)AorBphys.angSize;em.optVARCHARprincipalSEX_MAG_GSEx AUTO magnitude (Kron)magphot.mag;em.optVARCHARprincipalSEX_MAG_HSEx AUTO magnitude (Kron)magphot.mag;em.IR.HVARCHARprincipalSEX_MAG_ISEx AUTO magnitude (Kron)magphot.mag;em.opt.IVARCHARprincipalSEX_MAG_JSEx AUTO magnitude (Kron)magphot.mag;em.IR.JVARCHARprincipalSEX_MAG_KSEx AUTO magnitude (Kron)magphot.mag;em.IR.KVARCHARprincipalSEX_MAG_RSEx AUTO magnitude (Kron)magphot.mag;em.opt.RVARCHARprincipalSEX_MAG_USEx AUTO magnitude (Kron)magphot.mag;em.opt.UVARCHARprincipalSEX_MAG_YSEx AUTO magnitude (Kron)magphot.mag;em.IR.NIRVARCHARprincipalSEX_MAG_ZSEx AUTO magnitude (Kron)magphot.mag;em.optVARCHARprincipalSEX_PA_GSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.optVARCHARprincipalSEX_PA_HSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.IR.HVARCHARprincipalSEX_PA_ISEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.opt.IVARCHARprincipalSEX_PA_JSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.IR.JVARCHARprincipalSEX_PA_KSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.IR.KVARCHARprincipalSEX_PA_RSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.opt.RVARCHARprincipalSEX_PA_USEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.opt.UVARCHARprincipalSEX_PA_YSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.IR.NIRVARCHARprincipalSEX_PA_ZSEx Position Angle (x+, CCW) (see notes)degpos.posAng;em.optVARCHARprincipalSEX_PIXSEP_GSEx pixel separation from expected loc.pixelpos.angDistance;em.optVARCHARprincipalSEX_PIXSEP_HSEx pixel separation from expected loc.pixelpos.angDistance;em.IR.HVARCHARprincipalSEX_PIXSEP_ISEx pixel separation from expected loc.pixelpos.angDistance;em.opt.IVARCHARprincipalSEX_PIXSEP_JSEx pixel separation from expected loc.pixelpos.angDistance;em.IR.JVARCHARprincipalSEX_PIXSEP_KSEx pixel separation from expected loc.pixelpos.angDistance;em.IR.KVARCHARprincipalSEX_PIXSEP_RSEx pixel separation from expected loc.pixelpos.angDistance;em.opt.RVARCHARprincipalSEX_PIXSEP_USEx pixel separation from expected loc.pixelpos.angDistance;em.opt.UVARCHARprincipalSEX_PIXSEP_YSEx pixel separation from expected loc.pixelpos.angDistance;em.IR.NIRVARCHARprincipalSEX_PIXSEP_ZSEx pixel separation from expected loc.pixelpos.angDistance;em.optVARCHARprincipalSEX_RE_GSEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.optVARCHARprincipalSEX_RE_HSEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.IR.HVARCHARprincipalSEX_RE_ISEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.opt.IVARCHARprincipalSEX_RE_JSEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.IR.JVARCHARprincipalSEX_RE_KSEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.IR.KVARCHARprincipalSEX_RE_RSEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.opt.RVARCHARprincipalSEX_RE_USEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.opt.UVARCHARprincipalSEX_RE_YSEx half-light rad (semi-major,PSF corr)arcsecphys.angSize;em.IR.NIRVARCHARprincipalSEX_RE_ZSEx half-light rad (semi-major,PSF corr)rcsecphys.angSize;em.optVARCHARprincipalSEX_SKY_ERR_GSEx background sky error on meancountsstat.error;phot.count;em.optVARCHARprincipalSEX_SKY_ERR_HSEx background sky error on meancountsstat.error;phot.count;em.IR.HVARCHARprincipalSEX_SKY_ERR_ISEx background sky error on meancountsstat.error;phot.count;em.opt.IVARCHARprincipalSEX_SKY_ERR_JSEx background sky error on meancountsstat.error;phot.count;em.IR.JVARCHARprincipalSEX_SKY_ERR_KSEx background sky error on meancountsstat.error;phot.count;em.IR.KVARCHARprincipalSEX_SKY_ERR_RSEx background sky error on meancountsstat.error;phot.count;em.opt.RVARCHARprincipalSEX_SKY_ERR_USEx background sky error on meancountsstat.error;phot.count;em.opt.UVARCHARprincipalSEX_SKY_ERR_YSEx background sky error on meancountsstat.error;phot.count;em.IR.NIRVARCHARprincipalSEX_SKY_ERR_ZSEx background sky error on meancountsstat.error;phot.count;em.optVARCHARprincipalSEX_SKY_GSEx background skycountsinstr.skyLevel;phot.count;em.optVARCHARprincipalSEX_SKY_HSEx background skycountsinstr.skyLevel;phot.count;em.IR.HVARCHARprincipalSEX_SKY_ISEx background skycountsinstr.skyLevel;phot.count;em.opt.IVARCHARprincipalSEX_SKY_JSEx background skycountsinstr.skyLevel;phot.count;em.IR.JVARCHARprincipalSEX_SKY_KSEx background skycountsinstr.skyLevel;phot.count;em.IR.KVARCHARprincipalSEX_SKY_RSEx background skycountsinstr.skyLevel;phot.count;em.opt.RVARCHARprincipalSEX_SKY_RMS_HSEx background sky RMScountsphot.count;em.IR.HVARCHARprincipalSEX_SKY_RMS_ISEx background sky RMScountsphot.count;em.opt.IVARCHARprincipalSEX_SKY_RMS_JSEx background sky RMScountsphot.count;em.IR.JVARCHARprincipalSEX_SKY_RMS_KSEx background sky RMScountsphot.count;em.IR.KVARCHARprincipalSEX_SKY_RMS_RSEx background sky RMScountsphot.count;em.opt.RVARCHARprincipalSEX_SKY_RMS_USEx background sky RMScountsphot.count;em.opt.UVARCHARprincipalSEX_SKY_RMS_YSEx background sky RMScountsphot.count;em.IR.NIRVARCHARprincipalSEX_SKY_RMS_ZSEx background sky RMScountsphot.count;em.optVARCHARprincipalSEX_SKY_USEx background skycountsinstr.skyLevel;phot.count;em.opt.UVARCHARprincipalSEX_SKY_YSEx background skycountsinstr.skyLevel;phot.count;em.IR.NIRVARCHARprincipalSEX_SKY_ZSEx background skycountsinstr.skyLevel;phot.count;em.optVARCHARprincipalSEX_XCEN_GSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.optVARCHARprincipalSEX_XCEN_HSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.IR.HVARCHARprincipalSEX_XCEN_ISEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.opt.IVARCHARprincipalSEX_XCEN_JSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.IR.JVARCHARprincipalSEX_XCEN_KSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.IR.KVARCHARprincipalSEX_XCEN_RSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.opt.RVARCHARprincipalSEX_XCEN_USEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.opt.UVARCHARprincipalSEX_XCEN_YSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.IR.NIRVARCHARprincipalSEX_XCEN_ZSEx pixel pos. of object in cutout (x)pixelpos.cartesian.x;em.optVARCHARprincipalSEX_YCEN_GSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.optVARCHARprincipalSEX_YCEN_HSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.IR.HVARCHARprincipalSEX_YCEN_ISEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.opt.IVARCHARprincipalSEX_YCEN_JSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.IR.JVARCHARprincipalSEX_YCEN_KSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.IR.KVARCHARprincipalSEX_YCEN_RSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.opt.RVARCHARprincipalSEX_YCEN_USEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.opt.UVARCHARprincipalSEX_YCEN_YSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.IR.NIRVARCHARprincipalSEX_YCEN_ZSEx pixel pos. of object in cutout (y)pixelpos.cartesian.y;em.optVARCHARprincipalSIGMA_INDEXSIGMA Object ID (see notes)meta.idVARCHARprincipalSIG_TIME_Gtime taken to complete the fitstime.processing;em.optVARCHARprincipalSIG_TIME_Htime taken to complete the fitstime.processing;em.IR.HVARCHARprincipalSIG_TIME_Itime taken to complete the fitstime.processing;em.opt.IVARCHARprincipalSIG_TIME_Jtime taken to complete the fitstime.processing;em.IR.JVARCHARprincipalSIG_TIME_Ktime taken to complete the fitstime.processing;em.IR.KVARCHARprincipalSIG_TIME_Rtime taken to complete the fitstime.processing;em.opt.RVARCHARprincipalSIG_TIME_Utime taken to complete the fitstime.processing;em.opt.UVARCHARprincipalSIG_TIME_Ytime taken to complete the fitstime.processing;em.IR.NIRVARCHARprincipalSIG_TIME_Ztime taken to complete the fitstime.processing;em.optVARCHARprincipalURLURL of the object`s data dirmeta.ref.url;meta.fileVARCHARprincipalURL_KURL of K-band png filemeta.ref.url;meta.fileVARCHARprincipalURL_RURL of r-band png filemeta.ref.url;meta.fileVARCHARprincipalSEX_SKY_RMS_GSEx background sky RMScountsphot.count;em.optVARCHARprincipalgama_dr2.SersicCatThis catalogue contains the most useful subset of the output of the SersicPhotometry DMU, using SIGMA v0.9-0 (Structural Investigation of Galaxies via Model Analysis) to generate a single-Sersic fit to every GAMA DR2 object. This table is an exact subset of the table SersicCatAll.CATAIDGAMA Object IDmeta.idVARCHARprincipalFILENAMEFull path to object`s data directorymeta.id;meta.fileVARCHARprincipalGAL_CHI2_Greduced Chi^2 of output modelstat.fit.goodness;em.optVARCHARprincipalGAL_CHI2_Hreduced Chi^2 of output modelstat.fit.goodness;em.IR.HVARCHARprincipalGAL_CHI2_Ireduced Chi^2 of output modelstat.fit.goodness;em.opt.IVARCHARprincipalGAL_CHI2_Jreduced Chi^2 of output modelstat.fit.goodness;em.IR.JVARCHARprincipalGAL_CHI2_Kreduced Chi^2 of output modelstat.fit.goodness;em.IR.KVARCHARprincipalGAL_CHI2_Rreduced Chi^2 of output modelstat.fit.goodness;em.opt.RVARCHARprincipalGAL_CHI2_Ureduced Chi^2 of output modelstat.fit.goodness;em.opt.UVARCHARprincipalGAL_CHI2_Yreduced Chi^2 of output modelstat.fit.goodness;em.IR.NIRVARCHARprincipalGAL_CHI2_Zreduced Chi^2 of output modelstat.fit.goodness;em.optVARCHARprincipalGAL_DEC_GDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.optVARCHARprincipalGAL_DEC_HDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.HVARCHARprincipalGAL_DEC_IDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.IVARCHARprincipalGAL_DEC_JDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.JVARCHARprincipalGAL_DEC_KDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.KVARCHARprincipalGAL_DEC_RDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.RVARCHARprincipalGAL_DEC_UDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.UVARCHARprincipalGAL_DEC_YDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.NIRVARCHARprincipalGAL_DEC_ZDeclination as determined by GALFITdegpos.eq.dec;meta.modelled;em.optVARCHARprincipalGAL_ELLIP_Gellipticity (1-(b/a))src.ellipticity;meta.modelled;em.optVARCHARprincipalGAL_ELLIP_Hellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.HVARCHARprincipalGAL_ELLIP_Iellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.IVARCHARprincipalGAL_ELLIP_Jellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.JVARCHARprincipalGAL_ELLIP_Kellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.KVARCHARprincipalGAL_ELLIP_Rellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.RVARCHARprincipalGAL_ELLIP_Uellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.UVARCHARprincipalGAL_ELLIP_Yellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.NIRVARCHARprincipalGAL_ELLIP_Zellipticity (1-(b/a))src.ellipticity;meta.modelled;em.optVARCHARprincipalGAL_INDEX_GSersic indexstat.fit.param;meta.modelled;em.optVARCHARprincipalGAL_INDEX_HSersic indexstat.fit.param;meta.modelled;em.IR.HVARCHARprincipalGAL_INDEX_ISersic indexstat.fit.param;meta.modelled;em.opt.IVARCHARprincipalGAL_INDEX_JSersic indexstat.fit.param;meta.modelled;em.IR.JVARCHARprincipalGAL_INDEX_KSersic indexstat.fit.param;meta.modelled;em.IR.KVARCHARprincipalGAL_INDEX_RSersic indexstat.fit.param;meta.modelled;em.opt.RVARCHARprincipalGAL_INDEX_USersic indexstat.fit.param;meta.modelled;em.opt.UVARCHARprincipalGAL_INDEX_YSersic indexstat.fit.param;meta.modelled;em.IR.NIRVARCHARprincipalGAL_INDEX_ZSersic indexstat.fit.param;meta.modelled;em.optVARCHARprincipalGAL_MAG_10RE_Gmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MAG_10RE_Hmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGAL_MAG_10RE_Imagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.IVARCHARprincipalGAL_MAG_10RE_Jmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGAL_MAG_10RE_Kmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGAL_MAG_10RE_Rmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.RVARCHARprincipalGAL_MAG_10RE_Umagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.UVARCHARprincipalGAL_MAG_10RE_Ymagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MAG_10RE_Zmagnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MAG_Gmagnitude of Sersic modelmagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MAG_Hmagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGAL_MAG_Imagnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.IVARCHARprincipalGAL_MAG_Jmagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGAL_MAG_Kmagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGAL_MAG_Rmagnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.RVARCHARprincipalGAL_MAG_Umagnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.UVARCHARprincipalGAL_MAG_Ymagnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MAG_Zmagnitude of Sersic modelmagphot.mag;meta.modelled;em.optVARCHARprincipalGAL_MU_0_Gcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_0_Hcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGAL_MU_0_Icentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.IVARCHARprincipalGAL_MU_0_Jcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGAL_MU_0_Kcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGAL_MU_0_Rcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.RVARCHARprincipalGAL_MU_0_Ucentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.UVARCHARprincipalGAL_MU_0_Ycentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MU_0_Zcentral surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_AVG_Geffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_AVG_Heffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGAL_MU_E_AVG_Ieffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.IVARCHARprincipalGAL_MU_E_AVG_Jeffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGAL_MU_E_AVG_Keffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGAL_MU_E_AVG_Reffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.RVARCHARprincipalGAL_MU_E_AVG_Ueffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.UVARCHARprincipalGAL_MU_E_AVG_Yeffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MU_E_AVG_Zeffective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_Geffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_MU_E_Heffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGAL_MU_E_Ieffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.IVARCHARprincipalGAL_MU_E_Jeffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGAL_MU_E_Keffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGAL_MU_E_Reffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.RVARCHARprincipalGAL_MU_E_Ueffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.UVARCHARprincipalGAL_MU_E_Yeffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.NIRVARCHARprincipalGAL_MU_E_Zeffective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.optVARCHARprincipalGAL_PA_Gposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.optVARCHARprincipalGAL_PA_Hposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.HVARCHARprincipalGAL_PA_Iposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.IVARCHARprincipalGAL_PA_Jposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.JVARCHARprincipalGAL_PA_Kposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.KVARCHARprincipalGAL_PA_Rposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.RVARCHARprincipalGAL_PA_Uposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.UVARCHARprincipalGAL_PA_Yposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.NIRVARCHARprincipalGAL_PA_Zposition angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.optVARCHARprincipalGAL_R90_Grad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_R90_Hrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGAL_R90_Irad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalGAL_R90_Jrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGAL_R90_Krad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGAL_R90_Rrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalGAL_R90_Urad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalGAL_R90_Yrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.IR.NIRVARCHARprincipalGAL_R90_Zrad containing 90% of total light (sma)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RA_GRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.optVARCHARprincipalGAL_RA_HRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.HVARCHARprincipalGAL_RA_IRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.IVARCHARprincipalGAL_RA_JRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.JVARCHARprincipalGAL_RA_KRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.KVARCHARprincipalGAL_RA_RRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.RVARCHARprincipalGAL_RA_URight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.UVARCHARprincipalGAL_RA_YRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.NIRVARCHARprincipalGAL_RA_ZRight Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.optVARCHARprincipalGAL_RE_C_Gcircularised effective radiusarcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RE_C_Hcircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGAL_RE_C_Icircularised effective radiusarcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalGAL_RE_C_Jcircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGAL_RE_C_Kcircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGAL_RE_C_Rcircularised effective radiusarcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalGAL_RE_C_Ucircularised effective radiusarcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalGAL_RE_C_Ycircularised effective radiusarcsecphys.angSize;meta.modelled;em.IR.NIRVARCHARprincipalGAL_RE_C_Zcircularised effective radiusarcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RE_Geffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_RE_Heffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGAL_RE_Ieffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalGAL_RE_Jeffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGAL_RE_Keffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGAL_RE_Reffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalGAL_RE_Ueffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalGAL_RE_Yeffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.IR.NIRVARCHARprincipalGAL_RE_Zeffective radius (hl rad) (semi-major)arcsecphys.angSize;meta.modelled;em.optVARCHARprincipalGAL_YCEN_Upixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.UVARCHARprincipalGAL_YCEN_Ypixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.NIRVARCHARprincipalGAL_YCEN_Zpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.optVARCHARprincipalPSF_FWHM_GPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.optVARCHARprincipalPSF_FWHM_HPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.HVARCHARprincipalPSF_FWHM_IPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.IVARCHARprincipalPSF_FWHM_JPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.JVARCHARprincipalPSF_FWHM_KPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.KVARCHARprincipalPSF_FWHM_RPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.RVARCHARprincipalPSF_FWHM_UPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.UVARCHARprincipalPSF_FWHM_YPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.NIRVARCHARprincipalPSF_FWHM_ZPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.optVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalSIGMA_INDEXSIGMA Object ID (see notes)meta.idVARCHARprincipalURLURL of the object`s data dirmeta.ref.url;meta.fileVARCHARprincipalURL_KURL of K-band png filemeta.ref.url;meta.fileVARCHARprincipalURL_RURL of r-band png filemeta.ref.url;meta.fileVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalGAL_XCEN_Gpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.optVARCHARprincipalGAL_XCEN_Hpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.HVARCHARprincipalGAL_XCEN_Ipixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.IVARCHARprincipalGAL_XCEN_Jpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.JVARCHARprincipalGAL_XCEN_Kpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.KVARCHARprincipalGAL_XCEN_Rpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.RVARCHARprincipalGAL_XCEN_Upixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.UVARCHARprincipalGAL_XCEN_Ypixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.NIRVARCHARprincipalGAL_XCEN_Zpixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.optVARCHARprincipalGAL_YCEN_Gpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.optVARCHARprincipalGAL_YCEN_Hpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.HVARCHARprincipalGAL_YCEN_Ipixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.IVARCHARprincipalGAL_YCEN_Jpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.JVARCHARprincipalGAL_YCEN_Kpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.KVARCHARprincipalGAL_YCEN_Rpixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.RVARCHARprincipalOBJNAMESIGMA Object name (see notes)meta.idVARCHARprincipalgama_dr2.GalexObsInfoThis catalogue provides basic GALEX observational information, i.e. exposure times, background levels and detection limits, for all GAMA DR2 objects.BKGRND_FLUX_FUVFUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.100-200nm;src.netVARCHARprincipalBKGRND_FLUX_NUVNUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.200-300nm;src.netVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalFUVFLUXLIMIT10S/N=10 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalFUVFLUXLIMIT2p5S/N=2.5 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalFUVFLUXLIMIT5S/N=5 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalFUVMAGLIMIT10S/N=10 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalFUVMAGLIMIT2p5S/N=2.5 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalFUVMAGLIMIT5S/N=5 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalNUVFLUXLIMIT10S/N=10 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalNUVFLUXLIMIT2p5S/N=2.5 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalNUVFLUXLIMIT5S/N=5 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalNUVMAGLIMIT10S/N=10 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalNUVMAGLIMIT2p5S/N=2.5 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalNUVMAGLIMIT5S/N=5 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalgama_dr2.GalexSimpleMatchThis catalogue contains the result of a simple nearest neighbour match between InputCatA and GalexPhot, listing only objects included in DR2. GAMA DR2 objects without a GALEX nearest neighbour within a distance of 4 arcsec are considered unmatched and are not included in this catalogue.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalFUVMATCHFlag indicating whether matched GALEX source has FUV flux with S/N >=2.5 (-1=no FUV data)meta.code;em.UV.100-200nmVARCHARprincipalGGOIDGlobal Object ID of nearest neighbour GALEX objectmeta.idVARCHARprincipalGNEIGHBOR_DISTString list of distances to all GALEX sources within 20 arcsecVARCHARprincipalGNEIGHBOR_NAMEString list of names of all GALEX sources within 20 arcsecVARCHARprincipalMANY2ONENumber of GAMA objects the GALEX object is matched tometa.numberVARCHARprincipalNMATCH4Number of GALEX objects found within 4 arcsec of GAMA objectmeta.numberVARCHARprincipalNN_DISTDistance between GAMA object and nearest neighbour GALEX objectarcsecpos.angDistanceVARCHARprincipalOBJIDSDSS objid of GAMA objectmeta.idVARCHARprincipalgama_dr2.GalexPhotThis catalogue provides GALEX NUV and FUV photometry for primary sources with S/N_NUV >= 2.5 in the GAMA I survey regions. This photometry was derived using the GALEX SExtractor-based pipeline.ARTIFACT_FUVFUV artifact flag (see notes)meta.code;em.UV.100-200nmVARCHARprincipalARTIFACT_NUVNUV artifact flag (see notes)meta.code;em.UV.200-300nmVARCHARprincipalBKGRND_FLUX_FUVFUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.100-200nm;src.netVARCHARprincipalBKGRND_FLUX_NUVNUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.200-300nm;src.netVARCHARprincipalBKGRND_MAG_FUVFUV sky background surface brightnessmag/arcsec^2phot.mag;em.UV.100-200nm;src.netVARCHARprincipalBKGRND_MAG_NUVNUV sky background surface brightnessmag/arcsec^2phot.mag;em.UV.200-300nm;src.netVARCHARprincipalCLASS_STARNUV Sextractor star/galaxy classifier outputmeta.code;em.UV.200-300nmVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEXPTIME_FUVFUV exposure time of tilesobs.exposure;em.UV.100-200nmVARCHARprincipalEXPTIME_NUVNUV exposure time of tilesobs.exposure;em.UV.200-300nmVARCHARprincipalFLAGS_FUVFUV Sextraxtor extraction flagsmeta.code;em.UV.100-200nmVARCHARprincipalFLAGS_NUVNUV Sextraxtor extraction flagsmeta.code;em.UV.200-300nmVARCHARprincipalFLUX20_RADIUS_FUVFUV 20 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX20_RADIUS_NUVNUV 20 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX50_RADIUS_FUVFUV 50 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX50_RADIUS_NUVNUV 50 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX80_RADIUS_FUVFUV 80 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX80_RADIUS_NUVNUV 80 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX90_RADIUS_FUVFUV 90 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX90_RADIUS_NUVNUV 90 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX95_RADIUS_FUVFUV 95 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX95_RADIUS_NUVNUV 95 percent fraction-of-light radiusarcsecVARCHARprincipalFLUXERR_D12p0_FUVFUV flux error in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D12p0_NUVNUV flux error in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D18p0_FUVFUV flux error in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D18p0_NUVNUV flux error in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D25p5_FUVFUV flux error in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D25p5_NUVNUV flux error in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D34p5_FUVFUV flux error in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D34p5_NUVNUV flux error in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D3p0_FUVFUV flux error in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D3p0_NUVNUV flux error in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D4p5_FUVFUV flux error in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D4p5_NUVNUV flux error in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D7p5_FUVFUV flux error in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D7p5_NUVNUV flux error in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_FUVFUV flux error using NUV aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_NUVNUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUX_D12p0_FUVFUV flux in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D12p0_NUVNUV flux in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D18p0_FUVFUV flux in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D18p0_NUVNUV flux in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D25p5_FUVFUV flux in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D25p5_NUVNUV flux in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D34p5_FUVFUV flux in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D34p5_NUVNUV flux in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D3p0_FUVFUV flux in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D3p0_NUVNUV flux in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D4p5_FUVFUV flux in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D4p5_NUVNUV flux in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D7p5_FUVFUV flux in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D7p5_NUVNUV flux in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_FUVFUV calibrated flux using NUV aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_MAX_FUVFUV peak flux above backgroundmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_MAX_NUVNUV peak flux above backgroundmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_NUVNUV calibrated fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFOV_RADIUSDistance of object from centre of FoVdegpos.angDistanceVARCHARprincipalFWHM_FUVFUV FWHM assuming a gaussian corearcsecphys.size;em.UV.100-200nmVARCHARprincipalFWHM_NUVNUV FWHM assuming a gaussian corearcsecphys.size;em.UV.200-300nmVARCHARprincipalGGOIDGALEX Global Object IDmeta.idVARCHARprincipalGLATGalactic latitudedegpos.galactic.latVARCHARprincipalGLONGalactic longitudedegpos.galactic.lonVARCHARprincipalHP_PIXELHEALPix pixel on sky coverage maps on GALEX-GAMA web site (nside = 16384; nested)VARCHARprincipalMAGERR_D12p0_FUVFUV AB magnitude error in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D12p0_NUVNUV AB magnitude error in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D18p0_FUVFUV AB magnitude error in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D18p0_NUVNUV AB magnitude error in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D25p5_FUVFUV AB magnitude error in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D25p5_NUVNUV AB magnitude error in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D34p5_FUVFUV AB magnitude error in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D34p5_NUVNUV AB magnitude error in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D3p0_FUVFUV AB magnitude error in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D3p0_NUVNUV AB magnitude error in 3.0 arcsec (2 pixel)diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D4p5_FUVFUV AB magnitude error in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D4p5_NUVNUV AB magnitude error in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D7p5_FUVFUV AB magnitude error in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D7p5_NUVNUV AB magnitude error in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_FUVFUV calibrated AB Kron magnitude error using NUV aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_NUVNUV calibrated AB Kron magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_D12p0_FUVFUV AB magnitude in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D12p0_NUVNUV AB magnitude in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D18p0_FUVFUV AB magnitude in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D18p0_NUVNUV AB magnitude in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D25p5_FUVFUV AB magnitude in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D25p5_NUVNUV AB magnitude in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D34p5_FUVFUV AB magnitude in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D34p5_NUVNUV AB magnitude in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D3p0_FUVFUV AB magnitude in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D3p0_NUVNUV AB magnitude in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D4p5_FUVFUV AB magnitude in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D4p5_NUVNUV AB magnitude in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D7p5_FUVFUV AB magnitude in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D7p5_NUVNUV AB magnitude in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_FUVFUV calibrated AB Kron magnitude using NUV aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_NUVNUV calibrated AB Kron magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalNAMEObject IAU format namemeta.idVARCHARprincipalNUMBER_MCATRunning object number from GALEX MCAT filemeta.idVARCHARprincipalPOSANGPosition angle (east of north)degpos.posAngVARCHARprincipalPOSANGERRPosition angle errordegpos.posAng;stat.errorVARCHARprincipalPOSERRPosition errorarcsecstat.errorVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalS2N_FUVFUV signal-to-noise from flux value (NB: can become negative for negative flux)stat.snr;em.UV.100-200nmVARCHARprincipalS2N_NUVNUV signal-to-noise from flux valuestat.snr;em.UV.200-300nmVARCHARprincipalSEMIMAJORSemimajor axisarcsecphys.size.radiusVARCHARprincipalSEMIMAJORERRSemimajor axis errorarcsecphys.size.radius;stat.errorVARCHARprincipalSEMIMINORSemiminor axisarcsecphys.size.radiusVARCHARprincipalSEMIMINORERRSemiminor axis errorarcsecphys.size.radius;stat.errorVARCHARprincipalTILEGALEX tile namemeta.idVARCHARprincipalTILENUMGALEX tile numbermeta.numberVARCHARprincipalXPEAK_IMAGEPixel position of the brightest NUV pixel on intensity mapspixelVARCHARprincipalX_IMAGEObject pixel position on intensity mapspixelVARCHARprincipalYPEAK_IMAGEPixel position of the brightest NUV pixel on intensity mapspixelVARCHARprincipalY_IMAGEObject pixel position on intensity mapspixelVARCHARprincipalgama_dr2.GalexMainThis is the main catalogue of the GalexPhotometry DMU. It reproduces the most important information from the other catalogues in this DMU and provides a best estimate of the NUV and FUV fluxes of all GAMA DR2 objects that were detected by GALEX.NN_DEC_GALEXDeclination of nearest neighbour GALEX object (J2000)degpos.eq.decVARCHARprincipalBEST_FLUXERR_FUVBest estimate FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalBEST_FLUXERR_NUVBest estimate NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalBEST_FLUX_FUVBest estimate of the GAMA object`s FUV fluxmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalBEST_FLUX_NUVBest estimate of the GAMA object`s NUV fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalBEST_MAGERR_FUVBest estimate FUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalBEST_MAGERR_NUVBest estimate NUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalBEST_MAG_FUVBest estimate of the GAMA object`s FUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalBEST_MAG_NUVBest estimate of the GAMA object`s NUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalBEST_METHODMethod used for the best flux estimates (AdvancedMatch or CoG)meta.codeVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalCOG_CONFSOURCE_FUVCoG FUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCOG_CONFSOURCE_NUVCoG NUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCOG_FLUXERR_FUVCoG FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_FLUXERR_NUVCoG NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalCOG_FLUX_FUVCoG FUV flux at the position of the GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalCOG_FLUX_NUVCoG NUV flux at the position of the GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalCOG_HP_RAD_FUVCoG FUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCOG_HP_RAD_NUVCoG NUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCOG_MAGERR_FUVCoG FUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_MAGERR_NUVCoG NUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalCOG_MAG_FUVCoG FUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalCOG_MAG_NUVCoG NUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalCOG_RE_CRIT_FUVCoG FUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCOG_RE_CRIT_NUVCoG NUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalDECDeclination of GAMA object (J2000)degpos.eq.decVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalFUVFLAGCombination of the FUV artifact flags of all GALEX objects involved in advanced matching proceduremeta.code;em.UV.100-200nmVARCHARprincipalNMATCHOPTNumber of GAMA objects involved in advanced matching proceduremeta.numberVARCHARprincipalNMATCHUVNumber of GALEX objects involved in advanced matching proceduremeta.numberVARCHARprincipalNN_ARTIFACT_FUVFUV artifact flag of nearest neighbour GALEX object (see GalexPhot notes)meta.code;em.UV.100-200nmVARCHARprincipalNN_ARTIFACT_NUVNUV artifact flag of nearest neighbour GALEX object (see GalexPhot notes)meta.code;em.UV.200-300nmVARCHARprincipalNN_DISTDistance between GAMA object and nearest neighbour GALEX objectarcsecpos.angDistanceVARCHARprincipalNN_FLUX50_RADIUS_FUVFUV 50 percent fraction-of-light radius of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalNN_FLUX50_RADIUS_NUVNUV 50 percent fraction-of-light radius of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_FLUXERR_FUVFUV flux error of nearest neighbour GALEX object using NUV aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalNN_FLUXERR_NUVNUV flux error of nearest neighbour GALEX objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalNN_FLUX_FUVFUV flux of nearest neighbour GALEX object using NUV aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalNN_FLUX_NUVNUV flux of nearest neighbour GALEX objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalNN_GGOIDGlobal Object ID of nearest neighbour GALEX objectmeta.idVARCHARprincipalNN_MAGERR_FUVFUV AB Kron magnitude error of nearest neighbour GALEX object using NUV aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalNN_MAGERR_NUVNUV AB Kron magnitude error of nearest neighbour GALEX objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalNN_MAG_FUVFUV AB Kron magnitude of nearest neighbour GALEX object using NUV aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalNN_MAG_NUVNUV AB Kron magnitude of nearest neighbour GALEX objectmagphot.mag;em.UV.200-300nmVARCHARprincipalNN_MANY2ONENumber of GAMA objects the nearest neighbour GALEX object is matched tometa.numberVARCHARprincipalNN_NMATCH4Number of GALEX objects found within 4 arcsec of GAMA objectmeta.numberVARCHARprincipalNN_POSANGERR_NUVNUV position angle error of nearest neighbour GALEX objectdegpos.posAng;stat.errorVARCHARprincipalNN_POSANG_NUVNUV position angle (east of north) of nearest neighbour GALEX objectdegpos.posAngVARCHARprincipalNN_RA_GALEXRight Ascension of nearest neighbour GALEX object (J2000)degpos.eq.raVARCHARprincipalNN_SEMIMAJORERR_NUVNUV semimajor axis error of nearest neighbour GALEX objectarcsecphys.size.radius;stat.errorVARCHARprincipalNN_SEMIMAJOR_NUVNUV semimajor axis of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_SEMIMINORERR_NUVNUV semiminor axis error of nearest neighbour GALEX objectarcsecphys.size.radius;stat.errorVARCHARprincipalNN_SEMIMINOR_NUVNUV semiminor axis of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_SFLAGS_FUVFUV Sextraxtor extraction flags of nearest neighbour GALEX objectmeta.code;em.UV.100-200nmVARCHARprincipalNN_SFLAGS_NUVNUV Sextraxtor extraction flags of nearest neighbour GALEX objectmeta.code;em.UV.200-300nmVARCHARprincipalNUVFLAGCombination of the NUV artifact flags of all GALEX objects involved in advanced matching proceduremeta.code;em.UV.200-300nmVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRARight Ascension of GAMA object (J2000)degpos.eq.raVARCHARprincipalSPLIT_FLUXERR_FUVError on redistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalSPLIT_FLUXERR_NUVError on redistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalSPLIT_FLUX_FUVRedistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalSPLIT_FLUX_NUVRedistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalSPLIT_MAGERR_FUVError on redistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalSPLIT_MAGERR_NUVError on redistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalSPLIT_MAG_FUVRedistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nmVARCHARprincipalSPLIT_MAG_NUVRedistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nmVARCHARprincipalTOT_FLUXERR_FUVError on total FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalTOT_FLUXERR_NUVError on the total NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalTOT_FLUX_FUVTotal FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.100-200nmVARCHARprincipalTOT_FLUX_NUVTotal NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.200-300nmVARCHARprincipalTOT_MAGERR_FUVError on total FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalTOT_MAGERR_NUVError on total NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalTOT_MAG_FUVTotal FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.100-200nmVARCHARprincipalTOT_MAG_NUVTotal NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.200-300nmVARCHARprincipalgama_dr2.GalexCoGPhotThis catalogue provides GALEX NUV and FUV curve-of-growth photometry for all GAMA DR2 objects.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalCONFSOURCE_FUVFUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCONFSOURCE_NUVNUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCPSERR_FUVFUV counts per second errorcounts/sphot.count;em.UV.100-200nm;stat.errorVARCHARprincipalCPSERR_NUVNUV counts per second errorcounts/sphot.count;em.UV.200-300nm;stat.errorVARCHARprincipalCPS_FUVFUV counts per secondcounts/sphot.count;em.UV.100-200nmVARCHARprincipalCPS_NUVNUV counts per secondcounts/sphot.count;em.UV.200-300nmVARCHARprincipalFLUXERR_FUVFUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_NUVNUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUX_FUVFUV fluxmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_NUVNUV fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalHP_RAD_FUVFUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalHP_RAD_NUVNUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalMAGERR_FUVFUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_NUVNUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_FUVFUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_NUVNUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRE_CRIT_FUVFUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalRE_CRIT_NUVNUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalgama_dr2.GalexAdvancedMatchThis catalogue contains the result of an advanced match between InputCatA and GalexPhot, listing only objects included in DR2. The matching procedure takes into account the possibility of multiple matches between GALEX and GAMA objects and seeks to reconstruct the original UV flux of a given GAMA object. GAMA DR2 objects without a GALEX match are not included in this catalogue.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalFLUXSPLITERR_FUVRedistributed FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXSPLITERR_NUVRedistributed NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXSPLIT_FUVRedistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXSPLIT_NUVRedistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXTOTERR_FUVTotal FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXTOTERR_NUVTotal NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXTOT_FUVTotal FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXTOT_NUVTotal NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.200-300nmVARCHARprincipalFUVFLAGCombination of the FUV artifact flags of all GALEX objects involved in the matchingmeta.code;em.UV.100-200nmVARCHARprincipalMAGSPLITERR_FUVRedistributed FUV AB magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGSPLITERR_NUVRedistributed NUV AB magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGSPLIT_FUVRedistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nmVARCHARprincipalMAGSPLIT_NUVRedistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nmVARCHARprincipalMAGTOTERR_FUVTotal FUV AB magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGTOTERR_NUVTotal NUV AB magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGTOT_FUVTotal FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.100-200nmVARCHARprincipalMAGTOT_NUVTotal NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.200-300nmVARCHARprincipalNMATCHOPTNumber of GAMA objects involved in the matchingmeta.numberVARCHARprincipalNMATCHUVNumber of GALEX objects involved in the matchingmeta.numberVARCHARprincipalNUVFLAGCombination of the NUV artifact flags of all GALEX objects involved in the matchingmeta.code;em.UV.200-300nmVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalOPTIDXLISTID list of GAMA objects used in the flux redistribution calculation using SDSS OBJID; string always ends with a commaVARCHARprincipalUVIDXLISTID list of GALEX object used in the flux redistribution calculation using NAME from GalexPhot; string always ends with a commaVARCHARprincipal6dfgs_fdr<p>The 6dF Galaxy Survey (6dFGS) measured the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The targets are all galaxies brighter than K_tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J, r_F, b_J) = (13.05, 13.75, 15.6, 16.75). Central to the survey is the Six-Degree Field (6dF) multifibre spectrograph, an instrument able to record 150 simultaneous spectra over the 5.7 degree field of the UK Schmidt Telescope. Spectra are obtained in two observations using separate V and R gratings, that together give R ~ 1000 over at least 400-750 nm and signal-to-noise ratio ~10 per pixel. Redshift measurements are obtained semi-automatically, and are assigned a quality value based on visual inspection.</p>6dfgs_fdr.SPECTRARedshifts and observational dataSPECIDunique ID no., used to generate GIF image of spectrumNonemeta.id;meta.mainINTEGERindexedprincipalTARGETIDID no. in Target tableNonemeta.id.crossINTEGERprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.id;meta.mainVARCHARindexedprincipalOBSRAobserved RA (J2000 degrees)degpos.eq.ra;meta.mainREALindexedprincipalOBSDECobserved Dec (J2000 degrees)degpos.eq.dec;meta.mainREALindexedprincipalMATCH_DRposition match error (arcsec)arcsecstat.error;posREALprincipalHTMIDHierarchical Triangular Mesh (20-deep), mainly useful internally for indexing on positionNonemeta.idBIGINTprincipalCXCartesian x of unit vector on celestial sphereNonemeta.crypticREALprincipalCYCartesian y of unit vector on celestial sphereNonemeta.crypticREALprincipalCZCartesian z of unit vector on celestial sphereNonemeta.crypticREALprincipalZ_ORIGINredshift from C=combined V or R frameNonesrc.redshiftVARCHARprincipalZraw measured redshift,(corrected for template offsets and slit vane shift)Nonesrc.redshiftREALprincipalZ_HELIOheliocentric redshift (corrected for heliocentric motion, template offsets and slit vane shift)Nonesrc.redshift;pos.heliocentricREALprincipalQUALITYredshift measurement quality: 4=good 1=bad (6=star)Nonemeta.code.qual;src.redshiftINTEGERprincipalABEMMAredshift type: abs=1,emi=2,man=3Nonemeta.code.member;src.redshiftINTEGERprincipalNMBESTemission lines for emission zNonespect.line;meta.numberINTEGERprincipalNGOODnumber of good emission linesNonespect.line;meta.numberINTEGERprincipalZ_EMIemission redshift (uncorrected)Nonesrc.redshiftREALprincipalQ_Z_EMIemission redshift qualityNonemeta.code.qual;src.redshiftINTEGERprincipalKBESTRcross-correlation templateNonemeta.idINTEGERprincipalR_CRCORcross-correlation peakNonemeta.crypticREALprincipalZ_ABScross-correlation redshift(uncorrected)Nonesrc.redshiftREALprincipalQ_Z_ABScross-correlation qualityNonemeta.code.qualINTEGERprincipalQ_FINALsuggested quality for redshiftNonemeta.code.qual;src.redshiftINTEGERprincipalIALTERIALTER=1 if automatic z alteredNonemeta.code.classINTEGERprincipalZ_COMMredshifter's commentNonemeta.noteVARCHARprincipalZEMIBESTERRerror on the selected emission line redshift, 0.0 if not measuredNonestat.error;src.redshiftREALprincipalZABSBESTERRerror on the selected absorption line redshift, 0.0 if not measuredNonestat.error;src.redshiftREALprincipalZFINALERRerror on final quoted redshift, 0.0 if not measuredNonestat.error;src.redshiftREALprincipalTITLE_Veg 1325m243p2.sds observation titleNonemeta.idVARCHARprincipalCENRA_VRA of field centredegpos.eq.raREALprincipalCENDEC_VDEC of field centredegpos.eq.decREALprincipalAPPRA_Vapparent RA of field centredegpos.eq.raREALprincipalAPPDEC_Vapparent DEC of field centredegpos.eq.decREALprincipalACTMJD_Vthe time the field was actually configuredNonetime.epoch;instr.setupREALprincipalCONMJD_Vtime which was specified when configure was runNonetime.epoch;instr.setupREALprincipalPROGID_Vprogramme ID in V frameNonemeta.idVARCHARprincipalLABEL_Vlabel in V frameNonemeta.idVARCHARprincipalOBSID_Vobsid in V frameNonemeta.idVARCHARprincipalRUN_VV run numberNonemeta.idINTEGERprincipalEXP_VV reference frame exposure time secondssecondstime.durationREALprincipalNCOMB_Vnumber of V frames combinedNonemeta.numberINTEGERprincipalGRATID_Vgrating ID in V frameNonemeta.idVARCHARprincipalGRATSET_VV grating micrometer settingTODOinstr.setupREALprincipalGRATSLOT_VV grating slot IDNonemeta.idVARCHARprincipalGRATBLAZ_VV blaze directionNoneinstr.setupVARCHARprincipalSOURCE_VV source plateNonemeta.idVARCHARprincipalFOCUS_VV frame spectrograph focus valueTODOinstr.setupREALprincipalTFOCUS_VV frame telescope focus valueTODOinstr.setupREALprincipalGAIN_VV gainTODOinstr.setupREALprincipalNOISE_vV readout noiseTODOinstr.det.noiseREALprincipalCCD_VV CCD nameNonemeta.idVARCHARprincipalUTDATE_VUT date in V frame, default 1900-01-01Nonetime.epoch;obsVARCHARprincipalUTSTRT_VUT start time of V reference frameNonetime.startVARCHARprincipalMJDOBS_VMJD of observationNonetime.epoch;obsREALprincipalNAME_Vname of object in V frameNonemeta.idVARCHARprincipalTHPUT_VV throughput of fibreNoneinstr.sensitivityREALprincipalRA_Vobserved RA (J2000 degrees)degpos.eq.raREALprincipalDEC_Vobserved Dec (J2000 degrees)degpos.eq.decREALprincipalX_Vx position of object from V frameTODOpos.cartesian.xINTEGERprincipalY_Vy position of object from V frameTODOpos.cartesian.yINTEGERprincipalXERR_Verror on X_V positionTODOstat.error;pos.cartesian.xINTEGERprincipalYERR_Verror on Y_V positionTODOstat.error;pos.cartesian.yINTEGERprincipalTHETA_Vfibre angle V framedeginstr.offsetREALprincipalFIBRE_Vfibre number (row on CCD)Nonemeta.idINTEGERprincipalPIVOT_VV pivot numberNoneinstr.setupINTEGERprincipalRECMAG_Vmagnitude read from V framemagphot.magREALprincipalPID_VPID number read from V frameNonemeta.crypticINTEGERprincipalTITLE_Reg 1325m243p2.sds observation titleNonemeta.idVARCHARprincipalCENRA_RRA of field centredegpos.eq.raREALprincipalCENDEC_RDEC of field centredegpos.eq.decREALprincipalAPPRA_Rapparent RA of field centredegpos.eq.raREALprincipalAPPDEC_Rapparent DEC of field centredegpos.eq.decREALprincipalACTMJD_Rthe time the field was actually configuredNonetime.epoch;instr.setupREALprincipalCONMJD_Rtime which was specified when configure was runNonetime.epoch;instr.setupREALprincipalPROGID_Rprogramme ID in R frameNonemeta.idVARCHARprincipalLABEL_Rlabel in R frameNonemeta.idVARCHARprincipalOBSID_Robsid in R frameNonemeta.idVARCHARprincipalRUN_RR run numberNonemeta.idINTEGERprincipalEXP_RR reference frame exposure time secondssecondstime.durationREALprincipalNCOMB_Rnumber of R frames combinedNonemeta.numberINTEGERprincipalGRATID_Rgrating ID in R frameNonemeta.idVARCHARprincipalGRATSET_RR grating micrometer settingTODOinstr.setupREALprincipalGRATSLOT_RR grating slot IDNonemeta.idVARCHARprincipalGRATBLAZ_RR blaze directionNoneinstr.setupVARCHARprincipalSOURCE_RR source plateNonemeta.idVARCHARprincipalFOCUS_RR frame spectrograph focus valueTODOinstr.setupREALprincipalTFOCUS_RR frame telescope focus valueTODOinstr.setupREALprincipalGAIN_RR gainTODOinstr.setupREALprincipalNOISE_RR readout noiseTODOinstr.det.noiseREALprincipalCCD_RR CCD nameNonemeta.idVARCHARprincipalUTDATE_RUT date in R frame, default 1900-01-01Nonetime.epoch;obsVARCHARprincipalUTSTRT_RUT start time of R reference frameNonetime.startVARCHARprincipalMJDOBS_RMJD of observationNonetime.epoch;obsREALprincipalNAME_Rname of object in R frameNonemeta.idVARCHARprincipalTHPUT_RR throughput of fibreNoneinstr.sensitivityREALprincipalRA_Robserved RA (J2000 degrees)degpos.eq.raREALprincipalDEC_Robserved Dec (J2000 degrees)degpos.eq.decREALprincipalX_Rx position of object from R frameTODOpos.cartesian.xINTEGERprincipalY_Ry position of object from R frameTODOpos.cartesian.yINTEGERprincipalXERR_Rerror on X_R positionTODOstat.error;pos.cartesian.xINTEGERprincipalYERR_Rerror on Y_R positionTODOstat.error;pos.cartesian.yINTEGERprincipalTHETA_Rfibre angle R frameTODOinstr.offsetREALprincipalFIBRE_Rfibre number (row on CCD)TODOmeta.idINTEGERprincipalPIVOT_RR pivot numberNoneinstr.setupINTEGERprincipalRECMAG_Rmagnitude read from R framemagphot.magREALprincipalPID_RPID number read from R frameNonemeta.crypticINTEGERprincipalFRAMENAMEname of the observed field frameNonemeta.idVARCHARprincipalAXISSTART_Vstarting wavelength of the V-frameangstromem.wl;instr.setupREALprincipalAXISEND_Vend wavelength of the V-frameangstromem.wl;instr.setupREALprincipalAXISSTART_Rstarting wavelength of the R-frameangstromem.wl;instr.setupREALprincipalAXISEND_Rend wavelength of the R-frameangstromem.wl;instr.setupREALprincipalMATCHSPECIDSPECID of same object observation already ingested (usually = 0, helps flag frames objects that were re-analysedNonemeta.idINTEGERprincipalZ_INITIALvalue of attribute Z at initial ingest i.e. before correctionsNonesrc.redshiftREALprincipalZ_HELIO_INITIALvalue of attribute Z_HELIO at initial ingest i.e. before further correctionsNonesrc.redshiftREALprincipalZ_UPDATE_FLAG0 - uncorrected, 1 - slit vane corrected, 2 - template corrected, 3 - template and slit vane correctedNonemeta.codeINTEGERprincipalZ_UPDATE_COMMnot currently usedNonemeta.noteVARCHARprincipalSLIT_VANE_CORRslit vane redshift correction in km/skm/sarith.factor;src.redshiftREALprincipalQUALITY_INITIALQUALITY value at initial ingestNonemeta.code.qualINTEGERprincipalXTALKFLAG-1 if object is a contaminator, 0 (default) objects is neither contaminator or contaminated, +N object contaminated by fibre N. Details on cross-talk contaminationNonemeta.code.classINTEGERprincipalXTALKSCORE0 (uncontaminated) to 5 (likely cross-talk)Nonemeta.code.qualINTEGERprincipalXTALKVELOFFvelocity offset between contaminated and contaminator objectskm/sspect.dopplerVeloc;arith.diffREALprincipalXTALKCOMMcomment on crosstalkNonemeta.noteVARCHARprincipalQUALITY_UPDATE_COMMcomment on quality changeNonemeta.noteVARCHARprincipalDEPRECATEDflag used to expunge rows prior to releaseNonemeta.codeINTEGERprincipalREVTEMPLATEcode of template used in redshift revisionNonemeta.codeINTEGERprincipalREVCOMMENTcomment/origin of redshift revisionNonemeta.noteVARCHARprincipalPROGIDhighest priority programme ID of observed objectNonemeta.idINTEGERprincipalZ_COMM_INITIALredshifter's comment prior to revisionNonemeta.noteVARCHARprincipalGIFSPECTRUMURLURL for spectrum in GIF format (defunct)Nonemeta.ref.urlVARCHARprincipalFITSFILEURLURL for spectrum in FITS format (defunct)Nonemeta.ref.urlVARCHARprincipalDISPLAYURLURL for spectrum display (defunct)Nonemeta.ref.urlVARCHARprincipalFITS1DURLURL for 1D spectrum in FITS format (defunct)Nonemeta.ref.urlVARCHARprincipal6dfgs_fdr.TARGETThe master target listTARGETIDunique ID no., used to link tablesNonemeta.id;meta.mainINTEGERindexedprincipalTARGETNAMEname in config file, used to name FITS file and generate thumbnail imagesNonemeta.idVARCHARprincipalHTMIDHierarchical Triangular Mesh (20-deep) number, mainly useful internally for indexing on positionNonepos.HTMBIGINTprincipalRAmaster RA J2000 (decimal degrees)degpos.eq.ra;meta.mainREALindexedprincipalDECmaster Dec J2000 (decimal degrees)degpos.eq.dec;meta.mainREALindexedprincipalCXCartesian x of unit (RA,Dec) vector on celestial sphereNonemeta.crypticREALprincipalCYCartesian y of unit (RA,Dec) vector on celestial sphereNonemeta.crypticREALprincipalCZCartesian z of unit (RA,Dec) vector on celestial sphereNonemeta.crypticREALprincipalGLgalactic longitudedegpos.galactic.lonREALprincipalGBgalactic latitudedegpos.galactic.latREALprincipalA_VSchlegel V extinctionmagem.opt.V;phys.absorption.galREALprincipalPROGIDhighest priority programme IDNonemeta.idINTEGERprincipalBMAGBj galaxy magnitude from recalibrated SuperCOSMOS data (0.00 is null)magphot.mag;em.opt.BREALprincipalRMAGRf galaxy magnitude from recalibrated SuperCOSMOS data (0.00 is null)magphot.mag;em.opt.RREALprincipalSGSSS star/galaxy flag 1=galaxy 2=star 3=unclass 4=noiseNonemeta.idINTEGERprincipalZCATVELvelocity in ZCATkm/sphys.velocINTEGERprincipalZCATERRerror on velocity in ZCATkm/sphys.veloc;stat.errorINTEGERprincipalZCATREFZCAT referenceNonemeta.idINTEGERprincipalBMAGSELBj magnitude from online SuperCOSMOS Sky Surveys (99.99 and 23.0 are nulls), appeared as BMAG in the EDR and DR1magphot.mag;em.opt.BREALprincipalRMAGSELRf magnitude from online SuperCOSMOS Sky Surveys (99.99 and 22.0 are nulls), appeared as RMAG in the EDR and DR1magphot.mag;em.opt.RREALprincipalTEMPLATECODEcode for x-correlation templateNonemeta.idVARCHARprincipalFRAMENAMEname of SDF frameNonemeta.idVARCHARprincipal6dfgs_fdr.SUMSSBright radio sources from SUMSSOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipal6dfgs_fdr.NVSSCandidate QSOs from NVSSOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipal6dfgs_fdr.HESCandidate QSOs from the Hamburg/ESO SurveyOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipal6dfgs_fdr.AGN2MASSCandidate AGN from the 2MASS red AGN surveyOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipalMAG_3supplied magnitude 3magphot.magREALprincipal6dfgs_fdr.DENISJgalaxies from DENIS J < 13.85OBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipalCOMMENTsupplied commentsNonemeta.noteVARCHARprincipal6dfgs_fdr.DENISIGalaxies from DENIS I < 14.85OBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipalCOMMENTsupplied commentsNonemeta.noteVARCHARprincipal6dfgs_fdr.SHAPLEYGalaxies from the Shapley superclusterOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipal6dfgs_fdr.DURUKSTExtension to Durham/UKST galaxy surveyOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipal6dfgs_fdr.HIPASSSources from the HIPASS HI surveyOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipal6dfgs_fdr.RASSCandidate AGN from the ROSAT All-Sky SurveyOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipalCOMMENTsupplied commentsNonemeta.noteVARCHARprincipal6dfgs_fdr.FSCSources from the IRAS FAINT Source CatalogueOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitude 1magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitude 2magphot.magREALprincipalCOMMENTsupplied commentsNonemeta.noteVARCHARprincipal6dfgs_fdr.SUPERCOSSuperCOSMOS bright galaxies Bj and ROBJIDunique ID numberNonemeta.id;meta.mainmeta.id;meta.mainINTEGERindexedprincipalCATNAMEsupplied catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipalRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1Bj magnitude, SuperCOSMOS magnitudes generated from a revised calibration, done at the time of input catalogue preparation, tuned to the magnitude range of interest.magphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2R magnitude, SuperCOSMOS magnitudes generated from a revised calibration, done at the time of input catalogue preparation, tuned to the magnitude range of interest.magphot.magREALprincipalCOMMENTSuperCOSMOS reference (field no. + B_index + R_index)Nonemeta.noteVARCHARprincipal6dfgs_fdr.TWOMASS2MASS input catalogue J, H and KRARA J2000degpos.eq.ra;meta.mainREALindexedprincipalDECDec J2000degpos.eq.dec;meta.mainREALindexedprincipalPRIORITYsurvey weightNonemeta.code.classINTEGERprincipalMAG_1supplied magnitudemagphot.magREALprincipalPROGIDprogramme IDNonemeta.idINTEGERprincipalMAG_2supplied magnitudemagphot.magREALprincipalJ_M_K20FEJ 20mag/sq." isophotal fiducial elliptical aperture magnitudemagphot.mag;em.IR.JREALprincipalH_M_K20FEH 20mag/sq." isophotal fiducial elliptical aperture magnitudemagphot.mag;em.IR.HREALprincipalK_M_K20FEK 20mag/sq." isophotal fiducial elliptical aperture magnitudemagphot.mag;em.IR.KREALprincipalRADIUS20mag/sq." isophotal K fiducial elliptical aperture semi-major axisarcsecphys.angSize.smajAxisREALprincipalA_Bminor/major axis ratio fit to 3-sigma super-coadd isophotearcsecphys.size.axisRatio;meta.modelledREALprincipalMUK20FEaverage surface brightness within the mu_K = 20mag/sq arcsec elliptical isophote (derived from K_M_K20FE, RADIUS and A_B)magphot.mag.sb;stat.meanREALprincipalCORRcorrection, based on MUK20FE, made to the isophotal magnitude K_M_K20FE to get a pseudo-total magnitude Kmagphot.mag;em.IR.K;arith.factorREALprincipalJJ magnitude (JEXT) used for J selectionmagphot.mag;em.IR.JREALprincipalHH magnitude (HEXT) used for H selectionmagphot.mag;em.IR.HREALprincipalKEXTKEXT magnitudemagphot.mag;em.IR.KREALprincipalKK magnitude (corrected) used for K selectionmagphot.mag;em.IR.KREALprincipalKEXT_KKEXT minus K (corrected)magphot.mag;em.IR.KREALprincipalJTOTJ total magnitudemagphot.mag;em.IR.JREALprincipalHTOTH total magnitudemagphot.mag;em.IR.HREALprincipalKTOTK total magnitudemagphot.mag;em.IR.KREALprincipalRTOTradius of the total size of the galaxyarcsecphys.size.radiusREALprincipalOBJIDunique ID numberNonemeta.id;meta.mainINTEGERindexedprincipalCATNAME2MASS catalogue nameNonemeta.idVARCHARprincipalprevCATNAMEoriginal catalogue nameNonemeta.idVARCHARprincipalTARGETNAMEmatching name in target table, used to name FITS files and generate thumbnail imagesNonemeta.idVARCHARprincipalTARGETIDmatching ID number in targetNonemeta.id.crossINTEGERprincipal6dfgs_fdr.dc_source_listSource list of all objects contained within 6dFGSTARGETNAMEunique ID used for identifying sourcesNonemeta.id;meta.mainVARCHARindexedprincipalRAmaster RA J2000 (decimal degrees)degpos.eq.ra;meta.mainREALindexedprincipalDECmaster Dec J2000 (decimal degrees)degpos.eq.dec;meta.mainREALindexedprincipalsource_nameunique ID used for identifying sourcesNonemeta.id;meta.mainVARCHARindexedprincipalrapos.eq.raREALprincipaldecpos.eq.decREALprincipalgalah_dr3Studying galaxy evolution through galactic archaeologygalah_dr3.main_starGALAH DR3 Main Allstar (Clean)star_id2MASS identifiermeta.id.crossVARCHARprincipalsobject_idGALAH identifiermeta.id;meta.mainBIGINTindexedprincipalsource_idGaia DR2 source_idmeta.id.crossBIGINTprincipalsurvey_nameName of survey as part of GALAH+DR3meta.idVARCHARprincipalfield_idGALAH fco fieldmeta.idINTEGERprincipalflag_repeatRepeat observation flag, indicating if used for clean catalogmeta.code.qual,stat.fitINTEGERprincipalwg4_fieldGALAH WG4 fieldmeta.numberVARCHARprincipalwg4_pipelineSME pipeline version free/lbol/seismeta.versionVARCHARprincipalflag_spStellar parameter quality flagmeta.code.qual,stat.fitINTEGERprincipalteffSpectroscopic effective temperature (used for fitting)Kphys.temperature.effectiveREALprincipale_teffUncertainty teffKstat.error;phys.temperature.effectiveREALprincipalirfm_teffIRFM temperature (not used for synthesis)Kphys.temperature.effective,photREALprincipalirfm_ebvE(B-V) used for IRFM teff estimationmagphys.absorption.galREALprincipalirfm_ebv_refReference irfm_ebvmeta.bibVARCHARprincipalloggSurface gravity (not fitted via spectra if wg4_pipeline not free)log(cm.s**-2)phys.gravityREALprincipale_loggUncertainty logglog(cm.s**-2)stat.error;phys.gravityREALprincipalfe_hFe atomic abundance from Fe lines (final, 1D-NLTE)phys.abund.FeREALprincipale_fe_hUncertainty fe_hstat.error;phys.abund.FeREALprincipalflag_fe_hQuality flag fe_hmeta.code.qual,stat.fitINTEGERprincipalfe_h_atmosme.feh from stellar parameter run, fitted from H, Ti, Sc, Festat.fit.paramREALprincipalvmicMicroturbulence velocity (from empirical relation)km s-1phys.veloc.microTurbREALprincipalvbroadBroadening velocity (fitted sme.vsini with sme.vmac=0)km s-1phys.veloc.rotatREALprincipale_vbroadUncertainty of vbroadkm s-1stat.error;phys.veloc.rotatREALprincipalchi2_spChi2 value of stellar parameter fittingstat.fit.chi2REALprincipalalpha_feCombined, weighted alpha-process element abundancephys.abundREALprincipale_alpha_feUncertainty of alpha_festat.error;phys.abundREALprincipalnr_alpha_feBitmask of used measurements for alpha_femeta.numberREALprincipalflag_alpha_feQuality flag of measurements for alpha_femeta.code.qual,stat.fitINTEGERprincipalflux_A_FeNormalised maximum absorption strength of in iron linesspectr.lineREALprincipalchi_A_FeChi2 value of iron abundance fittingstat.fit.chi2REALprincipalLi_feNeutral Li atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Li_feUncertainty Li_festat.error;phys.abundREALprincipalnr_Li_feBitmask of used Li ind linesmeta.numberINTEGERprincipalflag_Li_feQuality flag of Li_femeta.code.qual,stat.fitINTEGERprincipalC_feNeutral C atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_C_feUncertainty C_festat.error;phys.abundREALprincipalnr_C_feBitmask of used C ind linesmeta.numberINTEGERprincipalflag_C_feQuality flag of C_femeta.code.qual,stat.fitINTEGERprincipalO_feNeutral O atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_O_feUncertainty O_festat.error;phys.abundREALprincipalnr_O_feBitmask of used O ind linesmeta.numberINTEGERprincipalflag_O_feQuality flag of O_femeta.code.qual,stat.fitINTEGERprincipalNa_feNeutral Na atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Na_feUncertainty Na_festat.error;phys.abundREALprincipalnr_Na_feBitmask of used Na ind linesmeta.numberINTEGERprincipalflag_Na_feQuality flag of Na_femeta.code.qual,stat.fitINTEGERprincipalMg_feNeutral Mg atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Mg_feUncertainty Mg_festat.error;phys.abundREALprincipalnr_Mg_feBitmask of used Mg ind linesmeta.numberINTEGERprincipalflag_Mg_feQuality flag of Mg_femeta.code.qual,stat.fitINTEGERprincipalAl_feNeutral Al atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Al_feUncertainty Al_festat.error;phys.abundREALprincipalnr_Al_feBitmask of used Al ind linesmeta.numberINTEGERprincipalflag_Al_feQuality flag of Al_femeta.code.qual,stat.fitINTEGERprincipalSi_feNeutral Si atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Si_feUncertainty Si_festat.error;phys.abundREALprincipalnr_Si_feBitmask of used Si ind linesmeta.numberINTEGERprincipalflag_Si_feQuality flag of Si_femeta.code.qual,stat.fitINTEGERprincipalK_feNeutral K atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_K_feUncertainty K_festat.error;phys.abundREALprincipalnr_K_feBitmask of used K ind linesmeta.numberINTEGERprincipalflag_K_feQuality flag of K_femeta.code.qual,stat.fitINTEGERprincipalCa_feNeutral Ca atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Ca_feUncertainty Ca_festat.error;phys.abundREALprincipalnr_Ca_feBitmask of used Ca ind linesmeta.numberINTEGERprincipalflag_Ca_feQuality flag of Ca_femeta.code.qual,stat.fitINTEGERprincipalSc_feNeutral Sc atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sc_feUncertainty Sc_festat.error;phys.abundREALprincipalnr_Sc_feBitmask of used Sc ind linesmeta.numberINTEGERprincipalflag_Sc_feQuality flag of Sc_femeta.code.qual,stat.fitINTEGERprincipalTi_feNeutral Ti atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ti_feUncertainty Ti_festat.error;phys.abundREALprincipalnr_Ti_feBitmask of used Ti ind linesmeta.numberINTEGERprincipalflag_Ti_feQuality flag of Ti_femeta.code.qual,stat.fitINTEGERprincipalTi2_feSingle-ionised Ti2 atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ti2_feUncertainty Ti2_festat.error;phys.abundREALprincipalnr_Ti2_feBitmask of used Ti2 ind linesmeta.numberINTEGERprincipalflag_Ti2_feQuality flag of Ti2_femeta.code.qual,stat.fitINTEGERprincipalV_feNeutral V atomic abundance (final, 1D-LTE)phys.abundREALprincipale_V_feUncertainty V_festat.error;phys.abundREALprincipalnr_V_feBitmask of used V ind linesmeta.numberINTEGERprincipalflag_V_feQuality flag of V_femeta.code.qual,stat.fitINTEGERprincipalCr_feNeutral Cr atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Cr_feUncertainty Cr_festat.error;phys.abundREALprincipalnr_Cr_feBitmask of used Cr ind linesmeta.numberINTEGERprincipalflag_Cr_feQuality flag of Cr_femeta.code.qual,stat.fitINTEGERprincipalMn_feNeutral Mn atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Mn_feUncertainty Mn_festat.error;phys.abundREALprincipalnr_Mn_feBitmask of used Mn ind linesmeta.numberINTEGERprincipalflag_Mn_feQuality flag of Mn_femeta.code.qual,stat.fitINTEGERprincipalCo_feNeutral Co atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Co_feUncertainty Co_festat.error;phys.abundREALprincipalnr_Co_feBitmask of used Co ind linesmeta.numberINTEGERprincipalflag_Co_feQuality flag of Co_femeta.code.qual,stat.fitINTEGERprincipalNi_feNeutral Ni atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ni_feUncertainty Ni_festat.error;phys.abundREALprincipalnr_Ni_feBitmask of used Ni ind linesmeta.numberINTEGERprincipalflag_Ni_feQuality flag of Ni_femeta.code.qual,stat.fitINTEGERprincipalCu_feNeutral Cu atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Cu_feUncertainty Cu_festat.error;phys.abundREALprincipalnr_Cu_feBitmask of used Cu ind linesmeta.numberINTEGERprincipalflag_Cu_feQuality flag of Cu_femeta.code.qual,stat.fitINTEGERprincipalZn_feNeutral Zn atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Zn_feUncertainty Zn_festat.error;phys.abundREALprincipalnr_Zn_feBitmask of used Zn ind linesmeta.numberINTEGERprincipalflag_Zn_feQuality flag of Zn_femeta.code.qual,stat.fitINTEGERprincipalRb_feNeutral Rb atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Rb_feUncertainty Rb_festat.error;phys.abundREALprincipalnr_Rb_feBitmask of used Rb ind linesmeta.numberINTEGERprincipalflag_Rb_feQuality flag of Rb_femeta.code.qual,stat.fitINTEGERprincipalSr_feNeutral Sr atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sr_feUncertainty Sr_festat.error;phys.abundREALprincipalnr_Sr_feBitmask of used Sr ind linesmeta.numberINTEGERprincipalflag_Sr_feQuality flag of Sr_femeta.code.qual,stat.fitINTEGERprincipalY_feNeutral Y atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Y_feUncertainty Y_festat.error;phys.abundREALprincipalnr_Y_feBitmask of used Y ind linesmeta.numberINTEGERprincipalflag_Y_feQuality flag of Y_femeta.code.qual,stat.fitINTEGERprincipalZr_feNeutral Zr atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Zr_feUncertainty Zr_festat.error;phys.abundREALprincipalnr_Zr_feBitmask of used Zr ind linesmeta.numberINTEGERprincipalflag_Zr_feQuality flag of Zr_femeta.code.qual,stat.fitINTEGERprincipalMo_feNeutral Mo atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Mo_feUncertainty Mo_festat.error;phys.abundREALprincipalnr_Mo_feBitmask of used Mo ind linesmeta.numberINTEGERprincipalflag_Mo_feQuality flag of Mo_femeta.code.qual,stat.fitINTEGERprincipalRu_feNeutral Ru atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ru_feUncertainty Ru_festat.error;phys.abundREALprincipalnr_Ru_feBitmask of used Ru ind linesmeta.numberINTEGERprincipalflag_Ru_feQuality flag of Ru_femeta.code.qual,stat.fitINTEGERprincipalBa_feSingle-ionised Ba atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Ba_feUncertainty Ba_festat.error;phys.abundREALprincipalnr_Ba_feBitmask of used Ba ind linesmeta.numberINTEGERprincipalflag_Ba_feQuality flag of Ba_femeta.code.qual,stat.fitINTEGERprincipalLa_feSingle-ionised La atomic abundance (final, 1D-LTE)phys.abundREALprincipale_La_feUncertainty La_festat.error;phys.abundREALprincipalnr_La_feBitmask of used La ind linesmeta.numberINTEGERprincipalflag_La_feQuality flag of La_femeta.code.qual,stat.fitINTEGERprincipalCe_feSingle-ionised Ce atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ce_feUncertainty Ce_festat.error;phys.abundREALprincipalnr_Ce_feBitmask of used Ce ind linesmeta.numberINTEGERprincipalflag_Ce_feQuality flag of Ce_femeta.code.qual,stat.fitINTEGERprincipalNd_feSingle-ionised Nd atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Nd_feUncertainty Nd_festat.error;phys.abundREALprincipalnr_Nd_feBitmask of used Nd ind linesmeta.numberINTEGERprincipalflag_Nd_feQuality flag of Nd_femeta.code.qual,stat.fitINTEGERprincipalSm_feSingle-ionised Sm atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sm_feUncertainty Sm_festat.error;phys.abundREALprincipalnr_Sm_feBitmask of used Sm ind linesmeta.numberINTEGERprincipalflag_Sm_feQuality flag of Sm_femeta.code.qual,stat.fitINTEGERprincipalEu_feSingle-ionised Eu atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Eu_feUncertainty Eu_festat.error;phys.abundREALprincipalnr_Eu_feBitmask of used Eu ind linesmeta.numberINTEGERprincipalflag_Eu_feQuality flag of Eu_femeta.code.qual,stat.fitINTEGERprincipalrapropagated from Gaia DR2degpos.eq.ra;meta.mainREALindexedprincipalra_errorpropagated from Gaia DR2masstat.error;pos.eq.raREALprincipaldecpropagated from Gaia DR2degpos.eq.dec;meta.mainREALindexedprincipaldec_errorpropagated from Gaia DR2masstat.error;pos.eq.decREALprincipallpropagated from Gaia DR2degpos.galactic.lonREALprincipalbpropagated from Gaia DR2degpos.galactic.latREALprincipalr_estpropagated from 2018AJ....156...58Bpcpos.distanceREALprincipalr_lopropagated from 2018AJ....156...58Bpcstat.error;stat.min;pos.distanceREALprincipalr_hipropagated from 2018AJ....156...58Bpcstat.error;stat.max;pos.distanceREALprincipalr_lenpropagated from 2018AJ....156...58Bpcstat.fit.param;pos.distanceREALprincipalpmrapropagated from Gaia DR2mas yr-1pos.pm;pos.eq.raREALprincipalpmra_errorpropagated from Gaia DR2mas yr-1stat.error;pos.pm;pos.eq.raREALprincipalpmdecpropagated from Gaia DR2mas yr-1pos.pm;pos.eq.decREALprincipalpmdec_errorpropagated from Gaia DR2mas yr-1stat.error;pos.pm;pos.eq.decREALprincipalra_dec_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.eq.decREALprincipalra_parallax_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.parallaxREALprincipalra_pmra_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.pm;pos.eq.raREALprincipalra_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.pm;pos.eq.decREALprincipaldec_parallax_corrpropagated from Gaia DR2stat.correlation;pos.eq.dec;pos.parallaxREALprincipaldec_pmra_corrpropagated from Gaia DR2stat.correlation;pos.eq.dec;pos.pm;pos.eq.raREALprincipaldec_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.eq.dec;pos.pm;pos.eq.decREALprincipalparallax_pmra_corrpropagated from Gaia DR2stat.correlation;pos.parallax;pos.pm;pos.eq.raREALprincipalparallax_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.parallax;pos.pm;pos.eq.decREALprincipalpmra_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.pm;pos.eq.ra;pos.pm;pos.eq.decREALprincipalrv_galahSME fitted radial velocity from GALAH spectrakm s-1spect.dopplerVeloc.optREALprincipale_rv_galahUncertainty of rv_galahkm s-1stat.error;spect.dopplerVeloc.optREALprincipalrv_gaiapropagated from Gaia DR2km s-1spect.dopplerVeloc.optREALprincipale_rv_gaiapropagated from Gaia DR2km s-1stat.error;spect.dopplerVeloc.optREALprincipalred_flageduction pipeline quality flagmeta.code.qual;INTEGERprincipalsnr_c1_irafAverage SNR/px CCD1stat.snrREALprincipalsnr_c2_irafAverage SNR/px CCD2stat.snrREALprincipalsnr_c3_irafAverage SNR/px CCD3stat.snrREALprincipalsnr_c4_irafAverage SNR/px CCD4stat.snrREALprincipalflag_guessGUESS reduction pipeline quality flagmeta.code.qual,stat.fitINTEGERprincipalv_jkV magnitude estimated from 2MASS J and Ks magmagphot.magREALprincipalj_mpropagated from 2MASSmagphot.mag;em.IR.JREALprincipalj_msigcompropagated from 2MASSmagstat.error;phot.mag;em.IR.JREALprincipalh_mpropagated from 2MASSmagphot.mag;em.IR.HREALprincipalh_msigcompropagated from 2MASSmagstat.error;phot.mag;em.IR.HREALprincipalks_mpropagated from 2MASSmagphot.mag;em.IR.KREALprincipalks_msigcompropagated from 2MASSmagstat.error;phot.mag;em.IR.KREALprincipalph_qual_tmasspropagated from 2MASS ph_qualmeta.code.qual;photVARCHARprincipalw2mpropropagated from AllWISEmagphot.mag;em.IR.4-8umREALprincipalw2mpro_errorpropagated from AllWISEmagstat.error;phot.magREALprincipalph_qual_wisepropagated from AllWISE ph_qualmeta.code.qual;photVARCHARprincipala_ksUsed Ks band extinctionmagphys.absorption.galREALprincipale_a_ksUncertainty of a_ksmagstat.error,phys.absorption.galREALprincipalbc_ksUsed Bolometric Correction for Ks bandmagphot.mag.bc;em.IR.KREALprincipalparallaxpropagated from Gaia DR2maspos.parallaxREALprincipalparallax_errorpropagated from Gaia DR2masstat.error;pos.parallaxREALprincipalruwepropagated from Gaia DR2stat.errorREALprincipalphot_g_mean_magpropagated from Gaia DR2magphot.mag;stat.mean;em.optREALprincipalbp_rppropagated from Gaia DR2magphot.colorREALprincipalgalah_dr3.main_specGALAH DR3 Main Allspec (Extended Caution)h_msigcompropagated from 2MASSmagstat.error;phot.mag;em.IR.HREALprincipalstar_id2MASS identifiermeta.id.crossVARCHARprincipalsobject_idGALAH identifiermeta.id;meta.mainBIGINTindexedprincipalsource_idGaia DR2 source_idmeta.id.crossBIGINTprincipalsurvey_nameName of survey as part of GALAH+DR3meta.idVARCHARprincipalfield_idGALAH fco fieldmeta.idINTEGERprincipalflag_repeatRepeat observation flag, indicating if used for clean catalogmeta.code.qual,stat.fitINTEGERprincipalwg4_fieldGALAH WG4 fieldmeta.numberVARCHARprincipalwg4_pipelineSME pipeline version free/lbol/seismeta.versionVARCHARprincipalflag_spStellar parameter quality flagmeta.code.qual,stat.fitINTEGERprincipalteffSpectroscopic effective temperature (used for fitting)Kphys.temperature.effectiveREALprincipale_teffUncertainty teffKstat.error;phys.temperature.effectiveREALprincipalirfm_teffIRFM temperature (not used for synthesis)Kphys.temperature.effective,photREALprincipalirfm_ebvE(B-V) used for IRFM teff estimationmagphys.absorption.galREALprincipalirfm_ebv_refReference irfm_ebvmeta.bibVARCHARprincipalcov_e_teffSME covariance fitting uncertainty teffKfit.param;stat.error;phys.temperature.effectiveREALprincipalinit_teffSME initial teffKfit.param;phys.temperature.effectiveREALprincipalloggSurface gravity (not fitted via spectra if wg4_pipeline not free)log(cm.s**-2)phys.gravityREALprincipale_loggUncertainty logglog(cm.s**-2)stat.error;phys.gravityREALprincipalcov_e_loggMonteCarlo uncertainty logglog(cm.s**-2)fit.param;stat.error;phys.gravityREALprincipalinit_loggSME initial logglog(cm.s**-2)fit.param;phys.gravityREALprincipalfe_hFe atomic abundance from Fe lines (final, 1D-NLTE)phys.abund.FeREALprincipale_fe_hUncertainty fe_hstat.error;phys.abund.FeREALprincipalcov_e_fe_hSME covariance fitting uncertainty fe_hfit.param;stat.error;phys.abund.FeREALprincipalflag_fe_hQuality flag fe_hmeta.code.qual,stat.fitINTEGERprincipalfe_h_atmosme.feh from stellar parameter run, fitted from H, Ti, Sc, Festat.fit.paramREALprincipale_fe_h_atmoUncertainty fe_h_atmofit.param;phys.abund.FeREALprincipalcov_e_fe_h_atmoSME covariance fitting uncertainty sme.fehfit.param;stat.error;phys.abund.FeREALprincipalinit_fe_h_atmoSME initial sme.fehfit.param;stat.error;phys.abund.FeREALprincipalvmicMicroturbulence velocity (from empirical relation)km s-1phys.veloc.microTurbREALprincipalvbroadBroadening velocity (fitted sme.vsini with sme.vmac=0)km s-1phys.veloc.rotatREALprincipale_vbroadUncertainty of vbroadkm s-1stat.error;phys.veloc.rotatREALprincipalcov_e_vbroadSME covariance fitting uncertainty sme.vsinikm s-1fit.param;stat.error;phys.veloc.rotatREALprincipalinit_vbroadSME initial broadening velocitykm s-1fit.param;stat.error;phys.veloc.rotatREALprincipalmassStellar parameter fitting product of stellar masssolMassfit.param;phys.massREALprincipallbolStellar parameter fitting product of bolometric luminositysolLumfit.param;phys.luminosityREALprincipalageStellar parameter fitting product of stellar ageGyrfit.param;time.ageREALprincipalchi2_spChi2 value of stellar parameter fittingstat.fit.chi2REALprincipalalpha_feCombined, weighted alpha-process element abundancephys.abundREALprincipale_alpha_feUncertainty of alpha_festat.error;phys.abundREALprincipalnr_alpha_feBitmask of used measurements for alpha_femeta.numberREALprincipalflag_alpha_feQuality flag of measurements for alpha_femeta.code.qual,stat.fitINTEGERprincipalflux_A_FeNormalised maximum absorption strength of in iron linesspectr.lineREALprincipalchi_A_FeChi2 value of iron abundance fittingstat.fit.chi2REALprincipalind_Li6708_feIndividual uncalibrated measurmenet of line/combo Li6708 with local RV fittedphys.abundREALprincipalind_cov_e_Li6708SME covariance fitting uncertainty ind_Li6708_fefit.param;stat.error;phys.abundREALprincipalind_flag_Li6708Quality flag fit for ind_Li6708_femeta.code.qual,stat.fitINTEGERprincipalind_Li6708_NoRV_feIndividual uncalibrated measurmenet of line/combo Li6708_NoRV with RV fixedphys.abundREALprincipalind_cov_e_Li6708_NoRVSME covariance fitting uncertainty ind_Li6708_NoRV_fefit.param;stat.error;phys.abundREALprincipalind_flag_Li6708_NoRVQuality flag fit for ind_Li6708_NoRV_femeta.code.qual,stat.fitINTEGERprincipalind_C6588_feIndividual uncalibrated measurmenet of line/combo C6588phys.abundREALprincipalind_cov_e_C6588SME covariance fitting uncertainty ind_C6588_fefit.param;stat.error;phys.abundREALprincipalind_flag_C6588Quality flag fit for ind_C6588_femeta.code.qual,stat.fitINTEGERprincipalind_O_feIndividual uncalibrated measurmenet of line/combo Ophys.abundREALprincipalind_cov_e_OSME covariance fitting uncertainty ind_O_fefit.param;stat.error;phys.abundREALprincipalind_flag_OQuality flag fit for ind_O_femeta.code.qual,stat.fitINTEGERprincipalind_Na_feIndividual uncalibrated measurmenet of line/combo Naphys.abundREALprincipalind_cov_e_NaSME covariance fitting uncertainty ind_Na_fefit.param;stat.error;phys.abundREALprincipalind_flag_NaQuality flag fit for ind_Na_femeta.code.qual,stat.fitINTEGERprincipalind_Mg5711_feIndividual uncalibrated measurmenet of line/combo Mg5711phys.abundREALprincipalind_cov_e_Mg5711SME covariance fitting uncertainty ind_Mg5711_fefit.param;stat.error;phys.abundREALprincipalind_flag_Mg5711Quality flag fit for ind_Mg5711_femeta.code.qual,stat.fitINTEGERprincipalind_Al_feIndividual uncalibrated measurmenet of line/combo Alphys.abundREALprincipalind_cov_e_AlSME covariance fitting uncertainty ind_Al_fefit.param;stat.error;phys.abundREALprincipalind_flag_AlQuality flag fit for ind_Al_femeta.code.qual,stat.fitINTEGERprincipalind_Si_feIndividual uncalibrated measurmenet of line/combo Siphys.abundREALprincipalind_cov_e_SiSME covariance fitting uncertainty ind_Si_fefit.param;stat.error;phys.abundREALprincipalind_flag_SiQuality flag fit for ind_Si_femeta.code.qual,stat.fitINTEGERprincipalind_K7699_feIndividual uncalibrated measurmenet of line/combo K7699phys.abundREALprincipalind_cov_e_K7699SME covariance fitting uncertainty ind_K7699_fefit.param;stat.error;phys.abundREALprincipalind_flag_K7699Quality flag fit for ind_K7699_femeta.code.qual,stat.fitINTEGERprincipalind_Ca_feIndividual uncalibrated measurmenet of line/combo Caphys.abundREALprincipalind_cov_e_CaSME covariance fitting uncertainty ind_Ca_fefit.param;stat.error;phys.abundREALprincipalind_flag_CaQuality flag fit for ind_Ca_femeta.code.qual,stat.fitINTEGERprincipalind_Sc_feIndividual uncalibrated measurmenet of line/combo Scphys.abundREALprincipalind_cov_e_ScSME covariance fitting uncertainty ind_Sc_fefit.param;stat.error;phys.abundREALprincipalind_flag_ScQuality flag fit for ind_Sc_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4758_feIndividual uncalibrated measurmenet of line/combo Ti4758phys.abundREALprincipalind_cov_e_Ti4758SME covariance fitting uncertainty ind_Ti4758_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4758Quality flag fit for ind_Ti4758_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4759_feIndividual uncalibrated measurmenet of line/combo Ti4759phys.abundREALprincipalind_cov_e_Ti4759SME covariance fitting uncertainty ind_Ti4759_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4759Quality flag fit for ind_Ti4759_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4778_feIndividual uncalibrated measurmenet of line/combo Ti4778phys.abundREALprincipalind_cov_e_Ti4778SME covariance fitting uncertainty ind_Ti4778_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4778Quality flag fit for ind_Ti4778_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4782_feIndividual uncalibrated measurmenet of line/combo Ti4782phys.abundREALprincipalind_cov_e_Ti4782SME covariance fitting uncertainty ind_Ti4782_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4782Quality flag fit for ind_Ti4782_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4798_feIndividual uncalibrated measurmenet of line/combo Ti4798phys.abundREALprincipalind_cov_e_Ti4798SME covariance fitting uncertainty ind_Ti4798_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4798Quality flag fit for ind_Ti4798_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4802_feIndividual uncalibrated measurmenet of line/combo Ti4802phys.abundREALprincipalind_cov_e_Ti4802SME covariance fitting uncertainty ind_Ti4802_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4802Quality flag fit for ind_Ti4802_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4820_feIndividual uncalibrated measurmenet of line/combo Ti4820phys.abundREALprincipalind_cov_e_Ti4820SME covariance fitting uncertainty ind_Ti4820_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4820Quality flag fit for ind_Ti4820_femeta.code.qual,stat.fitINTEGERprincipalind_Ti5689_feIndividual uncalibrated measurmenet of line/combo Ti5689phys.abundREALprincipalind_cov_e_Ti5689SME covariance fitting uncertainty ind_Ti5689_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti5689Quality flag fit for ind_Ti5689_femeta.code.qual,stat.fitINTEGERprincipalind_Ti5716_feIndividual uncalibrated measurmenet of line/combo Ti5716phys.abundREALprincipalind_cov_e_Ti5716SME covariance fitting uncertainty ind_Ti5716_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti5716Quality flag fit for ind_Ti5716_femeta.code.qual,stat.fitINTEGERprincipalind_Ti5720_feIndividual uncalibrated measurmenet of line/combo Ti5720phys.abundREALprincipalind_cov_e_Ti5720SME covariance fitting uncertainty ind_Ti5720_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti5720Quality flag fit for ind_Ti5720_femeta.code.qual,stat.fitINTEGERprincipalind_Ti5739_feIndividual uncalibrated measurmenet of line/combo Ti5739phys.abundREALprincipalind_cov_e_Ti5739SME covariance fitting uncertainty ind_Ti5739_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti5739Quality flag fit for ind_Ti5739_femeta.code.qual,stat.fitINTEGERprincipalind_Ti5866_feIndividual uncalibrated measurmenet of line/combo Ti5866phys.abundREALprincipalind_cov_e_Ti5866SME covariance fitting uncertainty ind_Ti5866_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti5866Quality flag fit for ind_Ti5866_femeta.code.qual,stat.fitINTEGERprincipalind_Ti6599_feIndividual uncalibrated measurmenet of line/combo Ti6599phys.abundREALprincipalind_cov_e_Ti6599SME covariance fitting uncertainty ind_Ti6599_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti6599Quality flag fit for ind_Ti6599_femeta.code.qual,stat.fitINTEGERprincipalind_Ti6717_feIndividual uncalibrated measurmenet of line/combo Ti6717phys.abundREALprincipalind_cov_e_Ti6717SME covariance fitting uncertainty ind_Ti6717_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti6717Quality flag fit for ind_Ti6717_femeta.code.qual,stat.fitINTEGERprincipalind_Ti7853_feIndividual uncalibrated measurmenet of line/combo Ti7853phys.abundREALprincipalind_cov_e_Ti7853SME covariance fitting uncertainty ind_Ti7853_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti7853Quality flag fit for ind_Ti7853_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4720_feIndividual uncalibrated measurmenet of line/combo Ti4720phys.abundREALprincipalind_cov_e_Ti4720SME covariance fitting uncertainty ind_Ti4720_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4720Quality flag fit for ind_Ti4720_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4765_feIndividual uncalibrated measurmenet of line/combo Ti4765phys.abundREALprincipalind_cov_e_Ti4765SME covariance fitting uncertainty ind_Ti4765_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4765Quality flag fit for ind_Ti4765_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4799_feIndividual uncalibrated measurmenet of line/combo Ti4799phys.abundREALprincipalind_cov_e_Ti4799SME covariance fitting uncertainty ind_Ti4799_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4799Quality flag fit for ind_Ti4799_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4849_feIndividual uncalibrated measurmenet of line/combo Ti4849phys.abundREALprincipalind_cov_e_Ti4849SME covariance fitting uncertainty ind_Ti4849_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4849Quality flag fit for ind_Ti4849_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4866_feIndividual uncalibrated measurmenet of line/combo Ti4866phys.abundREALprincipalind_cov_e_Ti4866SME covariance fitting uncertainty ind_Ti4866_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4866Quality flag fit for ind_Ti4866_femeta.code.qual,stat.fitINTEGERprincipalind_Ti4874_feIndividual uncalibrated measurmenet of line/combo Ti4874phys.abundREALprincipalind_cov_e_Ti4874SME covariance fitting uncertainty ind_Ti4874_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ti4874Quality flag fit for ind_Ti4874_femeta.code.qual,stat.fitINTEGERprincipalind_V4832_feIndividual uncalibrated measurmenet of line/combo V4832phys.abundREALprincipalind_cov_e_V4832SME covariance fitting uncertainty ind_V4832_fefit.param;stat.error;phys.abundREALprincipalind_flag_V4832Quality flag fit for ind_V4832_femeta.code.qual,stat.fitINTEGERprincipalind_V4784_feIndividual uncalibrated measurmenet of line/combo V4784phys.abundREALprincipalind_cov_e_V4784SME covariance fitting uncertainty ind_V4784_fefit.param;stat.error;phys.abundREALprincipalind_flag_V4784Quality flag fit for ind_V4784_femeta.code.qual,stat.fitINTEGERprincipalind_V4797_feIndividual uncalibrated measurmenet of line/combo V4797phys.abundREALprincipalind_cov_e_V4797SME covariance fitting uncertainty ind_V4797_fefit.param;stat.error;phys.abundREALprincipalind_flag_V4797Quality flag fit for ind_V4797_femeta.code.qual,stat.fitINTEGERprincipalind_Cr_feIndividual uncalibrated measurmenet of line/combo Crphys.abundREALprincipalind_cov_e_CrSME covariance fitting uncertainty ind_Cr_fefit.param;stat.error;phys.abundREALprincipalind_flag_CrQuality flag fit for ind_Cr_femeta.code.qual,stat.fitINTEGERprincipalind_Mn_feIndividual uncalibrated measurmenet of line/combo Mnphys.abundREALprincipalind_cov_e_MnSME covariance fitting uncertainty ind_Mn_fefit.param;stat.error;phys.abundREALprincipalind_flag_MnQuality flag fit for ind_Mn_femeta.code.qual,stat.fitINTEGERprincipalind_Co4781_feIndividual uncalibrated measurmenet of line/combo Co4781phys.abundREALprincipalind_cov_e_Co4781SME covariance fitting uncertainty ind_Co4781_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co4781Quality flag fit for ind_Co4781_femeta.code.qual,stat.fitINTEGERprincipalind_Co4900_feIndividual uncalibrated measurmenet of line/combo Co4900phys.abundREALprincipalind_cov_e_Co4900SME covariance fitting uncertainty ind_Co4900_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co4900Quality flag fit for ind_Co4900_femeta.code.qual,stat.fitINTEGERprincipalind_Co5647_feIndividual uncalibrated measurmenet of line/combo Co5647phys.abundREALprincipalind_cov_e_Co5647SME covariance fitting uncertainty ind_Co5647_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co5647Quality flag fit for ind_Co5647_femeta.code.qual,stat.fitINTEGERprincipalind_Co6490_feIndividual uncalibrated measurmenet of line/combo Co6490phys.abundREALprincipalind_cov_e_Co6490SME covariance fitting uncertainty ind_Co6490_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co6490Quality flag fit for ind_Co6490_femeta.code.qual,stat.fitINTEGERprincipalind_Co6551_feIndividual uncalibrated measurmenet of line/combo Co6551phys.abundREALprincipalind_cov_e_Co6551SME covariance fitting uncertainty ind_Co6551_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co6551Quality flag fit for ind_Co6551_femeta.code.qual,stat.fitINTEGERprincipalind_Co6632_feIndividual uncalibrated measurmenet of line/combo Co6632phys.abundREALprincipalind_cov_e_Co6632SME covariance fitting uncertainty ind_Co6632_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co6632Quality flag fit for ind_Co6632_femeta.code.qual,stat.fitINTEGERprincipalind_Co6679_feIndividual uncalibrated measurmenet of line/combo Co6679phys.abundREALprincipalind_cov_e_Co6679SME covariance fitting uncertainty ind_Co6679_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co6679Quality flag fit for ind_Co6679_femeta.code.qual,stat.fitINTEGERprincipalind_Co7713_feIndividual uncalibrated measurmenet of line/combo Co7713phys.abundREALprincipalind_cov_e_Co7713SME covariance fitting uncertainty ind_Co7713_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co7713Quality flag fit for ind_Co7713_femeta.code.qual,stat.fitINTEGERprincipalind_Co7838_feIndividual uncalibrated measurmenet of line/combo Co7838phys.abundREALprincipalind_cov_e_Co7838SME covariance fitting uncertainty ind_Co7838_fefit.param;stat.error;phys.abundREALprincipalind_flag_Co7838Quality flag fit for ind_Co7838_femeta.code.qual,stat.fitINTEGERprincipalind_Ni5847_feIndividual uncalibrated measurmenet of line/combo Ni5847phys.abundREALprincipalind_cov_e_Ni5847SME covariance fitting uncertainty ind_Ni5847_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ni5847Quality flag fit for ind_Ni5847_femeta.code.qual,stat.fitINTEGERprincipalind_Ni6586_feIndividual uncalibrated measurmenet of line/combo Ni6586phys.abundREALprincipalind_cov_e_Ni6586SME covariance fitting uncertainty ind_Ni6586_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ni6586Quality flag fit for ind_Ni6586_femeta.code.qual,stat.fitINTEGERprincipalind_Cu5700_feIndividual uncalibrated measurmenet of line/combo Cu5700phys.abundREALprincipalind_cov_e_Cu5700SME covariance fitting uncertainty ind_Cu5700_fefit.param;stat.error;phys.abundREALprincipalind_flag_Cu5700Quality flag fit for ind_Cu5700_femeta.code.qual,stat.fitINTEGERprincipalind_Cu5782_feIndividual uncalibrated measurmenet of line/combo Cu5782phys.abundREALprincipalind_cov_e_Cu5782SME covariance fitting uncertainty ind_Cu5782_fefit.param;stat.error;phys.abundREALprincipalind_flag_Cu5782Quality flag fit for ind_Cu5782_femeta.code.qual,stat.fitINTEGERprincipalind_Zn4722_feIndividual uncalibrated measurmenet of line/combo Zn4722phys.abundREALprincipalind_cov_e_Zn4722SME covariance fitting uncertainty ind_Zn4722_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zn4722Quality flag fit for ind_Zn4722_femeta.code.qual,stat.fitINTEGERprincipalind_Zn4811_feIndividual uncalibrated measurmenet of line/combo Zn4811phys.abundREALprincipalind_cov_e_Zn4811SME covariance fitting uncertainty ind_Zn4811_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zn4811Quality flag fit for ind_Zn4811_femeta.code.qual,stat.fitINTEGERprincipalind_Rb7800_feIndividual uncalibrated measurmenet of line/combo Rb7800phys.abundREALprincipalind_cov_e_Rb7800SME covariance fitting uncertainty ind_Rb7800_fefit.param;stat.error;phys.abundREALprincipalind_flag_Rb7800Quality flag fit for ind_Rb7800_femeta.code.qual,stat.fitINTEGERprincipalind_Sr6550_feIndividual uncalibrated measurmenet of line/combo Sr6550phys.abundREALprincipalind_cov_e_Sr6550SME covariance fitting uncertainty ind_Sr6550_fefit.param;stat.error;phys.abundREALprincipalind_flag_Sr6550Quality flag fit for ind_Sr6550_femeta.code.qual,stat.fitINTEGERprincipalind_Y_feIndividual uncalibrated measurmenet of line/combo Yphys.abundREALprincipalind_cov_e_YSME covariance fitting uncertainty ind_Y_fefit.param;stat.error;phys.abundREALprincipalind_flag_YQuality flag fit for ind_Y_femeta.code.qual,stat.fitINTEGERprincipalind_Y4820_feIndividual uncalibrated measurmenet of line/combo Y4820phys.abundREALprincipalind_cov_e_Y4820SME covariance fitting uncertainty ind_Y4820_fefit.param;stat.error;phys.abundREALprincipalind_flag_Y4820Quality flag fit for ind_Y4820_femeta.code.qual,stat.fitINTEGERprincipalind_Y4855_feIndividual uncalibrated measurmenet of line/combo Y4855phys.abundREALprincipalind_cov_e_Y4855SME covariance fitting uncertainty ind_Y4855_fefit.param;stat.error;phys.abundREALprincipalind_flag_Y4855Quality flag fit for ind_Y4855_femeta.code.qual,stat.fitINTEGERprincipalind_Y4884_feIndividual uncalibrated measurmenet of line/combo Y4884phys.abundREALprincipalind_cov_e_Y4884SME covariance fitting uncertainty ind_Y4884_fefit.param;stat.error;phys.abundREALprincipalind_flag_Y4884Quality flag fit for ind_Y4884_femeta.code.qual,stat.fitINTEGERprincipalind_Y5663_feIndividual uncalibrated measurmenet of line/combo Y5663phys.abundREALprincipalind_cov_e_Y5663SME covariance fitting uncertainty ind_Y5663_fefit.param;stat.error;phys.abundREALprincipalind_flag_Y5663Quality flag fit for ind_Y5663_femeta.code.qual,stat.fitINTEGERprincipalind_Y5729_feIndividual uncalibrated measurmenet of line/combo Y5729phys.abundREALprincipalind_cov_e_Y5729SME covariance fitting uncertainty ind_Y5729_fefit.param;stat.error;phys.abundREALprincipalind_flag_Y5729Quality flag fit for ind_Y5729_femeta.code.qual,stat.fitINTEGERprincipalind_Zr4739_feIndividual uncalibrated measurmenet of line/combo Zr4739phys.abundREALprincipalind_cov_e_Zr4739SME covariance fitting uncertainty ind_Zr4739_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zr4739Quality flag fit for ind_Zr4739_femeta.code.qual,stat.fitINTEGERprincipalind_Zr4772_feIndividual uncalibrated measurmenet of line/combo Zr4772phys.abundREALprincipalind_cov_e_Zr4772SME covariance fitting uncertainty ind_Zr4772_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zr4772Quality flag fit for ind_Zr4772_femeta.code.qual,stat.fitINTEGERprincipalind_Zr4806_feIndividual uncalibrated measurmenet of line/combo Zr4806phys.abundREALprincipalind_cov_e_Zr4806SME covariance fitting uncertainty ind_Zr4806_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zr4806Quality flag fit for ind_Zr4806_femeta.code.qual,stat.fitINTEGERprincipalind_Zr4828_feIndividual uncalibrated measurmenet of line/combo Zr4828phys.abundREALprincipalind_cov_e_Zr4828SME covariance fitting uncertainty ind_Zr4828_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zr4828Quality flag fit for ind_Zr4828_femeta.code.qual,stat.fitINTEGERprincipalind_Zr5681_feIndividual uncalibrated measurmenet of line/combo Zr5681phys.abundREALprincipalind_cov_e_Zr5681SME covariance fitting uncertainty ind_Zr5681_fefit.param;stat.error;phys.abundREALprincipalind_flag_Zr5681Quality flag fit for ind_Zr5681_femeta.code.qual,stat.fitINTEGERprincipalind_Mo5689_feIndividual uncalibrated measurmenet of line/combo Mo5689phys.abundREALprincipalind_cov_e_Mo5689SME covariance fitting uncertainty ind_Mo5689_fefit.param;stat.error;phys.abundREALprincipalind_flag_Mo5689Quality flag fit for ind_Mo5689_femeta.code.qual,stat.fitINTEGERprincipalind_Mo5751_feIndividual uncalibrated measurmenet of line/combo Mo5751phys.abundREALprincipalind_cov_e_Mo5751SME covariance fitting uncertainty ind_Mo5751_fefit.param;stat.error;phys.abundREALprincipalind_flag_Mo5751Quality flag fit for ind_Mo5751_femeta.code.qual,stat.fitINTEGERprincipalind_Mo5858_feIndividual uncalibrated measurmenet of line/combo Mo5858phys.abundREALprincipalind_cov_e_Mo5858SME covariance fitting uncertainty ind_Mo5858_fefit.param;stat.error;phys.abundREALprincipalind_flag_Mo5858Quality flag fit for ind_Mo5858_femeta.code.qual,stat.fitINTEGERprincipalind_Mo6619_feIndividual uncalibrated measurmenet of line/combo Mo6619phys.abundREALprincipalind_cov_e_Mo6619SME covariance fitting uncertainty ind_Mo6619_fefit.param;stat.error;phys.abundREALprincipalind_flag_Mo6619Quality flag fit for ind_Mo6619_femeta.code.qual,stat.fitINTEGERprincipalind_Ru4758_feIndividual uncalibrated measurmenet of line/combo Ru4758phys.abundREALprincipalind_cov_e_Ru4758SME covariance fitting uncertainty ind_Ru4758_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ru4758Quality flag fit for ind_Ru4758_femeta.code.qual,stat.fitINTEGERprincipalind_Ru4869_feIndividual uncalibrated measurmenet of line/combo Ru4869phys.abundREALprincipalind_cov_e_Ru4869SME covariance fitting uncertainty ind_Ru4869_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ru4869Quality flag fit for ind_Ru4869_femeta.code.qual,stat.fitINTEGERprincipalind_Ru5699_feIndividual uncalibrated measurmenet of line/combo Ru5699phys.abundREALprincipalind_cov_e_Ru5699SME covariance fitting uncertainty ind_Ru5699_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ru5699Quality flag fit for ind_Ru5699_femeta.code.qual,stat.fitINTEGERprincipalind_Ba_feIndividual uncalibrated measurmenet of line/combo Baphys.abundREALprincipalind_cov_e_BaSME covariance fitting uncertainty ind_Ba_fefit.param;stat.error;phys.abundREALprincipalind_flag_BaQuality flag fit for ind_Ba_femeta.code.qual,stat.fitINTEGERprincipalind_La4716_feIndividual uncalibrated measurmenet of line/combo La4716phys.abundREALprincipalind_cov_e_La4716SME covariance fitting uncertainty ind_La4716_fefit.param;stat.error;phys.abundREALprincipalind_flag_La4716Quality flag fit for ind_La4716_femeta.code.qual,stat.fitINTEGERprincipalind_La4749_feIndividual uncalibrated measurmenet of line/combo La4749phys.abundREALprincipalind_cov_e_La4749SME covariance fitting uncertainty ind_La4749_fefit.param;stat.error;phys.abundREALprincipalind_flag_La4749Quality flag fit for ind_La4749_femeta.code.qual,stat.fitINTEGERprincipalind_La4804_feIndividual uncalibrated measurmenet of line/combo La4804phys.abundREALprincipalind_cov_e_La4804SME covariance fitting uncertainty ind_La4804_fefit.param;stat.error;phys.abundREALprincipalind_flag_La4804Quality flag fit for ind_La4804_femeta.code.qual,stat.fitINTEGERprincipalind_La5806_feIndividual uncalibrated measurmenet of line/combo La5806phys.abundREALprincipalind_cov_e_La5806SME covariance fitting uncertainty ind_La5806_fefit.param;stat.error;phys.abundREALprincipalind_flag_La5806Quality flag fit for ind_La5806_femeta.code.qual,stat.fitINTEGERprincipalind_Ce4774_feIndividual uncalibrated measurmenet of line/combo Ce4774phys.abundREALprincipalind_cov_e_Ce4774SME covariance fitting uncertainty ind_Ce4774_fefit.param;stat.error;phys.abundREALprincipalind_flag_Ce4774Quality flag fit for ind_Ce4774_femeta.code.qual,stat.fitINTEGERprincipalind_Nd4811_feIndividual uncalibrated measurmenet of line/combo Nd4811phys.abundREALprincipalind_cov_e_Nd4811SME covariance fitting uncertainty ind_Nd4811_fefit.param;stat.error;phys.abundREALprincipalind_flag_Nd4811Quality flag fit for ind_Nd4811_femeta.code.qual,stat.fitINTEGERprincipalind_Nd5741_feIndividual uncalibrated measurmenet of line/combo Nd5741phys.abundREALprincipalind_cov_e_Nd5741SME covariance fitting uncertainty ind_Nd5741_fefit.param;stat.error;phys.abundREALprincipalind_flag_Nd5741Quality flag fit for ind_Nd5741_femeta.code.qual,stat.fitINTEGERprincipalind_Nd5770_feIndividual uncalibrated measurmenet of line/combo Nd5770phys.abundREALprincipalind_cov_e_Nd5770SME covariance fitting uncertainty ind_Nd5770_fefit.param;stat.error;phys.abundREALprincipalind_flag_Nd5770Quality flag fit for ind_Nd5770_femeta.code.qual,stat.fitINTEGERprincipalind_Nd5812_feIndividual uncalibrated measurmenet of line/combo Nd5812phys.abundREALprincipalind_cov_e_Nd5812SME covariance fitting uncertainty ind_Nd5812_fefit.param;stat.error;phys.abundREALprincipalind_flag_Nd5812Quality flag fit for ind_Nd5812_femeta.code.qual,stat.fitINTEGERprincipalind_Nd5842_feIndividual uncalibrated measurmenet of line/combo Nd5842phys.abundREALprincipalind_cov_e_Nd5842SME covariance fitting uncertainty ind_Nd5842_fefit.param;stat.error;phys.abundREALprincipalind_flag_Nd5842Quality flag fit for ind_Nd5842_femeta.code.qual,stat.fitINTEGERprincipalind_Sm4720_feIndividual uncalibrated measurmenet of line/combo Sm4720phys.abundREALprincipalind_cov_e_Sm4720SME covariance fitting uncertainty ind_Sm4720_fefit.param;stat.error;phys.abundREALprincipalind_flag_Sm4720Quality flag fit for ind_Sm4720_femeta.code.qual,stat.fitINTEGERprincipalind_Sm4792_feIndividual uncalibrated measurmenet of line/combo Sm4792phys.abundREALprincipalind_cov_e_Sm4792SME covariance fitting uncertainty ind_Sm4792_fefit.param;stat.error;phys.abundREALprincipalind_flag_Sm4792Quality flag fit for ind_Sm4792_femeta.code.qual,stat.fitINTEGERprincipalind_Sm4837_feIndividual uncalibrated measurmenet of line/combo Sm4837phys.abundREALprincipalind_cov_e_Sm4837SME covariance fitting uncertainty ind_Sm4837_fefit.param;stat.error;phys.abundREALprincipalind_flag_Sm4837Quality flag fit for ind_Sm4837_femeta.code.qual,stat.fitINTEGERprincipalind_Sm4848_feIndividual uncalibrated measurmenet of line/combo Sm4848phys.abundREALprincipalind_cov_e_Sm4848SME covariance fitting uncertainty ind_Sm4848_fefit.param;stat.error;phys.abundREALprincipalind_flag_Sm4848Quality flag fit for ind_Sm4848_femeta.code.qual,stat.fitINTEGERprincipalind_Sm4854_feIndividual uncalibrated measurmenet of line/combo Sm4854phys.abundREALprincipalind_cov_e_Sm4854SME covariance fitting uncertainty ind_Sm4854_fefit.param;stat.error;phys.abundREALprincipalind_flag_Sm4854Quality flag fit for ind_Sm4854_femeta.code.qual,stat.fitINTEGERprincipalind_Eu5819_feIndividual uncalibrated measurmenet of line/combo Eu5819phys.abundREALprincipalind_cov_e_Eu5819SME covariance fitting uncertainty ind_Eu5819_fefit.param;stat.error;phys.abundREALprincipalind_flag_Eu5819Quality flag fit for ind_Eu5819_femeta.code.qual,stat.fitINTEGERprincipalind_Eu6645_feIndividual uncalibrated measurmenet of line/combo Eu6645phys.abundREALprincipalind_cov_e_Eu6645SME covariance fitting uncertainty ind_Eu6645_fefit.param;stat.error;phys.abundREALprincipalind_flag_Eu6645Quality flag fit for ind_Eu6645_femeta.code.qual,stat.fitINTEGERprincipalLi_feNeutral Li atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Li_feUncertainty Li_festat.error;phys.abundREALprincipalnr_Li_feBitmask of used Li ind linesmeta.numberINTEGERprincipalflag_Li_feQuality flag of Li_femeta.code.qual,stat.fitINTEGERprincipalC_feNeutral C atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_C_feUncertainty C_festat.error;phys.abundREALprincipalnr_C_feBitmask of used C ind linesmeta.numberINTEGERprincipalflag_C_feQuality flag of C_femeta.code.qual,stat.fitINTEGERprincipalO_feNeutral O atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_O_feUncertainty O_festat.error;phys.abundREALprincipalnr_O_feBitmask of used O ind linesmeta.numberINTEGERprincipalflag_O_feQuality flag of O_femeta.code.qual,stat.fitINTEGERprincipalNa_feNeutral Na atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Na_feUncertainty Na_festat.error;phys.abundREALprincipalnr_Na_feBitmask of used Na ind linesmeta.numberINTEGERprincipalflag_Na_feQuality flag of Na_femeta.code.qual,stat.fitINTEGERprincipalMg_feNeutral Mg atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Mg_feUncertainty Mg_festat.error;phys.abundREALprincipalnr_Mg_feBitmask of used Mg ind linesmeta.numberINTEGERprincipalflag_Mg_feQuality flag of Mg_femeta.code.qual,stat.fitINTEGERprincipalAl_feNeutral Al atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Al_feUncertainty Al_festat.error;phys.abundREALprincipalnr_Al_feBitmask of used Al ind linesmeta.numberINTEGERprincipalflag_Al_feQuality flag of Al_femeta.code.qual,stat.fitINTEGERprincipalSi_feNeutral Si atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Si_feUncertainty Si_festat.error;phys.abundREALprincipalnr_Si_feBitmask of used Si ind linesmeta.numberINTEGERprincipalflag_Si_feQuality flag of Si_femeta.code.qual,stat.fitINTEGERprincipalK_feNeutral K atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_K_feUncertainty K_festat.error;phys.abundREALprincipalnr_K_feBitmask of used K ind linesmeta.numberINTEGERprincipalflag_K_feQuality flag of K_femeta.code.qual,stat.fitINTEGERprincipalCa_feNeutral Ca atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Ca_feUncertainty Ca_festat.error;phys.abundREALprincipalnr_Ca_feBitmask of used Ca ind linesmeta.numberINTEGERprincipalflag_Ca_feQuality flag of Ca_femeta.code.qual,stat.fitINTEGERprincipalSc_feNeutral Sc atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sc_feUncertainty Sc_festat.error;phys.abundREALprincipalnr_Sc_feBitmask of used Sc ind linesmeta.numberINTEGERprincipalflag_Sc_feQuality flag of Sc_femeta.code.qual,stat.fitINTEGERprincipalSc2_feSingle-ionised Sc2 atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sc2_feUncertainty Sc2_festat.error;phys.abundREALprincipalnr_Sc2_feBitmask of used Sc2 ind linesmeta.numberINTEGERprincipalflag_Sc2_feQuality flag of Sc2_femeta.code.qual,stat.fitINTEGERprincipalTi_feNeutral Ti atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ti_feUncertainty Ti_festat.error;phys.abundREALprincipalnr_Ti_feBitmask of used Ti ind linesmeta.numberINTEGERprincipalflag_Ti_feQuality flag of Ti_femeta.code.qual,stat.fitINTEGERprincipalTi2_feSingle-ionised Ti2 atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ti2_feUncertainty Ti2_festat.error;phys.abundREALprincipalnr_Ti2_feBitmask of used Ti2 ind linesmeta.numberINTEGERprincipalflag_Ti2_feQuality flag of Ti2_femeta.code.qual,stat.fitINTEGERprincipalV_feNeutral V atomic abundance (final, 1D-LTE)phys.abundREALprincipale_V_feUncertainty V_festat.error;phys.abundREALprincipalnr_V_feBitmask of used V ind linesmeta.numberINTEGERprincipalflag_V_feQuality flag of V_femeta.code.qual,stat.fitINTEGERprincipalCr_feNeutral Cr atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Cr_feUncertainty Cr_festat.error;phys.abundREALprincipalnr_Cr_feBitmask of used Cr ind linesmeta.numberINTEGERprincipalflag_Cr_feQuality flag of Cr_femeta.code.qual,stat.fitINTEGERprincipalCr2_feSingle-ionised Cr2 atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Cr2_feUncertainty Cr2_festat.error;phys.abundREALprincipalnr_Cr2_feBitmask of used Cr2 ind linesmeta.numberINTEGERprincipalflag_Cr2_feQuality flag of Cr2_femeta.code.qual,stat.fitINTEGERprincipalMn_feNeutral Mn atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Mn_feUncertainty Mn_festat.error;phys.abundREALprincipalnr_Mn_feBitmask of used Mn ind linesmeta.numberINTEGERprincipalflag_Mn_feQuality flag of Mn_femeta.code.qual,stat.fitINTEGERprincipalCo_feNeutral Co atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Co_feUncertainty Co_festat.error;phys.abundREALprincipalnr_Co_feBitmask of used Co ind linesmeta.numberINTEGERprincipalflag_Co_feQuality flag of Co_femeta.code.qual,stat.fitINTEGERprincipalNi_feNeutral Ni atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ni_feUncertainty Ni_festat.error;phys.abundREALprincipalnr_Ni_feBitmask of used Ni ind linesmeta.numberINTEGERprincipalflag_Ni_feQuality flag of Ni_femeta.code.qual,stat.fitINTEGERprincipalCu_feNeutral Cu atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Cu_feUncertainty Cu_festat.error;phys.abundREALprincipalnr_Cu_feBitmask of used Cu ind linesmeta.numberINTEGERprincipalflag_Cu_feQuality flag of Cu_femeta.code.qual,stat.fitINTEGERprincipalZn_feNeutral Zn atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Zn_feUncertainty Zn_festat.error;phys.abundREALprincipalnr_Zn_feBitmask of used Zn ind linesmeta.numberINTEGERprincipalflag_Zn_feQuality flag of Zn_femeta.code.qual,stat.fitINTEGERprincipalRb_feNeutral Rb atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Rb_feUncertainty Rb_festat.error;phys.abundREALprincipalnr_Rb_feBitmask of used Rb ind linesmeta.numberINTEGERprincipalflag_Rb_feQuality flag of Rb_femeta.code.qual,stat.fitINTEGERprincipalSr_feNeutral Sr atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sr_feUncertainty Sr_festat.error;phys.abundREALprincipalnr_Sr_feBitmask of used Sr ind linesmeta.numberINTEGERprincipalflag_Sr_feQuality flag of Sr_femeta.code.qual,stat.fitINTEGERprincipalY_feNeutral Y atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Y_feUncertainty Y_festat.error;phys.abundREALprincipalnr_Y_feBitmask of used Y ind linesmeta.numberINTEGERprincipalflag_Y_feQuality flag of Y_femeta.code.qual,stat.fitINTEGERprincipalZr_feNeutral Zr atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Zr_feUncertainty Zr_festat.error;phys.abundREALprincipalnr_Zr_feBitmask of used Zr ind linesmeta.numberINTEGERprincipalflag_Zr_feQuality flag of Zr_femeta.code.qual,stat.fitINTEGERprincipalMo_feNeutral Mo atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Mo_feUncertainty Mo_festat.error;phys.abundREALprincipalnr_Mo_feBitmask of used Mo ind linesmeta.numberINTEGERprincipalflag_Mo_feQuality flag of Mo_femeta.code.qual,stat.fitINTEGERprincipalRu_feNeutral Ru atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ru_feUncertainty Ru_festat.error;phys.abundREALprincipalnr_Ru_feBitmask of used Ru ind linesmeta.numberINTEGERprincipalflag_Ru_feQuality flag of Ru_femeta.code.qual,stat.fitINTEGERprincipalBa_feSingle-ionised Ba atomic abundance (final, 1D-NLTE)phys.abundREALprincipale_Ba_feUncertainty Ba_festat.error;phys.abundREALprincipalnr_Ba_feBitmask of used Ba ind linesmeta.numberINTEGERprincipalflag_Ba_feQuality flag of Ba_femeta.code.qual,stat.fitINTEGERprincipalLa_feSingle-ionised La atomic abundance (final, 1D-LTE)phys.abundREALprincipale_La_feUncertainty La_festat.error;phys.abundREALprincipalnr_La_feBitmask of used La ind linesmeta.numberINTEGERprincipalflag_La_feQuality flag of La_femeta.code.qual,stat.fitINTEGERprincipalCe_feSingle-ionised Ce atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Ce_feUncertainty Ce_festat.error;phys.abundREALprincipalnr_Ce_feBitmask of used Ce ind linesmeta.numberINTEGERprincipalflag_Ce_feQuality flag of Ce_femeta.code.qual,stat.fitINTEGERprincipalNd_feSingle-ionised Nd atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Nd_feUncertainty Nd_festat.error;phys.abundREALprincipalnr_Nd_feBitmask of used Nd ind linesmeta.numberINTEGERprincipalflag_Nd_feQuality flag of Nd_femeta.code.qual,stat.fitINTEGERprincipalSm_feSingle-ionised Sm atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Sm_feUncertainty Sm_festat.error;phys.abundREALprincipalnr_Sm_feBitmask of used Sm ind linesmeta.numberINTEGERprincipalflag_Sm_feQuality flag of Sm_femeta.code.qual,stat.fitINTEGERprincipalEu_feSingle-ionised Eu atomic abundance (final, 1D-LTE)phys.abundREALprincipale_Eu_feUncertainty Eu_festat.error;phys.abundREALprincipalnr_Eu_feBitmask of used Eu ind linesmeta.numberINTEGERprincipalflag_Eu_feQuality flag of Eu_femeta.code.qual,stat.fitINTEGERprincipalrapropagated from Gaia DR2degpos.eq.ra;meta.mainREALindexedprincipalra_errorpropagated from Gaia DR2masstat.error;pos.eq.raREALprincipaldecpropagated from Gaia DR2degpos.eq.dec;meta.mainREALindexedprincipaldec_errorpropagated from Gaia DR2masstat.error;pos.eq.decREALprincipallpropagated from Gaia DR2degpos.galactic.lonREALprincipalbpropagated from Gaia DR2degpos.galactic.latREALprincipalparallaxpropagated from Gaia DR2maspos.parallaxREALprincipalparallax_errorpropagated from Gaia DR2masstat.error;pos.parallaxREALprincipalr_estpropagated from 2018AJ....156...58Bpcpos.distanceREALprincipalr_lopropagated from 2018AJ....156...58Bpcstat.error;stat.min;pos.distanceREALprincipalr_hipropagated from 2018AJ....156...58Bpcstat.error;stat.max;pos.distanceREALprincipalr_lenpropagated from 2018AJ....156...58Bpcstat.fit.param;pos.distanceREALprincipaldist_bstepDistance from BSTEP modellingfit.param;pos.distanceREALprincipale_dist_bstep1-sigma uncertainty of dist_bstepfit.param;stat.error;pos.distanceREALprincipalpmrapropagated from Gaia DR2mas yr-1pos.pm;pos.eq.raREALprincipalpmra_errorpropagated from Gaia DR2mas yr-1stat.error;pos.pm;pos.eq.raREALprincipalpmdecpropagated from Gaia DR2mas yr-1pos.pm;pos.eq.decREALprincipalpmdec_errorpropagated from Gaia DR2mas yr-1stat.error;pos.pm;pos.eq.decREALprincipalra_dec_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.eq.decREALprincipalra_parallax_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.parallaxREALprincipalra_pmra_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.pm;pos.eq.raREALprincipalra_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.eq.ra;pos.pm;pos.eq.decREALprincipaldec_parallax_corrpropagated from Gaia DR2stat.correlation;pos.eq.dec;pos.parallaxREALprincipaldec_pmra_corrpropagated from Gaia DR2stat.correlation;pos.eq.dec;pos.pm;pos.eq.raREALprincipaldec_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.eq.dec;pos.pm;pos.eq.decREALprincipalparallax_pmra_corrpropagated from Gaia DR2stat.correlation;pos.parallax;pos.pm;pos.eq.raREALprincipalparallax_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.parallax;pos.pm;pos.eq.decREALprincipalpmra_pmdec_corrpropagated from Gaia DR2stat.correlation;pos.pm;pos.eq.ra;pos.pm;pos.eq.decREALprincipalrv_galahSME fitted radial velocity from GALAH spectrakm s-1spect.dopplerVeloc.optREALprincipale_rv_galahUncertainty of rv_galahkm s-1stat.error;spect.dopplerVeloc.optREALprincipalcov_e_rv_galahSME covariance fitting uncertainty sme.vradkm s-1fit.param;stat.error;spect.dopplerVeloc.optREALprincipalrv_gaiapropagated from Gaia DR2km s-1spect.dopplerVeloc.optREALprincipale_rv_gaiapropagated from Gaia DR2km s-1stat.error;spect.dopplerVeloc.optREALprincipalred_flageduction pipeline quality flagmeta.code.qual;INTEGERprincipalebvSFD extinction valuemagphys.absorption.galREALprincipalsnr_c1_irafAverage SNR/px CCD1stat.snrREALprincipalsnr_c2_irafAverage SNR/px CCD2stat.snrREALprincipalsnr_c3_irafAverage SNR/px CCD3stat.snrREALprincipalsnr_c4_irafAverage SNR/px CCD4stat.snrREALprincipalflag_guessGUESS reduction pipeline quality flagmeta.code.qual,stat.fitINTEGERprincipalrv_guessReduction pipeline best radial velocitykm s-1fit.param;spect.dopplerVeloc.optREALprincipale_rv_guessReduction pipeline uncertainty radial velocitykm s-1fit.param;stat.error;spect.dopplerVeloc.optREALprincipalteff_guessReduction pipeline best teffKfit.param;phys.temperature.effectiveREALprincipallogg_guessReduction pipeline best logglog(cm.s**-2)fit.param;phys.gravityREALprincipalfeh_guessReduction pipeline best fe_hfit.param;phys.abund.FeREALprincipalrv_5854Local best fit to RV when fitting A(Ba5854)km s-1fit.param;spect.dopplerVeloc.optREALprincipalrv_6708Local best fit to RV when fitting A(Li6708)km s-1fit.param;spect.dopplerVeloc.optREALprincipalrv_6722Local best fit to RV when fitting A(Si6722)km s-1fit.param;spect.dopplerVeloc.optREALprincipalv_jkV magnitude estimated from 2MASS J and Ks magmagphot.magREALprincipalj_mpropagated from 2MASSmagphot.mag;em.IR.JREALprincipalj_msigcompropagated from 2MASSmagstat.error;phot.mag;em.IR.JREALprincipalh_mpropagated from 2MASSmagphot.mag;em.IR.HREALprincipalks_mpropagated from 2MASSmagphot.mag;em.IR.KREALprincipalks_msigcompropagated from 2MASSmagstat.error;phot.mag;em.IR.KREALprincipalph_qual_tmasspropagated from 2MASS ph_qualmeta.code.qual;photVARCHARprincipalw2mpropropagated from AllWISEmagphot.mag;em.IR.4-8umREALprincipalw2mpro_errorpropagated from AllWISEmagstat.error;phot.magREALprincipalph_qual_wisepropagated from AllWISE ph_qualmeta.code.qual;photVARCHARprincipala_ksUsed Ks band extinctionmagphys.absorption.galREALprincipale_a_ksUncertainty of a_ksmagstat.error,phys.absorption.galREALprincipalbc_ksUsed Bolometric Correction for Ks bandmagphot.mag.bc;em.IR.KREALprincipalruwepropagated from Gaia DR2stat.errorREALprincipalphot_g_mean_magpropagated from Gaia DR2magphot.mag;stat.mean;em.optREALprincipalbp_rppropagated from Gaia DR2magphot.colorREALprincipalgalah_dr3.vac_rvGALAH DR3 VAC RVsobject_idGALAH identifiermeta.id;meta.mainBIGINTindexedprincipalvbaryorigOriginal barycentric correction usedkm s-1obs.paramREALprincipalvbarycorrCorrect barycentric correctionkm s-1obs.paramREALprincipalrv_obstRadial Velocity with grav. redshift correctionkm s-1spect.dopplerVeloc.optREALprincipale_rv_obstUncertainty of rv_obstkm s-1stat.error;spect.dopplerVeloc.optREALprincipalrv_nogr_obstRadial Velocity without grav. redshift correctionkm s-1spect.dopplerVeloc.optREALprincipale_rv_nogr_obstUncertainty of rv_nogr_obstkm s-1stat.error;spect.dopplerVeloc.optREALprincipalMJD_localModified Julian Date, Middle of Exposuredtime.epochREALprincipalheliocentricJDHeliocentric Julian Datedtime.epochREALprincipalgalah_dr3.vac_dynamicsGALAH DR3 VAC Dyanmicssobject_idGALAH identifiermeta.id;meta.mainBIGINTindexedprincipalX_XYZBest-value heliocentric Galactic rectangular x-coordinatekpcpos.cartesian.x;pos.heliocentricREALprincipalY_XYZBest-value heliocentric Galactic rectangular y-coordinatekpcpos.cartesian.y;pos.heliocentricREALprincipalZ_XYZBest-value heliocentric Galactic rectangular z-coordinatekpcpos.cartesian.z;pos.heliocentricREALprincipalU_UVWBest-value heliocentric Galactic rectangular x-velocitykm s-1phys.vel.orbital;pos.heliocentricREALprincipalV_UVWBest-value heliocentric Galactic rectangular y-velocitykm s-1phys.vel.orbital;pos.heliocentricREALprincipalW_UVWBest-value heliocentric Galactic rectangular z-velocitykm s-1phys.vel.orbital;pos.heliocentricREALprincipalR_RzphiBest-value Galactocentric Radiuskpcpos.galactocentricREALprincipalz_RzphiBest-value Galactocentric heightkpcpos.galactocentricREALprincipalphi_RzphiBest-value Galactocentric azimuthradpos.galactocentricREALprincipalvR_RzphiBest-value Galactocentric radial velocitykm s-1phys.vel.orbital;pos.galactocentricREALprincipalvz_RzphiBest-value Galactocentric vertical velocitykm s-1phys.vel.orbital;pos.galactocentricREALprincipalvphi_RzphiBest-value Galactocentric azimuthal velocitykm s-1phys.vel.orbital;pos.galactocentricREALprincipalvT_RzphiBest-value Galactocentric tangential velocitykm s-1phys.vel.orbital;pos.galactocentricREALprincipalJ_RBest-value radial actionkm kpc s-1src.orbitalREALprincipalL_ZBest-value azimuthal action / angular momentumkm kpc s-1src.orbital;phys.angMomentumREALprincipalJ_ZBest-value vertical actionkm kpc s-1src.orbitalREALprincipalOmegarBest-value radial orbit frequencyGyr-1src.orbitalREALprincipalOmegaphiBest-value azimuthal orbit frequencyGyr-1src.orbitalREALprincipalOmegazBest-value vertical orbit frequencyGyr-1src.orbitalREALprincipaleccBest-value orbit eccentricitysrc.orbital.eccentricityREALprincipalzmaxBest-value maximum Galactocentric heightkpcsrc.orbitalREALprincipalR_periBest-value Galactocentric pericenter radiuskpcsrc.orbitalDOUBLEprincipalR_apBest-value Galactocentric apocenter radiuskpcsrc.orbitalREALprincipalEnergyBest-value orbit energykm-2 s-2src.orbital;phys.energyREALprincipalX_XYZ_55th Percentile MC heliocentric Galactic rectangular x-coordinatekpcstat.error;stat.min;pos.cartesian.x;pos.heliocentricREALprincipalX_XYZ_5050th Percentile MC heliocentric Galactic rectangular x-coordinatekpcstat.error;stat.median;pos.cartesian.x;pos.heliocentricREALprincipalX_XYZ_9595th Percentile MC heliocentric Galactic rectangular x-coordinatekpcstat.error;stat.max;pos.cartesian.x;pos.heliocentricREALprincipalY_XYZ_55th Percentile MC heliocentric Galactic rectangular y-coordinatekpcstat.error;stat.min;pos.cartesian.y;pos.heliocentricREALprincipalY_XYZ_5050th Percentile MC heliocentric Galactic rectangular y-coordinatekpcstat.error;stat.median;pos.cartesian.y;pos.heliocentricREALprincipalY_XYZ_9595th Percentile MC heliocentric Galactic rectangular y-coordinatekpcstat.error;stat.max;pos.cartesian.y;pos.heliocentricREALprincipalZ_XYZ_55th Percentile MC heliocentric Galactic rectangular z-coordinatekpcstat.error;stat.min;pos.cartesian.z;pos.heliocentricREALprincipalZ_XYZ_5050th Percentile MC heliocentric Galactic rectangular z-coordinatekpcstat.error;stat.median;pos.cartesian.z;pos.heliocentricREALprincipalZ_XYZ_9595th Percentile MC heliocentric Galactic rectangular z-coordinatekpcstat.error;stat.max;pos.cartesian.z;pos.heliocentricREALprincipalU_UVW_55th Percentile MC heliocentric Galactic rectangular x-velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.heliocentricREALprincipalU_UVW_5050th Percentile MC heliocentric Galactic rectangular x-velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.heliocentricREALprincipalU_UVW_9595th Percentile MC heliocentric Galactic rectangular x-velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.heliocentricREALprincipalV_UVW_55th Percentile MC heliocentric Galactic rectangular y-velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.heliocentricREALprincipalV_UVW_5050th Percentile MC heliocentric Galactic rectangular y-velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.heliocentricREALprincipalV_UVW_9595th Percentile MC heliocentric Galactic rectangular y-velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.heliocentricREALprincipalW_UVW_55th Percentile MC heliocentric Galactic rectangular z-velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.heliocentricREALprincipalW_UVW_5050th Percentile MC heliocentric Galactic rectangular z-velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.heliocentricREALprincipalW_UVW_9595th Percentile MC heliocentric Galactic rectangular z-velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.heliocentricREALprincipalR_Rzphi_55th Percentile MC Galactocentric Radiuskpcstat.error;stat.min;pos.galactocentricREALprincipalR_Rzphi_5050th Percentile MC Galactocentric Radiuskpcstat.error;stat.median;pos.galactocentricREALprincipalR_Rzphi_9595th Percentile MC Galactocentric Radiuskpcstat.error;stat.max;pos.galactocentricREALprincipalz_Rzphi_55th Percentile MC Galactocentric heightkpcstat.error;stat.min;pos.galactocentricREALprincipalz_Rzphi_5050th Percentile MC Galactocentric heightkpcstat.error;stat.median;pos.galactocentricREALprincipalz_Rzphi_9595th Percentile MC Galactocentric heightkpcstat.error;stat.max;pos.galactocentricREALprincipalphi_Rzphi_55th Percentile MC Galactocentric azimuthradstat.error;stat.min;pos.galactocentricREALprincipalphi_Rzphi_5050th Percentile MC Galactocentric azimuthradstat.error;stat.median;pos.galactocentricREALprincipalphi_Rzphi_9595th Percentile MC Galactocentric azimuthradstat.error;stat.max;pos.galactocentricREALprincipalvR_Rzphi_55th Percentile MC Galactocentric radial velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.galactocentricREALprincipalvR_Rzphi_5050th Percentile MC Galactocentric radial velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.galactocentricREALprincipalvR_Rzphi_9595th Percentile MC Galactocentric radial velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.galactocentricREALprincipalvz_Rzphi_55th Percentile MC Galactocentric vertical velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.galactocentricREALprincipalvz_Rzphi_5050th Percentile MC Galactocentric vertical velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.galactocentricREALprincipalvz_Rzphi_9595th Percentile MC Galactocentric vertical velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.galactocentricREALprincipalvphi_Rzphi_55th Percentile MC Galactocentric azimuthal velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.galactocentricREALprincipalvphi_Rzphi_5050th Percentile MC Galactocentric azimuthal velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.galactocentricREALprincipalvphi_Rzphi_9595th Percentile MC Galactocentric azimuthal velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.galactocentricREALprincipalvT_Rzphi_55th Percentile MC Galactocentric tangential velocitykm s-1stat.error;stat.min;phys.vel.orbital;pos.galactocentricREALprincipalvT_Rzphi_5050th Percentile MC Galactocentric tangential velocitykm s-1stat.error;stat.median;phys.vel.orbital;pos.galactocentricREALprincipalvT_Rzphi_9595th Percentile MC Galactocentric tangential velocitykm s-1stat.error;stat.max;phys.vel.orbital;pos.galactocentricREALprincipalJ_R_55th Percentile MC radial actionkm kpc s-1stat.error;stat.min;src.orbitalREALprincipalJ_R_5050th Percentile MC radial actionkm kpc s-1stat.error;stat.median;src.orbitalREALprincipalJ_R_9595th Percentile MC radial actionkm kpc s-1stat.error;stat.max;src.orbitalREALprincipalL_Z_55th Percentile MC azimuthal action / angular momentumkm kpc s-1stat.error;stat.min;src.orbital;phys.angMomentumREALprincipalL_Z_5050th Percentile MC azimuthal action / angular momentumkm kpc s-1stat.error;stat.median;src.orbital;phys.angMomentumREALprincipalL_Z_9595th Percentile MC azimuthal action / angular momentumkm kpc s-1stat.error;stat.max;src.orbital;phys.angMomentumREALprincipalJ_Z_55th Percentile MC vertical actionkm kpc s-1stat.error;stat.min;src.orbitalREALprincipalJ_Z_5050th Percentile MC vertical actionkm kpc s-1stat.error;stat.median;src.orbitalREALprincipalJ_Z_9595th Percentile MC vertical actionkm kpc s-1stat.error;stat.max;src.orbitalREALprincipalOmegar_55th Percentile MC radial orbit frequencyGyr-1stat.error;stat.min;src.orbitalREALprincipalOmegar_5050th Percentile MC radial orbit frequencyGyr-1stat.error;stat.median;src.orbitalREALprincipalOmegar_9595th Percentile MC radial orbit frequencyGyr-1stat.error;stat.max;src.orbitalREALprincipalOmegaphi_55th Percentile MC azimuthal orbit frequencyGyr-1stat.error;stat.min;src.orbitalREALprincipalOmegaphi_5050th Percentile MC azimuthal orbit frequencyGyr-1stat.error;stat.median;src.orbitalREALprincipalOmegaphi_9595th Percentile MC azimuthal orbit frequencyGyr-1stat.error;stat.max;src.orbitalREALprincipalOmegaz_55th Percentile MC vertical orbit frequencyGyr-1stat.error;stat.min;src.orbitalREALprincipalOmegaz_5050th Percentile MC vertical orbit frequencyGyr-1stat.error;stat.median;src.orbitalREALprincipalOmegaz_9595th Percentile MC vertical orbit frequencyGyr-1stat.error;stat.max;src.orbitalREALprincipalecc_55th Percentile MC orbit eccentricitystat.error;stat.min;src.orbital.eccentricityREALprincipalecc_5050th Percentile MC orbit eccentricitystat.error;stat.median;src.orbital.eccentricityREALprincipalecc_9595th Percentile MC orbit eccentricitystat.error;stat.max;src.orbital.eccentricityREALprincipalzmax_55th Percentile MC maximum Galactocentric heightkpcstat.error;stat.min;src.orbitalREALprincipalzmax_5050th Percentile MC maximum Galactocentric heightkpcstat.error;stat.median;src.orbitalREALprincipalzmax_9595th Percentile MC maximum Galactocentric heightkpcstat.error;stat.max;src.orbitalREALprincipalR_peri_55th Percentile MC Galactocentric pericenter radiuskpcstat.error;stat.min;src.orbitalDOUBLEprincipalR_peri_5050th Percentile MC Galactocentric pericenter radiuskpcstat.error;stat.median;src.orbitalDOUBLEprincipalR_peri_9595th Percentile MC Galactocentric pericenter radiuskpcstat.error;stat.max;src.orbitalDOUBLEprincipalR_ap_55th Percentile MC Galactocentric apocenter radiuskpcstat.error;stat.min;src.orbitalREALprincipalR_ap_5050th Percentile MC Galactocentric apocenter radiuskpcstat.error;stat.median;src.orbitalREALprincipalR_ap_9595th Percentile MC Galactocentric apocenter radiuskpcstat.error;stat.max;src.orbitalREALprincipalEnergy_55th Percentile MC orbit energykm-2 s-2stat.error;stat.min;src.orbital;phys.energyREALprincipalEnergy_5050th Percentile MC orbit energykm-2 s-2stat.error;stat.median;src.orbital;phys.energyREALprincipalEnergy_9595th Percentile MC orbit energykm-2 s-2stat.error;stat.max;src.orbital;phys.energyREALprincipalgalah_dr3.vac_agesGALAH DR3 VAC Agessobject_idGALAH identifiermeta.id;meta.mainBIGINTindexedprincipale16_radius_bstep16 percentile value for radius_bstepstat.error;stat.min;phys.size.radiusREALprincipale84_radius_bstep84 percentile value for radius_bstepstat.error;stat.max;phys.size.radiusREALprincipalis_redclump_bstepProbability to be a red clump star (1.0) or not (0.0) BSTEP-Mod.stat.probabilityDOUBLEprincipale_is_redclump_bstep1-sigma uncertainty of is_redclump_bstepstat.error;stat.stdev;stat.probabilityDOUBLEprincipale16_is_redclump_bstep16 percentile value for is_redclump_bstepstat.error;stat.min;stat.probabilityDOUBLEprincipale84_is_redclump_bstep84 percentile value for is_redclump_bstepstat.error;stat.max;stat.probabilityDOUBLEprincipaldistance_bstepDistance BSTEP-Mod.pos.distanceREALprincipale_distance_bstep1-sigma uncertainty of distance_bstepstat.error;stat.stdev;pos.distanceREALprincipale16_distance_bstep16 percentile value for distance_bstepstat.error;stat.min;pos.distanceREALprincipale84_distance_bstep84 percentile value for distance_bstepstat.error;stat.max;pos.distanceREALprincipalebv_bstepExtinction E(B-V) BSTEP-Mod.phys.absorption.galREALprincipale_ebv_bstep1-sigma uncertainty of ebv_bstepstat.error;stat.stdev;phys.absorption.galREALprincipale16_ebv_bstep16 percentile value for ebv_bstepstat.error;stat.min;phys.absorption.galREALprincipalage_bstepAge estimate BSTEP-Mod.time.ageREALprincipale_age_bstep1-sigma uncertainty of age_bstepstat.error;stat.stdev;time.ageREALprincipale16_age_bstep16 percentile value for age_bstepstat.error;stat.min;time.ageREALprincipale84_age_bstep84 percentile value for age_bstepstat.error;stat.max;time.ageREALprincipalm_act_bstepActual stellar mass after mass loss BSTEP-Mod.phys.massREALprincipale_m_act_bstep1-sigma uncertainty of m_act_bstepstat.error;stat.stdev;phys.massREALprincipale16_m_act_bstep16 percentile value for m_act_bstepstat.error;stat.min;phys.massREALprincipale84_m_act_bstep84 percentile value for m_act_bstepstat.error;stat.max;phys.massREALprincipalm_ini_bstepInitial stellar mass BSTEP-Mod.phys.massREALprincipale_m_ini_bstep1-sigma uncertainty of m_ini_bstepstat.error;stat.stdev;phys.massREALprincipale16_m_ini_bstep16 percentile value for m_ini_bstepstat.error;stat.min;phys.massREALprincipale84_m_ini_bstep84 percentile value for m_ini_bstepstat.error;stat.max;phys.massREALprincipalradius_bstepStellar Radius BSTEP-Mod.phys.size.radiusREALprincipale_radius_bstep1-sigma uncertainty of radius_bstepstat.error;stat.stdev;phys.size.radiusREALprincipale84_ebv_bstep84 percentile value for ebv_bstepstat.error;stat.max;phys.absorption.galREALprincipalteff_bstepEffective Temperature BSTEP-Mod.phys.temperature.effectiveREALprincipale_teff_bstep1-sigma uncertainty of teff_bstepstat.error;stat.stdev;phys.temperature.effectiveREALprincipale16_teff_bstep16 percentile value for teff_bstepstat.error;stat.min;phys.temperature.effectiveREALprincipale84_teff_bstep84 percentile value for teff_bstepstat.error;stat.max;phys.temperature.effectiveREALprincipallogg_bstepSurface gravity BSTEP-Mod.phys.gravityREALprincipale_logg_bstep1-sigma uncertainty of logg_bstepstat.error;stat.stdev;phys.gravityREALprincipale16_logg_bstep16 percentile value for logg_bstepstat.error;stat.min;phys.gravityREALprincipale84_logg_bstep84 percentile value for logg_bstepstat.error;stat.max;phys.gravityREALprincipalmeh_act_bstepSurface effective [M/H] BSTEP-Mod.phys.abundREALprincipale_meh_act_bstep1-sigma uncertainty of meh_act_bstepstat.error;stat.stdev;phys.abundREALprincipale16_meh_act_bstep16 percentile value for meh_act_bstepstat.error;stat.min;phys.abundREALprincipale84_meh_act_bstep84 percentile value for meh_act_bstepstat.error;stat.max;phys.abundREALprincipalmeh_ini_bstepIntial effective metallicity [M/H] from isochrones BSTEP-Mod.phys.abundREALprincipale_meh_ini_bstep1-sigma uncertainty of meh_ini_bstepstat.error;stat.stdev;phys.abundREALprincipale16_meh_ini_bstep16 percentile value for meh_ini_bstepstat.error;stat.min;phys.abundREALprincipale84_meh_ini_bstep84 percentile value for meh_ini_bstepstat.error;stat.max;phys.abundREALprincipallog_lum_bsteplog(Luminosity L/L_sun)phys.luminosityREALprincipale_log_lum_bstep1-sigma uncertainty of log_lum_bstepstat.error;stat.stdev;phys.luminosityREALprincipale16_log_lum_bstep16 percentile value for log_lum_bstepstat.error;stat.min;phys.luminosityREALprincipale84_log_lum_bstep84 percentile value for log_lum_bstepstat.error;stat.max;phys.luminosityREALprincipalg4jy_dr1The G4Jy catalogueg4jy_dr1.catalogue_18012020The G4Jy catalogueG4Jy_nameName of source belonging to the G4Jy Samplemeta.id.parent;src;meta.id;meta.mainVARCHARindexedprincipalG4Jy_componentLabel for an individual GLEAM componentmeta.id.partVARCHARprincipalncmp_GLEAMNumber of GLEAM components for this G4Jy sourcemeta.number;em.radio.170-231MHzSMALLINTprincipalGLEAM_nameName of the GLEAM componentmeta.idVARCHARprincipalrefitted_flagFlag for sources with re-fitted GLEAM measurementsmeta.codeSMALLINTprincipalcentroid_RAJ2000Right ascension for the centroid position (J2000)degpos.eq.ra;meta.main;em.radio.750-1500MHzDOUBLEindexedprincipalerr_centroid_RAJ2000Error on RA for the centroid positionarcsecstat.error;pos.eq.ra;em.radio.750-1500MHzREALprincipalcentroid_DEJ2000Declination for the centroid position (J2000)degpos.eq.dec;meta.main;em.radio.750-1500MHzDOUBLEindexedprincipalerr_centroid_DEJ2000Error on Dec for the centroid positionarcsecstat.error;pos.eq.dec;em.radio.750-1500MHzREALprincipalcentroid_flagFlag for sources with an updated centroid-positionmeta.code.qual;em.radio.750-1500MHzSMALLINTprincipalmorphologyMorphology of the source in NVSS/SUMSS/TGSSsrc.morphVARCHARprincipalncmp_NVSSorSUMSSNumber of NVSS/SUMSS componentsmeta.number;em.radio.750-1500MHzSMALLINTprincipalconfusion_flagFlag for sources affected by confusion in GLEAMmeta.code.qual;em.radio.750-1500MHzSMALLINTprincipalangular_size_limitIndicates that the angular size is an upper limitmeta.code.error;em.radio.750-1500MHzVARCHARprincipalangular_sizeAngular size in NVSS/SUMSSarcsecphys.angSize;em.radio.750-1500MHzREALprincipalS_NVSSorSUMSSTotal flux-density in NVSS/SUMSSJyphot.flux.density;em.radio.750-1500MHzREALprincipalerr_S_NVSSorSUMSSError on the total flux-density in NVSS/SUMSSJystat.error;phot.flux.density;em.radio.750-1500MHzREALprincipalFreqIndicates whether NVSS or SUMSS was usedMHzem.radio.750-1500MHzREALprincipalG4Jy_NVSS_alphaSpectral index between 151 and 1400 MHzspect.indexREALprincipalerr_G4Jy_NVSS_alphaError on spectral index between 151 and 1400 MHzstat.error;spect.indexREALprincipalG4Jy_SUMSS_alphaSpectral index between 151 and 843 MHzspect.indexREALprincipalerr_G4Jy_SUMSS_alphaError on spectral index between 151 and 843 MHzstat.error;spect.indexREALprincipalG4Jy_alphaFitted spectral-index using total GLEAM flux-densitiesstat.fit;spect.indexREALprincipalerr_G4Jy_alphaError on fitted, G4Jy spectral-indexstat.error;spect.indexREALprincipalreduced_chi2_G4Jy_alphaReduced chi^2 statistic for G4Jy spectral-index fitstat.fit.chi2;spect.indexREALprincipalhost_flagFlag for the type of host-galaxy identificationmeta.code.classVARCHARprincipalAllWISE_nameName of the host galaxy in AllWISEmeta.id.cross;srcVARCHARprincipalAllWISE_RAJ2000Right ascension for the host galaxy (J2000)degpos.eq.ra;em.IRREALprincipalAllWISE_DEJ2000Declination for the host galaxy (J2000)degpos.eq.dec;em.IRREALprincipalW1magW1 magnitude for the host galaxymagphot.mag;em.IRREALprincipalerr_W1magError on W1 magnitude for the host galaxymagstat.error;phot.mag;em.IRREALprincipalW2magW2 magnitude for the host galaxymagphot.mag;em.IRREALprincipalerr_W2magError on W2 magnitude for the host galaxymagstat.error;phot.mag;em.IRREALprincipalW3magW3 magnitude for the host galaxymagphot.mag;em.IRREALprincipalerr_W3magError on W3 magnitude for the host galaxymagstat.error;phot.mag;em.IRREALprincipalW4magW4 magnitude for the host galaxymagphot.mag;em.IRREALprincipalerr_W4magError on W4 magnitude for the host galaxymagstat.error;phot.mag;em.IRREALprincipalGLEAM_ra_strRight ascension for the GLEAM component (J2000)pos.eq.ra;em.radio.170-231MHzVARCHARprincipalGLEAM_dec_strDeclination for the GLEAM component (J2000)d:m:spos.eq.dec;em.radio.170-231MHzVARCHARprincipalGLEAM_RAJ2000Right ascension for the GLEAM component (J2000)degpos.eq.ra;em.radio.170-231MHzREALprincipalerr_GLEAM_RAJ2000Error on RA for the GLEAM componentdegstat.error;pos.eq.ra;em.radio.170-231MHzDOUBLEprincipalGLEAM_DEJ2000Declination for the GLEAM component (J2000)degpos.eq.dec;em.radio.170-231MHzREALprincipalerr_GLEAM_DEJ2000Error on Dec for the GLEAM componentdegstat.error;pos.eq.dec;em.radio.170-231MHzDOUBLEprincipalbackground_wideBackground level in wide-band imageJy / beamstat.median;phot.flux.density.sbREALprincipallocal_rms_wideLocal noise level in wide-band imageJy / beamstat.variance;phot.flux.density.sbREALprincipalpeak_flux_widePeak flux-density in wide-band imageJy / beamphot.flux.density.sb;em.radio.170-231MHzREALprincipalerr_peak_flux_wideUncertainty in fit for peak flux-density in wide-band imageJy / beamstat.error;phot.flux.density.sb;em.radio.170-231MHzREALprincipalint_flux_wideIntegrated flux-density in wide-band imageJyphot.flux.density;em.radio.170-231MHzREALprincipalerr_int_flux_wideUncertainty in fit for integrated flux-density in wide-band imageJystat.error;phot.flux.density;em.radio.170-231MHzREALprincipala_wideFitted semi-major axis in wide-band imagearcsecphys.angSize.smajAxis;meta.modelledREALprincipalerr_a_wideUncertainty in fitted semi-major axis in wide-band imagearcsecstat.error;phys.angSize.smajAxisREALprincipalb_wideFitted semi-minor axis in wide-band imagearcsecphys.angSize.sminAxis;meta.modelledREALprincipalerr_b_wideUncertainty in fitted semi-minor axis in wide-band imagearcsecstat.error;phys.angSize.sminAxisREALprincipalpa_wideFitted position angle in wide-band imagedegpos.posAng;meta.modelledREALprincipalerr_pa_wideUncertainty in fitted position angle in wide-band imagedegstat.error;pos.posAngREALprincipalresidual_mean_wideMean value of data-model in wide-band imageJy / beamstat.fit.residualREALprincipalresidual_std_wideStandard deviation of data-model in wide-band imageJy / beamstat.fit.residualREALprincipalpsf_a_wideSemi-major axis of the point spread function in wide-band imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_wideSemi-minor axis of the point spread function in wide-band imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_widePosition angle of the point spread function in wide-band imagedegpos.posAng;instr.det.psfREALprincipalbackground_076Background level in 72-80 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_076Local noise level in 72-80 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_076Peak flux-density in 72-80 MHz imageJy / beamphot.flux.density.sb;em.radio.72-80MHzREALprincipalerr_peak_flux_076Uncertainty in fit for peak flux-density in 72-80 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.72-80MHzREALprincipalint_flux_076Integrated flux-density in 72-80 MHz imageJyphot.flux.density;em.radio.72-80MHzREALprincipalerr_int_flux_076Uncertainty in fit for integrated flux-density in 72-80 MHz imageJystat.error;phot.flux.density;em.radio.72-80MHzREALprincipala_076Fitted semi-major axis in 72-80 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_076Fitted semi-minor axis in 72-80 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_076Fitted position angle in 72-80 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_076Mean value of data-model in 72-80 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_076Standard deviation of data-model in 72-80 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_076Semi-major axis of the point spread function in 72-80 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_076Semi-minor axis of the point spread function in 72-80 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_076Position angle of the point spread function in 72-80 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_084Background level in 80-88 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_084Local noise level in 80-88 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_084Peak flux-density in 80-88 MHz imageJy / beamphot.flux.density.sb;em.radio.80-88MHzREALprincipalerr_peak_flux_084Uncertainty in fit for peak flux-density in 80-88 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.80-88MHzREALprincipalint_flux_084Integrated flux-density in 80-88 MHz imageJyphot.flux.density;em.radio.80-88MHzREALprincipalerr_int_flux_084Uncertainty in fit for integrated flux-density in 80-88 MHz imageJystat.error;phot.flux.density;em.radio.80-88MHzREALprincipala_084Fitted semi-major axis in 80-88 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_084Fitted semi-minor axis in 80-88 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_084Fitted position angle in 80-88 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_084Mean value of data-model in 80-88 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_084Standard deviation of data-model in 80-88 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_084Semi-major axis of the point spread function in 80-88 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_084Semi-minor axis of the point spread function in 80-88 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_084Position angle of the point spread function in 80-88 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_092Background level in 88-95 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_092Local noise level in 88-95 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_092Peak flux-density in 88-95 MHz imageJy / beamphot.flux.density.sb;em.radio.88-95MHzREALprincipalerr_peak_flux_092Uncertainty in fit for peak flux-density in 88-95 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.88-95MHzREALprincipalint_flux_092Integrated flux-density in 88-95 MHz imageJyphot.flux.density;em.radio.88-95MHzREALprincipalerr_int_flux_092Uncertainty in fit for integrated flux-density in 88-95 MHz imageJystat.error;phot.flux.density;em.radio.88-95MHzREALprincipala_092Fitted semi-major axis in 88-95 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_092Fitted semi-minor axis in 88-95 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_092Fitted position angle in 88-95 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_092Mean value of data-model in 88-95 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_092Standard deviation of data-model in 88-95 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_092Semi-major axis of the point spread function in 88-95 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_092Semi-minor axis of the point spread function in 88-95 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_092Position angle of the point spread function in 88-95 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_099Background level in 95-103 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_099Local noise level in 95-103 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_099Peak flux-density in 95-103 MHz imageJy / beamphot.flux.density.sb;em.radio.95-103MHzREALprincipalerr_peak_flux_099Uncertainty in fit for peak flux-density in 95-103 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.95-103MHzREALprincipalint_flux_099Integrated flux-density in 95-103 MHz imageJyphot.flux.density;em.radio.95-103MHzREALprincipalerr_int_flux_099Uncertainty in fit for integrated flux-density in 95-103 MHz imageJystat.error;phot.flux.density;em.radio.95-103MHzREALprincipala_099Fitted semi-major axis in 95-103 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_099Fitted semi-minor axis in 95-103 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_099Fitted position angle in 95-103 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_099Mean value of data-model in 95-103 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_099Standard deviation of data-model in 95-103 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_099Semi-major axis of the point spread function in 95-103 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_099Semi-minor axis of the point spread function in 95-103 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_099Position angle of the point spread function in 95-103 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_107Background level in 103-111 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_107Local noise level in 103-111 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_107Peak flux-density in 103-111 MHz imageJy / beamphot.flux.density.sb;em.radio.103-111MHzREALprincipalerr_peak_flux_107Uncertainty in fit for peak flux-density in 103-111 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.103-111MHzREALprincipalint_flux_107Integrated flux-density in 103-111 MHz imageJyphot.flux.density;em.radio.103-111MHzREALprincipalerr_int_flux_107Uncertainty in fit for integrated flux-density in 103-111 MHz imageJystat.error;phot.flux.density;em.radio.103-111MHzREALprincipala_107Fitted semi-major axis in 103-111 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_107Fitted semi-minor axis in 103-111 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_107Fitted position angle in 103-111 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_107Mean value of data-model in 103-111 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_107Standard deviation of data-model in 103-111 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_107Semi-major axis of the point spread function in 103-111 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_107Semi-minor axis of the point spread function in 103-111 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_107Position angle of the point spread function in 103-111 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_115Background level in 111-118 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_115Local noise level in 111-118 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_115Peak flux-density in 111-118 MHz imageJy / beamphot.flux.density.sb;em.radio.111-118MHzREALprincipalerr_peak_flux_115Uncertainty in fit for peak flux-density in 111-118 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.111-118MHzREALprincipalint_flux_115Integrated flux-density in 111-118 MHz imageJyphot.flux.density;em.radio.111-118MHzREALprincipalerr_int_flux_115Uncertainty in fit for integrated flux-density in 111-118 MHz imageJystat.error;phot.flux.density;em.radio.111-118MHzREALprincipala_115Fitted semi-major axis in 111-118 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_115Fitted semi-minor axis in 111-118 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_115Fitted position angle in 111-118 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_115Mean value of data-model in 111-118 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_115Standard deviation of data-model in 111-118 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_115Semi-major axis of the point spread function in 111-118 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_115Semi-minor axis of the point spread function in 111-118 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_115Position angle of the point spread function in 111-118 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_122Background level in 118-126 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_122Local noise level in 118-126 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_122Peak flux-density in 118-126 MHz imageJy / beamphot.flux.density.sb;em.radio.118-126MHzREALprincipalerr_peak_flux_122Uncertainty in fit for peak flux-density in 118-126 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.118-126MHzREALprincipalint_flux_122Integrated flux-density in 118-126 MHz imageJyphot.flux.density;em.radio.118-126MHzREALprincipalerr_int_flux_122Uncertainty in fit for integrated flux-density in 118-126 MHz imageJystat.error;phot.flux.density;em.radio.118-126MHzREALprincipala_122Fitted semi-major axis in 118-126 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_122Fitted semi-minor axis in 118-126 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_122Fitted position angle in 118-126 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_122Mean value of data-model in 118-126 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_122Standard deviation of data-model in 118-126 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_122Semi-major axis of the point spread function in 118-126 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_122Semi-minor axis of the point spread function in 118-126 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_122Position angle of the point spread function in 118-126 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_130Background level in 126-134 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_130Local noise level in 126-134 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_130Peak flux-density in 126-134 MHz imageJy / beamphot.flux.density.sb;em.radio.126-134MHzREALprincipalerr_peak_flux_130Uncertainty in fit for peak flux-density in 126-134 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.126-134MHzREALprincipalint_flux_130Integrated flux-density in 126-134 MHz imageJyphot.flux.density;em.radio.126-134MHzREALprincipalerr_int_flux_130Uncertainty in fit for integrated flux-density in 126-134 MHz imageJystat.error;phot.flux.density;em.radio.126-134MHzREALprincipala_130Fitted semi-major axis in 126-134 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_130Fitted semi-minor axis in 126-134 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_130Fitted position angle in 126-134 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_130Mean value of data-model in 126-134 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_130Standard deviation of data-model in 126-134 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_130Semi-major axis of the point spread function in 126-134 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_130Semi-minor axis of the point spread function in 126-134 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_130Position angle of the point spread function in 126-134 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_143Background level in 139-147 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_143Local noise level in 139-147 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_143Peak flux-density in 139-147 MHz imageJy / beamphot.flux.density.sb;em.radio.139-147MHzREALprincipalerr_peak_flux_143Uncertainty in fit for peak flux-density in 139-147 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.139-147MHzREALprincipalint_flux_143Integrated flux-density in 139-147 MHz imageJyphot.flux.density;em.radio.139-147MHzREALprincipalerr_int_flux_143Uncertainty in fit for integrated flux-density in 139-147 MHz imageJystat.error;phot.flux.density;em.radio.139-147MHzREALprincipala_143Fitted semi-major axis in 139-147 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_143Fitted semi-minor axis in 139-147 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_143Fitted position angle in 139-147 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_143Mean value of data-model in 139-147 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_143Standard deviation of data-model in 139-147 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_143Semi-major axis of the point spread function in 139-147 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_143Semi-minor axis of the point spread function in 139-147 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_143Position angle of the point spread function in 139-147 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_151Background level in 147-154 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_151Local noise level in 147-154 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_151Peak flux-density in 147-154 MHz imageJy / beamphot.flux.density.sb;em.radio.147-154MHzREALprincipalerr_peak_flux_151Uncertainty in fit for peak flux-density in 147-154 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.147-154MHzREALprincipalint_flux_151Integrated flux-density in 147-154 MHz imageJyphot.flux.density;em.radio.147-154MHzREALprincipalerr_int_flux_151Uncertainty in fit for integrated flux-density in 147-154 MHz imageJystat.error;phot.flux.density;em.radio.147-154MHzREALprincipala_151Fitted semi-major axis in 147-154 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_151Fitted semi-minor axis in 147-154 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_151Fitted position angle in 147-154 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_151Mean value of data-model in 147-154 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_151Standard deviation of data-model in 147-154 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_151Semi-major axis of the point spread function in 147-154 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_151Semi-minor axis of the point spread function in 147-154 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_151Position angle of the point spread function in 147-154 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_158Background level in 154-162 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_158Local noise level in 154-162 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_158Peak flux-density in 154-162 MHz imageJy / beamphot.flux.density.sb;em.radio.154-162MHzREALprincipalerr_peak_flux_158Uncertainty in fit for peak flux-density in 154-162 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.154-162MHzREALprincipalint_flux_158Integrated flux-density in 154-162 MHz imageJyphot.flux.density;em.radio.154-162MHzREALprincipalerr_int_flux_158Uncertainty in fit for integrated flux-density in 154-162 MHz imageJystat.error;phot.flux.density;em.radio.154-162MHzREALprincipala_158Fitted semi-major axis in 154-162 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_158Fitted semi-minor axis in 154-162 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_158Fitted position angle in 154-162 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_158Mean value of data-model in 154-162 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_158Standard deviation of data-model in 154-162 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_158Semi-major axis of the point spread function in 154-162 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_158Semi-minor axis of the point spread function in 154-162 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_158Position angle of the point spread function in 154-162 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_166Background level in 162-170 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_166Local noise level in 162-170 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_166Peak flux-density in 162-170 MHz imageJy / beamphot.flux.density.sb;em.radio.162-170MHzREALprincipalerr_peak_flux_166Uncertainty in fit for peak flux-density in 162-170 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.162-170MHzREALprincipalint_flux_166Integrated flux-density in 162-170 MHz imageJyphot.flux.density;em.radio.162-170MHzREALprincipalerr_int_flux_166Uncertainty in fit for integrated flux-density in 162-170 MHz imageJystat.error;phot.flux.density;em.radio.162-170MHzREALprincipala_166Fitted semi-major axis in 162-170 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_166Fitted semi-minor axis in 162-170 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_166Fitted position angle in 162-170 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_166Mean value of data-model in 162-170 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_166Standard deviation of data-model in 162-170 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_166Semi-major axis of the point spread function in 162-170 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_166Semi-minor axis of the point spread function in 162-170 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_166Position angle of the point spread function in 162-170 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_174Background level in 170-177 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_174Local noise level in 170-177 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_174Peak flux-density in 170-177 MHz imageJy / beamphot.flux.density.sb;em.radio.170-177MHzREALprincipalerr_peak_flux_174Uncertainty in fit for peak flux-density in 170-177 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.170-177MHzREALprincipalint_flux_174Integrated flux-density in 170-177 MHz imageJyphot.flux.density;em.radio.170-177MHzREALprincipalerr_int_flux_174Uncertainty in fit for integrated flux-density in 170-177 MHz imageJystat.error;phot.flux.density;em.radio.170-177MHzREALprincipala_174Fitted semi-major axis in 170-177 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_174Fitted semi-minor axis in 170-177 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_174Fitted position angle in 170-177 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_174Mean value of data-model in 170-177 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_174Standard deviation of data-model in 170-177 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_174Semi-major axis of the point spread function in 170-177 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_174Semi-minor axis of the point spread function in 170-177 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_174Position angle of the point spread function in 170-177 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_181Background level in 177-185 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_181Local noise level in 177-185 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_181Peak flux-density in 177-185 MHz imageJy / beamphot.flux.density.sb;em.radio.177-185MHzREALprincipalerr_peak_flux_181Uncertainty in fit for peak flux-density in 177-185 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.177-185MHzREALprincipalint_flux_181Integrated flux-density in 177-185 MHz imageJyphot.flux.density;em.radio.177-185MHzREALprincipalerr_int_flux_181Uncertainty in fit for integrated flux-density in 177-185 MHz imageJystat.error;phot.flux.density;em.radio.177-185MHzREALprincipala_181Fitted semi-major axis in 177-185 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_181Fitted semi-minor axis in 177-185 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_181Fitted position angle in 177-185 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_181Mean value of data-model in 177-185 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_181Standard deviation of data-model in 177-185 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_181Semi-major axis of the point spread function in 177-185 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_181Semi-minor axis of the point spread function in 177-185 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_181Position angle of the point spread function in 177-185 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_189Background level in 185-193 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_189Local noise level in 185-193 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_189Peak flux-density in 185-193 MHz imageJy / beamphot.flux.density.sb;em.radio.185-193MHzREALprincipalerr_peak_flux_189Uncertainty in fit for peak flux-density in 185-193 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.185-193MHzREALprincipalint_flux_189Integrated flux-density in 185-193 MHz imageJyphot.flux.density;em.radio.185-193MHzREALprincipalerr_int_flux_189Uncertainty in fit for integrated flux-density in 185-193 MHz imageJystat.error;phot.flux.density;em.radio.185-193MHzREALprincipala_189Fitted semi-major axis in 185-193 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_189Fitted semi-minor axis in 185-193 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_189Fitted position angle in 185-193 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_189Mean value of data-model in 185-193 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_189Standard deviation of data-model in 185-193 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_189Semi-major axis of the point spread function in 185-193 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_189Semi-minor axis of the point spread function in 185-193 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_189Position angle of the point spread function in 185-193 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_197Background level in 193-200 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_197Local noise level in 193-200 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_197Peak flux-density in 193-200 MHz imageJy / beamphot.flux.density.sb;em.radio.193-200MHzREALprincipalerr_peak_flux_197Uncertainty in fit for peak flux-density in 193-200 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.193-200MHzREALprincipalint_flux_197Integrated flux-density in 193-200 MHz imageJyphot.flux.density;em.radio.193-200MHzREALprincipalerr_int_flux_197Uncertainty in fit for integrated flux-density in 193-200 MHz imageJystat.error;phot.flux.density;em.radio.193-200MHzREALprincipala_197Fitted semi-major axis in 193-200 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_197Fitted semi-minor axis in 193-200 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_197Fitted position angle in 193-200 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_197Mean value of data-model in 193-200 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_197Standard deviation of data-model in 193-200 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_197Semi-major axis of the point spread function in 193-200 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_197Semi-minor axis of the point spread function in 193-200 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_197Position angle of the point spread function in 193-200 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_204Background level in 200-208 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_204Local noise level in 200-208 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_204Peak flux-density in 200-208 MHz imageJy / beamphot.flux.density.sb;em.radio.200-208MHzREALprincipalerr_peak_flux_204Uncertainty in fit for peak flux-density in 200-208 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.200-208MHzREALprincipalint_flux_204Integrated flux-density in 200-208 MHz imageJyphot.flux.density;em.radio.200-208MHzREALprincipalerr_int_flux_204Uncertainty in fit for integrated flux-density in 200-208 MHz imageJystat.error;phot.flux.density;em.radio.200-208MHzREALprincipala_204Fitted semi-major axis in 200-208 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_204Fitted semi-minor axis in 200-208 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_204Fitted position angle in 200-208 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_204Mean value of data-model in 200-208 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_204Standard deviation of data-model in 200-208 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_204Semi-major axis of the point spread function in 200-208 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_204Semi-minor axis of the point spread function in 200-208 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_204Position angle of the point spread function in 200-208 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_212Background level in 208-216 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_212Local noise level in 208-216 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_212Peak flux-density in 208-216 MHz imageJy / beamphot.flux.density.sb;em.radio.208-216MHzREALprincipalerr_peak_flux_212Uncertainty in fit for peak flux-density in 208-216 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.208-216MHzREALprincipalint_flux_212Integrated flux-density in 208-216 MHz imageJyphot.flux.density;em.radio.208-216MHzREALprincipalerr_int_flux_212Uncertainty in fit for integrated flux-density in 208-216 MHz imageJystat.error;phot.flux.density;em.radio.208-216MHzREALprincipala_212Fitted semi-major axis in 208-216 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_212Fitted semi-minor axis in 208-216 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_212Fitted position angle in 208-216 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_212Mean value of data-model in 208-216 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_212Standard deviation of data-model in 208-216 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_212Semi-major axis of the point spread function in 208-216 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_212Semi-minor axis of the point spread function in 208-216 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_212Position angle of the point spread function in 208-216 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_220Background level in 216-223 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_220Local noise level in 216-223 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_220Peak flux-density in 216-223 MHz imageJy / beamphot.flux.density.sb;em.radio.216-223MHzREALprincipalerr_peak_flux_220Uncertainty in fit for peak flux-density in 216-223 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.216-223MHzREALprincipalint_flux_220Integrated flux-density in 216-223 MHz imageJyphot.flux.density;em.radio.216-223MHzREALprincipalerr_int_flux_220Uncertainty in fit for integrated flux-density in 216-223 MHz imageJystat.error;phot.flux.density;em.radio.216-223MHzREALprincipala_220Fitted semi-major axis in 216-223 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_220Fitted semi-minor axis in 216-223 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_220Fitted position angle in 216-223 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_220Mean value of data-model in 216-223 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_220Standard deviation of data-model in 216-223 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_220Semi-major axis of the point spread function in 216-223 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_220Semi-minor axis of the point spread function in 216-223 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_220Position angle of the point spread function in 216-223 MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_227Background level in 223-231 MHz imageJy / beamstat.median;src;phot.flux.density.sbREALprincipallocal_rms_227Local noise level in 223-231 MHz imageJy / beamstat.variance;src;phot.flux.density.sbREALprincipalpeak_flux_227Peak flux-density in 223-231 MHz imageJy / beamphot.flux.density.sb;em.radio.223-231MHzREALprincipalerr_peak_flux_227Uncertainty in fit for peak flux-density in 223-231 MHz imageJy / beamstat.error;phot.flux.density.sb;em.radio.223-231MHzREALprincipalint_flux_227Integrated flux-density in 223-231 MHz imageJyphot.flux.density;em.radio.223-231MHzREALprincipalerr_int_flux_227Uncertainty in fit for integrated flux-density in 223-231 MHz imageJystat.error;phot.flux.density;em.radio.223-231MHzREALprincipala_227Fitted semi-major axis in 223-231 MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_227Fitted semi-minor axis in 223-231 MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_227Fitted position angle in 223-231 MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_227Mean value of data-model in 223-231 MHz imageJy / beamstat.fit.residualREALprincipalresidual_std_227Standard deviation of data-model in 223-231 MHz imageJy / beamstat.fit.residualREALprincipalpsf_a_227Semi-major axis of the point spread function in 223-231 MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_227Semi-minor axis of the point spread function in 223-231 MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_227Position angle of the point spread function in 223-231 MHz imagedegpos.posAng;instr.det.psfREALprincipalGLEAM_alphaFitted spectral-index using GLEAM-component flux-densitiesstat.fit;spect.indexREALprincipalerr_GLEAM_alphaError on fitted, GLEAM spectral-indexstat.error;spect.indexREALprincipalreduced_chi2_GLEAM_alphaReduced chi^2 statistic for GLEAM spectral-index fitstat.fit.chi2;spect.indexREALprincipaltotal_int_flux_076Total, integrated flux-density in 72-80 MHz imageJyphot.flux.density;em.radio.72-80MHzREALprincipalerr_total_int_flux_076Error on total, integrated flux-density in 72-80 MHz imageJystat.error;phot.flux.density;em.radio.72-80MHzREALprincipaltotal_int_flux_084Total, integrated flux-density in 80-88 MHz imageJyphot.flux.density;em.radio.80-88MHzREALprincipalerr_total_int_flux_084Error on total, integrated flux-density in 80-88 MHz imageJystat.error;phot.flux.density;em.radio.80-88MHzREALprincipaltotal_int_flux_092Total, integrated flux-density in 88-95 MHz imageJyphot.flux.density;em.radio.88-95MHzREALprincipalerr_total_int_flux_092Error on total, integrated flux-density in 88-95 MHz imageJystat.error;phot.flux.density;em.radio.88-95MHzREALprincipaltotal_int_flux_099Total, integrated flux-density in 95-103 MHz imageJyphot.flux.density;em.radio.95-103MHzREALprincipalerr_total_int_flux_099Error on total, integrated flux-density in 95-103 MHz imageJystat.error;phot.flux.density;em.radio.95-103MHzREALprincipaltotal_int_flux_107Total, integrated flux-density in 103-111 MHz imageJyphot.flux.density;em.radio.103-111MHzREALprincipalerr_total_int_flux_107Error on total, integrated flux-density in 103-111 MHz imageJystat.error;phot.flux.density;em.radio.103-111MHzREALprincipaltotal_int_flux_115Total, integrated flux-density in 111-118 MHz imageJyphot.flux.density;em.radio.111-118MHzREALprincipalerr_total_int_flux_115Error on total, integrated flux-density in 111-118 MHz imageJystat.error;phot.flux.density;em.radio.111-118MHzREALprincipaltotal_int_flux_122Total, integrated flux-density in 118-126 MHz imageJyphot.flux.density;em.radio.118-126MHzREALprincipalerr_total_int_flux_122Error on total, integrated flux-density in 118-126 MHz imageJystat.error;phot.flux.density;em.radio.118-126MHzREALprincipaltotal_int_flux_130Total, integrated flux-density in 126-134 MHz imageJyphot.flux.density;em.radio.126-134MHzREALprincipalerr_total_int_flux_130Error on total, integrated flux-density in 126-134 MHz imageJystat.error;phot.flux.density;em.radio.126-134MHzREALprincipaltotal_int_flux_143Total, integrated flux-density in 139-147 MHz imageJyphot.flux.density;em.radio.139-147MHzREALprincipalerr_total_int_flux_143Error on total, integrated flux-density in 139-147 MHz imageJystat.error;phot.flux.density;em.radio.139-147MHzREALprincipaltotal_int_flux_151Total, integrated flux-density in 147-154 MHz imageJyphot.flux.density;em.radio.147-154MHzREALprincipalerr_total_int_flux_151Error on total, integrated flux-density in 147-154 MHz imageJystat.error;phot.flux.density;em.radio.147-154MHzREALprincipaltotal_int_flux_158Total, integrated flux-density in 154-162 MHz imageJyphot.flux.density;em.radio.154-162MHzREALprincipalerr_total_int_flux_158Error on total, integrated flux-density in 154-162 MHz imageJystat.error;phot.flux.density;em.radio.154-162MHzREALprincipaltotal_int_flux_166Total, integrated flux-density in 162-170 MHz imageJyphot.flux.density;em.radio.162-170MHzREALprincipalerr_total_int_flux_166Error on total, integrated flux-density in 162-170 MHz imageJystat.error;phot.flux.density;em.radio.162-170MHzREALprincipaltotal_int_flux_174Total, integrated flux-density in 170-177 MHz imageJyphot.flux.density;em.radio.170-177MHzREALprincipalerr_total_int_flux_174Error on total, integrated flux-density in 170-177 MHz imageJystat.error;phot.flux.density;em.radio.170-177MHzREALprincipaltotal_int_flux_181Total, integrated flux-density in 177-185 MHz imageJyphot.flux.density;em.radio.177-185MHzREALprincipalerr_total_int_flux_181Error on total, integrated flux-density in 177-185 MHz imageJystat.error;phot.flux.density;em.radio.177-185MHzREALprincipaltotal_int_flux_189Total, integrated flux-density in 185-193 MHz imageJyphot.flux.density;em.radio.185-193MHzREALprincipalerr_total_int_flux_189Error on total, integrated flux-density in 185-193 MHz imageJystat.error;phot.flux.density;em.radio.185-193MHzREALprincipaltotal_int_flux_197Total, integrated flux-density in 193-200 MHz imageJyphot.flux.density;em.radio.193-200MHzREALprincipalerr_total_int_flux_197Error on total, integrated flux-density in 193-200 MHz imageJystat.error;phot.flux.density;em.radio.193-200MHzREALprincipaltotal_int_flux_204Total, integrated flux-density in 200-208 MHz imageJyphot.flux.density;em.radio.200-208MHzREALprincipalerr_total_int_flux_204Error on total, integrated flux-density in 200-208 MHz imageJystat.error;phot.flux.density;em.radio.200-208MHzREALprincipaltotal_int_flux_212Total, integrated flux-density in 208-216 MHz imageJyphot.flux.density;em.radio.208-216MHzREALprincipalerr_total_int_flux_212Error on total, integrated flux-density in 208-216 MHz imageJystat.error;phot.flux.density;em.radio.208-216MHzREALprincipaltotal_int_flux_220Total, integrated flux-density in 216-223 MHz imageJyphot.flux.density;em.radio.216-223MHzREALprincipalerr_total_int_flux_220Error on total, integrated flux-density in 216-223 MHz imageJystat.error;phot.flux.density;em.radio.216-223MHzREALprincipaltotal_int_flux_227Total, integrated flux-density in 223-231 MHz imageJyphot.flux.density;em.radio.223-231MHzREALprincipalerr_total_int_flux_227Error on total, integrated flux-density in 223-231 MHz imageJystat.error;phot.flux.density;em.radio.223-231MHzREALprincipal2dfgrs_fdr<p>The 2dF Galaxy Redshift Survey (2dFGRS) is a major spectroscopic survey taking full advantage of the unique capabilities of the 2dF facility built by the Anglo-Australian Observatory. The 2dFGRS is integrated with the 2dF QSO survey (Croom et al., 2004). The 2dFGRS obtained spectra for 245591 objects, mainly galaxies, brighter than a nominal extinction-corrected magnitude limit of bJ=19.45. Reliable (quality>=3) redshifts were obtained for 221414 galaxies. The galaxies cover an area of approximately 1500 square degrees selected from the extended APM Galaxy Survey in three regions: a North Galactic Pole (NGP) strip, a South Galactic Pole (SGP) strip, and random fields scattered around the SGP strip. Redshifts are measured from spectra covering 3600-8000 Angstroms at a two-pixel resolution of 9.0 Angstrom and a median S/N of 13 per pixel. All redshift identifications are visually checked and assigned a quality parameter Q in the range 1-5; Q>=3 redshifts are 98.4% reliable and have an rms uncertainty of 85 km/s. The overall redshift completeness for Q>=3 redshifts is 91.8% but this varies with magnitude from 99% for the brightest galaxies to 90% for objects at the survey limit (Colless et al., 2007).</p>2dfgrs_fdr.spec_allAll the spectroscopic informationserial2dFGRS serial numberNonemeta.idINTEGERprincipalname2dFGRS nameNonemeta.id;meta.mainVARCHARindexedprincipalUKSTUKST sky survey field numberNoneobs.fieldINTEGERprincipalOBSRUNObserving run year and monthNoneobs.param;obsVARCHARprincipalTDFgg2dFGRS field number (+NGP,-SGP)Noneobs.fieldINTEGERprincipalbestIn extension 0, extension number with best spectrum; in extension>0, 1 if best spectrum and 0 otherwiseNonemeta.codeINTEGERprincipalspectraNumber of spectra for this objectNonemeta.numberINTEGERprincipalextnumExtension numberNonemeta.codeINTEGERprincipalOBSNAMEObserved object nameNonemeta.idVARCHARprincipalOBSRAObserved RAradianspos.eq.raVARCHARprincipalOBSDECObserved Decradianspos.eq.decVARCHARprincipalMATCH_DRPosition match dr in arcsecarcsecpos.angDistanceVARCHARprincipalZRaw measured redshiftNonesrc.redshiftVARCHARprincipalZ_HELIOHeliocentric corrected redshiftNonesrc.redshift;pos.heliocentricVARCHARprincipalQUALITYRedshift measurement quality (quality=1-5; reliable redshifts have quality>=3)Nonemeta.code.qual;src.redshiftINTEGERprincipalABEMMARedshift type (abs=1, emi=2, man=3)Nonemeta.code;src.redshiftINTEGERprincipalNMBESTNumber of emission lines for Z_EMINonemeta.numberINTEGERprincipalNGOODNumber of good emmision linesNonemeta.numberINTEGERprincipalZ_EMIEmission redshiftNonesrc.redshift;pos.heliocentricVARCHARprincipalQ_Z_EMIEmission redshift qualityNonemeta.code.qual;src.redshiftVARCHARprincipalKBESTRCross-correlation template from best spectrumNonestat.fit.paramINTEGERprincipalR_CRCORCross-correlation peakNonestat.fit.paramVARCHARprincipalZ_ABSCross-correlation redshiftNonestat.fit.paramVARCHARprincipalQ_Z_ABSCross-correlation qualityNonemeta.code.qualVARCHARprincipalQ_FINALSuggested quality for redshiftNonemeta.code.qualVARCHARprincipalIALTERNo ideaNonemeta.crypticINTEGERprincipalZ_COMMObservers CommentNonemeta.noteVARCHARprincipalTHPUTFibre ThroughputNoneinstr.paramVARCHARprincipalSPFILE2dF reduced data fileNonemeta.fileVARCHARprincipalPLATE2dF plate number (0 or 1); -99 if noneNoneobs.paramINTEGERprincipalPIVOT2dF pivot numberNoneobs.paramINTEGERprincipalFIBRE2dF fibre numberNoneobs.paramINTEGERprincipalGRS_DATE2dF YYMMDD observed date; -99 if noneNonetime.epochVARCHARprincipalUTDATEUT date of observationYYYY:MM:DDtime.epoch;obsVARCHARprincipalSPECTID2dF spectrograph IDNonemeta.id;instrVARCHARprincipalGRATID2dF grating IDNonemeta.id;instrVARCHARprincipalGRATLPMM2dF grating line per mmNoneinstr.paramINTEGERprincipalGRATBLAZ2dF grating blaze directionNoneinstr.paramVARCHARprincipalGRATANGL2dF grating angledeginstr.paramVARCHARprincipalLAMBDACCentral wavelengthAngstromem.wl.centralVARCHARprincipalOBJX2dF object x positionpixelspos.cartesian.xINTEGERprincipalOBJY2dF object y positionpixelspos.cartesian.yINTEGERprincipalOBJXERR2dF object x position errorpixelsstat.error;pos.cartesian.xINTEGERprincipalOBJYERR2dF object y position errorpixelsstat.error;pos.cartesian.yINTEGERprincipalOBJMAG2dF object magnitudemagphot.magVARCHARprincipalTHETA2dF fibre angledeginstr.paramVARCHARprincipalPTRTYPE2dF ptrtypeNonemeta.codeVARCHARprincipalPID2dF pidNonemeta.codeINTEGERprincipalOBSFLD2dF observed field numberNoneobs.fieldVARCHARprincipalNCOMBNumber of frames combinedNonemeta.numberINTEGERprincipalREFRUNAAT Run number of reference frameNoneobs.paramINTEGERprincipalREFEXPExposure time (secs) of reference runsobs.exposureVARCHARprincipalSNRMedian signal-to-noise ratio per pixelNonestat.snr;stat.medianVARCHARprincipalOBSRAJ2000Observed RA (J2000)degpos.eq.raVARCHARprincipalOBSDECJ2000Observed Dec (J2000)degpos.eq.decVARCHARprincipal2dfgrs_fdr.phot_allAll the photometric informationserial2dFGRS serial numberNonemeta.idINTEGERprincipalalphaR.A. (B1950) in radiansradianspos.eq.raVARCHARprincipaldeltaDec. (B1950) in radiansradianspos.eq.decVARCHARprincipalname2dFGRS nameNonemeta.id;meta.mainVARCHARindexedprincipalraRA (B1950) in HH MM SS.SShh mm ss.sspos.eq.raVARCHARprincipaldecDEC (B1950) in DD MM SS.Sdd mm ss.sspos.eq.decVARCHARprincipalra2000RA (J2000) in HH MM SS.SShh mm ss.sspos.eq.ra;meta.mainVARCHARindexedprincipaldec2000DEC (J2000) in DD MM SS.Sdd mm ss.sspos.eq.dec;meta.mainVARCHARindexedprincipall2Galactic longitudedegpos.galactic.lonVARCHARprincipalb2Galactic latitudedegpos.galactic.latVARCHARprincipalUKSTUKST sky survey field numberNoneobs.fieldINTEGERprincipalbestIn extension 0, extension number with best spectrum; in extension>0, 1 if best spectrum and 0 otherwiseNonemeta.codeINTEGERprincipalspectraNumber of spectra for this objectNonemeta.numberINTEGERprincipalextnumExtension numberNonemeta.codeINTEGERprincipalSEQNUMSequence number: Database Primary KeyNonemeta.idINTEGERprincipalNAME_2dFgg2dFgg assigned nameNonemeta.idVARCHARprincipalRA_radiansRA in radiansradianspos.eq.raVARCHARprincipalDEC_radiansDec in radiansradianspos.eq.decVARCHARprincipalAPMEQNXEquinox of RA and DecNonetime.equinoxVARCHARprincipalBJSELFinal bj mag used in the object selectionmagphot.mag;em.opt.BVARCHARprincipalPROBpsi classification parameterNonesrc.morph.paramVARCHARprincipalPARKk classification parameterNonesrc.morph.paramVARCHARprincipalPARMUmu classification parameterNonesrc.morph.paramVARCHARprincipalIGALFinal class flag (equals 1 for a galaxy)Nonesrc.class.starGalaxyINTEGERprincipalJONEyeball class flagNonesrc.classINTEGERprincipalORIENTOrientation in degrees clockwise from E-Wdegpos.posAngVARCHARprincipalECCENTEccentricityNonesrc.morph.paramVARCHARprincipalAREAIsophotal area in pixelspixelsphys.areaVARCHARprincipalBJGFinal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalIFIELDUKST fieldNoneobs.fieldINTEGERprincipalREGIONGSSS Region nameNoneobs.fieldVARCHARprincipalOBJEQNXEquinox of the plate reference frameNonetime.equinoxVARCHARprincipalOBJRARA in radiansradianspos.eq.raVARCHARprincipalOBJDECDec in radiansradianspos.eq.decVARCHARprincipalBJSELOLDOriginal bj magnitude with extinction correction used in the object selectionmagphot.mag;em.opt.BVARCHARprincipalBJG_OLDOriginal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJSEL100bj mag used in the object selection (100k)magphot.mag;em.opt.BVARCHARprincipalBJG_100bj without extinction correction (100k)magphot.mag;em.opt.BVARCHARprincipalGALEXTGalactic extinctionmagphys.absorptionVARCHARprincipalVISCHECKVisual check flagNonemeta.codeINTEGERprincipalVISCOMMVisual check commentsNonemeta.noteVARCHARprincipalSBRAObject RA (J2000.0)degpos.eq.raVARCHARprincipalSBDECObject declination (J2000.0)degpos.eq.decVARCHARprincipalSBBJMAGUK-J (Bj) magnitudemagphot.mag;em.opt.BVARCHARprincipalSBAREATotal areapixelsphys.areaINTEGERprincipalSBAIWeighted semi-major axis0.01 micronsphys.angSize.smajAxisINTEGERprincipalSBBIWeighted semi-minor axis0.01 micronsphys.angSize.sminAxisINTEGERprincipalSBPACelestial position angledegpos.posAngINTEGERprincipalSBCLASSClassification flagNonemeta.codeINTEGERprincipalSBSIGMAProfile classification statisticNonestat.valueVARCHARprincipalSBBLENDDeblending flagNonemeta.codeINTEGERprincipalSBQUALQuality flagNonemeta.code.qualINTEGERprincipalSBAPMAPM-Supercosmos Bj-band match classificationNonemeta.codeINTEGERprincipalSRRAObject RA (J2000.0)degpos.eq.raVARCHARprincipalSRDECObject declination (J2000.0)degpos.eq.decVARCHARprincipalSRRMAGUK-J (R) magnitudemagphot.mag;em.opt.RVARCHARprincipalSRAREATotal areapixelsphys.areaINTEGERprincipalSRAIWeighted semi-major axis0.01 micronsphys.angSize.smajAxisINTEGERprincipalSRBIWeighted semi-minor axis0.01 micronsphys.angSize.sminAxisINTEGERprincipalSRPACelestial position angledegpos.posAngINTEGERprincipalSRCLASSClassification flagNonemeta.codeINTEGERprincipalSRSIGMAProfile classification statisticNonestat.valueVARCHARprincipalSRBLENDDeblending flagNonemeta.codeINTEGERprincipalSRQUALQuality flagNonemeta.code.qualINTEGERprincipalSRSBSupercosmos R vrs Bj match classificationNonemeta.codeINTEGERprincipal2dfgrs_fdr.spec_bestThe best spectrum of each surveyed galaxyserialDatabase serial number (=SEQNUM)Nonemeta.idINTEGERprincipalspectraNumber of spectra obtainedNonemeta.numberINTEGERprincipalname2dFGRS name (=NAME)Nonemeta.id;meta.mainVARCHARindexedprincipalUKSTUKST plate (=IFIELD)Noneobs.fieldINTEGERprincipalraR.A. (B1950)hh mm ss.sspos.eq.raVARCHARprincipaldecDec. (B1950)dd mm ss.sspos.eq.decVARCHARprincipalra2000R.A. (J2000)hh mm ss.sspos.eq.ra;meta.mainVARCHARindexedprincipaldec2000Dec. (J2000)dd mm ss.sspos.eq.dec;meta.mainVARCHARindexedprincipalBJGFinal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJSELFinal bj magnitude with extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJG_OLDOriginal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJSELOLDOriginal bj magnitude with extinction correctionmagphot.mag;em.opt.BVARCHARprincipalGALEXTGalactic extinction valuemagphys.absorptionVARCHARprincipalSB_BJSuperCosmos bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalSR_RSuperCosmos R magnitude without extinction correctionmagphot.mag;em.opt.RVARCHARprincipalzBest redshift (observed)Nonesrc.redshiftVARCHARprincipalz_helioBest redshift (heliocentric)Nonesrc.redshift;pos.heliocentricVARCHARprincipalobsrunObservation run of best spectrumNoneobs.param;obsVARCHARprincipalqualityRedshift quality parameter for best spectrum (quality=1-5; reliable redshifts have quality>=3)Nonemeta.code.qual;src.redshiftINTEGERprincipalabemmaRedshift type (abs=1, emi=2, man=3)Nonemeta.code;src.redshiftINTEGERprincipalZ_ABSCross-correlation redshift from best spectrumNonestat.fit.paramVARCHARprincipalKBESTRCross-correlation template from best spectrumNonestat.fit.paramINTEGERprincipalR_CRCORCross-correlation R value from best spectrumNonestat.fit.paramVARCHARprincipalZ_EMIEmission redshift from best spectrumNonesrc.redshift;pos.heliocentricVARCHARprincipalNMBESTNumber of emission lines for Z_EMI from best spectrumNonemeta.numberINTEGERprincipalSNRMedian S/N per pixel from best spectrumNonestat.snr;stat.medianVARCHARprincipalETA_TYPEEta spectral type parameter from best spectrum (-99.9 if none)Nonestat.fit.paramVARCHARprincipal2dfgrs_fdr.spec_keyKey spectroscopic information for each observationserialDatabase serial number (=SEQNUM)Nonemeta.idINTEGERprincipalname2dFGRS name (=NAME)Nonemeta.id;meta.mainVARCHARindexedprincipalUTDATEUT date of observationYYYY:MM:DDtime.epoch;obsVARCHARprincipalOBSRUNObservation runNoneobs.param;obsVARCHARprincipalZRedshift (observed)Nonesrc.redshiftVARCHARprincipalZ_HELIORedshift (heliocentric)Nonesrc.redshift;pos.heliocentricVARCHARprincipalQUALITYRedshift quality parameterNonemeta.code.qual;src.redshiftINTEGERprincipalABEMMARedshift type (abs=1, emi=2, man=3)Nonemeta.code;src.redshiftINTEGERprincipalZ_ABSCross-correlation redshiftNonestat.fit.paramVARCHARprincipalKBESTRCross-correlation templateNonestat.fit.paramINTEGERprincipalR_CRCORCross-correlation R valueNonestat.fit.paramVARCHARprincipalZ_EMIEmission redshiftNonesrc.redshift;pos.heliocentricVARCHARprincipalNMBESTNumber of emission lines for Z_EMINonemeta.numberINTEGERprincipalSNRMedian S/N per pixelNonestat.snr;stat.medianVARCHARprincipalETA_TYPEEta spectral type parameter (-99.9 if none)Nonestat.fit.paramVARCHARprincipal2dfgrs_fdr.spec_sumSummary of spectroscopic informationserialDatabase serial number (=SEQNUM)Nonemeta.idINTEGERprincipalspectraNumber of spectraNonemeta.numberINTEGERprincipalname2dFGRS name (=NAME)Nonemeta.id;meta.mainVARCHARindexedprincipalUKSTUKST plate (=IFIELD)Noneobs.fieldINTEGERprincipalraR.A. (B1950)hh mm ss.sspos.eq.raVARCHARprincipaldecDec. (B1950)dd mm ss.sspos.eq.decVARCHARprincipalra2000R.A. (J2000)hh mm ss.sspos.eq.ra;meta.mainVARCHARindexedprincipaldec2000Dec. (J2000)dd mm ss.sspos.eq.dec;meta.mainVARCHARindexedprincipalBJGFinal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJSELFinal bj magnitude with extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJG_OLDOriginal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalBJSELOLDOriginal bj magnitude with extinction correctionmagphot.mag;em.opt.BVARCHARprincipalGALEXTGalactic extinction valuemagphys.absorptionVARCHARprincipalSB_BJSupercosmos bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalSR_RSupercosmos R magnitude without extinction correctionmagphot.mag;em.opt.RVARCHARprincipalbestFITS extension number of the best spectrumNonemeta.codeINTEGERprincipalzBest redshift (observed)Nonesrc.redshiftVARCHARprincipalz_helioBest redshift (heliocentric)Nonesrc.redshift;pos.heliocentricVARCHARprincipalqualityRedshift quality parameter (quality=1-5; reliable redshifts have quality>=3)Nonemeta.code.qual;src.redshiftINTEGERprincipalobsrunObservation run of best spectrumNoneobs.param;obsVARCHARprincipal2dfgrs_fdr.phot_keyKey photometric informationSEQNUMAssigned sequence number to this object; determines the filename (SEQNUM.fits)Nonemeta.idINTEGERprincipalraR.A. (B1950) in HH MM SS.SShh mm ss.sspos.eq.raVARCHARprincipaldecDec. (B1950) in DD MM SS.Sdd mm ss.sspos.eq.decVARCHARprincipalBJSELFinal bj magnitude with extinction correction (i.e. with corrections for isophote, field-effects and plate-matching, then calibrated to total mags with saturation correction, and then extinction corrected)magphot.mag;em.opt.BVARCHARprincipalPROBpsi classification parameter: for eyeballed galaxies, psi*1000 = (10000 + abs(jon) + psi*100); for eyeballed non-galaxies, psi*1000 = -(10000 + abs(jon) + psi*100)Nonesrc.morph.paramVARCHARprincipalPARKk classification parameter = k / k_starNonesrc.morph.paramVARCHARprincipalPARMUmu classification parameter = mu / mu_starNonesrc.morph.paramVARCHARprincipalIGALFinal classification: -4 = noise, -3 = star + star, -2 = star + fuzz, -1 = star, 0 = galaxy + star merger, 1 = galaxy, 2 = galaxy + galaxy mergerNonesrc.class.starGalaxyINTEGERprincipalJONEyeball classification, value > 0 only for galaxies brighter than about 18th mag: 0 = noise, 1 = S0, 2 = elliptical, 3 = spiral, 4 = irregular, 5 = undetermined galaxy, 6 = star, 7 = star + star merger, 8 = galaxy + star merger, 9 = galaxy + galaxy mergerNonesrc.classINTEGERprincipalORIENTOrientation measured in degrees clockwise from E to W: orient = 180/pi * atan(2*sxy/((sxx + syy)*(1 + e)-syy))degpos.posAngVARCHARprincipalECCENTEccentricity (e): e*200 = 200*(((sxx-syy)**2 + 4sxy**2)**0.5)/(sxx + syy)Nonesrc.morph.paramVARCHARprincipalAREAIsophotal area in pixelspixelsphys.areaVARCHARprincipalX_BJPlate x_bj in 8 micron pixelsNoneinstr.scaleVARCHARprincipalY_BJPlate y_bj in 8 micron pixelsNoneinstr.scaleVARCHARprincipalDXDistortion corrected difference (x_bj - x_R)*100Nonearith.diffVARCHARprincipalDYDistortion corrected difference (y_bj - y_R)*100Nonearith.diffVARCHARprincipalBJGFinal bj magnitude without extinction correctionmagphot.mag;em.opt.BVARCHARprincipalRMAGUnmatched APM 'total' magmagphot.magVARCHARprincipalPMAGUnmatched raw APM profile integrated magmagphot.magVARCHARprincipalFMAGUnmatched raw APM 2" profile integrated magmagphot.magVARCHARprincipalSMAGUnmatched raw stellar mag (from APMCAL)magphot.magVARCHARprincipalREDMAGNot usedmagphot.mag;em.opt.RVARCHARprincipalIFIELDUKST fieldNoneobs.fieldINTEGERprincipalIGFIELDGalaxy number in UKST fieldNonemeta.numberINTEGERprincipalNAME2dFGRS assigned name; if either (i) BJSELOLD is fainter than 19.45, or (ii) the object could not be allocated to a fibre by the configuration algorithm, then NAME is blankNonemeta.idVARCHARprincipalBJG_OLDOriginal bj magnitude without extinction correction (prior to re-calibration to BJG)magphot.mag;em.opt.BVARCHARprincipalBJSELOLDOriginal bj magnitude with extinction correction (prior to re-calibration to BJSEL); used to select survey samplemagphot.mag;em.opt.BVARCHARprincipal100_BJG100k release bj magnitude without extinction correction (prior to re-calibration to BJG)magphot.mag;em.opt.BVARCHARprincipal100BJSEL100k release bj magnitude with extinction correction (prior to re-calibration to BJSEL)magphot.mag;em.opt.BVARCHARprincipal2dfgrs_fdr.dc_source_listSource list of all objects contained within 6dFGSsource_nameunique ID used for identifying sourcesNonemeta.id;meta.mainVARCHARindexedprincipalrapos.eq.raREALindexedprincipaldecpos.eq.decREALindexedprincipalTARGETNAMEunique ID used for identifying sourcesNonemeta.id;meta.mainVARCHARindexedprincipalRAmaster RA J2000 (decimal degrees)degpos.eq.ra;meta.mainREALindexedprincipalDECmaster Dec J2000 (decimal degrees)degpos.eq.dec;meta.mainREALindexedprincipalwigglez_finalThe WiggleZ Dark Energy Survey was a large-scale galaxy redshift survey of bright emission-line galaxies with median redshift z = 0.6, carried out at the Anglo-Australian Telescope at Siding Spring, Australia between 2006 and 2011. More than 200,000 redshifts were obtained, covering 1000 square degrees of equatorial sky in seven well-separated regions. WiggleZ galaxies were selected for observation using colour and magnitude cuts from a combination of optical and UV imaging. The optical imaging employed was from the SDSS in the Northern Galactic Pole and from the RCS2 survey in the Southern Galactic Pole, and UV imaging was provided by the GALEX satellite. The WiggleZ data were used to produce some of the first high-redshift baryon acoustic oscillation measurements and growth of structure measurements, BAO measurements including density-field reconstruction, constraints on cosmological parameters and the properties of neutrinos, and many other scientific results.wigglez_final.WiggleZCatThis catalogue lists all galaxies described in the final data release paper, Drinkwater et al. (2018, MNRAS, 474, 4151, BIBCODE= 2018MNRAS.474.4151D, https://doi.org/10.1093/mnras/stx2963). The data include photometry used to select the galaxies, measured redshifts, absolute FUV magnitudes and stellar mass estimates.WiggleZ_NameGalaxy Namemeta.idVARCHARindexedprincipalRARight Ascension (J2000degpos.eq.raVARCHARindexedprincipalDecDeclination (J2000degpos.eq.decVARCHARindexedprincipalredshiftredshiftsrc.redshiftVARCHARprincipalDredshiftredshift uncertaintysrc.redshift;stat.stdevVARCHARprincipalQredshift qualitymeta.code.classINTEGERprincipalFUVFUV magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipalNUVNUV magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipaluu magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipalgg magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipalrr magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipaliI magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipalzz magnitude dereddenedmagphot.mag.reddFreeVARCHARprincipalDFUVFUV magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalDNUVNUV magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalDuu magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalDgg magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalDrr magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalDiI magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalDzz magnitude uncertaintymagphot.mag.reddFree;stat.stdevVARCHARprincipalE_B_VE(B-V) reddeningmagphot.color.excessVARCHARprincipalclassSelection class flagmeta.code.classVARCHARprincipalUTdateUniversal Time date when spectrum observed, YYYYMMDDtime.epochINTEGERprincipalMFUVAbsolute magnitude in the FUV bandmagphot.magVARCHARprincipalMassStellar Mass log(M*/Msun)dexphys.massVARCHARprincipalDMassStellar Mass uncertaintydexphys.mass;stat.stdevVARCHARprincipalSpecFileName of spectrum filemeta.fileVARCHARprincipalcommentsComment on spectrummeta.noteVARCHARprincipalgalah_dr2Studying galaxy evolution through galactic archaeologygalah_dr2.galahdr2catThis table contains photometry, stellar parameters and abundances for GALAH DR2al_feAluminium abundanceDexphys.abundVARCHARprincipalalpha_feAlpha enhancementDexphys.abundVARCHARprincipalba_feBarium abundanceDexphys.abundVARCHARprincipalc_feCarbon abundanceDexphys.abundVARCHARprincipalca_feCalcium abundanceDexphys.abundVARCHARprincipalchi2_cannonChi squared of best-fit synthetic spectrumstat.fit.chi2VARCHARprincipalco_feCobalt abundanceDexphys.abundVARCHARprincipalcr_feChromium abundanceDexphys.abundVARCHARprincipalcu_feCopper abundanceDexphys.abundVARCHARprincipaldej2000DeclinationDegpos.eq.decVARCHARindexedprincipale_al_feUncertainty on al_feDexstat.errorVARCHARprincipale_alpha_feUncertainty on alpha_feDexstat.errorVARCHARprincipale_ba_feUncertainty on ba_feDexstat.errorVARCHARprincipale_c_feUncertainty on c_feDexstat.errorVARCHARprincipale_ca_feUncertainty on ca_feDexstat.errorVARCHARprincipale_co_feUncertainty on co_feDexstat.errorVARCHARprincipale_cr_feUncertainty on cr_feDexstat.errorVARCHARprincipale_cu_feUncertainty on cu_feDexstat.errorVARCHARprincipale_eu_feUncertainty on eu_feDexstat.errorVARCHARprincipale_fe_hUncertainty on fe_hDexstat.errorVARCHARprincipale_hmagUncertainty in H magMagphot.magVARCHARprincipale_jmagUncertainty in J magMagphot.magVARCHARprincipale_k_feUncertainty on k_feDexstat.errorVARCHARprincipale_kmagUncertainty in K magMagphot.magVARCHARprincipale_la_feUncertainty on la_feDexstat.errorVARCHARprincipale_li_feUncertainty on li_feDexstat.errorVARCHARprincipale_loggUncertainty on logglog(cm/s**2)stat.errorVARCHARprincipale_mg_feUncertainty on mg_feDexstat.errorVARCHARprincipale_mn_feUncertainty on mn_feDexstat.errorVARCHARprincipale_na_feUncertainty on na_feDexstat.errorVARCHARprincipale_ni_feUncertainty on ni_feDexstat.errorVARCHARprincipale_o_feUncertainty on o_feDexstat.errorVARCHARprincipale_rv_nogr_obstUncertainty on rv_obstkm/sstat.errorVARCHARprincipale_rv_obstUncertainty on rv_obstkm/sstat.errorVARCHARprincipale_rv_syntUncertainty on rv_syntkm/sstat.errorVARCHARprincipale_sc_feUncertainty on sc_feDexstat.errorVARCHARprincipale_si_feUncertainty on si_feDexstat.errorVARCHARprincipale_teffUncertainty on teffKstat.errorVARCHARprincipale_ti_feUncertainty on ti_feDexstat.errorVARCHARprincipale_v_feUncertainty on v_feDexstat.errorVARCHARprincipale_vmicUncertainty on vmickm/sstat.errorVARCHARprincipale_vsiniUncertainty on vsinikm/sstat.errorVARCHARprincipale_y_feUncertainty on y_feDexstat.errorVARCHARprincipale_zn_feUncertainty on zn_feDexstat.errorVARCHARprincipaleu_feEuropium abundanceDexphys.abundVARCHARprincipalfe_hIron abundanceDexphys.abund.feVARCHARprincipalfield_idGALAH field IDmeta.id.parentVARCHARprincipalflag_al_feBitmask for al_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_ba_feBitmask for ba_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_c_feBitmask for c_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_ca_feBitmask for ca_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_cannonBitmask for analysis difficultiesmeta.code.qualVARCHARprincipalflag_co_feBitmask for co_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_cr_feBitmask for cr_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_cu_feBitmask for cu_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_eu_feBitmask for eu_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_k_feBitmask for k_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_la_feBitmask for la_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_li_feBitmask for li_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_mg_feBitmask for mg_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_mn_feBitmask for mn_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_na_feBitmask for na_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_ni_feBitmask for ni_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_o_feBitmask for o_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_sc_feBitmask for sc_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_si_feBitmask for si_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_ti_feBitmask for ti_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_v_feBitmask for v_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_y_feBitmask for y_fe abundance difficultiesmeta.code.qualVARCHARprincipalflag_zn_feBitmask for zn_fe abundance difficultiesmeta.code.qualVARCHARprincipalgaia_dr2_idGaia SOURCE_IDmeta.id.crossVARCHARprincipalhmag2MASS H magnitudeMagphot.magVARCHARprincipaljmag2MASS J magnitudeMagphot.magVARCHARprincipalk_fePotassium abundanceDexphys.abundVARCHARprincipalkmag2MASS K magnitudeMagphot.magVARCHARprincipalla_feLanthanum abundanceDexphys.abundVARCHARprincipalli_feLithium abundanceDexphys.abundVARCHARprincipalloggSurface gravitylog(cm/s**2)phys.gravityVARCHARprincipalmg_feMagnesium abundanceDexphys.abundVARCHARprincipalmn_feManganese abundanceDexphys.abundVARCHARprincipalna_feSodium abundanceDexphys.abundVARCHARprincipalndfclassObservation typeobs.paramVARCHARprincipalni_feNickel abundanceDexphys.abundVARCHARprincipalo_feOxygen abundanceDexphys.abundVARCHARprincipalraj2000Right ascensionDegpos.eq.raVARCHARindexedprincipalrv_nogr_obstRadial velocity, cross correlation to real spectra, uncorrected for gravitational redshiftkm/sspec.dopplerVeloc.optVARCHARprincipalrv_obstRadial velocity, cross correlation to real spectrakm/sspec.dopplerVeloc.optVARCHARprincipalrv_syntRadial velocity, cross correlation to synthetic spectrakm/sspec.dopplerVeloc.optVARCHARprincipalsc_feScandium abundanceDexphys.abundVARCHARprincipalsi_feSilicon abundanceDexphys.abundVARCHARprincipalsnr_c1SNR in HERMES blue channelstat.snrVARCHARprincipalsnr_c2SNR in HERMES green channelstat.snrVARCHARprincipalsnr_c3SNR in HERMES red channelstat.snrVARCHARprincipalsnr_c4SNR in HERMES IR channelstat.snrVARCHARprincipalsobject_idGALAH observation IDmeta.id.parentVARCHARprincipalsp_label_distanceDistance from the training set in stellar parameter spacestat.valueVARCHARprincipalstar_id2MASS (preferred) or UCAC4 (secondary) ID numbermeta.id.crossVARCHARindexedprincipalteffEffective temperatureKphys.temperature.effectiveVARCHARprincipalti_feTitanium abundanceDexphys.abundVARCHARprincipalv_feVanadium abundanceDexphys.abundVARCHARprincipalvmag_jkSynthetic V magnitude calculated from JHKMagphot.magVARCHARprincipalvmicMicroturbulent velocitykm/sphys.veloc.microTurbVARCHARprincipalvsiniRotational velocitykm/sphys.veloc.rotatVARCHARprincipaly_feYttrium abundanceDexphys.abundVARCHARprincipalzn_feZinc abundanceDexphys.abundVARCHARprincipalgalah_dr1Studying galaxy evolution through galactic archaeologygalah_dr1.CatalogueGALAH object properties for Data Release 1DECDeclination (Equinox J2000)degpos.eq.decREALprincipalOzDES_IDOzDES IDmeta.idVARCHARprincipalRARight ascension (Equinox J2000)degpos.eq.raREALprincipalflagredshift quality flagmeta.code.classVARCHARprincipaltypesMain object typemeta.code.classVARCHARprincipalzredshiftsrc.redshiftREALprincipalalpha_feAlpha enhancementVARCHARprincipaldecDeclination (J2000.0)VARCHARindexedprincipale_b_v?=99.999 ReddeningVARCHARprincipalfe_hMetallicityVARCHARprincipalgalah_idGALAH Survey ID numberVARCHARindexedprincipalloggSurface gravityVARCHARprincipalm_m_v?=99.999 V-band distance modulusVARCHARprincipalraRight ascension (J2000.0)VARCHARindexedprincipalteffEffective temparatureVARCHARprincipaltmass_id2MASS ID numberVARCHARprincipaltycho2_idTycho-2 ID numberVARCHARprincipalvradRadial velocityVARCHARprincipalsami_dr2<div id="project_overview_text"><p>The SAMI Galaxy Survey is a spatially resolved spectroscopic survey of a large sample of nearby (z<0.1) galaxies, conducted with the Sydney – Australian Astronomical Observatory Multi-Object Integral Field Spectrograph (SAMI). SAMI is mounted on the 3.9 meter Anglo-Australian Telescope at Siding Spring Observatory. Survey observations began in March 2013 and were completed in May 2018. At the completion of survey observing, just over 3000 total galaxies were observed.</p><p>The key science goals of the SAMI Survey are to answer the following questions:</p><ul><li>What is the physical role of environment in galaxy evolution?</li><li>What is the relationship between stellar mass growth and angular momentum development in galaxies?</li><li>How does gas get into and out of galaxies, and how does this drive star formation?</li></ul></div>sami_dr2.DR2SampleSAMI sample catalogueCATIDSAMI Galaxy IDmeta.idINTEGERindexedprincipalRAJ2000 Right Ascensiondegpos.eq.raDOUBLEindexedprincipalDecJ2000 Declinationdegpos.eq.decDOUBLEindexedprincipalz_specSpectroscopic redshiftsrc.redshiftDOUBLEprincipalz_tonryFlow-corrected redshiftsrc.redshiftDOUBLEprincipalM_rAbsolute r-band magnitudemagphot.magAbs;em.opt.RDOUBLEprincipalmu_within_1reMean r-band surface brightness with 1 effective radiusmag/arcsec^2phot.mag.sbDOUBLEprincipalmu_1rer-band surface brightness at 1 effective radiusmag/arcsec^2phot.mag.sbDOUBLEprincipalmu_2rer-band surface brightness at 2 effective radiimag/arcsec^2phot.mag.sbDOUBLEprincipalr_petror-band Petrosian radiusarcsecphys.angSizeDOUBLEprincipalr_autor-band Kron radiusarcsecphys.angSizeDOUBLEprincipalr_er-band effective radiusarcsecphys.angSizeDOUBLEprincipalellipr-band ellipticitysrc.ellipticityDOUBLEprincipalPAr-band position angledegpos.posAngDOUBLEprincipalg_i(g-i) colourmagphot.colorDOUBLEprincipalA_gg-band extinctionmagphys.absorptionDOUBLEprincipalMstarLogarithm of stellar massdexphys.massDOUBLEprincipalmorphmorphological type indicator (0 = elliptical, 1 = S0, 2 = Sa/Sb, 3 = Sc/Sd/Irr)src.morphREALprincipalmorph_flagflag indicating whether galaxy was classified in the first or second iterationmeta.code.statusINTEGERprincipalsami_dr2.StellarKinematicsGlobal and aperture stellar kinematics measurementsCATIDCatalog ID from Bryant et al. 2015 and Owers et al. 2017meta.idBIGINTprincipalPA_STELKINKinematic position angle. Anticlockwise, North=0 degreesdegpos.posAngREALprincipalE_PA_STELKIN1-sigma error on the kinematic position angledegpos.posAng;stat.errorREALprincipalSIGMA_REVelocity dispersion from Re aperture spectrakm/sphys.veloc.dispersionREALprincipalE_SIGMA_RE1-sigma error on sigma_rekm/sphys.veloc.dispersion;stat.errorREALprincipalSIGMA_3KPCVelocity dispersion from 3kpc aperture spectrakm/sphys.veloc.dispersionREALprincipalE_SIGMA_3KPC1-sigma error on sigma_3kpckm/sphys.veloc.dispersion;stat.errorREALprincipalSIGMA_1_4_ARCSECVelocity dispersion from 1.4 arcsec aperture spectrakm/sphys.veloc.dispersion;stat.errorREALprincipalE_SIGMA_1_4_ARCSEC1-sigma error on sigma_1_4_arcseckm/sphys.veloc.dispersion;stat.errorREALprincipalSIGMA_2_ARCSECVelocity dispersion from 2 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalE_SIGMA_2_ARCSEC1-sigma error on sigma_2_arcseckm/sphys.veloc.dispersion;stat.errorREALprincipalSIGMA_3_ARCSECVelocity dispersion from 3 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalE_SIGMA_3_ARCSEC1-sigma error on sigma_3_arcseckm/sphys.veloc.dispersion;stat.errorREALprincipalSIGMA_4_ARCSECVelocity dispersion from 4 arcsec aperture spectrakm/sphys.veloc.dispersionREALprincipalE_SIGMA_4_ARCSEC1-sigma error on sigma_4_arcseckm/sphys.veloc.dispersion;stat.errorREALprincipalAPER_CORR_FLAGFlag to indicate whether lambdar_re and vsigma_re have been aperture corrected. 0 = no aperture correction applied. 1 = inside-out aperture corrected (rmax < re). 2 = from outside in (re < hwhm_psf)meta.code.qualREALprincipalRMAX_APER_CORRRadius at which the aperture corrected value was determined fromphysics.size.radius;arith.ratioREALprincipalLAMBDAR_RESpin Parameter proxy within effective ellipse as defined in van de Sande et al. 2017phys.angMomentumREALprincipalE_LAMBDAR_RE1-sigma error on lambdar_rephys.angMomentum;stat.errorREALprincipalLAMBDAR_MAXLambdar at maximum radius that is used for aperture correction (where APER_CORR_FLAG = 1)phys.angMomentumREALprincipalE_LAMBDAR_MAX1-sigma error on lambdar_Maxphys.angMomentum;stat.errorREALprincipalVSIGMA_REFlux weighted V/sigma within Re effective ellipsephys.veloc;phys.veloc.dispersion;arith.ratioREALprincipalE_VSIGMA_RE1-sigma error on vsigma_ephys.veloc;phys.veloc.dispersion;arith.ratio;stat.errorREALprincipalVSIGMA_MAXV/sigma at maximum radius that is used for aperture correction (where APER_CORR_FLAG = 1)phys.veloc;phys.veloc.dispersion;arith.ratioREALprincipalE_VSIGMA_MAX1-sigma error on VSigma_maxphys.veloc;phys.veloc.dispersion;arith.ratio;stat.errorREALprincipalMEAN_K51_REkinematic asymmetry estimate from kinemetry within Restat.Fourier.amplitudeREALprincipalE_MEAN_K51_RE1-sigma error on mean_k51_restat.Fourier.amplitude;stat.errorREALprincipalsami_dr2.GasRecomcompAperturesAperture recommended-component emission line fluxes, ionised gas kinematics, and star formation ratesSFR_3_ARCSECONDStar formation rate in 3-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_3_ARCSECONDUncertainty in star formation rate in 3-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalNPIX_4_ARCSECONDNumber of pixels in 4-ARCSECOND aperture_meta.valueVARCHARprincipalAREA_COV_4_ARCSECONDFraction of SAMI FoV covered by 4-ARCSECOND aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_4_ARCSECOND1-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_4_ARCSECONDUncertainty on 1-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_4_ARCSECOND2-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_ERR_4_ARCSECONDUncertainty on 2-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_4_ARCSECOND3-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_ERR_4_ARCSECONDUncertainty on 3-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_4_ARCSECOND1-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_4_ARCSECONDUncertainty on 1-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_2_COMP_4_ARCSECOND2-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_2_COMP_4_ARCSECONDUncertainty on 2-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_3_COMP_4_ARCSECOND3-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_3_COMP_4_ARCSECONDUncertainty on 3-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalOII3727_4_ARCSECONDTotal [OII]3727 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOII3727_ERR_4_ARCSECONDUncertainty on total [OII]3727 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_4_ARCSECONDTotal Hbeta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_ERR_4_ARCSECONDUncertainty on total Hbeta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_4_ARCSECONDTotal [OIII]5007 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_ERR_4_ARCSECONDUncertainty on total [OIII]5007 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_4_ARCSECONDTotal [OI]6300 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_ERR_4_ARCSECONDUncertainty on total [OI]6300 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_4_ARCSECONDTotal Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_4_ARCSECONDUncertainty on total Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_4_ARCSECOND1-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_4_ARCSECONDUncertainty on 1-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_4_ARCSECOND2-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_ERR_4_ARCSECONDUncertainty on 2-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_4_ARCSECOND3-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_ERR_4_ARCSECONDUncertainty on 3-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_4_ARCSECONDTotal [NII]6583 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_ERR_4_ARCSECONDUncertainty on total [NII]6583 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_4_ARCSECONDTotal [SII]6716 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_ERR_4_ARCSECONDUncertainty on total [SII]6716 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_4_ARCSECONDTotal [SII]6731 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_ERR_4_ARCSECONDUncertainty on total [SII]6731 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalEXTINCTION_CORR_4_ARCSECONDExtinction correction on total Halpha flux in 4-ARCSECOND aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_4_ARCSECONDUncertainty in extinction correction on total Halpha flux in 4-ARCSECOND aperturphys.fluxcorrVARCHARprincipalSFR_4_ARCSECONDStar formation rate in 4-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_4_ARCSECONDUncertainty in star formation rate in 4-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalCATIDSAMI galaxy IDmeta.idVARCHARprincipalRASAMI galaxy Right AscensionDegreesmeta.idVARCHARprincipalDECSAMI galaxy DeclinationDegreesmeta.idVARCHARprincipalZSAMI galaxy Redshift assumedmeta.idVARCHARprincipalR_ESAMI galaxy effective radiusarcsecondmeta.idVARCHARprincipalELLIPSAMI galaxy ellipticitymeta.idVARCHARprincipalPASAMI galaxy Position AngleDegreesmeta.idVARCHARprincipalNPIX_RENumber of pixels in RE aperture_meta.valueVARCHARprincipalAREA_COV_REFraction of SAMI FoV covered by RE aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_RE1-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_REUncertainty on 1-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_RE2-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_ERR_REUncertainty on 2-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_RE3-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_ERR_REUncertainty on 3-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_RE1-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_REUncertainty on 1-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_2_COMP_RE2-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_2_COMP_REUncertainty on 2-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_3_COMP_RE3-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_3_COMP_REUncertainty on 3-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalOII3727_RETotal [OII]3727 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOII3727_ERR_REUncertainty on total [OII]3727 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_RETotal Hbeta flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_ERR_REUncertainty on total Hbeta flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_RETotal [OIII]5007 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_ERR_REUncertainty on total [OIII]5007 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_RETotal [OI]6300 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_ERR_REUncertainty on total [OI]6300 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_RETotal Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_REUncertainty on total Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_RE1-component Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_REUncertainty on 1-component Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_RE2-component Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_ERR_REUncertainty on 2-component Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_RE3-component Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_ERR_REUncertainty on 3-component Halpha flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_RETotal [NII]6583 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_ERR_REUncertainty on total [NII]6583 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_RETotal [SII]6716 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_ERR_REUncertainty on total [SII]6716 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_RETotal [SII]6731 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_ERR_REUncertainty on total [SII]6731 flux in RE aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalEXTINCTION_CORR_REExtinction correction on total Halpha flux in RE aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_REUncertainty in extinction correction on total Halpha flux in RE aperturephys.fluxcorrVARCHARprincipalSFR_REStar formation rate in RE apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_REUncertainty in star formation rate in RE apertureMsun/yrphys.sfrVARCHARprincipalNPIX_3KPC_ROUNDNumber of pixels in 3KPC-ROUND aperture_meta.valueVARCHARprincipalAREA_COV_3KPC_ROUNDFraction of SAMI FoV covered by 3KPC-ROUND aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_3KPC_ROUND1-component Gas velocity in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_3KPC_ROUNDUncertainty on 1-component Gas velocity in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_3KPC_ROUND2-component Gas velocity in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_ERR_3KPC_ROUNDUncertainty on 2-component Gas velocity in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_3KPC_ROUND3-component Gas velocity in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_ERR_3KPC_ROUNDUncertainty on 3-component Gas velocity in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_3KPC_ROUND1-component Gas velocity dispersion in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_3KPC_ROUNDUncertainty on 1-component Gas velocity dispersion in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_2_COMP_3KPC_ROUND2-component Gas velocity dispersion in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_2_COMP_3KPC_ROUNDUncertainty on 2-component Gas velocity dispersion in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_3_COMP_3KPC_ROUND3-component Gas velocity dispersion in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_3_COMP_3KPC_ROUNDUncertainty on 3-component Gas velocity dispersion in 3KPC-ROUND aperturekm/sphys.velocityVARCHARprincipalOII3727_3KPC_ROUNDTotal [OII]3727 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOII3727_ERR_3KPC_ROUNDUncertainty on total [OII]3727 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_3KPC_ROUNDTotal Hbeta flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_ERR_3KPC_ROUNDUncertainty on total Hbeta flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_3KPC_ROUNDTotal [OIII]5007 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_ERR_3KPC_ROUNDUncertainty on total [OIII]5007 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_3KPC_ROUNDTotal [OI]6300 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_ERR_3KPC_ROUNDUncertainty on total [OI]6300 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_3KPC_ROUNDTotal Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_3KPC_ROUNDUncertainty on total Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_3KPC_ROUND1-component Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_3KPC_ROUNDUncertainty on 1-component Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_3KPC_ROUND2-component Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_ERR_3KPC_ROUNDUncertainty on 2-component Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_3KPC_ROUND3-component Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_ERR_3KPC_ROUNDUncertainty on 3-component Halpha flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_3KPC_ROUNDTotal [NII]6583 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_ERR_3KPC_ROUNDUncertainty on total [NII]6583 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_3KPC_ROUNDTotal [SII]6716 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_ERR_3KPC_ROUNDUncertainty on total [SII]6716 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_3KPC_ROUNDTotal [SII]6731 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_ERR_3KPC_ROUNDUncertainty on total [SII]6731 flux in 3KPC-ROUND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalEXTINCTION_CORR_3KPC_ROUNDExtinction correction on total Halpha flux in 3KPC-ROUND aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_3KPC_ROUNDUncertainty in extinction correction on total Halpha flux in 3KPC-ROUND aperturephys.fluxcorrVARCHARprincipalSFR_3KPC_ROUNDStar formation rate in 3KPC-ROUND apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_3KPC_ROUNDUncertainty in star formation rate in 3KPC-ROUND apertureMsun/yrphys.sfrVARCHARprincipalNPIX_1_4_ARCSECONDNumber of pixels in 4-ARCSECOND aperture_meta.valueVARCHARprincipalAREA_COV_1_4_ARCSECONDFraction of SAMI FoV covered by 4-ARCSECOND aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_1_4_ARCSECOND1-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_1_4_ARCSECONDUncertainty on 1-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_1_4_ARCSECOND2-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_ERR_1_4_ARCSECONDUncertainty on 2-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_1_4_ARCSECOND3-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_ERR_1_4_ARCSECONDUncertainty on 3-component Gas velocity in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_1_4_ARCSECOND1-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_1_4_ARCSECONDUncertainty on 1-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_2_COMP_1_4_ARCSECOND2-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_2_COMP_1_4_ARCSECONDUncertainty on 2-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_3_COMP_1_4_ARCSECOND3-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_3_COMP_1_4_ARCSECONDUncertainty on 3-component Gas velocity dispersion in 4-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalOII3727_1_4_ARCSECONDTotal [OII]3727 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOII3727_ERR_1_4_ARCSECONDUncertainty on total [OII]3727 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_1_4_ARCSECONDTotal Hbeta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_ERR_1_4_ARCSECONDUncertainty on total Hbeta flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_1_4_ARCSECONDTotal [OIII]5007 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_ERR_1_4_ARCSECONDUncertainty on total [OIII]5007 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_1_4_ARCSECONDTotal [OI]6300 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_ERR_1_4_ARCSECONDUncertainty on total [OI]6300 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_1_4_ARCSECONDTotal Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_1_4_ARCSECONDUncertainty on total Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_1_4_ARCSECOND1-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_1_4_ARCSECONDUncertainty on 1-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_1_4_ARCSECOND2-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_ERR_1_4_ARCSECONDUncertainty on 2-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_1_4_ARCSECOND3-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_ERR_1_4_ARCSECONDUncertainty on 3-component Halpha flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_1_4_ARCSECONDTotal [NII]6583 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_ERR_1_4_ARCSECONDUncertainty on total [NII]6583 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_1_4_ARCSECONDTotal [SII]6716 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_ERR_1_4_ARCSECONDUncertainty on total [SII]6716 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_1_4_ARCSECONDTotal [SII]6731 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_ERR_1_4_ARCSECONDUncertainty on total [SII]6731 flux in 4-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalEXTINCTION_CORR_1_4_ARCSECONDExtinction correction on total Halpha flux in 4-ARCSECOND aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_1_4_ARCSECONDUncertainty in extinction correction on total Halpha flux in 4-ARCSECOND aperturphys.fluxcorrVARCHARprincipalSFR_1_4_ARCSECONDStar formation rate in 4-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_1_4_ARCSECONDUncertainty in star formation rate in 4-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalNPIX_2_ARCSECONDNumber of pixels in 2-ARCSECOND aperture_meta.valueVARCHARprincipalAREA_COV_2_ARCSECONDFraction of SAMI FoV covered by 2-ARCSECOND aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_2_ARCSECOND1-component Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_2_ARCSECONDUncertainty on 1-component Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_2_ARCSECOND2-component Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_ERR_2_ARCSECONDUncertainty on 2-component Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_2_ARCSECOND3-component Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_ERR_2_ARCSECONDUncertainty on 3-component Gas velocity in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_2_ARCSECOND1-component Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_2_ARCSECONDUncertainty on 1-component Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_2_COMP_2_ARCSECOND2-component Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_2_COMP_2_ARCSECONDUncertainty on 2-component Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_3_COMP_2_ARCSECOND3-component Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_3_COMP_2_ARCSECONDUncertainty on 3-component Gas velocity dispersion in 2-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalOII3727_2_ARCSECONDTotal [OII]3727 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOII3727_ERR_2_ARCSECONDUncertainty on total [OII]3727 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_2_ARCSECONDTotal Hbeta flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_ERR_2_ARCSECONDUncertainty on total Hbeta flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_2_ARCSECONDTotal [OIII]5007 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_ERR_2_ARCSECONDUncertainty on total [OIII]5007 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_2_ARCSECONDTotal [OI]6300 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_ERR_2_ARCSECONDUncertainty on total [OI]6300 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_2_ARCSECONDTotal Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_2_ARCSECONDUncertainty on total Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_2_ARCSECOND1-component Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_2_ARCSECONDUncertainty on 1-component Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_2_ARCSECOND2-component Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_ERR_2_ARCSECONDUncertainty on 2-component Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_2_ARCSECOND3-component Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_ERR_2_ARCSECONDUncertainty on 3-component Halpha flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_2_ARCSECONDTotal [NII]6583 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_ERR_2_ARCSECONDUncertainty on total [NII]6583 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_2_ARCSECONDTotal [SII]6716 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_ERR_2_ARCSECONDUncertainty on total [SII]6716 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_2_ARCSECONDTotal [SII]6731 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_ERR_2_ARCSECONDUncertainty on total [SII]6731 flux in 2-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalEXTINCTION_CORR_2_ARCSECONDExtinction correction on total Halpha flux in 2-ARCSECOND aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_2_ARCSECONDUncertainty in extinction correction on total Halpha flux in 2-ARCSECOND aperturphys.fluxcorrVARCHARprincipalSFR_2_ARCSECONDStar formation rate in 2-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_2_ARCSECONDUncertainty in star formation rate in 2-ARCSECOND apertureMsun/yrphys.sfrVARCHARprincipalNPIX_3_ARCSECONDNumber of pixels in 3-ARCSECOND aperture_meta.valueVARCHARprincipalAREA_COV_3_ARCSECONDFraction of SAMI FoV covered by 3-ARCSECOND aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_3_ARCSECOND1-component Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_3_ARCSECONDUncertainty on 1-component Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_3_ARCSECOND2-component Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_2_COMP_ERR_3_ARCSECONDUncertainty on 2-component Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_3_ARCSECOND3-component Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalV_GAS_3_COMP_ERR_3_ARCSECONDUncertainty on 3-component Gas velocity in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_3_ARCSECOND1-component Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_3_ARCSECONDUncertainty on 1-component Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_2_COMP_3_ARCSECOND2-component Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_2_COMP_3_ARCSECONDUncertainty on 2-component Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_3_COMP_3_ARCSECOND3-component Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_3_COMP_3_ARCSECONDUncertainty on 3-component Gas velocity dispersion in 3-ARCSECOND aperturekm/sphys.velocityVARCHARprincipalOII3727_3_ARCSECONDTotal [OII]3727 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOII3727_ERR_3_ARCSECONDUncertainty on total [OII]3727 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_3_ARCSECONDTotal Hbeta flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHBETA_ERR_3_ARCSECONDUncertainty on total Hbeta flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_3_ARCSECONDTotal [OIII]5007 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOIII5007_ERR_3_ARCSECONDUncertainty on total [OIII]5007 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_3_ARCSECONDTotal [OI]6300 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalOI6300_ERR_3_ARCSECONDUncertainty on total [OI]6300 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_3_ARCSECONDTotal Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_3_ARCSECONDUncertainty on total Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_3_ARCSECOND1-component Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_3_ARCSECONDUncertainty on 1-component Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_3_ARCSECOND2-component Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_2_COMP_ERR_3_ARCSECONDUncertainty on 2-component Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_3_ARCSECOND3-component Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalHALPHA_3_COMP_ERR_3_ARCSECONDUncertainty on 3-component Halpha flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_3_ARCSECONDTotal [NII]6583 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalNII6583_ERR_3_ARCSECONDUncertainty on total [NII]6583 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_3_ARCSECONDTotal [SII]6716 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6716_ERR_3_ARCSECONDUncertainty on total [SII]6716 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_3_ARCSECONDTotal [SII]6731 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalSII6731_ERR_3_ARCSECONDUncertainty on total [SII]6731 flux in 3-ARCSECOND aperture1E-16 erg/s/cm2phys.fluxVARCHARprincipalEXTINCTION_CORR_3_ARCSECONDExtinction correction on total Halpha flux in 3-ARCSECOND aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_3_ARCSECONDUncertainty in extinction correction on total Halpha flux in 3-ARCSECOND aperturphys.fluxcorrVARCHARprincipalsami_dr2.IndexAperturesLick index measurements from aperture spectraCATIDSAMI galaxy IDmeta.idINTEGERprincipalHdeltaA_3KPC_ROUNDHdeltaA index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_3KPC_ROUNDHdeltaF index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_3KPC_ROUNDHgammaA index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_3KPC_ROUNDHgammaF index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_3KPC_ROUNDHbeta index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_3KPC_ROUNDMgb index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_3KPC_ROUNDFe4383 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_3KPC_ROUNDFe4668 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_3KPC_ROUNDFe5015 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_3KPC_ROUNDFe5270 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_3KPC_ROUNDFe5335 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_3KPC_ROUNDCN1 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalCN2_3KPC_ROUNDCN2 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalCa4227_3KPC_ROUNDCa4227 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_3KPC_ROUNDG4300 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_3KPC_ROUNDMg1 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalMg2_3KPC_ROUNDMg2 index strength within the 3KPC aperturemagspect.line;phot.magDOUBLEprincipalFe4531_3KPC_ROUNDFe4531 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_3KPC_ROUNDFe5406 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_3KPC_ROUNDCa4455 index strength within the 3KPC apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_3KPC_ROUND_errUncertainty on the HdeltaA index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_3KPC_ROUND_errUncertainty on the HdeltaF index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_3KPC_ROUND_errUncertainty on the HgammaA index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_3KPC_ROUND_errUncertainty on the HgammaF index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_3KPC_ROUND_errUncertainty on the Hbeta index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_3KPC_ROUND_errUncertainty on the Mgb index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_3KPC_ROUND_errUncertainty on the Fe4383 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_3KPC_ROUND_errUncertainty on the Fe4668 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_3KPC_ROUND_errUncertainty on the Fe5015 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_3KPC_ROUND_errUncertainty on the Fe5270 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_3KPC_ROUND_errUncertainty on the Fe5335 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_3KPC_ROUND_errUncertainty on the CN1 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_3KPC_ROUND_errUncertainty on the CN2 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_3KPC_ROUND_errUncertainty on the Ca4227 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_3KPC_ROUND_errUncertainty on the G4300 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_3KPC_ROUND_errUncertainty on the Mg1 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_3KPC_ROUND_errUncertainty on the Mg2 index strength within the 3KPC aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_3KPC_ROUND_errUncertainty on the Fe4531 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_3KPC_ROUND_errUncertainty on the Fe5406 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_3KPC_ROUND_errUncertainty on the Ca4455 index strength within the 3KPC apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_3_ARCSECONDHdeltaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_3_ARCSECONDHdeltaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_3_ARCSECONDHgammaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_3_ARCSECONDHgammaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_3_ARCSECONDHbeta index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_3_ARCSECONDMgb index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_3_ARCSECONDFe4383 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_3_ARCSECONDFe4668 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_3_ARCSECONDFe5015 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_3_ARCSECONDFe5270 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_3_ARCSECONDFe5335 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_3_ARCSECONDCN1 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_3_ARCSECONDCN2 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_3_ARCSECONDCa4227 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_3_ARCSECONDG4300 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_3_ARCSECONDMg1 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_3_ARCSECONDMg2 index strength within the 3 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_3_ARCSECONDFe4531 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_3_ARCSECONDFe5406 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_3_ARCSECONDCa4455 index strength within the 3 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_3_ARCSECOND_errUncertainty on the HdeltaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_3_ARCSECOND_errUncertainty on the HdeltaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_3_ARCSECOND_errUncertainty on the HgammaA index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_3_ARCSECOND_errUncertainty on the HgammaF index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_3_ARCSECOND_errUncertainty on the Hbeta index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_3_ARCSECOND_errUncertainty on the Mgb index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_3_ARCSECOND_errUncertainty on the Fe4383 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_3_ARCSECOND_errUncertainty on the Fe4668 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_3_ARCSECOND_errUncertainty on the Fe5015 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_3_ARCSECOND_errUncertainty on the Fe5270 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_3_ARCSECOND_errUncertainty on the Fe5335 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_3_ARCSECOND_errUncertainty on the CN1 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_3_ARCSECOND_errUncertainty on the CN2 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_3_ARCSECOND_errUncertainty on the Ca4227 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_3_ARCSECOND_errUncertainty on the G4300 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_3_ARCSECOND_errUncertainty on the Mg1 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_3_ARCSECOND_errUncertainty on the Mg2 index strength within the 3 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_3_ARCSECOND_errUncertainty on the Fe4531 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_3_ARCSECOND_errUncertainty on the Fe5406 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_3_ARCSECOND_errUncertainty on the Ca4455 index strength within the 3 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_REHdeltaA index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_REHdeltaF index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_REHgammaA index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_REHgammaF index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_REHbeta index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_REMgb index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_REFe4383 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_REFe4668 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_REFe5015 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_REFe5270 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_REFe5335 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_RECN1 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalCN2_RECN2 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalCa4227_RECa4227 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_REG4300 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_REMg1 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalMg2_REMg2 index strength within the RE aperturemagspect.line;phot.magDOUBLEprincipalFe4531_REFe4531 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_REFe5406 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_RECa4455 index strength within the RE apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_RE_errUncertainty on the HdeltaA index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_RE_errUncertainty on the HdeltaF index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_RE_errUncertainty on the HgammaA index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_RE_errUncertainty on the HgammaF index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_RE_errUncertainty on the Hbeta index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_RE_errUncertainty on the Mgb index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_RE_errUncertainty on the Fe4383 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_RE_errUncertainty on the Fe4668 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_RE_errUncertainty on the Fe5015 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_RE_errUncertainty on the Fe5270 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_RE_errUncertainty on the Fe5335 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_RE_errUncertainty on the CN1 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_RE_errUncertainty on the CN2 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_RE_errUncertainty on the Ca4227 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_RE_errUncertainty on the G4300 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_RE_errUncertainty on the Mg1 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_RE_errUncertainty on the Mg2 index strength within the RE aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_RE_errUncertainty on the Fe4531 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_RE_errUncertainty on the Fe5406 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_RE_errUncertainty on the Ca4455 index strength within the RE apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_2_ARCSECONDHdeltaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_2_ARCSECONDHdeltaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_2_ARCSECONDHgammaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_2_ARCSECONDHgammaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_2_ARCSECONDHbeta index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_2_ARCSECONDMgb index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_2_ARCSECONDFe4383 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_2_ARCSECONDFe4668 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_2_ARCSECONDFe5015 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_2_ARCSECONDFe5270 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_2_ARCSECONDFe5335 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_2_ARCSECONDCN1 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_2_ARCSECONDCN2 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_2_ARCSECONDCa4227 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_2_ARCSECONDG4300 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_2_ARCSECONDMg1 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_2_ARCSECONDMg2 index strength within the 2 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_2_ARCSECONDFe4531 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_2_ARCSECONDFe5406 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_2_ARCSECONDCa4455 index strength within the 2 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_2_ARCSECOND_errUncertainty on the HdeltaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_2_ARCSECOND_errUncertainty on the HdeltaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_2_ARCSECOND_errUncertainty on the HgammaA index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_2_ARCSECOND_errUncertainty on the HgammaF index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_2_ARCSECOND_errUncertainty on the Hbeta index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_2_ARCSECOND_errUncertainty on the Mgb index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_2_ARCSECOND_errUncertainty on the Fe4383 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_2_ARCSECOND_errUncertainty on the Fe4668 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_2_ARCSECOND_errUncertainty on the Fe5015 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_2_ARCSECOND_errUncertainty on the Fe5270 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_2_ARCSECOND_errUncertainty on the Fe5335 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_2_ARCSECOND_errUncertainty on the CN1 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_2_ARCSECOND_errUncertainty on the CN2 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_2_ARCSECOND_errUncertainty on the Ca4227 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_2_ARCSECOND_errUncertainty on the G4300 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_2_ARCSECOND_errUncertainty on the Mg1 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_2_ARCSECOND_errUncertainty on the Mg2 index strength within the 2 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_2_ARCSECOND_errUncertainty on the Fe4531 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_2_ARCSECOND_errUncertainty on the Fe5406 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_2_ARCSECOND_errUncertainty on the Ca4455 index strength within the 2 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_1_4_ARCSECONDHdeltaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_1_4_ARCSECONDHdeltaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_1_4_ARCSECONDHgammaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_1_4_ARCSECONDHgammaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_1_4_ARCSECONDHbeta index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_1_4_ARCSECONDMgb index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_1_4_ARCSECONDFe4383 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_1_4_ARCSECONDFe4668 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_1_4_ARCSECONDFe5015 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_1_4_ARCSECONDFe5270 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_1_4_ARCSECONDFe5335 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_1_4_ARCSECONDCN1 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_1_4_ARCSECONDCN2 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_1_4_ARCSECONDCa4227 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_1_4_ARCSECONDG4300 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_1_4_ARCSECONDMg1 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_1_4_ARCSECONDMg2 index strength within the 1.4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_1_4_ARCSECONDFe4531 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_1_4_ARCSECONDFe5406 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_1_4_ARCSECONDCa4455 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_1_4_ARCSECOND_errUncertainty on the HdeltaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_1_4_ARCSECOND_errUncertainty on the HdeltaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_1_4_ARCSECOND_errUncertainty on the HgammaA index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_1_4_ARCSECOND_errUncertainty on the HgammaF index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_1_4_ARCSECOND_errUncertainty on the Hbeta index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_1_4_ARCSECOND_errUncertainty on the Mgb index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_1_4_ARCSECOND_errUncertainty on the Fe4383 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_1_4_ARCSECOND_errUncertainty on the Fe4668 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_1_4_ARCSECOND_errUncertainty on the Fe5015 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_1_4_ARCSECOND_errUncertainty on the Fe5270 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_1_4_ARCSECOND_errUncertainty on the Fe5335 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_1_4_ARCSECOND_errUncertainty on the CN1 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_1_4_ARCSECOND_errUncertainty on the CN2 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_1_4_ARCSECOND_errUncertainty on the Ca4227 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_1_4_ARCSECOND_errUncertainty on the G4300 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_1_4_ARCSECOND_errUncertainty on the Mg1 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_1_4_ARCSECOND_errUncertainty on the Mg2 index strength within the 1.4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_1_4_ARCSECOND_errUncertainty on the Fe4531 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_1_4_ARCSECOND_errUncertainty on the Fe5406 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_1_4_ARCSECOND_errUncertainty on the Ca4455 index strength within the 1.4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaA_4_ARCSECONDHdeltaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaF_4_ARCSECONDHdeltaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaA_4_ARCSECONDHgammaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHgammaF_4_ARCSECONDHgammaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHbeta_4_ARCSECONDHbeta index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMgb_4_ARCSECONDMgb index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4383_4_ARCSECONDFe4383 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe4668_4_ARCSECONDFe4668 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5015_4_ARCSECONDFe5015 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5270_4_ARCSECONDFe5270 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5335_4_ARCSECONDFe5335 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCN1_4_ARCSECONDCN1 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCN2_4_ARCSECONDCN2 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalCa4227_4_ARCSECONDCa4227 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalG4300_4_ARCSECONDG4300 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalMg1_4_ARCSECONDMg1 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalMg2_4_ARCSECONDMg2 index strength within the 4 arcsec aperturemagspect.line;phot.magDOUBLEprincipalFe4531_4_ARCSECONDFe4531 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalFe5406_4_ARCSECONDFe5406 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalCa4455_4_ARCSECONDCa4455 index strength within the 4 arcsec apertureAngstromspect.line.eqWidthDOUBLEprincipalHdeltaA_4_ARCSECOND_errUncertainty on the HdeltaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHdeltaF_4_ARCSECOND_errUncertainty on the HdeltaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaA_4_ARCSECOND_errUncertainty on the HgammaA index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHgammaF_4_ARCSECOND_errUncertainty on the HgammaF index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalHbeta_4_ARCSECOND_errUncertainty on the Hbeta index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMgb_4_ARCSECOND_errUncertainty on the Mgb index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4383_4_ARCSECOND_errUncertainty on the Fe4383 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe4668_4_ARCSECOND_errUncertainty on the Fe4668 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5015_4_ARCSECOND_errUncertainty on the Fe5015 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5270_4_ARCSECOND_errUncertainty on the Fe5270 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5335_4_ARCSECOND_errUncertainty on the Fe5335 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCN1_4_ARCSECOND_errUncertainty on the CN1 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCN2_4_ARCSECOND_errUncertainty on the CN2 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalCa4227_4_ARCSECOND_errUncertainty on the Ca4227 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalG4300_4_ARCSECOND_errUncertainty on the G4300 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalMg1_4_ARCSECOND_errUncertainty on the Mg1 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalMg2_4_ARCSECOND_errUncertainty on the Mg2 index strength within the 4 arcsec aperturemagspect.line;phot.mag;stat.errorDOUBLEprincipalFe4531_4_ARCSECOND_errUncertainty on the Fe4531 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFe5406_4_ARCSECOND_errUncertainty on the Fe5406 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalCa4455_4_ARCSECOND_errUncertainty on the Ca4455 index strength within the 4 arcsec apertureAngstromspect.line.eqWidth;stat.errorDOUBLEprincipalFLAG_3KPC_ROUNDQuality flag for index measurements in the 3KPC aperture (0 = good, 1 = potentially unreliable)meta.code.qualINTEGERprincipalFLAG_3_ARCSECONDQuality flag for index measurements in the 3 arcsec aperture (0 = good, 1 = potentially unreliable)meta.code.qualINTEGERprincipalFLAG_REQuality flag for index measurements in the RE aperture (0 = good, 1 = potentially unreliable)meta.code.qualINTEGERprincipalFLAG_2_ARCSECONDQuality flag for index measurements in the 2 arcsec aperture (0 = good, 1 = potentially unreliable)meta.code.qualINTEGERprincipalFLAG_1_4_ARCSECONDQuality flag for index measurements in the 1.4 arcsec aperture (0 = good, 1 = potentially unreliable)meta.code.qualINTEGERprincipalFLAG_4_ARCSECONDQuality flag for index measurements in the 4 arcsec aperture (0 = good, 1 = potentially unreliable)meta.code.qualINTEGERprincipalsami_dr2.SSPAperturesSingle stellar population equivalent age, [Z/H] and [alpha/Fe] measured from aperture spectraCATIDSAMI galaxy IDmeta.idINTEGERprincipalAge_3KPC_ROUNDSSP Age within the 3KPC apertureGyrstime.ageDOUBLEprincipalZ_3KPC_ROUNDSSP Z within the 3KPC aperturephys.abundDOUBLEprincipalalpha_3KPC_ROUNDSSP alpha within the 3KPC aperturephys.abundDOUBLEprincipalAge_3KPC_ROUND_errUncertainty on SSP Age within the 3KPC apertureGyrstime.age;stat.errorDOUBLEprincipalZ_3KPC_ROUND_errUncertainty on SSP Z within the 3KPC aperturephys.abund;stat.errorDOUBLEprincipalalpha_3KPC_ROUND_errUncertainty on SSP alpha within the 3KPC aperturephys.abund;stat.errorDOUBLEprincipalAge_3_ARCSECONDSSP Age within the 3 arcsec apertureGyrstime.ageDOUBLEprincipalZ_3_ARCSECONDSSP Z within the 3 arcsec aperturephys.abundDOUBLEprincipalalpha_3_ARCSECONDSSP alpha within the 3 arcsec aperturephys.abundDOUBLEprincipalAge_3_ARCSECOND_errUncertainty on SSP Age within the 3 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_3_ARCSECOND_errUncertainty on SSP Z within the 3 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_3_ARCSECOND_errUncertainty on SSP alpha within the 3 arcsec aperturephys.abund;stat.errorDOUBLEprincipalAge_RESSP Age within the RE apertureGyrstime.ageDOUBLEprincipalZ_RESSP Z within the RE aperturephys.abundDOUBLEprincipalalpha_RESSP alpha within the RE aperturephys.abundDOUBLEprincipalAge_RE_errUncertainty on SSP Age within the RE apertureGyrstime.age;stat.errorDOUBLEprincipalZ_RE_errUncertainty on SSP Z within the RE aperturephys.abund;stat.errorDOUBLEprincipalalpha_RE_errUncertainty on SSP alpha within the RE aperturephys.abund;stat.errorDOUBLEprincipalAge_2_ARCSECONDSSP Age within the 2 arcsec apertureGyrstime.ageDOUBLEprincipalZ_2_ARCSECONDSSP Z within the 2 arcsec aperturephys.abundDOUBLEprincipalalpha_2_ARCSECONDSSP alpha within the 2 arcsec aperturephys.abundDOUBLEprincipalAge_2_ARCSECOND_errUncertainty on SSP Age within the 2 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_2_ARCSECOND_errUncertainty on SSP Z within the 2 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_2_ARCSECOND_errUncertainty on SSP alpha within the 2 arcsec aperturephys.abund;stat.errorDOUBLEprincipalAge_1_4_ARCSECONDSSP Age within the 1.4 arcsec apertureGyrstime.ageDOUBLEprincipalZ_1_4_ARCSECONDSSP Z within the 1.4 arcsec aperturephys.abundDOUBLEprincipalalpha_1_4_ARCSECONDSSP alpha within the 1.4 arcsec aperturephys.abundDOUBLEprincipalAge_1_4_ARCSECOND_errUncertainty on SSP Age within the 1.4 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_1_4_ARCSECOND_errUncertainty on SSP Z within the 1.4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_1_4_ARCSECOND_errUncertainty on SSP alpha within the 1.4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalAge_4_ARCSECONDSSP Age within the 4 arcsec apertureGyrstime.ageDOUBLEprincipalZ_4_ARCSECONDSSP Z within the 4 arcsec aperturephys.abundDOUBLEprincipalalpha_4_ARCSECONDSSP alpha within the 4 arcsec aperturephys.abundDOUBLEprincipalAge_4_ARCSECOND_errUncertainty on SSP Age within the 4 arcsec apertureGyrstime.age;stat.errorDOUBLEprincipalZ_4_ARCSECOND_errUncertainty on SSP Z within the 4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalalpha_4_ARCSECOND_errUncertainty on SSP alpha within the 4 arcsec aperturephys.abund;stat.errorDOUBLEprincipalsami_dr2.Gas1compAperturesAperture 1-component emission line fluxes, ionised gas kinematics, and star formation ratesCATIDSAMI galaxy IDmeta.idVARCHARprincipalRASAMI galaxy Right AscensionDegreesmeta.idVARCHARprincipalDECSAMI galaxy DeclinationDegreesmeta.idVARCHARprincipalZSAMI galaxy Redshift assumedmeta.idVARCHARprincipalR_ESAMI galaxy effective radiusarcsecondmeta.idVARCHARprincipalELLIPSAMI galaxy ellipticitymeta.idVARCHARprincipalPASAMI galaxy Position AngleDegreesmeta.idVARCHARprincipalNPIX_RENumber of pixels in RE aperture_meta.valueVARCHARprincipalAREA_COV_REFraction of SAMI FoV covered by RE aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_RE1-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_REUncertainty on 1-component Gas velocity in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_RE1-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_REUncertainty on 1-component Gas velocity dispersion in RE aperturekm/sphys.velocityVARCHARprincipalOII3727_RETotal [OII]3727 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOII3727_ERR_REUncertainty on total [OII]3727 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_RETotal Hbeta flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_ERR_REUncertainty on total Hbeta flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_RETotal [OIII]5007 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_ERR_REUncertainty on total [OIII]5007 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_RETotal [OI]6300 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_ERR_REUncertainty on total [OI]6300 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_RETotal Halpha flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_REUncertainty on total Halpha flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_RE1-component Halpha flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_REUncertainty on 1-component Halpha flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_RETotal [NII]6583 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_ERR_REUncertainty on total [NII]6583 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_RETotal [SII]6716 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_ERR_REUncertainty on total [SII]6716 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_RETotal [SII]6731 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_ERR_REUncertainty on total [SII]6731 flux in RE aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalEXTINCTION_CORR_REExtinction correction on total Halpha flux in RE aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_REUncertainty in extinction correction on total Halpha flux in RE aperturephys.fluxcorrVARCHARprincipalSFR_REStar formation rate in RE apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_REUncertainty in star formation rate in RE apertureMsun/yrphys.sfrVARCHARprincipalNPIX_3KPC_ROUNDNumber of pixels in 3KPC aperture_meta.valueVARCHARprincipalAREA_COV_3KPC_ROUNDFraction of SAMI FoV covered by 3KPC aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_3KPC_ROUND1-component Gas velocity in 3KPC aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_3KPC_ROUNDUncertainty on 1-component Gas velocity in 3KPC aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_3KPC_ROUND1-component Gas velocity dispersion in 3KPC aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_3KPC_ROUNDUncertainty on 1-component Gas velocity dispersion in 3KPC aperturekm/sphys.velocityVARCHARprincipalOII3727_3KPC_ROUNDTotal [OII]3727 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOII3727_ERR_3KPC_ROUNDUncertainty on total [OII]3727 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_3KPC_ROUNDTotal Hbeta flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_ERR_3KPC_ROUNDUncertainty on total Hbeta flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_3KPC_ROUNDTotal [OIII]5007 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_ERR_3KPC_ROUNDUncertainty on total [OIII]5007 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_3KPC_ROUNDTotal [OI]6300 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_ERR_3KPC_ROUNDUncertainty on total [OI]6300 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_3KPC_ROUNDTotal Halpha flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_3KPC_ROUNDUncertainty on total Halpha flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_3KPC_ROUND1-component Halpha flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_3KPC_ROUNDUncertainty on 1-component Halpha flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_3KPC_ROUNDTotal [NII]6583 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_ERR_3KPC_ROUNDUncertainty on total [NII]6583 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_3KPC_ROUNDTotal [SII]6716 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_ERR_3KPC_ROUNDUncertainty on total [SII]6716 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_3KPC_ROUNDTotal [SII]6731 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_ERR_3KPC_ROUNDUncertainty on total [SII]6731 flux in 3KPC aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalEXTINCTION_CORR_3KPC_ROUNDExtinction correction on total Halpha flux in 3KPC aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_3KPC_ROUNDUncertainty in extinction correction on total Halpha flux in 3KPC aperturephys.fluxcorrVARCHARprincipalSFR_3KPC_ROUNDStar formation rate in 3KPC apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_3KPC_ROUNDUncertainty in star formation rate in 3KPC apertureMsun/yrphys.sfrVARCHARprincipalNPIX_1_4_ARCSECONDNumber of pixels in the 1.4 arcsecond aperture_meta.valueVARCHARprincipalAREA_COV_1_4_ARCSECONDFraction of SAMI FoV covered by the 1.4 arcsecond aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_1_4_ARCSECOND1-component Gas velocity in the 1.4 arcsecond aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_1_4_ARCSECONDUncertainty on 1-component Gas velocity in the 1.4 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_1_4_ARCSECOND1-component Gas velocity dispersion in the 1.4 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_1_4_ARCSECONDUncertainty on 1-component Gas velocity dispersion in the 1.4 arcsecond aperturekm/sphys.velocityVARCHARprincipalOII3727_1_4_ARCSECONDTotal [OII]3727 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOII3727_ERR_1_4_ARCSECONDUncertainty on total [OII]3727 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_1_4_ARCSECONDTotal Hbeta flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_ERR_1_4_ARCSECONDUncertainty on total Hbeta flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_1_4_ARCSECONDTotal [OIII]5007 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_ERR_1_4_ARCSECONDUncertainty on total [OIII]5007 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_1_4_ARCSECONDTotal [OI]6300 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_ERR_1_4_ARCSECONDUncertainty on total [OI]6300 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_1_4_ARCSECONDTotal Halpha flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_1_4_ARCSECONDUncertainty on total Halpha flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_1_4_ARCSECOND1-component Halpha flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_1_4_ARCSECONDUncertainty on 1-component Halpha flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_1_4_ARCSECONDTotal [NII]6583 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_ERR_1_4_ARCSECONDUncertainty on total [NII]6583 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_1_4_ARCSECONDTotal [SII]6716 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_ERR_1_4_ARCSECONDUncertainty on total [SII]6716 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_1_4_ARCSECONDTotal [SII]6731 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_ERR_1_4_ARCSECONDUncertainty on total [SII]6731 flux in the 1.4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalEXTINCTION_CORR_1_4_ARCSECONDExtinction correction on total Halpha flux in the 1.4 arcsecond aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_1_4_ARCSECONDUncertainty in extinction correction on total Halpha flux in the 1.4 arcsecond aperturephys.fluxcorrVARCHARprincipalSFR_1_4_ARCSECONDStar formation rate in the 1.4 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_1_4_ARCSECONDUncertainty in star formation rate in the 1.4 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalNPIX_2_ARCSECONDNumber of pixels in the 2 arcsecond aperture_meta.valueVARCHARprincipalAREA_COV_2_ARCSECONDFraction of SAMI FoV covered by the 2 arcsecond aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_2_ARCSECOND1-component Gas velocity in the 2 arcsecond aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_2_ARCSECONDUncertainty on 1-component Gas velocity in the 2 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_2_ARCSECOND1-component Gas velocity dispersion in the 2 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_2_ARCSECONDUncertainty on 1-component Gas velocity dispersion in the 2 arcsecond aperturekm/sphys.velocityVARCHARprincipalOII3727_2_ARCSECONDTotal [OII]3727 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOII3727_ERR_2_ARCSECONDUncertainty on total [OII]3727 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_2_ARCSECONDTotal Hbeta flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_ERR_2_ARCSECONDUncertainty on total Hbeta flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_2_ARCSECONDTotal [OIII]5007 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_ERR_2_ARCSECONDUncertainty on total [OIII]5007 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_2_ARCSECONDTotal [OI]6300 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_ERR_2_ARCSECONDUncertainty on total [OI]6300 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_2_ARCSECONDTotal Halpha flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_2_ARCSECONDUncertainty on total Halpha flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_2_ARCSECOND1-component Halpha flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_2_ARCSECONDUncertainty on 1-component Halpha flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_2_ARCSECONDTotal [NII]6583 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_ERR_2_ARCSECONDUncertainty on total [NII]6583 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_2_ARCSECONDTotal [SII]6716 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_ERR_2_ARCSECONDUncertainty on total [SII]6716 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_2_ARCSECONDTotal [SII]6731 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_ERR_2_ARCSECONDUncertainty on total [SII]6731 flux in the 2 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalEXTINCTION_CORR_2_ARCSECONDExtinction correction on total Halpha flux in the 2 arcsecond aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_2_ARCSECONDUncertainty in extinction correction on total Halpha flux in the 2 arcsecond aperturephys.fluxcorrVARCHARprincipalSFR_2_ARCSECONDStar formation rate in the 2 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_2_ARCSECONDUncertainty in star formation rate in the 2 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalNPIX_3_ARCSECONDNumber of pixels in the 3 arcsecond aperture_meta.valueVARCHARprincipalAREA_COV_3_ARCSECONDFraction of SAMI FoV covered by the 3 arcsecond aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_3_ARCSECOND1-component Gas velocity in the 3 arcsecond aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_3_ARCSECONDUncertainty on 1-component Gas velocity in the 3 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_3_ARCSECOND1-component Gas velocity dispersion in the 3 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_3_ARCSECONDUncertainty on 1-component Gas velocity dispersion in the 3 arcsecond aperturekm/sphys.velocityVARCHARprincipalOII3727_3_ARCSECONDTotal [OII]3727 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOII3727_ERR_3_ARCSECONDUncertainty on total [OII]3727 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_3_ARCSECONDTotal Hbeta flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_ERR_3_ARCSECONDUncertainty on total Hbeta flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_3_ARCSECONDTotal [OIII]5007 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_ERR_3_ARCSECONDUncertainty on total [OIII]5007 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_3_ARCSECONDTotal [OI]6300 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_ERR_3_ARCSECONDUncertainty on total [OI]6300 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_3_ARCSECONDTotal Halpha flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_3_ARCSECONDUncertainty on total Halpha flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_3_ARCSECOND1-component Halpha flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_3_ARCSECONDUncertainty on 1-component Halpha flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_3_ARCSECONDTotal [NII]6583 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_ERR_3_ARCSECONDUncertainty on total [NII]6583 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_3_ARCSECONDTotal [SII]6716 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_ERR_3_ARCSECONDUncertainty on total [SII]6716 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_3_ARCSECONDTotal [SII]6731 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_ERR_3_ARCSECONDUncertainty on total [SII]6731 flux in the 3 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalEXTINCTION_CORR_3_ARCSECONDExtinction correction on total Halpha flux in the 3 arcsecond aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_3_ARCSECONDUncertainty in extinction correction on total Halpha flux in the 3 arcsecond aperturephys.fluxcorrVARCHARprincipalSFR_3_ARCSECONDStar formation rate in the 3 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_3_ARCSECONDUncertainty in star formation rate in the 3 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalNPIX_4_ARCSECONDNumber of pixels in the 4 arcsecond aperture_meta.valueVARCHARprincipalAREA_COV_4_ARCSECONDFraction of SAMI FoV covered by the 4 arcsecond aperturemeta.valueVARCHARprincipalV_GAS_1_COMP_4_ARCSECOND1-component Gas velocity in the 4 arcsecond aperturekm/sphys.velocityVARCHARprincipalV_GAS_1_COMP_ERR_4_ARCSECONDUncertainty on 1-component Gas velocity in the 4 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_1_COMP_4_ARCSECOND1-component Gas velocity dispersion in the 4 arcsecond aperturekm/sphys.velocityVARCHARprincipalVDISP_GAS_ERR_1_COMP_4_ARCSECONDUncertainty on 1-component Gas velocity dispersion in the 4 arcsecond aperturekm/sphys.velocityVARCHARprincipalOII3727_4_ARCSECONDTotal [OII]3727 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOII3727_ERR_4_ARCSECONDUncertainty on total [OII]3727 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_4_ARCSECONDTotal Hbeta flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHBETA_ERR_4_ARCSECONDUncertainty on total Hbeta flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_4_ARCSECONDTotal [OIII]5007 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOIII5007_ERR_4_ARCSECONDUncertainty on total [OIII]5007 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_4_ARCSECONDTotal [OI]6300 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalOI6300_ERR_4_ARCSECONDUncertainty on total [OI]6300 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_4_ARCSECONDTotal Halpha flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_TOTAL_ERR_4_ARCSECONDUncertainty on total Halpha flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_4_ARCSECOND1-component Halpha flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalHALPHA_1_COMP_ERR_4_ARCSECONDUncertainty on 1-component Halpha flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_4_ARCSECONDTotal [NII]6583 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalNII6583_ERR_4_ARCSECONDUncertainty on total [NII]6583 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_4_ARCSECONDTotal [SII]6716 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6716_ERR_4_ARCSECONDUncertainty on total [SII]6716 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_4_ARCSECONDTotal [SII]6731 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalSII6731_ERR_4_ARCSECONDUncertainty on total [SII]6731 flux in the 4 arcsecond aperture1E-16 erg/s/cm^2phys.fluxVARCHARprincipalEXTINCTION_CORR_4_ARCSECONDExtinction correction on total Halpha flux in the 4 arcsecond aperturephys.fluxcorrVARCHARprincipalEXTINCTION_CORR_ERR_4_ARCSECONDUncertainty in extinction correction on total Halpha flux in the 4 arcsecond aperturephys.fluxcorrVARCHARprincipalSFR_4_ARCSECONDStar formation rate in the 4 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalSFR_ERR_4_ARCSECONDUncertainty in star formation rate in the 4 arcsecond apertureMsun/yrphys.sfrVARCHARprincipalgleamx_dr1placeholdergleamx_dr1.idr1_subset_filtered_seds_paperGLEAM-X DR1 cataloguera_strRight Ascension J2000pos.eq.ra;meta.mainVARCHARindexedprincipalpeak_flux_widePeak flux in wide imageJy/beamphot.flux.density;em.radio.170-231MHzREALprincipalint_flux_wideIntegrated flux in wide imageJyphot.flux;em.radio.170-231MHzREALprincipalpeak_flux_084Peak flux in 080-088MHz imageJy/beamphot.flux.density;em.radio.080-088MHzREALprincipalpeak_flux_189Peak flux in 185-193MHz imageJy/beamphot.flux.density;em.radio.185-193MHzREALprincipalpsf_a_W_087Semi-major axis of the point spread function in 072-103MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_087Semi-minor axis of the point spread function in 072-103MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_087Position angle of the point spread function in 072-103MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_118Background level in 103-134MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_118Local noise level in 103-134MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_118Peak flux in 103-134MHz imageJy/beamphot.flux.density;em.radio.103-134MHzREALprincipalerr_peak_flux_W_118Uncertainty in fit for peak flux in 103-134MHz imageJy/beamstat.error;phot.flux.density;em.radio.103-134MHzREALprincipalint_flux_W_118Integrated flux in 103-134MHz imageJyphot.flux;em.radio.103-134MHzREALprincipalbackground_W_154Background level in 139-170MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_154Local noise level in 139-170MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipala_wideFitted semi-major axis in wide imagearcsecphys.angSize.smajAxis;meta.modelledREALprincipalerr_a_wideUncertainty in fitted semi-major axis in wide imagearcsecstat.error;phys.angSize.smajAxisREALprincipalb_wideFitted semi-minor axis in wide imagearcsecphys.angSize.sminAxis;meta.modelledREALprincipalerr_b_wideUncertainty in fitted semi-minor axis in wide imagearcsecstat.error;phys.angSize.sminAxisREALprincipalerr_pa_wideUncertainty in fitted position angle in wide imagedegstat.error;pos.posAngREALprincipalresidual_mean_wideMean value of data-model in wide imageJy/beamstat.fit.residualREALprincipalpsf_a_wideSemi-major axis of the point spread function in wide imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalerr_abs_flux_pctPercent error in absolute flux scale - all frequencies%stat.error;phot.flux;em.radioREALprincipalerr_fit_flux_pctPercent error on internal flux scale - all frequencies%stat.error;phot.flux;em.radioREALprincipalpsf_b_wideSemi-minor axis of the point spread function in wide imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_widePosition angle of the point spread function in wide imagedegpos.posAng;instr.det.psfREALprincipalbackground_076Background level in 072-080MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_076Local noise level in 072-080MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_076Peak flux in 072-080MHz imageJy/beamphot.flux.density;em.radio.072-080MHzREALprincipalint_flux_076Integrated flux in 072-080MHz imageJyphot.flux;em.radio.072-080MHzREALprincipalerr_int_flux_076Uncertainty in fit for integrated flux in 072-080MHz imageJystat.error;phot.flux;em.radio.072-080MHzREALprincipala_076Fitted semi-major axis in 072-080MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalpsf_b_076Semi-minor axis of the point spread function in 072-080MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_076Position angle of the point spread function in 072-080MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_084Background level in 080-088MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_084Local noise level in 080-088MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpsf_pa_227Position angle of the point spread function in 223-231MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_087Background level in 072-103MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipalNameIAU Namemeta.id;srcVARCHARindexedprincipalpa_wideFitted position angle in wide imagedegpos.posAng;meta.modelledREALprincipalerr_peak_flux_084Uncertainty in fit for peak flux in 080-088MHz imageJy/beamstat.error;phot.flux.density;em.radio.080-088MHzREALprincipalint_flux_084Integrated flux in 080-088MHz imageJyphot.flux;em.radio.080-088MHzREALprincipalerr_int_flux_084Uncertainty in fit for integrated flux in 080-088MHz imageJystat.error;phot.flux;em.radio.080-088MHzREALprincipala_084Fitted semi-major axis in 080-088MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_084Fitted semi-minor axis in 080-088MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_084Fitted position angle in 080-088MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_084Mean value of data-model in 080-088MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_084Standard deviation of data-model in 080-088MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_084Semi-major axis of the point spread function in 080-088MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_084Semi-minor axis of the point spread function in 080-088MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_084Position angle of the point spread function in 080-088MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_092Background level in 088-095MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipalpeak_flux_099Peak flux in 095-103MHz imageJy/beamphot.flux.density;em.radio.095-103MHzREALprincipalerr_peak_flux_076Uncertainty in fit for peak flux in 072-080MHz imageJy/beamstat.error;phot.flux.density;em.radio.072-080MHzREALprincipalerr_peak_flux_099Uncertainty in fit for peak flux in 095-103MHz imageJy/beamstat.error;phot.flux.density;em.radio.095-103MHzREALprincipalint_flux_099Integrated flux in 095-103MHz imageJyphot.flux;em.radio.095-103MHzREALprincipalerr_int_flux_099Uncertainty in fit for integrated flux in 095-103MHz imageJystat.error;phot.flux;em.radio.095-103MHzREALprincipalb_076Fitted semi-minor axis in 072-080MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_076Fitted position angle in 072-080MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_076Mean value of data-model in 072-080MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_076Standard deviation of data-model in 072-080MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_076Semi-major axis of the point spread function in 072-080MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipala_099Fitted semi-major axis in 095-103MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_099Fitted semi-minor axis in 095-103MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_099Fitted position angle in 095-103MHz imagedegpos.posAng;meta.modelledREALprincipallocal_rms_wideLocal noise leve in wide imageJy/beamstat.variance;phot.flux.densityREALprincipaldec_strDeclination J2000d:m:spos.eq.dec;meta.mainVARCHARindexedprincipalRAJ2000Right Ascension J2000degpos.eq.raREALindexedprincipalerr_RAJ2000Uncertainty in Right Ascensiondegstat.error;pos.eq.raREALprincipalDEJ2000Declination J2000degpos.eq.decREALindexedprincipalerr_DEJ2000Uncertainty in Declinationdegstat.error;pos.eq.decREALprincipalresidual_mean_099Mean value of data-model in 095-103MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_099Standard deviation of data-model in 095-103MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_099Semi-major axis of the point spread function in 095-103MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_099Semi-minor axis of the point spread function in 095-103MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_099Position angle of the point spread function in 095-103MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_107Background level in 103-111MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_107Local noise level in 103-111MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_107Peak flux in 103-111MHz imageJy/beamphot.flux.density;em.radio.103-111MHzREALprincipalerr_peak_flux_107Uncertainty in fit for peak flux in 103-111MHz imageJy/beamstat.error;phot.flux.density;em.radio.103-111MHzREALprincipalint_flux_107Integrated flux in 103-111MHz imageJyphot.flux;em.radio.103-111MHzREALprincipalerr_int_flux_107Uncertainty in fit for integrated flux in 103-111MHz imageJystat.error;phot.flux;em.radio.103-111MHzREALprincipala_107Fitted semi-major axis in 103-111MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_107Fitted semi-minor axis in 103-111MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_107Fitted position angle in 103-111MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_107Mean value of data-model in 103-111MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_107Standard deviation of data-model in 103-111MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_107Semi-major axis of the point spread function in 103-111MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_107Semi-minor axis of the point spread function in 103-111MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_107Position angle of the point spread function in 103-111MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_115Background level in 111-118MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_115Local noise level in 111-118MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_115Peak flux in 111-118MHz imageJy/beamphot.flux.density;em.radio.111-118MHzREALprincipalerr_peak_flux_115Uncertainty in fit for peak flux in 111-118MHz imageJy/beamstat.error;phot.flux.density;em.radio.111-118MHzREALprincipalint_flux_115Integrated flux in 111-118MHz imageJyphot.flux;em.radio.111-118MHzREALprincipalerr_int_flux_115Uncertainty in fit for integrated flux in 111-118MHz imageJystat.error;phot.flux;em.radio.111-118MHzREALprincipala_115Fitted semi-major axis in 111-118MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_115Fitted semi-minor axis in 111-118MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_115Fitted position angle in 111-118MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_115Mean value of data-model in 111-118MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_115Standard deviation of data-model in 111-118MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_115Semi-major axis of the point spread function in 111-118MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_115Semi-minor axis of the point spread function in 111-118MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_115Position angle of the point spread function in 111-118MHz imagedegpos.posAng;instr.det.psfREALprincipallocal_rms_122Local noise level in 118-126MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_122Peak flux in 118-126MHz imageJy/beamphot.flux.density;em.radio.118-126MHzREALprincipalerr_peak_flux_122Uncertainty in fit for peak flux in 118-126MHz imageJy/beamstat.error;phot.flux.density;em.radio.118-126MHzREALprincipalint_flux_122Integrated flux in 118-126MHz imageJyphot.flux;em.radio.118-126MHzREALprincipalerr_int_flux_122Uncertainty in fit for integrated flux in 118-126MHz imageJystat.error;phot.flux;em.radio.118-126MHzREALprincipala_122Fitted semi-major axis in 118-126MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_122Fitted semi-minor axis in 118-126MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_122Fitted position angle in 118-126MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_122Mean value of data-model in 118-126MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_122Standard deviation of data-model in 118-126MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_122Semi-major axis of the point spread function in 118-126MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalbackground_wideBackground level in wide imageJy/beamstat.median;phot.flux.densityREALprincipalresidual_std_wideStandard deviation of data-model in wide imageJy/beamstat.fit.residualREALprincipalpsf_b_122Semi-minor axis of the point spread function in 118-126MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_122Position angle of the point spread function in 118-126MHz imagedegpos.posAng;instr.det.psfREALprincipalerr_peak_flux_130Uncertainty in fit for peak flux in 126-134MHz imageJy/beamstat.error;phot.flux.density;em.radio.126-134MHzREALprincipalint_flux_130Integrated flux in 126-134MHz imageJyphot.flux;em.radio.126-134MHzREALprincipalerr_int_flux_130Uncertainty in fit for integrated flux in 126-134MHz imageJystat.error;phot.flux;em.radio.126-134MHzREALprincipala_130Fitted semi-major axis in 126-134MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_130Fitted semi-minor axis in 126-134MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_130Fitted position angle in 126-134MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_130Mean value of data-model in 126-134MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_130Standard deviation of data-model in 126-134MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_130Semi-major axis of the point spread function in 126-134MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_130Semi-minor axis of the point spread function in 126-134MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_130Position angle of the point spread function in 126-134MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_143Background level in 139-147MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_143Local noise level in 139-147MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalerr_peak_flux_143Uncertainty in fit for peak flux in 139-147MHz imageJy/beamstat.error;phot.flux.density;em.radio.139-147MHzREALprincipalint_flux_143Integrated flux in 139-147MHz imageJyphot.flux;em.radio.139-147MHzREALprincipalerr_int_flux_143Uncertainty in fit for integrated flux in 139-147MHz imageJystat.error;phot.flux;em.radio.139-147MHzREALprincipala_143Fitted semi-major axis in 139-147MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_143Fitted semi-minor axis in 139-147MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_143Fitted position angle in 139-147MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_143Mean value of data-model in 139-147MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_143Standard deviation of data-model in 139-147MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_143Semi-major axis of the point spread function in 139-147MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_143Semi-minor axis of the point spread function in 139-147MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_143Position angle of the point spread function in 139-147MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_151Background level in 147-154MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_151Local noise level in 147-154MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_151Peak flux in 147-154MHz imageJy/beamphot.flux.density;em.radio.147-154MHzREALprincipalerr_peak_flux_151Uncertainty in fit for peak flux in 147-154MHz imageJy/beamstat.error;phot.flux.density;em.radio.147-154MHzREALprincipalint_flux_151Integrated flux in 147-154MHz imageJyphot.flux;em.radio.147-154MHzREALprincipalerr_int_flux_151Uncertainty in fit for integrated flux in 147-154MHz imageJystat.error;phot.flux;em.radio.147-154MHzREALprincipala_151Fitted semi-major axis in 147-154MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_151Fitted semi-minor axis in 147-154MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_151Fitted position angle in 147-154MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_151Mean value of data-model in 147-154MHz imageJy/beamstat.fit.residualREALprincipalpsf_b_151Semi-minor axis of the point spread function in 147-154MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_151Position angle of the point spread function in 147-154MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_158Background level in 154-162MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_158Local noise level in 154-162MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_158Peak flux in 154-162MHz imageJy/beamphot.flux.density;em.radio.154-162MHzREALprincipalerr_peak_flux_158Uncertainty in fit for peak flux in 154-162MHz imageJy/beamstat.error;phot.flux.density;em.radio.154-162MHzREALprincipalint_flux_158Integrated flux in 154-162MHz imageJyphot.flux;em.radio.154-162MHzREALprincipalerr_int_flux_158Uncertainty in fit for integrated flux in 154-162MHz imageJystat.error;phot.flux;em.radio.154-162MHzREALprincipala_158Fitted semi-major axis in 154-162MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_158Fitted semi-minor axis in 154-162MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_158Fitted position angle in 154-162MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_158Mean value of data-model in 154-162MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_158Standard deviation of data-model in 154-162MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_158Semi-major axis of the point spread function in 154-162MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_158Semi-minor axis of the point spread function in 154-162MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_158Position angle of the point spread function in 154-162MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_166Background level in 162-170MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_166Local noise level in 162-170MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_166Peak flux in 162-170MHz imageJy/beamphot.flux.density;em.radio.162-170MHzREALprincipalerr_peak_flux_166Uncertainty in fit for peak flux in 162-170MHz imageJy/beamstat.error;phot.flux.density;em.radio.162-170MHzREALprincipalint_flux_166Integrated flux in 162-170MHz imageJyphot.flux;em.radio.162-170MHzREALprincipalerr_int_flux_166Uncertainty in fit for integrated flux in 162-170MHz imageJystat.error;phot.flux;em.radio.162-170MHzREALprincipala_166Fitted semi-major axis in 162-170MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_166Fitted semi-minor axis in 162-170MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_166Fitted position angle in 162-170MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_166Mean value of data-model in 162-170MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_166Standard deviation of data-model in 162-170MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_166Semi-major axis of the point spread function in 162-170MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_166Semi-minor axis of the point spread function in 162-170MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_166Position angle of the point spread function in 162-170MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_174Background level in 170-177MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_174Local noise level in 170-177MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_174Peak flux in 170-177MHz imageJy/beamphot.flux.density;em.radio.170-177MHzREALprincipalerr_peak_flux_174Uncertainty in fit for peak flux in 170-177MHz imageJy/beamstat.error;phot.flux.density;em.radio.170-177MHzREALprincipalresidual_std_181Standard deviation of data-model in 177-185MHz imageJy/beamstat.fit.residualREALprincipalerr_peak_flux_189Uncertainty in fit for peak flux in 185-193MHz imageJy/beamstat.error;phot.flux.density;em.radio.185-193MHzREALprincipalint_flux_189Integrated flux in 185-193MHz imageJyphot.flux;em.radio.185-193MHzREALprincipalerr_int_flux_189Uncertainty in fit for integrated flux in 185-193MHz imageJystat.error;phot.flux;em.radio.185-193MHzREALprincipala_189Fitted semi-major axis in 185-193MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_189Fitted semi-minor axis in 185-193MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_189Fitted position angle in 185-193MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_189Mean value of data-model in 185-193MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_189Standard deviation of data-model in 185-193MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_189Semi-major axis of the point spread function in 185-193MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_189Semi-minor axis of the point spread function in 185-193MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_189Position angle of the point spread function in 185-193MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_197Background level in 193-200MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_197Local noise level in 193-200MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_197Peak flux in 193-200MHz imageJy/beamphot.flux.density;em.radio.193-200MHzREALprincipalerr_peak_flux_197Uncertainty in fit for peak flux in 193-200MHz imageJy/beamstat.error;phot.flux.density;em.radio.193-200MHzREALprincipalint_flux_197Integrated flux in 193-200MHz imageJyphot.flux;em.radio.193-200MHzREALprincipalerr_int_flux_197Uncertainty in fit for integrated flux in 193-200MHz imageJystat.error;phot.flux;em.radio.193-200MHzREALprincipala_197Fitted semi-major axis in 193-200MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_197Fitted semi-minor axis in 193-200MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_197Fitted position angle in 193-200MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_197Mean value of data-model in 193-200MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_197Standard deviation of data-model in 193-200MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_197Semi-major axis of the point spread function in 193-200MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_197Semi-minor axis of the point spread function in 193-200MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_197Position angle of the point spread function in 193-200MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_204Background level in 200-208MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_204Local noise level in 200-208MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_204Peak flux in 200-208MHz imageJy/beamphot.flux.density;em.radio.200-208MHzREALprincipalerr_peak_flux_204Uncertainty in fit for peak flux in 200-208MHz imageJy/beamstat.error;phot.flux.density;em.radio.200-208MHzREALprincipalerr_int_flux_204Uncertainty in fit for integrated flux in 200-208MHz imageJystat.error;phot.flux;em.radio.200-208MHzREALprincipala_204Fitted semi-major axis in 200-208MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_204Fitted semi-minor axis in 200-208MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_204Fitted position angle in 200-208MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_204Mean value of data-model in 200-208MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_204Standard deviation of data-model in 200-208MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_204Semi-major axis of the point spread function in 200-208MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_204Semi-minor axis of the point spread function in 200-208MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_204Position angle of the point spread function in 200-208MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_212Background level in 208-216MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipalpeak_flux_143Peak flux in 139-147MHz imageJy/beamphot.flux.density;em.radio.139-147MHzREALprincipallocal_rms_212Local noise level in 208-216MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_212Peak flux in 208-216MHz imageJy/beamphot.flux.density;em.radio.208-216MHzREALprincipalerr_peak_flux_212Uncertainty in fit for peak flux in 208-216MHz imageJy/beamstat.error;phot.flux.density;em.radio.208-216MHzREALprincipalint_flux_212Integrated flux in 208-216MHz imageJyphot.flux;em.radio.208-216MHzREALprincipalerr_int_flux_212Uncertainty in fit for integrated flux in 208-216MHz imageJystat.error;phot.flux;em.radio.208-216MHzREALprincipala_212Fitted semi-major axis in 208-216MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_212Fitted semi-minor axis in 208-216MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_212Fitted position angle in 208-216MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_212Mean value of data-model in 208-216MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_212Standard deviation of data-model in 208-216MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_212Semi-major axis of the point spread function in 208-216MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_212Semi-minor axis of the point spread function in 208-216MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_212Position angle of the point spread function in 208-216MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_220Background level in 216-223MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_220Local noise level in 216-223MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_220Peak flux in 216-223MHz imageJy/beamphot.flux.density;em.radio.216-223MHzREALprincipalerr_peak_flux_220Uncertainty in fit for peak flux in 216-223MHz imageJy/beamstat.error;phot.flux.density;em.radio.216-223MHzREALprincipalint_flux_220Integrated flux in 216-223MHz imageJyphot.flux;em.radio.216-223MHzREALprincipalerr_int_flux_220Uncertainty in fit for integrated flux in 216-223MHz imageJystat.error;phot.flux;em.radio.216-223MHzREALprincipala_220Fitted semi-major axis in 216-223MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_220Fitted semi-minor axis in 216-223MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_220Fitted position angle in 216-223MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_220Mean value of data-model in 216-223MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_220Standard deviation of data-model in 216-223MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_220Semi-major axis of the point spread function in 216-223MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_220Semi-minor axis of the point spread function in 216-223MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_220Position angle of the point spread function in 216-223MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_227Background level in 223-231MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_227Local noise level in 223-231MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_227Peak flux in 223-231MHz imageJy/beamphot.flux.density;em.radio.223-231MHzREALprincipalerr_peak_flux_227Uncertainty in fit for peak flux in 223-231MHz imageJy/beamstat.error;phot.flux.density;em.radio.223-231MHzREALprincipalint_flux_227Integrated flux in 223-231MHz imageJyphot.flux;em.radio.223-231MHzREALprincipalerr_int_flux_227Uncertainty in fit for integrated flux in 223-231MHz imageJystat.error;phot.flux;em.radio.223-231MHzREALprincipala_227Fitted semi-major axis in 223-231MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_227Fitted semi-minor axis in 223-231MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_227Fitted position angle in 223-231MHz imagedegpos.posAng;meta.modelledREALprincipalbackground_130Background level in 126-134MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_130Local noise level in 126-134MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalresidual_mean_227Mean value of data-model in 223-231MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_227Standard deviation of data-model in 223-231MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_227Semi-major axis of the point spread function in 223-231MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_227Semi-minor axis of the point spread function in 223-231MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipallocal_rms_W_087Local noise level in 072-103MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_087Peak flux in 072-103MHz imageJy/beamphot.flux.density;em.radio.072-103MHzREALprincipalerr_peak_flux_W_087Uncertainty in fit for peak flux in 072-103MHz imageJy/beamstat.error;phot.flux.density;em.radio.072-103MHzREALprincipalint_flux_W_087Integrated flux in 072-103MHz imageJyphot.flux;em.radio.072-103MHzREALprincipalerr_int_flux_W_087Uncertainty in fit for integrated flux in 072-103MHz imageJystat.error;phot.flux;em.radio.072-103MHzREALprincipala_W_087Fitted semi-major axis in 072-103MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_087Fitted semi-minor axis in 072-103MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_087Fitted position angle in 072-103MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_087Mean value of data-model in 072-103MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_087Standard deviation of data-model in 072-103MHz imageJy/beamstat.fit.residualREALprincipalpeak_flux_W_154Peak flux in 139-170MHz imageJy/beamphot.flux.density;em.radio.139-170MHzREALprincipalerr_peak_flux_W_154Uncertainty in fit for peak flux in 139-170MHz imageJy/beamstat.error;phot.flux.density;em.radio.139-170MHzREALprincipalint_flux_W_154Integrated flux in 139-170MHz imageJyphot.flux;em.radio.139-170MHzREALprincipalerr_int_flux_W_154Uncertainty in fit for integrated flux in 139-170MHz imageJystat.error;phot.flux;em.radio.139-170MHzREALprincipala_W_154Fitted semi-major axis in 139-170MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_154Fitted semi-minor axis in 139-170MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_154Fitted position angle in 139-170MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_154Mean value of data-model in 139-170MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_154Standard deviation of data-model in 139-170MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_154Semi-major axis of the point spread function in 139-170MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_154Semi-minor axis of the point spread function in 139-170MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalb_W_185Fitted semi-minor axis in 170-200MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_185Fitted position angle in 170-200MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_185Mean value of data-model in 170-200MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_185Standard deviation of data-model in 170-200MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_185Semi-major axis of the point spread function in 170-200MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_185Semi-minor axis of the point spread function in 170-200MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_185Position angle of the point spread function in 170-200MHz imagedegpos.posAng;instr.det.psfREALprincipalresidual_std_151Standard deviation of data-model in 147-154MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_151Semi-major axis of the point spread function in 147-154MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalint_flux_174Integrated flux in 170-177MHz imageJyphot.flux;em.radio.170-177MHzREALprincipalerr_int_flux_174Uncertainty in fit for integrated flux in 170-177MHz imageJystat.error;phot.flux;em.radio.170-177MHzREALprincipala_174Fitted semi-major axis in 170-177MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_174Fitted semi-minor axis in 170-177MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_174Fitted position angle in 170-177MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_174Mean value of data-model in 170-177MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_174Standard deviation of data-model in 170-177MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_174Semi-major axis of the point spread function in 170-177MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_174Semi-minor axis of the point spread function in 170-177MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_174Position angle of the point spread function in 170-177MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_181Background level in 177-185MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipalpeak_flux_181Peak flux in 177-185MHz imageJy/beamphot.flux.density;em.radio.177-185MHzREALprincipalerr_peak_flux_181Uncertainty in fit for peak flux in 177-185MHz imageJy/beamstat.error;phot.flux.density;em.radio.177-185MHzREALprincipalint_flux_181Integrated flux in 177-185MHz imageJyphot.flux;em.radio.177-185MHzREALprincipalerr_int_flux_181Uncertainty in fit for integrated flux in 177-185MHz imageJystat.error;phot.flux;em.radio.177-185MHzREALprincipala_181Fitted semi-major axis in 177-185MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_181Fitted semi-minor axis in 177-185MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_181Fitted position angle in 177-185MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_181Mean value of data-model in 177-185MHz imageJy/beamstat.fit.residualREALprincipalpsf_b_181Semi-minor axis of the point spread function in 177-185MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_181Position angle of the point spread function in 177-185MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_189Background level in 185-193MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipalerr_int_flux_W_185Uncertainty in fit for integrated flux in 170-200MHz imageJystat.error;phot.flux;em.radio.170-200MHzREALprincipalbackground_W_215Background level in 200-231MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_215Local noise level in 200-231MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_215Peak flux in 200-231MHz imageJy/beamphot.flux.density;em.radio.200-231MHzREALprincipalerr_peak_flux_W_215Uncertainty in fit for peak flux in 200-231MHz imageJy/beamstat.error;phot.flux.density;em.radio.200-231MHzREALprincipalint_flux_W_215Integrated flux in 200-231MHz imageJyphot.flux;em.radio.200-231MHzREALprincipalerr_int_flux_W_215Uncertainty in fit for integrated flux in 200-231MHz imageJystat.error;phot.flux;em.radio.200-231MHzREALprincipala_W_215Fitted semi-major axis in 200-231MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_215Fitted semi-minor axis in 200-231MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpsf_pa_W_215Position angle of the point spread function in 200-231MHz imagedegpos.posAng;instr.det.psfREALprincipalsp_int_flux_fit_200Power-law fitted flux density at 200 MHzJyphot.flux;em.radio.200MHzREALprincipalerr_sp_int_flux_fit_200Error on power-law fitted flux density at 200 MHzJystat.error;phot.flux;em.radio.200MHzREALprincipalsp_alphaFitted spectral index assuming power-law SEDspec.index;em.radioREALprincipalpsf_a_181Semi-major axis of the point spread function in 177-185MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipallocal_rms_189Local noise level in 185-193MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_130Peak flux in 126-134MHz imageJy/beamphot.flux.density;em.radio.126-134MHzREALprincipallocal_rms_181Local noise level in 177-185MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpsf_a_W_215Semi-major axis of the point spread function in 200-231MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_215Semi-minor axis of the point spread function in 200-231MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalcsp_alphaFitted spectral index assuming curved SEDspec.index;em.radioREALprincipalerr_csp_alphaError on fitted spectral index assuming curved SEDstat.error;spec.index;em.radioREALprincipalint_flux_204Integrated flux in 200-208MHz imageJyphot.flux;em.radio.200-208MHzREALprincipalpsf_a_W_118Semi-major axis of the point spread function in 103-134MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_118Semi-minor axis of the point spread function in 103-134MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_118Position angle of the point spread function in 103-134MHz imagedegpos.posAng;instr.det.psfREALprincipalerr_int_flux_W_118Uncertainty in fit for integrated flux in 103-134MHz imageJystat.error;phot.flux;em.radio.103-134MHzREALprincipala_W_118Fitted semi-major axis in 103-134MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_118Fitted semi-minor axis in 103-134MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_118Fitted position angle in 103-134MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_118Mean value of data-model in 103-134MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_118Standard deviation of data-model in 103-134MHz imageJy/beamstat.fit.residualREALprincipalerr_peak_flux_wideUncertainty in fit for peak flux in wide imageJy/beamstat.error;phot.flux.density;em.radio.170-231MHzREALprincipalerr_int_flux_wideUncertainty in fit for integrated flux in wide imageJystat.error;phot.flux;em.radio.170-231MHzREALprincipallocal_rms_092Local noise level in 088-095MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_092Peak flux in 088-095MHz imageJy/beamphot.flux.density;em.radio.088-095MHzREALprincipalerr_peak_flux_092Uncertainty in fit for peak flux in 088-095MHz imageJy/beamstat.error;phot.flux.density;em.radio.088-095MHzREALprincipalint_flux_092Integrated flux in 088-095MHz imageJyphot.flux;em.radio.088-095MHzREALprincipalerr_int_flux_092Uncertainty in fit for integrated flux in 088-095MHz imageJystat.error;phot.flux;em.radio.088-095MHzREALprincipala_092Fitted semi-major axis in 088-095MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_092Fitted semi-minor axis in 088-095MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_092Fitted position angle in 088-095MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_092Mean value of data-model in 088-095MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_092Standard deviation of data-model in 088-095MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_092Semi-major axis of the point spread function in 088-095MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_092Semi-minor axis of the point spread function in 088-095MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_092Position angle of the point spread function in 088-095MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_099Background level in 095-103MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_099Local noise level in 095-103MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipala_W_185Fitted semi-major axis in 170-200MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalbackground_122Background level in 118-126MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipalpsf_pa_W_154Position angle of the point spread function in 139-170MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_185Background level in 170-200MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_185Local noise level in 170-200MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_185Peak flux in 170-200MHz imageJy/beamphot.flux.density;em.radio.170-200MHzREALprincipalerr_peak_flux_W_185Uncertainty in fit for peak flux in 170-200MHz imageJy/beamstat.error;phot.flux.density;em.radio.170-200MHzREALprincipalint_flux_W_185Integrated flux in 170-200MHz imageJyphot.flux;em.radio.170-200MHzREALprincipalpa_W_215Fitted position angle in 200-231MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_215Mean value of data-model in 200-231MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_215Standard deviation of data-model in 200-231MHz imageJy/beamstat.fit.residualREALprincipalerr_sp_alphaError on fitted spectral index assuming power-law SEDstat.error;spec.index;em.radioREALprincipalsp_reduced_chi2Reduced chi-squared statistic for power-law SED fitstat.fit.goodnessREALprincipalcsp_int_flux_fit_200Curved SED fitted flux density at 200 MHzJyphot.flux;em.radio.200MHzREALprincipalerr_csp_int_flux_fit_200Error on curved SED fitted flux density at 200 MHzJystat.error;phot.flux;em.radio.200MHzREALprincipalcsp_betaFitted curvature index assuming curved SEDstat.fitREALprincipalerr_csp_betaError on fitted curvature index assuming curved SEDstat.errorREALprincipalcsp_reduced_chi2Reduced chi-squared statistic for curved SED fitstat.fit.goodnessREALprincipaldc_conesearchData Central conesearch tables.dc_conesearch.sami_dr3Data Central cone search table for sami_dr3 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.2dfgrs_fdrData Central cone search table for 2dfgrs_fdr with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.gleamx_dr1Data Central cone search table for gleamx_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.ozdes_dr1Data Central cone search table for ozdes_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.gama_dr2Data Central cone search table for gama_dr2 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.wigglez_finalData Central cone search table for wigglez_final with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.2mass_fdrData Central cone search table for 2mass_fdr with ra and dec both in ICRS degrees.raRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipalnameUnique source name.meta.id;meta.mainVARCHARindexedprincipaldc_conesearch.galahtess_dr1Data Central cone search table for galahtess_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.6dfgs_fdrData Central cone search table for 6dfgs_fdr with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.galah_dr2Data Central cone search table for galah_dr2 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.sami_dr1Data Central cone search table for sami_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.gleam_dr1Data Central cone search table for gleam_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaltable_nameTable name the source originates from within the schema.meta.idVARCHARprincipaldc_conesearch.totalData Central conesearch view consolidating all with dc_conesearch tables.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipalsurvey_drSurvey data release origin for object.degmeta.idVARCHARindexedprincipaldc_conesearch.galah_dr3Data Central cone search table for galah_dr3 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.galah_dr1Data Central cone search table for galah_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.lobes_dr1Data Central cone search table for lobes_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.g4jy_dr1Data Central cone search table for g4jy_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.sami_dr2Data Central cone search table for sami_dr2 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.s5_dr1Data Central cone search table for s5_dr1 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.ozdes_dr2Data Central cone search table for ozdes_dr2 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaldc_conesearch.gama_pdr4v2Data Central cone search table for gama_pdr4v2 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaltable_nameTable name the source originates from within the schema.meta.idVARCHARprincipaldc_conesearch.gama_dr4Data Central cone search table for gama_dr4 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaltable_nameTable name the source originates from within the schema.meta.idVARCHARprincipaldc_conesearch.gleamx_dr2Data Central cone search table for gleamx_dr2 with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaltable_nameTable name the source originates from within the schema.meta.idVARCHARprincipaldc_conesearch.devils_dr1Data Central cone search table for devils_dr1 with ra and dec both in ICRS degrees.raRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipalnameUnique source name.meta.id;meta.mainVARCHARindexedprincipaltable_nameTable name the source originates from within the schema.meta.idVARCHARprincipaldc_conesearch.2dflens_fdrData Central cone search table for 2dflens_fdr with ra and dec both in ICRS degrees.nameUnique source name.meta.id;meta.mainVARCHARindexedprincipaldecDeclination in ICRS degrees.degpos.eq.dec;meta.mainREALindexedprincipaltable_nameTable name the source originates from within the schema.meta.idVARCHARprincipalraRight Ascension in ICRS degrees.degpos.eq.ra;meta.mainREALindexedprincipalnoirlab_test1Test table from noirlab to crossmatch with EMU cataloguesnoirlab_test1.nlabTest table from noirlab to crossmatch with EMU cataloguesa_imagemajor axis size based on an isophotal model [pixel]pixREALprincipalb_imageminor axis size based on an isophotal model [pixel]pixREALprincipaltheta_j2000position angle of source in j2000 coordinates, from non-windowed measurement [degrees]degREALprincipalflags_yy-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_zz-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflux_radius_gg-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixREALprincipalflux_radius_ii-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixREALprincipalflux_radius_rr-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixREALprincipalflux_radius_yy-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixREALprincipalflux_radius_zz-band half-light radius for the object, from elliptical growth-curve, modeled in 2 dimensions [pixel]pixREALprincipalwavg_fluxerr_psf_gg-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_ii-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_rr-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_yy-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_fluxerr_psf_zz-band uncertainty of weighted averaged flux measurement of psf fit single epoch detections [adu]aduREALprincipalflux_auto_gg-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_ii-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_rr-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_yy-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflux_auto_zz-band aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_gg-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_ii-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_rr-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_yy-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalfluxerr_auto_zz-band uncertainty in aperture-flux measurement, elliptical model based on the kron radius [adu]aduREALprincipalflags_gg-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_ii-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalflags_rr-band additive flag describing cautionary advice about source extraction process. use less than 4 for well behaved objectsSMALLINTprincipalmag_auto_z_deredz-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalebv_sfd98e(b-v) reddening coefficient from schlegel, finkbeiner & davis, 1998 [mag]magDOUBLEprincipalwavg_flux_psf_gg-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_ii-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_rr-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_yy-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalwavg_flux_psf_zz-band weighted average flux measurement of psf fit single epoch detections [adu]aduREALprincipalra2Right ascension in right/second table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec2Declination in right/second table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipaldistanceDistance between ra1,dec1 and ra2,dec2 (arcsec)pos.angDistanceDOUBLEprincipalraright ascension, with quantized precision for indexing (alphawin_j2000 has full precision but not indexed) [degrees]degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecdeclination, with quantized precision for indexing (deltawin_j2000 has full precision but not indexed) [degrees]degpos.eq.dec;meta.mainDOUBLEindexedprincipalalphawin_j2000right ascension for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipaldeltawin_j2000declination for the object, j2000 in icrs system (full precision but not indexed) [degrees]degDOUBLEprincipalmag_auto_g_deredg-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipaldesignationUnique source IDmeta.idVARCHARprincipalid1ID in left/first table (coadd_object_id)meta.id;meta.mainBIGINTindexedprincipalra1Right ascension in left/first table (ra)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldec1Declination in left/first table (dec)degpos.eq.dec;meta.mainDOUBLEindexedprincipalid2ID in right/second table (source_id)meta.id;meta.mainVARCHARindexedprincipalmag_auto_i_deredi-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_r_deredr-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipalmag_auto_y_deredy-band dereddened magnitude estimation (using sfd98), for an elliptical model based on the kron radius [mag]magREALprincipal2mass_fdr<p>The Two Micron All Sky Survey (2MASS) project is designed to close the gap between our current technical capability and our knowledge of the near - infrared sky.In addition to providing a context for the interpretation of results obtained at infrared and other wavelengths, 2MASS will provide direct answers to immediate questions on the large-scale structure of the Milky Way and the Local Universe. To achieve these goals, 2MASS is uniformly scanning the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0".</p>2mass_fdr.pscThis table contains photometric measurements for the Point Source CatalograRight ascension (J2000)degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination (J2000)degpos.eq.dec;meta.mainDOUBLEindexedprincipalerr_majSemi-major axis of position error ellipsearcsstat.errorREALprincipalerr_minSemi-minor axis of position error ellipsearcsstat.errorREALprincipalerr_angPosition angle of error ellipse major axis (E of N)degstat.errorINTEGERprincipaldesignationSource designationNonemeta.id;meta.mainVARCHARindexedprincipalj_mJ selected default magnitudemagphot.mag;em.IR.JREALprincipalj_cmsigJ default magnitude uncertaintymagstat.error;phot.magREALprincipalj_msigcomJ total magnitude uncertaintymagstat.error;phot.mag;em.IR.JREALprincipalj_snrJ Signal-to-noise ratioNonestat.snrDOUBLEprincipalh_mH selected default magnitudemagphot.mag;em.IR.HREALprincipalh_cmsigH default magnitude uncertaintymagstat.error;phot.magREALprincipalh_msigcomH total magnitude uncertaintymagstat.error;phot.mag;em.IR.HREALprincipalh_snrH Signal-to-noise ratioNonestat.snrDOUBLEprincipalk_mK selected default magnitudemagphot.mag;em.IR.KREALprincipalk_cmsigK default magnitude uncertaintymagstat.error;phot.magREALprincipalk_msigcomK total magnitude uncertaintymagstat.error;phot.mag;em.IR.KREALprincipalk_snrK Signal-to-noise ratioNonestat.snrDOUBLEprincipalph_qualJHK Photometric quality flagNonemeta.code.qual;photVARCHARprincipalrd_flgSource of JHK default magNonemeta.refVARCHARprincipalbl_flgJHK components fit to sourceNonemeta.codeVARCHARprincipalcc_flgArtifact contamination, confusionNonemeta.codeVARCHARprincipalndetNumber of aperture measurements (jjhhkk)Nonemeta.numberVARCHARprincipalproxDistance between source and nearest neighbourarcspos.angDistanceREALprincipalpxpaPosition angle of vector from source to nearest neighbour (E of N)degpos.posAngINTEGERprincipalpxcntrSequence number of nearest neighbourNonemeta.numberBIGINTprincipalgal_contamExtended source contaminationNonemeta.codeSMALLINTprincipalmp_flgAssociation with asteroid or cometNonemeta.codeSMALLINTprincipalpts_keyUnique source identifier in catalogueNonemeta.id;meta.tableINTEGERprincipalhemisHemisphere of observationNoneobs.param;obsVARCHARprincipaldateObservation dateNonetime.epoch;obsVARCHARprincipalscanScan number (within date)Noneobs.fieldINTEGERprincipalglonGalactic longitudedegpos.galactic.lonDOUBLEprincipalglatGalactic latitudedegpos.galactic.latDOUBLEprincipalx_scanDistance of source from focal plane centerlinearcspos.cartesian;instr.detREALprincipaljdateJulian date of source measurementdtime.epochDOUBLEprincipalj_psfchiJ band reduced $\chi^2$ value of fitNonestat.fit.chi2;stat.valueREALprincipalh_psfchiH band reduced $\chi^2$ value of fitNonestat.fit.chi2;stat.valueREALprincipalk_psfchiK band reduced $\chi^2$ value of fitNonestat.fit.chi2;stat.valueREALprincipalj_m_stdapJ standard aperture magnitudemagphot.mag;em.IR.JREALprincipalj_msig_stdaperror on Jstdapmagstat.errorREALprincipalh_m_stdapH standard aperture magnitudemagphot.mag;em.IR.HREALprincipalh_msig_stdaperror on Hstdapmagstat.errorREALprincipalk_m_stdapK standard aperture magnitudemagphot.mag;em.IR.KREALprincipalk_msig_stdaperror on Kstdapmagstat.errorREALprincipaldist_edge_nsDistance from the source to the nearest North or South scan edgearcspos;arith.diffINTEGERprincipaldist_edge_ewDistance from the source to the nearest East or West scan edgearcspos;arith.diffINTEGERprincipaldist_edge_flgflag indicating to which edges the edgeNS and edgeEW values referNonepos.cartesian;instr.detVARCHARprincipaldup_srcFlag indicating duplicate sourceNonemeta.codeSMALLINTprincipaluse_srcUse source flagNonemeta.codeSMALLINTprincipalaAssociated optical sourceNonemeta.id;meta.datasetVARCHARprincipaldist_optDistance to associated optical sourcearcspos.angDistanceREALprincipalphi_optposition angle from optical source to the 2MASS source positiondegpos.posAngINTEGERprincipalb_m_optBlue magnitude of associated optical sourcemagphot.mag;em.opt.BREALprincipalvr_m_optVisual or red mag of associated optical sourcemagphot.mag;em.opt.RREALprincipalnopt_mchsNumber of optical sources within 5arcsecNonemeta.numberSMALLINTprincipalext_keyRecord Identifier in XSCNonemeta.id.crossINTEGERprincipalscan_keyRecord Identifier in the Scan Information TableNonemeta.idINTEGERprincipalcoadd_keyRecord Identifier in the Atlas Image Data TableNonemeta.id;meta.datasetINTEGERprincipalcoaddSequence number of the Atlas ImageNonemeta.numberINTEGERprincipal2mass_fdr.xscThis table contains photometric measurements for the Extended Source Catalogh_flg_70Confusion flags of h_m_70Nonemeta.codeSMALLINTprincipalk_m_70K magnitude in 70arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_70$\sigma$ k_m_70magstat.error;phot.mag;em.IR.KREALprincipalk_flg_70Confusion flags of k_m_70Nonemeta.codeSMALLINTprincipalj_m_sysJ system magnitudemagphot.mag;em.IR.JREALprincipalj_msig_sys$\sigma$ j_m_sysmagstat.error;phot.mag;em.IR.JREALprincipalh_m_sysH system magnitudemagphot.mag;em.IR.HREALprincipalh_msig_sys$\sigma$ h_m_sysmagstat.error;phot.mag;em.IR.HREALprincipalk_m_sysK system magnitudemagphot.mag;em.IR.KREALprincipalk_msig_sys$\sigma$ k_m_sysmagstat.error;phot.mag;em.IR.KREALprincipalsys_flgsystem flag: 0=no system, 1=nearby galaxy fluxNonemeta.codeSMALLINTprincipalcontam_flgcontamination flag: 0=no stars, 1=stellar fluxNonemeta.codeSMALLINTprincipalj_5sig_baJ minor/major axis ratio to 5$\sigma$ fitNonephys.size.axisRatioREALprincipalj_5sig_phiJ pos.angle to 5$\sigma$ fitdegpos.posAngINTEGERprincipalh_5sig_baH minor/major axis ratio to 5$\sigma$ fitNonephys.size.axisRatioREALprincipalh_5sig_phiH pos.angle to 5$\sigma$ fitdegpos.posAngINTEGERprincipalk_5sig_baK minor/major axis ratio to 5$\sigma$ fitNonephys.size.axisRatioREALprincipalk_5sig_phiK pos.angle to 5 $\sigma$ fitdegpos.posAngINTEGERprincipalj_d_areaJ 5$\sigma$/3$\sigma$ differential areaNonephys.angSizeINTEGERprincipalj_perc_dareaJ 5$\sigma$/3$\sigma$ relative area changeNonephys.angSizeINTEGERprincipaljdateJulian date of the observationdtime.epochDOUBLEprincipaldesignationSource name (HHMMSSss+DDMMSSs, J2000)Nonemeta.id;meta.mainVARCHARindexedprincipalraRight ascension (J2000), based on peak pixeldegpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination (J2000), based on peak pixeldegpos.eq.dec;meta.mainDOUBLEindexedprincipalsup_raSuper-coadd centroid RA (J2000)degpos.eq.raDOUBLEindexedprincipalsup_decSuper-coadd centroid Dec (J2000)degpos.eq.decDOUBLEindexedprincipalglonGalactic longitudedegpos.galactic.lonDOUBLEprincipalglatGalactic latitudedegpos.galactic.latDOUBLEprincipaldensityCoadd log(density) of stars with k<14magNonephys.densityREALprincipalr_k20feSemi-major axis of fiducial ellipse at isophote K=20mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalj_m_k20feJ magnitude in r_k20fe ellipsemagphot.mag;em.IR.JREALprincipalj_msig_k20fe$\sigma$ j_m_k20femagstat.errorREALprincipalj_flg_k20feConfusion flags of j_m_k20feNonemeta.codeSMALLINTprincipalh_m_k20feH magnitude in k20fe ellipsemagphot.mag;em.IR.HREALprincipalh_msig_k20fe$\sigma$ h_m_k20femagstat.errorREALprincipalh_flg_k20feConfusion flags of h_m_k20feNonemeta.codeSMALLINTprincipalk_m_k20feK magnitude in k20fe ellipsemagphot.mag;em.IR.KREALprincipalk_msig_k20fe$\sigma$ k_m_k20femagstat.errorREALprincipalk_flg_k20feConfusion flags of k_m_k20feNonemeta.codeSMALLINTprincipalr_3sigSemi-major axis of 3$\sigma$ K isophotal ellipsearcsecphys.angSize.smajAxis;em.IR.KREALprincipalj_baJ minor/major axis ratio to 3$\sigma$Nonephys.size.axisRatioREALprincipalj_phiJ pos.angle of 3$\sigma$ ellipsedegpos.posAngINTEGERprincipalh_baH minor/major axis ratio to 3$\sigma$Nonephys.size.axisRatioREALprincipalh_phiH pos.angle to 3$\sigma$ ellipsedegpos.posAngINTEGERprincipalk_baK minor/major axis ratio to 3$\sigma$Nonephys.size.axisRatioREALprincipalk_phiK pos.angle to 3$\sigma$ ellipsedegpos.posAngINTEGERprincipalsup_r_3sigSemi-major axis of super-coadd 3$\sigma$ isophotal ellipsearcsecphys.angSize.smajAxisREALprincipalsup_baMinor/major axis ratio to sup_r_3sigNonephys.size.axisRatioREALprincipalsup_phiPos.angle of sup_r_3sigdegpos.posAngINTEGERprincipalr_feK fiducial Kron elliptical aperture semi-major axisarcsecphys.angSize.smajAxis;srcREALprincipalj_m_feJ magnitude in r_femagphot.mag;em.IR.JREALprincipalj_msig_fe$\sigma$ j_m_femagstat.errorREALprincipalj_flg_feConfusion flags of j_m_feNonemeta.codeSMALLINTprincipalh_m_feH magnitude in r_femagphot.mag;em.IR.HREALprincipalh_msig_fe$\sigma$ h_m_femagstat.errorREALprincipalh_flg_feConfusion flags of h_m_feNonemeta.codeSMALLINTprincipalk_m_feK magnitude in r_femagphot.mag;em.IR.KREALprincipalk_msig_fe$\sigma$ k_m_femagstat.errorREALprincipalk_flg_feConfusion flags of k_m_feNonemeta.codeSMALLINTprincipalr_extExtrapolation/total radius of fit to radial profilearcsecphys.angSize;srcREALprincipalj_m_extJ magnitude in r_extmagphot.mag;em.IR.JREALprincipalj_msig_ext$\sigma$ j_m_extmagstat.errorREALprincipalj_pchi$\chi^2$ j_m_extNonemeta.noteREALprincipalh_m_extH magnitude in r_extmagphot.mag;em.IR.HREALprincipalh_msig_ext$\sigma$ r_extmagstat.errorREALprincipalh_pchi$\chi^2$ r_extNonemeta.noteREALprincipalk_m_extK magnitude in r_extmagphot.mag;em.IR.KREALprincipalk_msig_ext$\sigma$ r_extmagstat.errorREALprincipalk_pchi$\chi^2$ r_extNonemeta.noteREALprincipalj_r_effJ half-light radiusarcsecphys.angSize;srcREALprincipalj_mnsurfb_effJ mean surface brightnessmag / arcsec$^2$phot.mag.sb;em.IR.J;stat.meanREALprincipalh_r_effH half-light radiusarcsecphys.angSize;srcREALprincipalh_mnsurfb_effH mean surface brightnessmag / arcsec$^2$phot.mag.sb;em.IR.H;stat.meanREALprincipalk_r_effK half-light radiusarcsecphys.angSize;srcREALprincipalk_mnsurfb_effK mean surface brightnessmag / arcsec$^2$phot.mag.sb;em.IR.K;stat.meanREALprincipalj_con_indxJ concentration indexNonemeta.codeREALprincipalh_con_indxH concentration indexNonemeta.codeREALprincipalk_con_indxK concentration indexNonemeta.codeREALprincipalj_peakJ peak pixel brightnessmag / arcsec$^2$phot.mag.sb;em.IR.JREALprincipalh_peakH peak pixel brightnessmag / arcsec$^2$phot.mag.sb;em.IR.HREALprincipalk_peakK peak pixel brightnessmag / arcsec$^2$phot.mag.sb;em.IR.KREALprincipalj_5surfJ central surface brightness (r<=5 arcsec)mag / arcsec$^2$phot.mag.sb;em.IR.JREALprincipalh_5surfH central surface brightness (r<=5 arcsec)mag / arcsec$^2$phot.mag.sb;em.IR.HREALprincipalk_5surfK central surface brightness (r<=5 arcsec)mag / arcsec$^2$phot.mag.sb;em.IR.KREALprincipale_scoreextended scoreNonesrc.class.starGalaxyREALprincipalg_scoregalaxy scoreNonesrc.class.starGalaxyREALprincipalvcVisual verification of sourceNonemeta.codeINTEGERprincipalcc_flgContamination or confusion flagNonemeta.codeVARCHARprincipalim_nxSize of postage stamp imageNonemeta.numberINTEGERprincipalr_k20fcRadius of fiducial circle at isophote K=20mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalj_m_k20fcJ magnitude in r_k20fcmagphot.mag;em.IR.JREALprincipalj_msig_k20fc$\sigma$ j_m_k20fcmagstat.error;phot.mag;em.IR.JREALprincipalj_flg_k20fcConfusion flags of j_m_k20fcNonemeta.codeSMALLINTprincipalh_m_k20fcH magnitude in r_k20fcmagphot.mag;em.IR.HREALprincipalh_msig_k20fc$\sigma$ h_m_k20fcmagstat.error;phot.mag;em.IR.KREALprincipalh_flg_k20fcConfusion flags of h_m_k20fcNonemeta.codeSMALLINTprincipalk_m_k20fcK magnitude in r_k20fcmagphot.mag;em.IR.KREALprincipalk_msig_k20fc$\sigma$ k_m_k20fcmagstat.error;phot.mag;em.IR.KREALprincipalk_flg_k20fcConfusion flags of k_m_k20fcNonemeta.codeSMALLINTprincipalj_r_eJ Kron ellipse semi-major axisarcsecphys.angSize.smajAxis;srcREALprincipalj_m_eJ magnitude in j_r_emagphot.mag;em.IR.JREALprincipalj_msig_e$\sigma$ j_m_emagstat.errorREALprincipalj_flg_eConfusion flags of j_m_eNonemeta.codeSMALLINTprincipalh_r_eH Kron ellipse semi-major axisarcsecphys.angSize.smajAxis;srcREALprincipalh_m_eH magnitude in h_r_emagphot.mag;em.IR.HREALprincipalh_msig_e$\sigma$ h_m_emagstat.errorREALprincipalh_flg_eConfusion flags of h_m_eNonemeta.codeSMALLINTprincipalk_r_eK Kron ellipse semi-major axisarcsecphys.angSize.smajAxis;srcREALprincipalk_m_eK magnitude in k_r_emagphot.mag;em.IR.KREALprincipalk_msig_e$\sigma$ k_m_emagstat.errorREALprincipalk_flg_eConfusion flags of k_m_eNonemeta.codeSMALLINTprincipalj_r_cKron circular aperture radiusarcsecphys.angSize;srcREALprincipalj_m_cJ Kron circular aperture magnitudemagphot.mag;em.IR.JREALprincipalj_msig_c$\sigma$ j_m_cmagstat.errorREALprincipalj_flg_cConfusion flags of j_m_cNonemeta.codeSMALLINTprincipalh_r_cH Kron circular aperture radiusarcsecphys.angSize;srcREALprincipalh_m_cH Kron circular aperture magnitudemagphot.mag;em.IR.HREALprincipalh_msig_c$\sigma$ h_m_cmagstat.errorREALprincipalh_flg_cConfusion flags of h_m_cNonemeta.codeSMALLINTprincipalk_r_cK Kron circular aperture radiusarcsecphys.angSize;srcREALprincipalk_m_cK Kron circular aperture magnitudemagphot.mag;em.IR.KREALprincipalk_msig_c$\sigma$ k_m_cmagstat.errorREALprincipalk_flg_cConfusion flags of k_m_cNonemeta.codeSMALLINTprincipalr_fcK fiducial Kron circular radiusarcsecphys.angSize;srcREALprincipalj_m_fcJ magnitude in r_fcmagphot.mag;em.IR.JREALprincipalj_msig_fc$\sigma$ j_m_fcmagstat.error;phot.mag;em.IR.JREALprincipalj_flg_fcConfusion flags of j_m_fcNonemeta.codeSMALLINTprincipalh_m_fcH fiducial Kron circular magnitudemagphot.mag;em.IR.HREALprincipalh_msig_fc$\sigma$ h_m_fcmagstat.error;phot.mag;em.IR.HREALprincipalh_flg_fcConfusion flags of h_m_fcNonemeta.codeSMALLINTprincipalk_m_fcK fiducial Kron circular magnitudemagphot.mag;em.IR.KREALprincipalk_msig_fc$\sigma$ k_m_fcmagstat.error;phot.mag;em.IR.KREALprincipalk_flg_fcConfusion flags of k_m_fcNonemeta.codeSMALLINTprincipalj_r_i20eSemi-major axis of elliptical aperture at isophote J=20mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalj_m_i20eJ magnitude in j_r_i20emagphot.mag;em.IR.JREALprincipalj_msig_i20e$\sigma$ j_m_i20emagstat.errorREALprincipalj_flg_i20eConfusion flags of j_m_i20eNonemeta.codeSMALLINTprincipalh_r_i20eSemi-major axis of elliptical aperture at isophote H=20mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalh_m_i20eH magnitude in h_r_i20emagphot.mag;em.IR.HREALprincipalh_msig_i20e$\sigma$ h_m_i20emagstat.errorREALprincipalh_flg_i20eConfusion flags of h_m_i20eNonemeta.codeSMALLINTprincipalk_r_i20eSemi-major axis of elliptical aperture at isophote K=20mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalk_m_i20eK magnitude in k_r_i20emagphot.mag;em.IR.KREALprincipalk_msig_i20e$\sigma$ k_m_i20emagstat.errorREALprincipalk_flg_i20eConfusion flags of k_m_i20eNonemeta.codeSMALLINTprincipalj_r_i20cRadius of circular aperture at isophote J=20mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalj_m_i20cJ magnitude in j_r_i20cmagphot.mag;em.IR.JREALprincipalj_msig_i20c$\sigma$ j_m_i20cmagstat.error;phot.mag;em.IR.JREALprincipalj_flg_i20cConfusion flags of j_m_i20cNonemeta.codeSMALLINTprincipalh_r_i20cRadius of circular aperture at isophote H=20mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalh_m_i20cH magnitude in h_r_i20cmagphot.mag;em.IR.HREALprincipalh_msig_i20c$\sigma$ h_m_i20cmagstat.error;phot.mag;em.IR.HREALprincipalh_flg_i20cConfusion flags of h_m_i20cNonemeta.codeSMALLINTprincipalk_r_i20cRadius of circular aperture at isophote H=20mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalk_m_i20cK magnitude in k_r_i20cmagphot.mag;em.IR.KREALprincipalk_msig_i20c$\sigma$ k_m_i20cmagphot.mag;em.IR.KREALprincipalk_flg_i20cConfusion flags of k_m_i20cmagstat.error;phot.mag;em.IR.KREALprincipalj_r_i21eSemi-major axis of elliptical aperture at isophote J=21mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalj_m_i21eJ magnitude in j_r_i21emagphot.mag;em.IR.JREALprincipalj_msig_i21e$\sigma$ j_m_121emagstat.error;phot.mag;em.IR.JREALprincipalj_flg_i21eConfusion flags of j_m_121eNonemeta.codeSMALLINTprincipalh_r_i21eSemi-major axis of elliptical aperture at isophote h=21mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalh_m_i21eH magnitude in h_r_i21emagphot.mag;em.IR.HREALprincipalh_msig_i21e$\sigma$ h_m_121emagstat.error;phot.mag;em.IR.HREALprincipalh_flg_i21eConfusion flags of h_m_121eNonemeta.codeSMALLINTprincipalk_r_i21eSemi-major axis of elliptical aperture at isophote at K=21mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalk_m_i21eK magnitude in k_r_i21emagphot.mag;em.IR.KREALprincipalk_msig_i21e$\sigma$ k_m_121emagstat.error;phot.mag;em.IR.KREALprincipalk_flg_i21eConfusion flags of k_m_121eNonemeta.codeSMALLINTprincipalr_j21feSemi-major axis of fiducial elliptical aperture at J=21mag/arcsec$^2$arcsecphys.angSize.smajAxis;srcREALprincipalj_m_j21feJ magnitude in r_j21femagphot.mag;em.IR.JREALprincipalj_msig_j21fe$\sigma$ j_m_21femagstat.error;phot.mag;em.IR.JREALprincipalj_flg_j21feConfusion flags of j_m_21feNonemeta.codeSMALLINTprincipalh_m_j21feH magnitude in r_j21femagphot.mag;em.IR.HREALprincipalh_msig_j21fe$\sigma$ h_m_21femagstat.error;phot.mag;em.IR.HREALprincipalh_flg_j21feConfusion flags of h_m_21feNonemeta.codeSMALLINTprincipalk_m_j21feK magnitude in r_j21femagphot.mag;em.IR.KREALprincipalk_msig_j21fe$\sigma$ k_m_21femagstat.error;phot.mag;em.IR.KREALprincipalk_flg_j21feConfusion flags of k_m_21feNonemeta.codeSMALLINTprincipalj_r_i21cRadius of circular aperture at isophote J=21mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalj_m_i21cJ magnitude in j_r_i21cmagphot.mag;em.IR.JREALprincipalj_msig_i21c$\sigma$ j_m_i21cmagstat.error;phot.mag;em.IR.JREALprincipalj_flg_i21cConfusion flags of j_m_i21cNonemeta.codeSMALLINTprincipalh_r_i21cRadius of circular aperture at isophote H=21mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalh_m_i21cH magnitude in h_r_i21cmagphot.mag;em.IR.HREALprincipalh_msig_i21c$\sigma$ h_m_i21cmagstat.error;phot.mag;em.IR.HREALprincipalh_flg_i21cConfusion flags of h_m_i21cNonemeta.codeSMALLINTprincipalk_r_i21cRadius of circular aperture at isophote K=21mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalk_m_i21cK magnitude in k_r_i21cmagphot.mag;em.IR.KREALprincipalk_msig_i21c$\sigma$ k_m_i21cmagstat.error;phot.mag;em.IR.KREALprincipalk_flg_i21cConfusion flags of k_m_i21cNonemeta.codeSMALLINTprincipalr_j21fcJ fiducial Kron circular radius at isophote J=21mag/arcsec$^2$arcsecphys.angSize;srcREALprincipalj_m_j21fcJ magnitude in r_j21fcmagphot.mag;em.IR.JREALprincipalj_msig_j21fc$\sigma$ j_m_j21fcmagstat.error;phot.mag;em.IR.JREALprincipalj_flg_j21fcConfusion flags of j_m_j21fcNonemeta.codeSMALLINTprincipalh_m_j21fcH magnitude in r_j21fcmagphot.mag;em.IR.HREALprincipalh_msig_j21fc$\sigma$ h_m_j21fcmagstat.error;phot.mag;em.IR.HREALprincipalh_flg_j21fcConfusion flags of h_m_j21fcNonemeta.codeSMALLINTprincipalk_m_j21fcK magnitude in r_j21fcmagphot.mag;em.IR.KREALprincipalk_msig_j21fc$\sigma$ k_m_j21fcmagstat.error;phot.mag;em.IR.KREALprincipalk_flg_j21fcConfusion flags of k_m_j21fcNonemeta.codeSMALLINTprincipalj_m_5J magnitude in 5arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_5$\sigma$ j_m_5magstat.error;phot.mag;em.IR.JREALprincipalj_flg_5Confusion flags of j_m_5Nonemeta.codeSMALLINTprincipalh_m_5H magnitude in 5arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_5$\sigma$ h_m_5magstat.error;phot.mag;em.IR.HREALprincipalh_flg_5Confusion flags of h_m_5Nonemeta.codeSMALLINTprincipalk_m_5K magnitude in 5arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_5$\sigma$ k_m_5magstat.error;phot.mag;em.IR.KREALprincipalk_flg_5Confusion flags of k_m_5Nonemeta.codeSMALLINTprincipalj_m_7J magnitude in 7arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_7$\sigma$ j_m_7magstat.error;phot.mag;em.IR.JREALprincipalj_flg_7Confusion flags of j_m_7Nonemeta.codeSMALLINTprincipalh_m_7H magnitude in 7arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_7$\sigma$ h_m_7magstat.error;phot.mag;em.IR.HREALprincipalh_flg_7Confusion flags of h_m_7Nonemeta.codeSMALLINTprincipalk_m_7K magnitude in 7arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_7$\sigma$ k_m_7magstat.error;phot.mag;em.IR.KREALprincipalk_flg_7Confusion flags of k_m_7Nonemeta.codeSMALLINTprincipalj_m_10J magnitude in 10arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_10$\sigma$ j_m_10magstat.error;phot.mag;em.IR.JREALprincipalj_flg_10Confusion flags of j_m_10Nonemeta.codeSMALLINTprincipalh_m_10H magnitude in 10arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_10$\sigma$ h_m_10magstat.error;phot.mag;em.IR.HREALprincipalh_flg_10Confusion flags of h_m_10Nonemeta.codeSMALLINTprincipalk_m_10K magnitude in 10arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_10$\sigma$ k_m_10magstat.error;phot.mag;em.IR.KREALprincipalk_flg_10Confusion flags of k_m_10Nonemeta.codeSMALLINTprincipalj_m_15J magnitude in 15arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_15$\sigma$ j_m_15magstat.error;phot.mag;em.IR.JREALprincipalj_flg_15Confusion flags of j_m_15Nonemeta.codeSMALLINTprincipalh_m_15H magnitude in 15arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_15$\sigma$ h_m_15magstat.error;phot.mag;em.IR.HREALprincipalh_flg_15Confusion flags of h_m_15Nonemeta.codeSMALLINTprincipalk_m_15K magnitude in 15arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_15$\sigma$ k_m_15magstat.error;phot.mag;em.IR.KREALprincipalk_flg_15Confusion flags of k_m_15Nonemeta.codeSMALLINTprincipalj_m_20J magnitude in 20arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_20$\sigma$ j_m_20magstat.error;phot.mag;em.IR.JREALprincipalj_flg_20Confusion flags of j_m_20Nonemeta.codeSMALLINTprincipalh_m_20H magnitude in 20arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_20$\sigma$ h_m_20magstat.error;phot.mag;em.IR.HREALprincipalh_flg_20Confusion flags of h_m_20Nonemeta.codeSMALLINTprincipalk_m_20K magnitude in 20arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_20$\sigma$ k_m_20magstat.error;phot.mag;em.IR.KREALprincipalk_flg_20Confusion flags of k_m_20Nonemeta.codeSMALLINTprincipalj_m_25J magnitude in 25arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_25$\sigma$ j_m_25magstat.error;phot.mag;em.IR.JREALprincipalj_flg_25Confusion flags of j_m_25Nonemeta.codeSMALLINTprincipalh_m_25H magnitude in 25arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_25$\sigma$ h_m_25magstat.error;phot.mag;em.IR.HREALprincipalh_flg_25Confusion flags of h_m_25Nonemeta.codeSMALLINTprincipalk_m_25K magnitude in 25arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_25$\sigma$ k_m_25magstat.error;phot.mag;em.IR.KREALprincipalk_flg_25Confusion flags of k_m_25Nonemeta.codeSMALLINTprincipalj_m_30J magnitude in 30arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_30$\sigma$ j_m_30magstat.error;phot.mag;em.IR.JREALprincipalj_flg_30Confusion flags of j_m_30Nonemeta.codeSMALLINTprincipalh_m_30H magnitude in 30arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_30$\sigma$ h_m_30magstat.error;phot.mag;em.IR.HREALprincipalh_flg_30Confusion flags of h_m_30Nonemeta.codeSMALLINTprincipalk_m_30K magnitude in 30arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_30$\sigma$ k_m_30magstat.error;phot.mag;em.IR.KREALprincipalk_flg_30Confusion flags of k_m_30Nonemeta.codeSMALLINTprincipalj_m_40J magnitude in 40arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_40$\sigma$ j_m_40magstat.error;phot.mag;em.IR.JREALprincipalj_flg_40Confusion flags of j_m_40Nonemeta.codeSMALLINTprincipalh_m_40H magnitude in 40arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_40$\sigma$ h_m_40magstat.error;phot.mag;em.IR.HREALprincipalh_flg_40Confusion flags of h_m_40Nonemeta.codeSMALLINTprincipalk_m_40K magnitude in 40arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_40$\sigma$ k_m_40magstat.error;phot.mag;em.IR.KREALprincipalk_flg_40Confusion flags of k_m_40Nonemeta.codeSMALLINTprincipalj_m_50J magnitude in 50arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_50$\sigma$ j_m_50magstat.error;phot.mag;em.IR.JREALprincipalj_flg_50Confusion flags of j_m_50Nonemeta.codeSMALLINTprincipalh_m_50H magnitude in 50arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_50$\sigma$ h_m_50magstat.error;phot.mag;em.IR.HREALprincipalh_flg_50Confusion flags of h_m_50Nonemeta.codeSMALLINTprincipalk_m_50K magnitude in 50arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_50$\sigma$ k_m_50magstat.error;phot.mag;em.IR.KREALprincipalk_flg_50Confusion flags of k_m_50Nonemeta.codeSMALLINTprincipalj_m_60J magnitude in 60arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_60$\sigma$ j_m_60magstat.error;phot.mag;em.IR.JREALprincipalj_flg_60Confusion flags of j_m_60Nonemeta.codeSMALLINTprincipalh_m_60H magnitude in 60arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_60$\sigma$ h_m_60magstat.error;phot.mag;em.IR.HREALprincipalh_flg_60Confusion flags of h_m_60Nonemeta.codeSMALLINTprincipalk_m_60K magnitude in 60arcsec aperturemagphot.mag;em.IR.KREALprincipalk_msig_60$\sigma$ k_m_60magstat.error;phot.mag;em.IR.KREALprincipalk_flg_60Confusion flags of k_m_60Nonemeta.codeSMALLINTprincipalj_m_70J magnitude in 70arcsec aperturemagphot.mag;em.IR.JREALprincipalj_msig_70$\sigma$ j_m_70magstat.error;phot.mag;em.IR.JREALprincipalj_flg_70Confusion flags of j_m_70Nonemeta.codeSMALLINTprincipalh_m_70H magnitude in 70arcsec aperturemagphot.mag;em.IR.HREALprincipalh_msig_70$\sigma$ h_m_70magstat.error;phot.mag;em.IR.HREALprincipalh_d_areaH 5$\sigma$/3$\sigma$ differential areaNonephys.angSizeINTEGERprincipalh_perc_dareaH 5$\sigma$/3$\sigma$ relative area changeNonephys.angSizeINTEGERprincipalk_d_areaK 5$\sigma$/3$\sigma$ differential areaNonephys.angSizeINTEGERprincipalk_perc_dareaK 5$\sigma$/3$\sigma$ relative area changeNonephys.angSizeINTEGERprincipalj_bisym_ratJ bi-symmetric flux ratioNonestat.fit.paramREALprincipalj_bisym_chiJ bi-symmetric x-correlationNonestat.fit.chi2REALprincipalh_bisym_ratH bi-symmetric flux ratioNonestat.fit.paramREALprincipalh_bisym_chiH bi-symmetric x-correlationNonestat.fit.chi2REALprincipalk_bisym_ratK bi-symmetric flux ratioNonestat.fit.paramREALprincipalk_bisym_chiK bi-symmetric x-correlationNonestat.fit.chi2REALprincipalj_sh0J ridge shape (LCSB: BSNR limit)Nonesrc.morph.paramREALprincipalj_sig_sh0$\sigma$ j_sh0Nonestat.errorREALprincipalh_sh0H ridge shape (LCSB: BSNR limit)Nonesrc.morph.paramREALprincipalh_sig_sh0$\sigma$ h_sh0Nonestat.errorREALprincipalk_sh0K ridge shape (LCSB: BSNR limit)Nonesrc.morph.paramREALprincipalk_sig_sh0$\sigma$ k_sh0Nonestat.errorREALprincipalj_sc_mxdnJ mxdn score (LCSB: BSNR - block/smoothed SNR)Nonestat.fit.paramREALprincipalj_sc_shJ shape scoreNonestat.fit.paramREALprincipalj_sc_wshJ wsh score (LCSB: PSNR - peak raw SNR)Nonestat.fit.paramREALprincipalj_sc_r23J r23 score (LCSB: TSNR - integrated SNR for r=15)Nonestat.fit.paramREALprincipalj_sc_1mmJ 1st moment score (LCSB: super blk 2,4,8 SNR)Nonestat.fit.paramREALprincipalj_sc_2mmJ 2nd moment score (LCSB: SNRMAX - super SNR max.)Nonestat.fit.paramREALprincipalj_sc_vintJ vint scoreNonestat.fit.paramREALprincipalj_sc_r1J r1 scoreNonestat.fit.paramREALprincipalj_sc_mshJ median shape scoreNonestat.fit.paramREALprincipalh_sc_mxdnH mxdn score (LCSB: BSNR - block/smoothed SNR)Nonestat.fit.paramREALprincipalh_sc_shH shape scoreNonestat.fit.paramREALprincipalh_sc_wshH wsh score (LCSB: PSNR - peak raw SNR)Nonestat.fit.paramREALprincipalh_sc_r23H r23 score (LCSB: TSNR - integrated SNR for r=15)Nonestat.fit.paramREALprincipalh_sc_1mmH 1st moment score (LCSB: super blk 2,4,8 SNR)Nonestat.fit.paramREALprincipalh_sc_2mmH 2nd moment score (LCSB: SNRMAX - super SNR max.)Nonestat.fit.paramREALprincipalh_sc_vintH vint scoreNonestat.fit.paramREALprincipalh_sc_r1H r1 scoreNonestat.fit.paramREALprincipalh_sc_mshH median shape scoreNonestat.fit.paramREALprincipalk_sc_mxdnK mxdn score (LCSB: BSNR - block/smoothed SNR)Nonestat.fit.paramREALprincipalk_sc_shK shape scoreNonestat.fit.paramREALprincipalk_sc_wshK wsh score (LCSB: PSNR - peak raw SNR)Nonestat.fit.paramREALprincipalk_sc_r23K r23 score (LCSB: TSNR - integrated SNR for r=15)Nonestat.fit.paramREALprincipalk_sc_1mmK 1st moment score (LCSB: super blk 2,4,8 SNR)Nonestat.fit.paramREALprincipalk_sc_2mmK 2nd moment score (LCSB: SNRMAX - super SNR max.)Nonestat.fit.paramREALprincipalk_sc_vintK vint scoreNonestat.fit.paramREALprincipalk_sc_r1K r1 scoreNonestat.fit.paramREALprincipalk_sc_mshK median shape scoreNonestat.fit.paramREALprincipalj_chif_ellfJ chi-fraction for elliptical fit to 3$\sigma$ isophoteNonestat.fit.chi2REALprincipalk_chif_ellfK chi-fraction for elliptical fit to 3$\sigma$ isophoteNonestat.fit.chi2REALprincipalellfit_flgellipse fitting contamination flag (0=no contamination)Nonemeta.codeSMALLINTprincipalsup_chif_ellfsuper-coadd chi-fraction for elliptical fit to 3$\sigma$ isophoteNonestat.fit.chi2REALprincipaln_blankNumber of blanked sourcesNonemeta.numberINTEGERprincipaln_subNumber of subtracted sourcesNonemeta.numberINTEGERprincipalbl_sub_flgblanked/subtracted description flagNonemeta.codeSMALLINTprincipalid_flgType/galaxy sourceNonemeta.codeSMALLINTprincipalid_catMatched galaxy's catalog nameNonemeta.idVARCHARprincipalfg_flgFlux-growth convergence flagNonemeta.codeVARCHARprincipalblk_facLCSB blocking factor (1,2,4,8)Nonemeta.codeINTEGERprincipaldup_srcDuplicate source flagNonemeta.code.multipSMALLINTprincipaluse_srcUse source flagNonemeta.code.multipSMALLINTprincipalproxDistance to nearest neighbor in PSCarcsecpos.angDistanceREALprincipalpxpapos.angle of vector to proxdegpos.posAngINTEGERprincipalpxcntrext_key value of nearest XSC sourceNonemeta.idINTEGERprincipaldist_edge_nsDistance to nearest N/S edgearcsecmeta.codeINTEGERprincipaldist_edge_ewDistance to nearest E/W edgearcsecmeta.codeINTEGERprincipaldist_edge_flgnearest edgeNonemeta.codeVARCHARprincipalpts_keyKey to source data DB recordNonemeta.idINTEGERprincipalmp_keyKey to minor planet predictionNonemeta.idINTEGERprincipalnight_keykey to night data recordNonemeta.idINTEGERprincipalscan_keykey to scan data recordNonemeta.idINTEGERprincipalcoadd_keykey to coadd data recordNonemeta.idINTEGERprincipalhemishemisphere of observation: n = North/Mt.Hopkins; s= South/CTIONonemeta.id;instr.obstyVARCHARprincipaldateUT day of observationY:M:Dtime.epoch;obsVARCHARprincipalscanscan number (unique within date)Nonemeta.idINTEGERprincipalcoadd3-digit coadd number (unique within scan)Nonemeta.idVARCHARprincipalidsource ID number (unique within scan+coadd)Nonemeta.idINTEGERprincipalx_coaddx (cross-scan) positionarcsecpos.cartesian.x;instr.detREALprincipaly_coaddy (in-scan) positionarcsecpos.cartesian.y;instr.detREALprincipalj_subst2J residual background2 scoreNonestat.fit.paramREALprincipalh_subst2H residual background2 scoreNonestat.fit.paramREALprincipalk_subst2K residual background2 scoreNonestat.fit.paramREALprincipalj_backJ coadd median backgroundNoneinstr.backgroundREALprincipalh_backH coadd median backgroundNoneinstr.backgroundREALprincipalk_backK coadd median backgroundNoneinstr.backgroundREALprincipalj_resid_annJ residual annulus background medianNonestat.fit.residualREALprincipalh_resid_annH residual annulus background medianNonestat.fit.residualREALprincipalk_resid_annK residual annulus background medianNonestat.fit.residualREALprincipalj_bndg_perJ banding FT periodarcsecstat.fit.paramINTEGERprincipalj_bndg_ampJ banding maximum FT amplitudeNonestat.fit.paramREALprincipalh_bndg_perH banding FT periodarcsecstat.fit.paramINTEGERprincipalh_bndg_ampH banding maximum FT amplitudeNonestat.fit.paramREALprincipalk_bndg_perK banding FT periodarcsecstat.fit.paramINTEGERprincipalk_bndg_ampK banding maximum FT amplitudeNonestat.fit.paramREALprincipalj_seetrackJ band seetracking scoreNonestat.fit.paramREALprincipalh_seetrackH band seetracking scoreNonestat.fit.paramREALprincipalk_seetrackK band seetracking scoreNonestat.fit.paramREALprincipalext_keyentry counter (key) numberNonemeta.idINTEGERprincipal2mass_fdr.scnThe Scan Information Table contains the observational scan metadatara_3J2000 right ascension of the eastern corner at end of scan. This is the corner fully covered by all three bands.degpos.eq.raDOUBLEprincipalj_2mratJ-band average 2nd image moment ratio.Nonephot.calibREALprincipalh_2mratH-band average 2nd image moment ratio.Nonephot.calibREALprincipalk_2mratK_s-band average 2nd image moment ratio.Nonephot.calibREALprincipalj_pspJ-band photometric sensitivity parameter (PSP).Nonephot.calibDOUBLEprincipalh_pspH-band photometric sensitivity parameter (PSP).Nonephot.calibDOUBLEprincipalk_pspK_s-band photometric sensitivity parameter (PSP).Nonephot.calibDOUBLEprincipalj_pts_noiseThe base-10 logarithm of the characteristic J-band point source scan noise, in units of log(mJy). See notes for more details.log(mJy)phot.calibREALprincipalh_pts_noiseThe base-10 logarithm of the characteristic H-band point source scan noise, in units of log(mJy). See notes for more details.log(mJy)phot.calibREALprincipalk_pts_noiseThe base-10 logarithm of the characteristic Ks-band point source scan noise, in units of log(mJy). See notes for more details.log(mJy)phot.calibREALprincipalj_msnr10The J-band magnitude at which SNR=10 is achieved for this scan, estimated using the photometric sensitivity parameter j_psp and zero point offset j_zp_ap. This estimate does not take into account the effect of confusion noise in high source density regions.Nonephot.magREALprincipalh_msnr10The H-band magnitude at which SNR=10 is achieved for this scan, estimated using the photometric sensitivity parameter h_psp and zero point offset h_zp_ap. This estimate does not take into account the effect of confusion noise in high source density regions.Nonephot.magREALprincipalk_msnr10The K_s-band magnitude at which SNR=10 is achieved for this scan, estimated using the photometric sensitivity parameter k_psp and zero point offset k_zp_ap. This estimate does not take into account the effect of confusion noise in high source density regions.Nonephot.magREALprincipalrel0Flag indicating whether the scan is contained in the 2MASS Sampler Release."0" indicates non-inclusion in Sampler Release; "1" indicates inclusion in Sampler Release.Nonemeta.datasetBOOLEANprincipalrel1Flag indicating whether the scan is contained in the 2MASS First Incremental Data Release (IDR1)."0" indicates non-inclusion in IDR1; "1" indicates inclusion in IDR1.Nonemeta.datasetBOOLEANprincipalrel2Flag indicating whether the scan is contained in the 2MASS Second Incremental Data Release (IDR2)."0" indicates non-inclusion in IDR2; "1" indicates inclusion in IDR2.Nonemeta.datasetBOOLEANprincipalscan_keyThe unique identification number for this scan.Nonemeta.id;meta.mainINTEGERindexedprincipalhemisObservatory from which data were obtained: "n" = north = Mt. Hopkins; "s" = south = Cerro Tololo.Noneinstr.obstyVARCHARprincipaldateThe observation reference date for this scan expressed in ISO standard format. This is the UT date at sunrise for the night on which the scan was observed.Nonetime.epochVARCHARprincipalscanScan number (unique within date)Nonemeta.idINTEGERprincipaltileTile identification number.Nonemeta.idINTEGERprincipalraRight ascension of scan center for equinox J2000; this is computed from the interior corners ra_[1,2,3,4] and dec_[1,2,3,4].degpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination of scan center for equinox J2000; this is computed from the interior corners ra_[1,2,3,4] and dec_[1,2,3,4] (see below).degpos.eq.dec;meta.mainDOUBLEindexedprincipalglonGalactic longitude of scan center, as computed from ra and dec above. Galactic coordinates are derived by precessing reconstructed ra and dec to B1950, and performing rotational transformation into the l_II, b_II coordinate system.degpos.galatic.lon;meta.mainREALprincipalglatGalactic latitude of scan center, as computed from ra and dec above. Galactic coordinates are derived by precessing reconstructed ra and dec to B1950, and performing rotational transformation into the l_II, b_II coordinate system.degpos.galatic.lon;meta.mainREALprincipalra_1J2000 right ascension of the eastern corner at start of scan. This is the corner fully covered by all three bands.degpos.eq.raDOUBLEprincipaldec_1J2000 declination of the eastern corner at start of scan. This is the corner fully covered by all three bands.degpos.eq.decDOUBLEprincipalra_2J2000 right ascension of the western corner at start of scan. This is the corner fully covered by all three bands.degpos.eq.raDOUBLEprincipaldec_2J2000 declination of the western corner at start of scan. This is the corner fully covered by all three bands.degpos.eq.decDOUBLEprincipaldec_3J2000 declination of the eastern corner at end of scan. This is the corner fully covered by all three bands.degpos.eq.decDOUBLEprincipalra_4J2000 right ascension of the western corner at end of scan. This is the corner fully covered by all three bands.degpos.eq.raDOUBLEprincipaldec_4J2000 declination of the western corner at end of scan. This is the corner fully covered by all three bands.degpos.eq.decDOUBLEprincipalsdScanning direction: "n" = north-going; "s" = south-going.Noneobs.paramVARCHARprincipalqualQuality score for scan: "10" is highest grade; "0" is lowest.Nonemeta.code.qual;meta.mainINTEGERprincipalhglSpecial flag indicating whether or not this scan has a single-frame H-band or J-band electronic glitch: "0" indicates no glitch; "1" indicates glitch.Nonemeta.code.qualBOOLEANprincipalcldSpecial flag indicating whether or not a cloud was found in the scan after comparison of its photometry to that of overlapping scans in the database: "0" indicates no evidence for clouds; "1" indicates clouds.Nonemeta.code.qualBOOLEANprincipalxphSpecial flag indicating whether or not another photometric problem, not obviously cloud related, was found in the scan after comparing its photometry to that of overlapping scans: "0" indicates no problem; "1" indicates compromised photometry.Nonemeta.code.qualBOOLEANprincipalanomSpecial flag indicating whether or not an unusual problem was found in the Atlas Images for this scan. Such problem include, but are not limited to, residual meteor trails, satellite trails, insect trails, and unusual reflections or glints from bright stars: "0" indicates no such problem; "1" indicates an anomaly.Nonemeta.code.qualBOOLEANprincipalutUniversal Time (UT) at beginning of scan.hrtime.startDOUBLEprincipaljdateJulian Date at beginning of scan.julian daytime.startDOUBLEprincipalairmAirmass at beginning of scan.Noneobs.airMassREALprincipalzdScan's distance from the zenith at beginning of scan.degobs.paramREALprincipalhaHour angle at beginning of scan.hrpos.eq.haDOUBLEprincipalrhRelative humidity of telescope enclosure at beginning of scan.percentphysINTEGERprincipalair_tempAir temperature at beginning of scan.deg Cphys.temperatureREALprincipaltel_tempTelescope girdle temperature at beginning of scan. This temperature was used to adjust telescope focus to compensate for variations with temperature.deg Cphys.temperatureREALprincipalfocusFocus setting of telescope at beginning of scan. This is a measure of the position of the focus mechanism, in units of 1.25 microns, relative to a reference position. This reference position changed each time the telescope was collimated.Noneobs.paramINTEGERprincipalhryFlag indicating the H-band array configuration for the camera: "0" indicates the original configuration; "1" indicates the new (modified) configuration. For the southern camera, the array configuration was never changed, so this flag is always "0". For the northern camera a new H-band array, first used on 13 Sep 1999 (UT), was installed in mid-survey. Before this date the flag is "0" and on or after this date it is "1".Noneobs.paramBOOLEANprincipalc_stratFlag indicating the calibration strategy for this night's data: "0" indicates two calibration fields observed after every two-hour segment of regular survey scans; "1" indicates one calibration field observed after every hour segment of regular survey scans. For data taken from the southern hemisphere, this flag is always "1". For data taken from the northern hemisphere this flag is set to "0" on dates before 11 Oct 1997 (UT), and to "1" for dates of 11 Oct 1997 (UT) or thereafter.Noneobs.calibBOOLEANprincipalj_zp_apPhotometric zero-point for J-band aperture photometry.magphot.calibDOUBLEprincipalh_zp_apPhotometric zero-point for H-band aperture photometry.magphot.calibDOUBLEprincipalk_zp_apPhotometric zero-point for K_s-band aperture photometry.magphot.calibDOUBLEprincipalh_zperr_apRMS-error of zero-point for H-band aperture photometrymagphot.calib;stat.stdevDOUBLEprincipalk_zperr_apRMS-error of zero-point for K_s-band aperture photometrymagphot.calib;stat.stdevDOUBLEprincipalj_n_snr10Number of point sources at J-band with SNR>10 (instrumental mag <=15.8)Nonemeta.numberINTEGERprincipalh_n_snr10Number of point sources at H-band with SNR>10 (instrumental mag <=15.1)Nonemeta.numberINTEGERprincipalk_n_snr10Number of point sources at K_s-band with SNR>10 (instrumental mag <=14.3)Nonemeta.numberINTEGERprincipaln_extNumber of regular extended sources detected in scan.Nonemeta.numberINTEGERprincipalj_shape_avgJ-band average seeing shape for scan. The seeing full-width at half maximum (in arcseconds) can be obtained from the approximate relation FWHM(arcseconds) = 3.13*(j_shape_avg) - 0.46.Noneinstr.obsty.seeingREALprincipalh_shape_avgH-band average seeing shape for scan. The seeing full-width at half maximum (in arcseconds) can be obtained from the approximate relation FWHM(arcseconds) = 3.13*(h_shape_avg) - 0.46.Noneinstr.obsty.seeingREALprincipalk_shape_avgK_s-band average seeing shape for scan. The seeing full-width at half maximum (in arcseconds) can be obtained from the approximate relation FWHM(arcseconds) = 3.13*(k_shape_avg) - 0.46.Noneinstr.obsty.seeingREALprincipalj_shape_rmsRMS-error of J-band average seeing shape.Noneinstr.obsty.seeing;stat.rmsREALprincipalh_shape_rmsRMS-error of H-band average seeing shape.Noneinstr.obsty.seeing;stat.rmsREALprincipalk_shape_rmsRMS-error of K_s-band average seeing shape.Noneinstr.obsty.seeing;stat.rmsREALprincipalgleam_dr1A copy of GLEAM tables VIII/100/gleamegc, VIII/100/table1 and VIII/102/gleamgal from VizieR TAP service.gleam_dr1.gleamgalA copy of VizieR TAP table VIII_radio."VIII/102/gleamgal". GLEAM Galactic plane catalog ( Hurley-Walker N., Hancock P.J., Franzen T.M.O., et al.)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordINTEGERprincipalGLEAMGLEAM name (JHHMMSS+DDMMSS) (Name)meta.id;meta.mainVARCHARindexedprincipalFint099Integrated flux in 095-103MHz image (int_flux_099)Jyphot.fluxDOUBLEprincipalFint122Integrated flux in 118-126MHz image (int_flux_122)Jyphot.fluxDOUBLEprincipalbckwideBackground level in wide (170-231MHz) image (background_wide)Jy/beamphys.angSize;srcDOUBLEprincipallrmswideLocal noise leve in wide (170-231MHz) image (local_rms_wide)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalRAJ2000Right Ascension J2000 (RAJ2000)degpos.eq.ra;meta.mainDOUBLEindexedprincipale_RAJ2000rms uncertainty on RAdeg (err_RAJ2000) (1)degstat.error;pos.eq.raDOUBLEprincipalDEJ2000Declination J2000 (DEJ2000)degpos.eq.dec;meta.mainDOUBLEindexedprincipale_DEJ2000rms uncertainty on DEdeg (err_DEJ2000) (1)degstat.error;pos.eq.decDOUBLEprincipalFpwidePeak flux in wide (170-231MHz) image (peak_flux_wide)Jy/beamphot.flux.densityDOUBLEprincipale_Fpwiderms uncertainty in fit for peak flux in wide image (err_peak_flux_wide)Jy/beamstat.errorDOUBLEprincipalFintwideIntegrated flux in wide (170-231MHz) image (int_flux_wide)Jyphot.fluxDOUBLEprincipale_Fintwiderms uncertainty in fit for integrated flux in wide image (e_Fintwide)Jystat.errorDOUBLEprincipalawideFitted semi-major axis in wide (170-231MHz) image (a_wide)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipale_awiderms uncertainty in fitted semi-major axis in wide image (err_a_wide)arcsecstat.errorDOUBLEprincipalbwideFitted semi-minor axis in wide (170-231MHz) image (b_wide)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipale_bwiderms uncertainty in fitted semi-minor axis in wide image (err_b_wide)arcsecstat.errorDOUBLEprincipalpawideFitted position angle in wide (170-231MHz) image (pa_wide)degpos.posAng;meta.modelledDOUBLEprincipale_pawiderms uncertainty in fitted position angle in wide image (err_pa_wide)degstat.errorDOUBLEprincipalresmwideMean value of data-model in wide (170-231MHz) image (residual_mean_wide)Jy/beamstat.value;stat.meanDOUBLEprincipalresstdwideStandard deviation of data-model in wide (170-231MHz) image (residual_std_wide)Jy/beamstat.fit.residualDOUBLEprincipaleabsFpctPercent error in absolute flux scale - all frequencies (err_abs_flux_pct)%stat.errorSMALLINTprincipalefitFpctPercent error on internal flux scale - all frequencies (err_fit_flux_pct)%stat.errorSMALLINTprincipalpsfawideSemi-major axis of the point spread function in wide (170-231MHz) image (psf_a_wide)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfbwideSemi-minor axis of the point spread function in wide (170-231MHz) image (psf_b_wide)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPAwidePosition angle of the point spread function in wide (170-231MHz) image (psf_pa_wide)degpos.posAng;meta.modelledDOUBLEprincipalbck076Background level in 072-080MHz image (background_076)Jy/beamphys.angSize;srcDOUBLEprincipallrms076Local noise level in 072-080MHz image (local_rms_076)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp076Peak flux in 072-080MHz image (peak_flux_076)Jy/beamphot.flux.densityDOUBLEprincipale_Fp076rms uncertainty in fit for peak flux in 072-080MHz image (err_peak_flux_076)Jy/beamstat.errorDOUBLEprincipalFint076Integrated flux in 072-080MHz image (int_flux_076)Jyphot.fluxDOUBLEprincipale_Fint076rms uncertainty in fit for integrated flux in 072-080MHz image (err_int_flux_076)Jystat.errorDOUBLEprincipala076Fitted semi-major axis in 072-080MHz image (a_076)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb076Fitted semi-minor axis in 072-080MHz image (b_076)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa076Fitted position angle in 072-080MHz image (pa_076)degpos.posAng;meta.modelledDOUBLEprincipalresm076Mean value of data-model in 072-080MHz image (residual_mean_076)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd076Standard deviation of data-model in 072-080MHz image (residual_std_076)Jy/beamstat.fit.residualDOUBLEprincipalpsfa076Semi-major axis of the point spread function in 072-080MHz image (psf_a_076)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb076Semi-minor axis of the point spread function in 072-080MHz image (psf_b_076)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA076Position angle of the point spread function in 072-080MHz image (psf_pa_076)degpos.posAng;meta.modelledDOUBLEprincipalbck084Background level in 080-088MHz image (background_084)Jy/beamphys.angSize;srcDOUBLEprincipallrms084Local noise level in 080-088MHz image (local_rms_084)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp084Peak flux in 080-088MHz image (peak_flux_084)Jy/beamphot.flux.densityDOUBLEprincipale_Fp084rms uncertainty in fit for peak flux in 080-088MHz image (err_peak_flux_084)Jy/beamstat.errorDOUBLEprincipalFint084Integrated flux in 080-088MHz image (int_flux_084)Jyphot.fluxDOUBLEprincipale_Fint084rms uncertainty in fit for integrated flux in 080-088MHz image (err_int_flux_084)Jystat.errorDOUBLEprincipala084Fitted semi-major axis in 080-088MHz image (a_084)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb084Fitted semi-minor axis in 080-088MHz image (b_084)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa084Fitted position angle in 080-088MHz image (pa_084)degpos.posAng;meta.modelledDOUBLEprincipalresm084Mean value of data-model in 080-088MHz image (residual_mean_084)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd084Standard deviation of data-model in 080-088MHz image (residual_std_084)Jy/beamstat.fit.residualDOUBLEprincipalpsfa084Semi-major axis of the point spread function in 080-088MHz image (psf_a_084)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb084Semi-minor axis of the point spread function in 080-088MHz image (psf_b_084)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA084Position angle of the point spread function in 080-088MHz image (psf_pa_084)degpos.posAng;meta.modelledDOUBLEprincipalbck092Background level in 088-095MHz image (background_092)Jy/beamphys.angSize;srcDOUBLEprincipallrms092Local noise level in 088-095MHz image (local_rms_092)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp092Peak flux in 088-095MHz image (peak_flux_092)Jy/beamphot.flux.densityDOUBLEprincipale_Fp092rms uncertainty in fit for peak flux in 088-095MHz image (err_peak_flux_092)Jy/beamstat.errorDOUBLEprincipalFint092Integrated flux in 088-095MHz image (int_flux_092)Jyphot.fluxDOUBLEprincipale_Fint092rms uncertainty in fit for integrated flux in 088-095MHz image (err_int_flux_092)Jystat.errorDOUBLEprincipala092Fitted semi-major axis in 088-095MHz image (a_092)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb092Fitted semi-minor axis in 088-095MHz image (b_092)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa092Fitted position angle in 088-095MHz image (pa_092)degpos.posAng;meta.modelledDOUBLEprincipalresm092Mean value of data-model in 088-095MHz image (residual_mean_092)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd092Standard deviation of data-model in 088-095MHz image (residual_std_092)Jy/beamstat.fit.residualDOUBLEprincipalpsfa092Semi-major axis of the point spread function in 088-095MHz image (psf_a_092)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb092Semi-minor axis of the point spread function in 088-095MHz image (psf_b_092)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA092Position angle of the point spread function in 088-095MHz image (psf_pa_092)degpos.posAng;meta.modelledDOUBLEprincipalbck099Background level in 095-103MHz image (background_099)Jy/beamphys.angSize;srcDOUBLEprincipallrms099Local noise level in 095-103MHz image (local_rms_099)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp099Peak flux in 095-103MHz image (peak_flux_099)Jy/beamphot.flux.densityDOUBLEprincipale_Fp099rms uncertainty in fit for peak flux in 095-103MHz image (err_peak_flux_099)Jy/beamstat.errorDOUBLEprincipale_Fint099rms uncertainty in fit for integrated flux in 095-103MHz image (err_int_flux_099)Jystat.errorDOUBLEprincipala099Fitted semi-major axis in 095-103MHz image (a_099)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb099Fitted semi-minor axis in 095-103MHz image (b_099)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa099Fitted position angle in 095-103MHz image (pa_099)degpos.posAng;meta.modelledDOUBLEprincipalresm099Mean value of data-model in 095-103MHz image (residual_mean_099)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd099Standard deviation of data-model in 095-103MHz image (residual_std_099)Jy/beamstat.fit.residualDOUBLEprincipalpsfa099Semi-major axis of the point spread function in 095-103MHz image (psf_a_099)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb099Semi-minor axis of the point spread function in 095-103MHz image (psf_b_099)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA099Position angle of the point spread function in 095-103MHz image (psf_pa_099)degpos.posAng;meta.modelledDOUBLEprincipalbck107Background level in 103-111MHz image (background_107)Jy/beamphys.angSize;srcDOUBLEprincipallrms107Local noise level in 103-111MHz image (local_rms_107)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp107Peak flux in 103-111MHz image (peak_flux_107)Jy/beamphot.flux.densityDOUBLEprincipale_Fp107rms uncertainty in fit for peak flux in 103-111MHz image (err_peak_flux_107)Jy/beamstat.errorDOUBLEprincipalFint107Integrated flux in 103-111MHz image (int_flux_107)Jyphot.fluxDOUBLEprincipale_Fint107rms uncertainty in fit for integrated flux in 103-111MHz image (err_int_flux_107)Jystat.errorDOUBLEprincipala107Fitted semi-major axis in 103-111MHz image (a_107)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb107Fitted semi-minor axis in 103-111MHz image (b_107)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa107Fitted position angle in 103-111MHz image (pa_107)degpos.posAng;meta.modelledDOUBLEprincipalresm107Mean value of data-model in 103-111MHz image (residual_mean_107)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd107Standard deviation of data-model in 103-111MHz image (residual_std_107)Jy/beamstat.fit.residualDOUBLEprincipalpsfa107Semi-major axis of the point spread function in 103-111MHz image (psf_a_107)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb107Semi-minor axis of the point spread function in 103-111MHz image (psf_b_107)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA107Position angle of the point spread function in 103-111MHz image (psf_pa_107)degpos.posAng;meta.modelledDOUBLEprincipalbck115Background level in 111-118MHz image (background_115)Jy/beamphys.angSize;srcDOUBLEprincipallrms115Local noise level in 111-118MHz image (local_rms_115)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp115Peak flux in 111-118MHz image (peak_flux_115)Jy/beamphot.flux.densityDOUBLEprincipale_Fp115rms uncertainty in fit for peak flux in 111-118MHz image (err_peak_flux_115)Jy/beamstat.errorDOUBLEprincipalFint115Integrated flux in 111-118MHz image (int_flux_115)Jyphot.fluxDOUBLEprincipale_Fint115rms uncertainty in fit for integrated flux in 111-118MHz image (err_int_flux_115)Jystat.errorDOUBLEprincipala115Fitted semi-major axis in 111-118MHz image (a_115)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb115Fitted semi-minor axis in 111-118MHz image (b_115)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa115Fitted position angle in 111-118MHz image (pa_115)degpos.posAng;meta.modelledDOUBLEprincipalresm115Mean value of data-model in 111-118MHz image (residual_mean_115)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd115Standard deviation of data-model in 111-118MHz image (residual_std_115)Jy/beamstat.fit.residualDOUBLEprincipalpsfa115Semi-major axis of the point spread function in 111-118MHz image (psf_a_115)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb115Semi-minor axis of the point spread function in 111-118MHz image (psf_b_115)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA115Position angle of the point spread function in 111-118MHz image (psf_pa_115)degpos.posAng;meta.modelledDOUBLEprincipalbck122Background level in 118-126MHz image (background_122)Jy/beamphys.angSize;srcDOUBLEprincipallrms122Local noise level in 118-126MHz image (local_rms_122)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp122Peak flux in 118-126MHz image (peak_flux_122)Jy/beamphot.flux.densityDOUBLEprincipale_Fp122rms uncertainty in fit for peak flux in 118-126MHz image (err_peak_flux_122)Jy/beamstat.errorDOUBLEprincipale_Fint122rms uncertainty in fit for integrated flux in 118-126MHz image (err_int_flux_122)Jystat.errorDOUBLEprincipala122Fitted semi-major axis in 118-126MHz image (a_122)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb122Fitted semi-minor axis in 118-126MHz image (b_122)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa122Fitted semi-minor axis in 118-126MHz image (pa_122)degpos.posAng;meta.modelledDOUBLEprincipalresm122Mean value of data-model in 118-126MHz image (residual_mean_122)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd122Standard deviation of data-model in 118-126MHz image (residual_std_122)Jy/beamstat.fit.residualDOUBLEprincipalpsfa122Semi-major axis of the point spread function in 118-126MHz image (psf_a_122)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb122Semi-minor axis of the point spread function in 118-126MHz image (psf_b_122)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA122Position angle of the point spread function in 118-126MHz image (psf_pa_122)degpos.posAng;meta.modelledDOUBLEprincipalbck130Background level in 126-134MHz image (background_130)Jy/beamphys.angSize;srcDOUBLEprincipallrms130Local noise level in 126-134MHz image (local_rms_130)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp130Peak flux in 126-134MHz image (peak_flux_130)Jy/beamphot.flux.densityDOUBLEprincipale_Fp130rms uncertainty in fit for peak flux in 126-134MHz image (err_peak_flux_130)Jy/beamstat.errorDOUBLEprincipalFint130Integrated flux in 126-134MHz image (int_flux_130)Jyphot.fluxDOUBLEprincipale_Fint130rms uncertainty in fit for integrated flux in 126-134MHz image (err_int_flux_130)Jystat.errorDOUBLEprincipala130Fitted semi-major axis in 126-134MHz image (a_130)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb130Fitted semi-minor axis in 126-134MHz image (b_130)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa130Fitted position angle in 126-134MHz image (pa_130)degpos.posAng;meta.modelledDOUBLEprincipalresm130Mean value of data-model in 126-134MHz image (residual_mean_130)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd130Standard deviation of data-model in 126-134MHz image (residual_std_130)Jy/beamstat.fit.residualDOUBLEprincipalpsfa130Semi-major axis of the point spread function in 126-134MHz image (psf_a_130)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb130Semi-minor axis of the point spread function in 126-134MHz image (psf_b_130)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA130Position angle of the point spread function in 126-134MHz image (psf_pa_130)degpos.posAng;meta.modelledDOUBLEprincipalbck143Background level in 139-147MHz image (background_143)Jy/beamphys.angSize;srcDOUBLEprincipallrms143Local noise level in 139-147MHz image (local_rms_143)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp143Peak flux in 139-147MHz image (peak_flux_143)Jy/beamphot.flux.densityDOUBLEprincipale_Fp143rms uncertainty in fit for peak flux in 139-147MHz image (err_peak_flux_143)Jy/beamstat.errorDOUBLEprincipalFint143Integrated flux in 139-147MHz image (int_flux_143)Jyphot.fluxDOUBLEprincipale_Fint143rms uncertainty in fit for integrated flux in 139-147MHz image (err_int_flux_143)Jystat.errorDOUBLEprincipala143Fitted semi-major axis in 139-147MHz image (a_143)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb143Fitted semi-minor axis in 139-147MHz image (b_143)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa143Fitted position angle in 139-147MHz image (pa_143)degpos.posAng;meta.modelledDOUBLEprincipalresm143Mean value of data-model in 139-147MHz image (residual_mean_143)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd143Standard deviation of data-model in 139-147MHz image (residual_std_143)Jy/beamstat.fit.residualDOUBLEprincipalpsfa143Semi-major axis of the point spread function in 139-147MHz image (psf_a_143)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb143Semi-minor axis of the point spread function in 139-147MHz image (psf_b_143)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA143Position angle of the point spread function in 139-147MHz image (psf_pa_143)degpos.posAng;meta.modelledDOUBLEprincipalbck151Background level in 147-154MHz image (background_151)Jy/beamphys.angSize;srcDOUBLEprincipallrms151Local noise level in 147-154MHz image (local_rms_151)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp151Peak flux in 147-154MHz image (peak_flux_151)Jy/beamphot.flux.densityDOUBLEprincipale_Fp151rms uncertainty in fit for peak flux in 147-154MHz image (err_peak_flux_151)Jy/beamstat.errorDOUBLEprincipalFint151Integrated flux in 147-154MHz image (int_flux_151)Jyphot.fluxDOUBLEprincipale_Fint151rms uncertainty in fit for integrated flux in 147-154MHz image (err_int_flux_151)Jystat.errorDOUBLEprincipala151Fitted semi-major axis in 147-154MHz image (a_151)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb151Fitted semi-minor axis in 147-154MHz image (b_151)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa151Fitted position angle in 147-154MHz image (pa_151)degpos.posAng;meta.modelledDOUBLEprincipalresm151Mean value of data-model in 147-154MHz image (residual_mean_151)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd151Standard deviation of data-model in 147-154MHz image (residual_std_151)Jy/beamstat.fit.residualDOUBLEprincipalpsfa151Semi-major axis of the point spread function in 147-154MHz image (psf_a_151)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb151Semi-minor axis of the point spread function in 147-154MHz image (psf_b_151)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA151Position angle of the point spread function in 147-154MHz image (psf_pa_151)degpos.posAng;meta.modelledDOUBLEprincipalbck158Background level in 154-162MHz image (background_158)Jy/beamphys.angSize;srcDOUBLEprincipallrms158Local noise level in 154-162MHz image (local_rms_158)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp158Peak flux in 154-162MHz image (peak_flux_158)Jy/beamphot.flux.densityDOUBLEprincipale_Fp158rms uncertainty in fit for peak flux in 154-162MHz image (err_peak_flux_158)Jy/beamstat.errorDOUBLEprincipalFint158Integrated flux in 154-162MHz image (int_flux_158)Jyphot.fluxDOUBLEprincipale_Fint158rms uncertainty in fit for integrated flux in 154-162MHz image (err_int_flux_158)Jystat.errorDOUBLEprincipala158Fitted semi-major axis in 154-162MHz image (a_158)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb158Fitted semi-minor axis in 154-162MHz image (b_158)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa158Fitted position angle in 154-162MHz image (pa_158)degpos.posAng;meta.modelledDOUBLEprincipalresm158Mean value of data-model in 154-162MHz image (residual_mean_158)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd158Standard deviation of data-model in 154-162MHz image (residual_std_158)Jy/beamstat.fit.residualDOUBLEprincipalpsfa158Semi-major axis of the point spread function in 154-162MHz image (psf_a_158)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb158Semi-minor axis of the point spread function in 154-162MHz image (psf_b_158)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA158Position angle of the point spread function in 154-162MHz image (psf_pa_158)degpos.posAng;meta.modelledDOUBLEprincipalbck166Background level in 162-170MHz image (background_166)Jy/beamphys.angSize;srcDOUBLEprincipallrms166Local noise level in 162-170MHz image (local_rms_166)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp166Peak flux in 162-170MHz image (peak_flux_166)Jy/beamphot.flux.densityDOUBLEprincipale_Fp166rms uncertainty in fit for peak flux in 162-170MHz image (err_peak_flux_166)Jy/beamstat.errorDOUBLEprincipalFint166Integrated flux in 162-170MHz image (int_flux_166)Jyphot.fluxDOUBLEprincipale_Fint166rms uncertainty in fit for integrated flux in 162-170MHz image (err_int_flux_166)Jystat.errorDOUBLEprincipala166Fitted semi-major axis in 162-170MHz image (a_166)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb166Fitted semi-minor axis in 162-170MHz image (b_166)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa166Fitted position angle in 162-170MHz image (pa_166)degpos.posAng;meta.modelledDOUBLEprincipalresm166Mean value of data-model in 162-170MHz image (residual_mean_166)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd166Standard deviation of data-model in 162-170MHz image (residual_std_166)Jy/beamstat.fit.residualDOUBLEprincipalpsfa166Semi-major axis of the point spread function in 162-170MHz image (psf_a_166)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb166Semi-minor axis of the point spread function in 162-170MHz image (psf_b_166)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA166Position angle of the point spread function in 162-170MHz image (psf_pa_166)degpos.posAng;meta.modelledDOUBLEprincipalbck174Background level in 170-177MHz image (background_174)Jy/beamphys.angSize;srcDOUBLEprincipallrms174Local noise level in 170-177MHz image (local_rms_174)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp174Peak flux in 170-177MHz image (peak_flux_174)Jy/beamphot.flux.densityDOUBLEprincipale_Fp174rms uncertainty in fit for peak flux in 170-177MHz image (err_peak_flux_174)Jy/beamstat.errorDOUBLEprincipalFint174Integrated flux in 170-177MHz image (int_flux_174)Jyphot.fluxDOUBLEprincipale_Fint174rms uncertainty in fit for integrated flux in 170-177MHz image (err_int_flux_174)Jystat.errorDOUBLEprincipala174Fitted semi-major axis in 170-177MHz image (a_174)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb174Fitted semi-minor axis in 170-177MHz image (b_174)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa174Fitted position angle in 170-177MHz image (pa_174)degpos.posAng;meta.modelledDOUBLEprincipalresm174Mean value of data-model in 170-177MHz image (residual_mean_174)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd174Standard deviation of data-model in 170-177MHz image (residual_std_174)Jy/beamstat.fit.residualDOUBLEprincipalpsfa174Semi-major axis of the point spread function in 170-177MHz image (psf_a_174)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb174Semi-minor axis of the point spread function in 170-177MHz image (psf_b_174)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA174Position angle of the point spread function in 170-177MHz image (psf_pa_174)degpos.posAng;meta.modelledDOUBLEprincipalbck181Background level in 177-185MHz image (background_181)Jy/beamphys.angSize;srcDOUBLEprincipallrms181Local noise level in 177-185MHz image (local_rms_181)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp181Peak flux in 177-185MHz image (peak_flux_181)Jy/beamphot.flux.densityDOUBLEprincipale_Fp181rms uncertainty in fit for peak flux in 177-185MHz image (err_peak_flux_181)Jy/beamstat.errorDOUBLEprincipalFint181Integrated flux in 177-185MHz image (int_flux_181)Jyphot.fluxDOUBLEprincipale_Fint181rms uncertainty in fit for integrated flux in 177-185MHz image (err_int_flux_181)Jystat.errorDOUBLEprincipala181Fitted semi-major axis in 177-185MHz image (a_181)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb181Fitted semi-minor axis in 177-185MHz image (b_181)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa181Fitted position angle in 177-185MHz image (pa_181)degpos.posAng;meta.modelledDOUBLEprincipalresm181Mean value of data-model in 177-185MHz image (residual_mean_181)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd181Standard deviation of data-model in 177-185MHz image (residual_std_181)Jy/beamstat.fit.residualDOUBLEprincipalpsfa181Semi-major axis of the point spread function in 177-185MHz image (psf_a_181)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb181Semi-minor axis of the point spread function in 177-185MHz image (psf_b_181)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA181Position angle of the point spread function in 177-185MHz image (psf_pa_181)degpos.posAng;meta.modelledDOUBLEprincipalbck189Background level in 185-193MHz image (background_189)Jy/beamphys.angSize;srcDOUBLEprincipallrms189Local noise level in 185-193MHz image (local_rms_189)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp189Peak flux in 185-193MHz image (peak_flux_189)Jy/beamphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fp189rms uncertainty in fit for peak flux in 185-193MHz image (err_peak_flux_189)Jy/beamstat.errorDOUBLEprincipalFint189Integrated flux in 185-193MHz image (int_flux_189)Jyphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fint189rms uncertainty in fit for integrated flux in 185-193MHz image (err_int_flux_189)Jystat.errorDOUBLEprincipala189Fitted semi-major axis in 185-193MHz image (a_189)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb189Fitted semi-minor axis in 185-193MHz image (b_189)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa189Fitted position angle in 185-193MHz image (pa_189)degpos.posAng;meta.modelledDOUBLEprincipalresm189Mean value of data-model in 185-193MHz image (residual_mean_189)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd189Standard deviation of data-model in 185-193MHz image (residual_std_189)Jy/beamstat.fit.residualDOUBLEprincipalpsfa189Semi-major axis of the point spread function in 185-193MHz image (psf_a_189)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb189Semi-minor axis of the point spread function in 185-193MHz image (psf_b_189)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA189Position angle of the point spread function in 185-193MHz image (psf_pa_189)degpos.posAng;meta.modelledDOUBLEprincipalbck197Background level in 193-200MHz image (background_197)Jy/beamphys.angSize;srcDOUBLEprincipallrms197Local noise level in 193-200MHz image (local_rms_197)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp197Peak flux in 193-200MHz image (peak_flux_197)Jy/beamphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fp197rms uncertainty in fit for peak flux in 193-200MHz image (err_peak_flux_197)Jy/beamstat.errorDOUBLEprincipalFint197Integrated flux in 193-200MHz image (int_flux_197)Jyphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fint197rms uncertainty in fit for integrated flux in 193-200MHz image (err_int_flux_197)Jystat.errorDOUBLEprincipala197Fitted semi-major axis in 193-200MHz image (a_197)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb197Fitted semi-minor axis in 193-200MHz image (b_197)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa197Fitted position angle in 193-200MHz image (pa_197)degpos.posAng;meta.modelledDOUBLEprincipalresm197Mean value of data-model in 193-200MHz image (residual_mean_197)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd197Standard deviation of data-model in 193-200MHz image (residual_std_197)Jy/beamstat.fit.residualDOUBLEprincipalpsfa197Semi-major axis of the point spread function in 193-200MHz image (psf_a_197)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb197Semi-minor axis of the point spread function in 193-200MHz image (psf_b_197)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA197Position angle of the point spread function in 193-200MHz image (psf_pa_197)degpos.posAng;meta.modelledDOUBLEprincipalbck204Background level in 200-208MHz image (background_204)Jy/beamphys.angSize;srcDOUBLEprincipallrms204Local noise level in 200-208MHz image (local_rms_204)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp204Peak flux in 200-208MHz image (peak_flux_204)Jy/beamphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fp204rms uncertainty in fit for peak flux in 200-208MHz image (err_peak_flux_204)Jy/beamstat.errorDOUBLEprincipalFint204Integrated flux in 200-208MHz image (int_flux_204)Jyphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fint204rms uncertainty in fit for integrated flux in 200-208MHz image (err_int_flux_204)Jystat.errorDOUBLEprincipala204Fitted semi-major axis in 200-208MHz image (a_204)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb204Fitted semi-minor axis in 200-208MHz image (b_204)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa204Fitted position angle in 200-208MHz image (pa_204)degpos.posAng;meta.modelledDOUBLEprincipalresm204Mean value of data-model in 200-208MHz image (residual_mean_204)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd204Standard deviation of data-model in 200-208MHz image (residual_std_204)Jy/beamstat.fit.residualDOUBLEprincipalpsfa204Semi-major axis of the point spread function in 200-208MHz image (psf_a_204)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb204Semi-minor axis of the point spread function in 200-208MHz image (psf_b_204)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA204Position angle of the point spread function in 200-208MHz image (psf_pa_204)degpos.posAng;meta.modelledDOUBLEprincipalbck212Background level in 208-216MHz image (background_212)Jy/beamphys.angSize;srcDOUBLEprincipallrms212Local noise level in 208-216MHz image (local_rms_212)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp212Peak flux in 208-216MHz image (peak_flux_212)Jy/beamphot.flux.densityDOUBLEprincipale_Fp212rms uncertainty in fit for peak flux in 208-216MHz image (err_peak_flux_212)Jy/beamstat.errorDOUBLEprincipalFint212Integrated flux in 208-216MHz image (int_flux_212)Jyphot.fluxDOUBLEprincipale_Fint212rms uncertainty in fit for integrated flux in 208-216MHz image (err_int_flux_212)Jystat.errorDOUBLEprincipala212Fitted semi-major axis in 208-216MHz image (a_212)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb212Fitted semi-minor axis in 208-216MHz image (b_212)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa212Fitted position angle in 208-216MHz image (pa_212)degpos.posAng;meta.modelledDOUBLEprincipalresm212Mean value of data-model in 208-216MHz image (residual_mean_212)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd212Standard deviation of data-model in 208-216MHz image (residual_std_212)Jy/beamstat.fit.residualDOUBLEprincipalpsfa212Semi-major axis of the point spread function in 208-216MHz image (psf_a_212)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb212Semi-minor axis of the point spread function in 208-216MHz image (psf_b_212)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA212Position angle of the point spread function in 208-216MHz image (psf_pa_212)degpos.posAng;meta.modelledDOUBLEprincipalbck220Background level in 216-223MHz image (background_220)Jy/beamphys.angSize;srcDOUBLEprincipallrms220Local noise level in 216-223MHz image (local_rms_220)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp220Peak flux in 216-223MHz image (peak_flux_220)Jy/beamphot.flux.densityDOUBLEprincipale_Fp220rms uncertainty in fit for peak flux in 216-223MHz image (err_peak_flux_220)Jy/beamstat.errorDOUBLEprincipalFint220Integrated flux in 216-223MHz image (int_flux_220)Jyphot.fluxDOUBLEprincipale_Fint220rms uncertainty in fit for integrated flux in 216-223MHz image (err_int_flux_220)Jystat.errorDOUBLEprincipala220Fitted semi-major axis in 216-223MHz image (a_220)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb220Fitted semi-minor axis in 216-223MHz image (b_220)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa220Fitted position angle in 216-223MHz image (pa_220)degpos.posAng;meta.modelledDOUBLEprincipalresm220Mean value of data-model in 216-223MHz image (residual_mean_220)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd220Standard deviation of data-model in 216-223MHz image (residual_std_220)Jy/beamstat.fit.residualDOUBLEprincipalpsfa220Semi-major axis of the point spread function in 216-223MHz image (psf_a_220)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb220Semi-minor axis of the point spread function in 216-223MHz image (psf_b_220)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA220Position angle of the point spread function in 216-223MHz image (psf_pa_220)degpos.posAng;meta.modelledDOUBLEprincipalbck227Background level in 223-231MHz image (background_227)Jy/beamphys.angSize;srcDOUBLEprincipallrms227Local noise level in 223-231MHz image (local_rms_227)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp227Peak flux in 223-231MHz image (peak_flux_227)Jy/beamphot.flux.densityDOUBLEprincipale_Fp227rms uncertainty in fit for peak flux in 223-231MHz image (err_peak_flux_227)Jy/beamstat.errorDOUBLEprincipalFint227Integrated flux in 223-231MHz image (int_flux_227)Jyphot.fluxDOUBLEprincipale_Fint227rms uncertainty in fit for integrated flux in 223-231MHz image (err_int_flux_227)Jystat.errorDOUBLEprincipala227Fitted semi-major axis in 223-231MHz image (a_227)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb227Fitted semi-minor axis in 223-231MHz image (b_227)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa227Fitted position angle in 223-231MHz image (pa_227)degpos.posAng;meta.modelledDOUBLEprincipalresm227Mean value of data-model in 223-231MHz image (residual_mean_227)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd227Standard deviation of data-model in 223-231MHz image (residual_std_227)Jy/beamstat.fit.residualDOUBLEprincipalpsfa227Semi-major axis of the point spread function in 223-231MHz image (psf_a_227)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb227Semi-minor axis of the point spread function in 223-231MHz image (psf_b_227)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA227Position angle of the point spread function in 223-231MHz image (psf_pa_227)degpos.posAng;meta.modelledDOUBLEprincipalalphaFitted spectral index (alpha)spect.index;meta.modelledDOUBLEprincipale_alphaError on fitted spectral index (err_alpha)stat.error;pos.eq.raDOUBLEprincipalchi2Reduced chi^2 statistic for spectral index fit (reduced_chi2)stat.fit.chi2DOUBLEprincipalFintfit200Fitted 200MHz integrated flux density (int_flux_fit_200)Jystat.fit;phot.fluxDOUBLEprincipale_Fintfit200Error on fitted 200MHz integrated flux density (err_int_flux_fit_200)Jystat.errorDOUBLEprincipalgleam_dr1.table1A copy of VizieR TAP table VIII_radio."VIII/100/table1". GLEAM first year observing parameters ( Hurley-Walker N., Callingham J.R., Hancock P.J., et al.)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordINTEGERprincipalObs_DateObservation date'Y:M:D'time.epoch;obsDOUBLEprincipalRA1RA rangehourpos.eq.ra;meta.mainDOUBLEindexedprincipalRA2RA rangehourpos.eq.raDOUBLEprincipalDEDeclinationdegpos.eq.dec;meta.mainDOUBLEindexedprincipalNflagNumber of flagged tiles out of the 128 availablemeta.numberSMALLINTprincipalCalCalibrator (1)meta.id;meta.mainVARCHARindexedprincipalgleam_dr1.gleamegcA copy of VizieR TAP table VIII_radio."VIII/100/gleamegc". GLEAM EGC catalog, version 2 ( Hurley-Walker N., Callingham J.R., Hancock P.J., et al.)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordINTEGERprincipalGLEAMGLEAM name (JHHMMSS+DDMMSS) (Name)meta.id;meta.mainVARCHARindexedprincipalbckwideBackground level in wide (170-231MHz) image (background_wide)Jy/beamphys.angSize;srcDOUBLEprincipallrmswideLocal noise leve in wide (170-231MHz) image (local_rms_wide)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalRAJ2000Right Ascension J2000 (RAJ2000)degpos.eq.ra;meta.mainDOUBLEindexedprincipale_RAJ2000rms uncertainty on RAdeg (err_RAJ2000) (1)degstat.error;pos.eq.raDOUBLEprincipalDEJ2000Declination J2000 (DEJ2000)degpos.eq.dec;meta.mainDOUBLEindexedprincipale_DEJ2000rms uncertainty on DEdeg (err_DEJ2000) (1)degstat.error;pos.eq.decDOUBLEprincipalFpwidePeak flux in wide (170-231MHz) image (peak_flux_wide)Jy/beamphot.flux.densityDOUBLEprincipale_Fpwiderms uncertainty in fit for peak flux in wide image (err_peak_flux_wide)Jy/beamstat.errorDOUBLEprincipalFintwideIntegrated flux in wide (170-231MHz) image (int_flux_wide)Jyphot.fluxDOUBLEprincipale_Fintwiderms uncertainty in fit for integrated flux in wide image (e_Fintwide)Jystat.errorDOUBLEprincipalawideFitted semi-major axis in wide (170-231MHz) image (a_wide)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipale_awiderms uncertainty in fitted semi-major axis in wide image (err_a_wide)arcsecstat.errorDOUBLEprincipalbwideFitted semi-minor axis in wide (170-231MHz) image (b_wide)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipale_bwiderms uncertainty in fitted semi-minor axis in wide image (err_b_wide)arcsecstat.errorDOUBLEprincipalpawideFitted position angle in wide (170-231MHz) image (pa_wide)degpos.posAng;meta.modelledDOUBLEprincipale_pawiderms uncertainty in fitted position angle in wide image (err_pa_wide)degstat.errorDOUBLEprincipalresmwideMean value of data-model in wide (170-231MHz) image (residual_mean_wide)Jy/beamstat.value;stat.meanDOUBLEprincipalresstdwideStandard deviation of data-model in wide (170-231MHz) image (residual_std_wide)Jy/beamstat.fit.residualDOUBLEprincipaleabsFpctPercent error in absolute flux scale - all frequencies (err_abs_flux_pct)%stat.errorSMALLINTprincipalefitFpctPercent error on internal flux scale - all frequencies (err_fit_flux_pct)%stat.errorSMALLINTprincipalpsfawideSemi-major axis of the point spread function in wide (170-231MHz) image (psf_a_wide)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfbwideSemi-minor axis of the point spread function in wide (170-231MHz) image (psf_b_wide)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPAwidePosition angle of the point spread function in wide (170-231MHz) image (psf_pa_wide)degpos.posAng;meta.modelledDOUBLEprincipalbck076Background level in 072-080MHz image (background_076)Jy/beamphys.angSize;srcDOUBLEprincipallrms076Local noise level in 072-080MHz image (local_rms_076)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp076Peak flux in 072-080MHz image (peak_flux_076)Jy/beamphot.flux.densityDOUBLEprincipale_Fp076rms uncertainty in fit for peak flux in 072-080MHz image (err_peak_flux_076)Jy/beamstat.errorDOUBLEprincipalFint076Integrated flux in 072-080MHz image (int_flux_076)Jyphot.fluxDOUBLEprincipale_Fint076rms uncertainty in fit for integrated flux in 072-080MHz image (err_int_flux_076)Jystat.errorDOUBLEprincipala076Fitted semi-major axis in 072-080MHz image (a_076)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb076Fitted semi-minor axis in 072-080MHz image (b_076)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa076Fitted position angle in 072-080MHz image (pa_076)degpos.posAng;meta.modelledDOUBLEprincipalresm076Mean value of data-model in 072-080MHz image (residual_mean_076)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd076Standard deviation of data-model in 072-080MHz image (residual_std_076)Jy/beamstat.fit.residualDOUBLEprincipalpsfa076Semi-major axis of the point spread function in 072-080MHz image (psf_a_076)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb076Semi-minor axis of the point spread function in 072-080MHz image (psf_b_076)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA076Position angle of the point spread function in 072-080MHz image (psf_pa_076)degpos.posAng;meta.modelledDOUBLEprincipalbck084Background level in 080-088MHz image (background_084)Jy/beamphys.angSize;srcDOUBLEprincipallrms084Local noise level in 080-088MHz image (local_rms_084)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp084Peak flux in 080-088MHz image (peak_flux_084)Jy/beamphot.flux.densityDOUBLEprincipale_Fp084rms uncertainty in fit for peak flux in 080-088MHz image (err_peak_flux_084)Jy/beamstat.errorDOUBLEprincipalFint084Integrated flux in 080-088MHz image (int_flux_084)Jyphot.fluxDOUBLEprincipale_Fint084rms uncertainty in fit for integrated flux in 080-088MHz image (err_int_flux_084)Jystat.errorDOUBLEprincipala084Fitted semi-major axis in 080-088MHz image (a_084)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb084Fitted semi-minor axis in 080-088MHz image (b_084)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa084Fitted position angle in 080-088MHz image (pa_084)degpos.posAng;meta.modelledDOUBLEprincipalresm084Mean value of data-model in 080-088MHz image (residual_mean_084)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd084Standard deviation of data-model in 080-088MHz image (residual_std_084)Jy/beamstat.fit.residualDOUBLEprincipalpsfa084Semi-major axis of the point spread function in 080-088MHz image (psf_a_084)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb084Semi-minor axis of the point spread function in 080-088MHz image (psf_b_084)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA084Position angle of the point spread function in 080-088MHz image (psf_pa_084)degpos.posAng;meta.modelledDOUBLEprincipalbck092Background level in 088-095MHz image (background_092)Jy/beamphys.angSize;srcDOUBLEprincipallrms092Local noise level in 088-095MHz image (local_rms_092)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp092Peak flux in 088-095MHz image (peak_flux_092)Jy/beamphot.flux.densityDOUBLEprincipale_Fp092rms uncertainty in fit for peak flux in 088-095MHz image (err_peak_flux_092)Jy/beamstat.errorDOUBLEprincipalFint092Integrated flux in 088-095MHz image (int_flux_092)Jyphot.fluxDOUBLEprincipale_Fint092rms uncertainty in fit for integrated flux in 088-095MHz image (err_int_flux_092)Jystat.errorDOUBLEprincipala092Fitted semi-major axis in 088-095MHz image (a_092)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb092Fitted semi-minor axis in 088-095MHz image (b_092)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa092Fitted position angle in 088-095MHz image (pa_092)degpos.posAng;meta.modelledDOUBLEprincipalresm092Mean value of data-model in 088-095MHz image (residual_mean_092)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd092Standard deviation of data-model in 088-095MHz image (residual_std_092)Jy/beamstat.fit.residualDOUBLEprincipalpsfa092Semi-major axis of the point spread function in 088-095MHz image (psf_a_092)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb092Semi-minor axis of the point spread function in 088-095MHz image (psf_b_092)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA092Position angle of the point spread function in 088-095MHz image (psf_pa_092)degpos.posAng;meta.modelledDOUBLEprincipalbck099Background level in 095-103MHz image (background_099)Jy/beamphys.angSize;srcDOUBLEprincipallrms099Local noise level in 095-103MHz image (local_rms_099)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp099Peak flux in 095-103MHz image (peak_flux_099)Jy/beamphot.flux.densityDOUBLEprincipale_Fp099rms uncertainty in fit for peak flux in 095-103MHz image (err_peak_flux_099)Jy/beamstat.errorDOUBLEprincipalFint099Integrated flux in 095-103MHz image (int_flux_099)Jyphot.fluxDOUBLEprincipale_Fint099rms uncertainty in fit for integrated flux in 095-103MHz image (err_int_flux_099)Jystat.errorDOUBLEprincipala099Fitted semi-major axis in 095-103MHz image (a_099)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb099Fitted semi-minor axis in 095-103MHz image (b_099)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa099Fitted position angle in 095-103MHz image (pa_099)degpos.posAng;meta.modelledDOUBLEprincipalresm099Mean value of data-model in 095-103MHz image (residual_mean_099)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd099Standard deviation of data-model in 095-103MHz image (residual_std_099)Jy/beamstat.fit.residualDOUBLEprincipalpsfa099Semi-major axis of the point spread function in 095-103MHz image (psf_a_099)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb099Semi-minor axis of the point spread function in 095-103MHz image (psf_b_099)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA099Position angle of the point spread function in 095-103MHz image (psf_pa_099)degpos.posAng;meta.modelledDOUBLEprincipalbck107Background level in 103-111MHz image (background_107)Jy/beamphys.angSize;srcDOUBLEprincipallrms107Local noise level in 103-111MHz image (local_rms_107)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp107Peak flux in 103-111MHz image (peak_flux_107)Jy/beamphot.flux.densityDOUBLEprincipale_Fp107rms uncertainty in fit for peak flux in 103-111MHz image (err_peak_flux_107)Jy/beamstat.errorDOUBLEprincipalFint107Integrated flux in 103-111MHz image (int_flux_107)Jyphot.fluxDOUBLEprincipale_Fint107rms uncertainty in fit for integrated flux in 103-111MHz image (err_int_flux_107)Jystat.errorDOUBLEprincipala107Fitted semi-major axis in 103-111MHz image (a_107)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb107Fitted semi-minor axis in 103-111MHz image (b_107)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa107Fitted position angle in 103-111MHz image (pa_107)degpos.posAng;meta.modelledDOUBLEprincipalresm107Mean value of data-model in 103-111MHz image (residual_mean_107)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd107Standard deviation of data-model in 103-111MHz image (residual_std_107)Jy/beamstat.fit.residualDOUBLEprincipalpsfa107Semi-major axis of the point spread function in 103-111MHz image (psf_a_107)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb107Semi-minor axis of the point spread function in 103-111MHz image (psf_b_107)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA107Position angle of the point spread function in 103-111MHz image (psf_pa_107)degpos.posAng;meta.modelledDOUBLEprincipalbck115Background level in 111-118MHz image (background_115)Jy/beamphys.angSize;srcDOUBLEprincipallrms115Local noise level in 111-118MHz image (local_rms_115)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp115Peak flux in 111-118MHz image (peak_flux_115)Jy/beamphot.flux.densityDOUBLEprincipale_Fp115rms uncertainty in fit for peak flux in 111-118MHz image (err_peak_flux_115)Jy/beamstat.errorDOUBLEprincipalFint115Integrated flux in 111-118MHz image (int_flux_115)Jyphot.fluxDOUBLEprincipale_Fint115rms uncertainty in fit for integrated flux in 111-118MHz image (err_int_flux_115)Jystat.errorDOUBLEprincipala115Fitted semi-major axis in 111-118MHz image (a_115)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb115Fitted semi-minor axis in 111-118MHz image (b_115)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa115Fitted position angle in 111-118MHz image (pa_115)degpos.posAng;meta.modelledDOUBLEprincipalresm115Mean value of data-model in 111-118MHz image (residual_mean_115)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd115Standard deviation of data-model in 111-118MHz image (residual_std_115)Jy/beamstat.fit.residualDOUBLEprincipalpsfa115Semi-major axis of the point spread function in 111-118MHz image (psf_a_115)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb115Semi-minor axis of the point spread function in 111-118MHz image (psf_b_115)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA115Position angle of the point spread function in 111-118MHz image (psf_pa_115)degpos.posAng;meta.modelledDOUBLEprincipalbck122Background level in 118-126MHz image (background_122)Jy/beamphys.angSize;srcDOUBLEprincipallrms122Local noise level in 118-126MHz image (local_rms_122)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp122Peak flux in 118-126MHz image (peak_flux_122)Jy/beamphot.flux.densityDOUBLEprincipale_Fp122rms uncertainty in fit for peak flux in 118-126MHz image (err_peak_flux_122)Jy/beamstat.errorDOUBLEprincipalFint122Integrated flux in 118-126MHz image (int_flux_122)Jyphot.fluxDOUBLEprincipale_Fint122rms uncertainty in fit for integrated flux in 118-126MHz image (err_int_flux_122)Jystat.errorDOUBLEprincipala122Fitted semi-major axis in 118-126MHz image (a_122)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb122Fitted semi-minor axis in 118-126MHz image (b_122)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa122Fitted semi-minor axis in 118-126MHz image (pa_122)degpos.posAng;meta.modelledDOUBLEprincipalresm122Mean value of data-model in 118-126MHz image (residual_mean_122)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd122Standard deviation of data-model in 118-126MHz image (residual_std_122)Jy/beamstat.fit.residualDOUBLEprincipalpsfa122Semi-major axis of the point spread function in 118-126MHz image (psf_a_122)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb122Semi-minor axis of the point spread function in 118-126MHz image (psf_b_122)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA122Position angle of the point spread function in 118-126MHz image (psf_pa_122)degpos.posAng;meta.modelledDOUBLEprincipalbck130Background level in 126-134MHz image (background_130)Jy/beamphys.angSize;srcDOUBLEprincipallrms130Local noise level in 126-134MHz image (local_rms_130)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp130Peak flux in 126-134MHz image (peak_flux_130)Jy/beamphot.flux.densityDOUBLEprincipale_Fp130rms uncertainty in fit for peak flux in 126-134MHz image (err_peak_flux_130)Jy/beamstat.errorDOUBLEprincipalFint130Integrated flux in 126-134MHz image (int_flux_130)Jyphot.fluxDOUBLEprincipale_Fint130rms uncertainty in fit for integrated flux in 126-134MHz image (err_int_flux_130)Jystat.errorDOUBLEprincipala130Fitted semi-major axis in 126-134MHz image (a_130)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb130Fitted semi-minor axis in 126-134MHz image (b_130)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa130Fitted position angle in 126-134MHz image (pa_130)degpos.posAng;meta.modelledDOUBLEprincipalresm130Mean value of data-model in 126-134MHz image (residual_mean_130)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd130Standard deviation of data-model in 126-134MHz image (residual_std_130)Jy/beamstat.fit.residualDOUBLEprincipalpsfa130Semi-major axis of the point spread function in 126-134MHz image (psf_a_130)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb130Semi-minor axis of the point spread function in 126-134MHz image (psf_b_130)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA130Position angle of the point spread function in 126-134MHz image (psf_pa_130)degpos.posAng;meta.modelledDOUBLEprincipalbck143Background level in 139-147MHz image (background_143)Jy/beamphys.angSize;srcDOUBLEprincipallrms143Local noise level in 139-147MHz image (local_rms_143)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp143Peak flux in 139-147MHz image (peak_flux_143)Jy/beamphot.flux.densityDOUBLEprincipale_Fp143rms uncertainty in fit for peak flux in 139-147MHz image (err_peak_flux_143)Jy/beamstat.errorDOUBLEprincipalFint143Integrated flux in 139-147MHz image (int_flux_143)Jyphot.fluxDOUBLEprincipale_Fint143rms uncertainty in fit for integrated flux in 139-147MHz image (err_int_flux_143)Jystat.errorDOUBLEprincipala143Fitted semi-major axis in 139-147MHz image (a_143)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb143Fitted semi-minor axis in 139-147MHz image (b_143)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa143Fitted position angle in 139-147MHz image (pa_143)degpos.posAng;meta.modelledDOUBLEprincipalresm143Mean value of data-model in 139-147MHz image (residual_mean_143)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd143Standard deviation of data-model in 139-147MHz image (residual_std_143)Jy/beamstat.fit.residualDOUBLEprincipalpsfa143Semi-major axis of the point spread function in 139-147MHz image (psf_a_143)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb143Semi-minor axis of the point spread function in 139-147MHz image (psf_b_143)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA143Position angle of the point spread function in 139-147MHz image (psf_pa_143)degpos.posAng;meta.modelledDOUBLEprincipalbck151Background level in 147-154MHz image (background_151)Jy/beamphys.angSize;srcDOUBLEprincipallrms151Local noise level in 147-154MHz image (local_rms_151)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp151Peak flux in 147-154MHz image (peak_flux_151)Jy/beamphot.flux.densityDOUBLEprincipale_Fp151rms uncertainty in fit for peak flux in 147-154MHz image (err_peak_flux_151)Jy/beamstat.errorDOUBLEprincipalFint151Integrated flux in 147-154MHz image (int_flux_151)Jyphot.fluxDOUBLEprincipale_Fint151rms uncertainty in fit for integrated flux in 147-154MHz image (err_int_flux_151)Jystat.errorDOUBLEprincipala151Fitted semi-major axis in 147-154MHz image (a_151)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb151Fitted semi-minor axis in 147-154MHz image (b_151)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa151Fitted position angle in 147-154MHz image (pa_151)degpos.posAng;meta.modelledDOUBLEprincipalresm151Mean value of data-model in 147-154MHz image (residual_mean_151)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd151Standard deviation of data-model in 147-154MHz image (residual_std_151)Jy/beamstat.fit.residualDOUBLEprincipalpsfa151Semi-major axis of the point spread function in 147-154MHz image (psf_a_151)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb151Semi-minor axis of the point spread function in 147-154MHz image (psf_b_151)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA151Position angle of the point spread function in 147-154MHz image (psf_pa_151)degpos.posAng;meta.modelledDOUBLEprincipalbck158Background level in 154-162MHz image (background_158)Jy/beamphys.angSize;srcDOUBLEprincipallrms158Local noise level in 154-162MHz image (local_rms_158)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp158Peak flux in 154-162MHz image (peak_flux_158)Jy/beamphot.flux.densityDOUBLEprincipale_Fp158rms uncertainty in fit for peak flux in 154-162MHz image (err_peak_flux_158)Jy/beamstat.errorDOUBLEprincipalFint158Integrated flux in 154-162MHz image (int_flux_158)Jyphot.fluxDOUBLEprincipalFint181Integrated flux in 177-185MHz image (int_flux_181)Jyphot.fluxDOUBLEprincipale_Fint158rms uncertainty in fit for integrated flux in 154-162MHz image (err_int_flux_158)Jystat.errorDOUBLEprincipala158Fitted semi-major axis in 154-162MHz image (a_158)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb158Fitted semi-minor axis in 154-162MHz image (b_158)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa158Fitted position angle in 154-162MHz image (pa_158)degpos.posAng;meta.modelledDOUBLEprincipalresm158Mean value of data-model in 154-162MHz image (residual_mean_158)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd158Standard deviation of data-model in 154-162MHz image (residual_std_158)Jy/beamstat.fit.residualDOUBLEprincipalpsfa158Semi-major axis of the point spread function in 154-162MHz image (psf_a_158)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb158Semi-minor axis of the point spread function in 154-162MHz image (psf_b_158)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA158Position angle of the point spread function in 154-162MHz image (psf_pa_158)degpos.posAng;meta.modelledDOUBLEprincipalbck166Background level in 162-170MHz image (background_166)Jy/beamphys.angSize;srcDOUBLEprincipallrms166Local noise level in 162-170MHz image (local_rms_166)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp166Peak flux in 162-170MHz image (peak_flux_166)Jy/beamphot.flux.densityDOUBLEprincipale_Fp166rms uncertainty in fit for peak flux in 162-170MHz image (err_peak_flux_166)Jy/beamstat.errorDOUBLEprincipalFint166Integrated flux in 162-170MHz image (int_flux_166)Jyphot.fluxDOUBLEprincipale_Fint166rms uncertainty in fit for integrated flux in 162-170MHz image (err_int_flux_166)Jystat.errorDOUBLEprincipala166Fitted semi-major axis in 162-170MHz image (a_166)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb166Fitted semi-minor axis in 162-170MHz image (b_166)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa166Fitted position angle in 162-170MHz image (pa_166)degpos.posAng;meta.modelledDOUBLEprincipalresm166Mean value of data-model in 162-170MHz image (residual_mean_166)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd166Standard deviation of data-model in 162-170MHz image (residual_std_166)Jy/beamstat.fit.residualDOUBLEprincipalpsfa166Semi-major axis of the point spread function in 162-170MHz image (psf_a_166)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb166Semi-minor axis of the point spread function in 162-170MHz image (psf_b_166)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA166Position angle of the point spread function in 162-170MHz image (psf_pa_166)degpos.posAng;meta.modelledDOUBLEprincipalbck174Background level in 170-177MHz image (background_174)Jy/beamphys.angSize;srcDOUBLEprincipallrms174Local noise level in 170-177MHz image (local_rms_174)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp174Peak flux in 170-177MHz image (peak_flux_174)Jy/beamphot.flux.densityDOUBLEprincipale_Fp174rms uncertainty in fit for peak flux in 170-177MHz image (err_peak_flux_174)Jy/beamstat.errorDOUBLEprincipalFint174Integrated flux in 170-177MHz image (int_flux_174)Jyphot.fluxDOUBLEprincipale_Fint174rms uncertainty in fit for integrated flux in 170-177MHz image (err_int_flux_174)Jystat.errorDOUBLEprincipala174Fitted semi-major axis in 170-177MHz image (a_174)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb174Fitted semi-minor axis in 170-177MHz image (b_174)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa174Fitted position angle in 170-177MHz image (pa_174)degpos.posAng;meta.modelledDOUBLEprincipalresm174Mean value of data-model in 170-177MHz image (residual_mean_174)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd174Standard deviation of data-model in 170-177MHz image (residual_std_174)Jy/beamstat.fit.residualDOUBLEprincipalpsfa174Semi-major axis of the point spread function in 170-177MHz image (psf_a_174)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb174Semi-minor axis of the point spread function in 170-177MHz image (psf_b_174)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA174Position angle of the point spread function in 170-177MHz image (psf_pa_174)degpos.posAng;meta.modelledDOUBLEprincipalbck181Background level in 177-185MHz image (background_181)Jy/beamphys.angSize;srcDOUBLEprincipallrms181Local noise level in 177-185MHz image (local_rms_181)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp181Peak flux in 177-185MHz image (peak_flux_181)Jy/beamphot.flux.densityDOUBLEprincipale_Fp181rms uncertainty in fit for peak flux in 177-185MHz image (err_peak_flux_181)Jy/beamstat.errorDOUBLEprincipale_Fint181rms uncertainty in fit for integrated flux in 177-185MHz image (err_int_flux_181)Jystat.errorDOUBLEprincipala181Fitted semi-major axis in 177-185MHz image (a_181)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb181Fitted semi-minor axis in 177-185MHz image (b_181)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa181Fitted position angle in 177-185MHz image (pa_181)degpos.posAng;meta.modelledDOUBLEprincipalresm181Mean value of data-model in 177-185MHz image (residual_mean_181)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd181Standard deviation of data-model in 177-185MHz image (residual_std_181)Jy/beamstat.fit.residualDOUBLEprincipalpsfa181Semi-major axis of the point spread function in 177-185MHz image (psf_a_181)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb181Semi-minor axis of the point spread function in 177-185MHz image (psf_b_181)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA181Position angle of the point spread function in 177-185MHz image (psf_pa_181)degpos.posAng;meta.modelledDOUBLEprincipalbck189Background level in 185-193MHz image (background_189)Jy/beamphys.angSize;srcDOUBLEprincipallrms189Local noise level in 185-193MHz image (local_rms_189)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp189Peak flux in 185-193MHz image (peak_flux_189)Jy/beamphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fp189rms uncertainty in fit for peak flux in 185-193MHz image (err_peak_flux_189)Jy/beamstat.errorDOUBLEprincipalFint189Integrated flux in 185-193MHz image (int_flux_189)Jyphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fint189rms uncertainty in fit for integrated flux in 185-193MHz image (err_int_flux_189)Jystat.errorDOUBLEprincipala189Fitted semi-major axis in 185-193MHz image (a_189)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb189Fitted semi-minor axis in 185-193MHz image (b_189)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa189Fitted position angle in 185-193MHz image (pa_189)degpos.posAng;meta.modelledDOUBLEprincipalresm189Mean value of data-model in 185-193MHz image (residual_mean_189)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd189Standard deviation of data-model in 185-193MHz image (residual_std_189)Jy/beamstat.fit.residualDOUBLEprincipalpsfa189Semi-major axis of the point spread function in 185-193MHz image (psf_a_189)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb189Semi-minor axis of the point spread function in 185-193MHz image (psf_b_189)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA189Position angle of the point spread function in 185-193MHz image (psf_pa_189)degpos.posAng;meta.modelledDOUBLEprincipalbck197Background level in 193-200MHz image (background_197)Jy/beamphys.angSize;srcDOUBLEprincipallrms197Local noise level in 193-200MHz image (local_rms_197)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp197Peak flux in 193-200MHz image (peak_flux_197)Jy/beamphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fp197rms uncertainty in fit for peak flux in 193-200MHz image (err_peak_flux_197)Jy/beamstat.errorDOUBLEprincipalFint197Integrated flux in 193-200MHz image (int_flux_197)Jyphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fint197rms uncertainty in fit for integrated flux in 193-200MHz image (err_int_flux_197)Jystat.errorDOUBLEprincipala197Fitted semi-major axis in 193-200MHz image (a_197)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb197Fitted semi-minor axis in 193-200MHz image (b_197)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa197Fitted position angle in 193-200MHz image (pa_197)degpos.posAng;meta.modelledDOUBLEprincipalresm197Mean value of data-model in 193-200MHz image (residual_mean_197)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd197Standard deviation of data-model in 193-200MHz image (residual_std_197)Jy/beamstat.fit.residualDOUBLEprincipalpsfa197Semi-major axis of the point spread function in 193-200MHz image (psf_a_197)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb197Semi-minor axis of the point spread function in 193-200MHz image (psf_b_197)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA197Position angle of the point spread function in 193-200MHz image (psf_pa_197)degpos.posAng;meta.modelledDOUBLEprincipalbck204Background level in 200-208MHz image (background_204)Jy/beamphys.angSize;srcDOUBLEprincipallrms204Local noise level in 200-208MHz image (local_rms_204)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp204Peak flux in 200-208MHz image (peak_flux_204)Jy/beamphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fp204rms uncertainty in fit for peak flux in 200-208MHz image (err_peak_flux_204)Jy/beamstat.errorDOUBLEprincipalFint204Integrated flux in 200-208MHz image (int_flux_204)Jyphot.flux.density;em.radio.200-400MHzDOUBLEprincipale_Fint204rms uncertainty in fit for integrated flux in 200-208MHz image (err_int_flux_204)Jystat.errorDOUBLEprincipala204Fitted semi-major axis in 200-208MHz image (a_204)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb204Fitted semi-minor axis in 200-208MHz image (b_204)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa204Fitted position angle in 200-208MHz image (pa_204)degpos.posAng;meta.modelledDOUBLEprincipalresm204Mean value of data-model in 200-208MHz image (residual_mean_204)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd204Standard deviation of data-model in 200-208MHz image (residual_std_204)Jy/beamstat.fit.residualDOUBLEprincipalpsfa204Semi-major axis of the point spread function in 200-208MHz image (psf_a_204)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb204Semi-minor axis of the point spread function in 200-208MHz image (psf_b_204)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA204Position angle of the point spread function in 200-208MHz image (psf_pa_204)degpos.posAng;meta.modelledDOUBLEprincipalbck212Background level in 208-216MHz image (background_212)Jy/beamphys.angSize;srcDOUBLEprincipallrms212Local noise level in 208-216MHz image (local_rms_212)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp212Peak flux in 208-216MHz image (peak_flux_212)Jy/beamphot.flux.densityDOUBLEprincipale_Fp212rms uncertainty in fit for peak flux in 208-216MHz image (err_peak_flux_212)Jy/beamstat.errorDOUBLEprincipalFint212Integrated flux in 208-216MHz image (int_flux_212)Jyphot.fluxDOUBLEprincipale_Fint212rms uncertainty in fit for integrated flux in 208-216MHz image (err_int_flux_212)Jystat.errorDOUBLEprincipala212Fitted semi-major axis in 208-216MHz image (a_212)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb212Fitted semi-minor axis in 208-216MHz image (b_212)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa212Fitted position angle in 208-216MHz image (pa_212)degpos.posAng;meta.modelledDOUBLEprincipalresm212Mean value of data-model in 208-216MHz image (residual_mean_212)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd212Standard deviation of data-model in 208-216MHz image (residual_std_212)Jy/beamstat.fit.residualDOUBLEprincipalpsfa212Semi-major axis of the point spread function in 208-216MHz image (psf_a_212)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb212Semi-minor axis of the point spread function in 208-216MHz image (psf_b_212)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA212Position angle of the point spread function in 208-216MHz image (psf_pa_212)degpos.posAng;meta.modelledDOUBLEprincipalbck220Background level in 216-223MHz image (background_220)Jy/beamphys.angSize;srcDOUBLEprincipallrms220Local noise level in 216-223MHz image (local_rms_220)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp220Peak flux in 216-223MHz image (peak_flux_220)Jy/beamphot.flux.densityDOUBLEprincipale_Fp220rms uncertainty in fit for peak flux in 216-223MHz image (err_peak_flux_220)Jy/beamstat.errorDOUBLEprincipalFint220Integrated flux in 216-223MHz image (int_flux_220)Jyphot.fluxDOUBLEprincipale_Fint220rms uncertainty in fit for integrated flux in 216-223MHz image (err_int_flux_220)Jystat.errorDOUBLEprincipala220Fitted semi-major axis in 216-223MHz image (a_220)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb220Fitted semi-minor axis in 216-223MHz image (b_220)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa220Fitted position angle in 216-223MHz image (pa_220)degpos.posAng;meta.modelledDOUBLEprincipalresm220Mean value of data-model in 216-223MHz image (residual_mean_220)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd220Standard deviation of data-model in 216-223MHz image (residual_std_220)Jy/beamstat.fit.residualDOUBLEprincipalpsfa220Semi-major axis of the point spread function in 216-223MHz image (psf_a_220)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb220Semi-minor axis of the point spread function in 216-223MHz image (psf_b_220)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA220Position angle of the point spread function in 216-223MHz image (psf_pa_220)degpos.posAng;meta.modelledDOUBLEprincipalbck227Background level in 223-231MHz image (background_227)Jy/beamphys.angSize;srcDOUBLEprincipallrms227Local noise level in 223-231MHz image (local_rms_227)Jy/beamstat.median;phot.flux.densityDOUBLEprincipalFp227Peak flux in 223-231MHz image (peak_flux_227)Jy/beamphot.flux.densityDOUBLEprincipale_Fp227rms uncertainty in fit for peak flux in 223-231MHz image (err_peak_flux_227)Jy/beamstat.errorDOUBLEprincipalFint227Integrated flux in 223-231MHz image (int_flux_227)Jyphot.fluxDOUBLEprincipale_Fint227rms uncertainty in fit for integrated flux in 223-231MHz image (err_int_flux_227)Jystat.errorDOUBLEprincipala227Fitted semi-major axis in 223-231MHz image (a_227)arcsecphys.angSize.smajAxis;meta.modelledDOUBLEprincipalb227Fitted semi-minor axis in 223-231MHz image (b_227)arcsecphys.angSize.sminAxis;meta.modelledDOUBLEprincipalpa227Fitted position angle in 223-231MHz image (pa_227)degpos.posAng;meta.modelledDOUBLEprincipalresm227Mean value of data-model in 223-231MHz image (residual_mean_227)Jy/beamstat.value;stat.meanDOUBLEprincipalresstd227Standard deviation of data-model in 223-231MHz image (residual_std_227)Jy/beamstat.fit.residualDOUBLEprincipalpsfa227Semi-major axis of the point spread function in 223-231MHz image (psf_a_227)arcsecphys.angSize.smajAxis;instr.det.psfDOUBLEprincipalpsfb227Semi-minor axis of the point spread function in 223-231MHz image (psf_b_227)arcsecphys.angSize.sminAxis;instr.det.psfDOUBLEprincipalpsfPA227Position angle of the point spread function in 223-231MHz image (psf_pa_227)degpos.posAng;meta.modelledDOUBLEprincipalalphaFitted spectral index (alpha)spect.index;meta.modelledDOUBLEprincipale_alphaError on fitted spectral index (err_alpha)stat.error;pos.eq.raDOUBLEprincipalchi2Reduced chi^2 statistic for spectral index fit (reduced_chi2)stat.fit.chi2DOUBLEprincipalFintfit200Fitted 200MHz integrated flux density (int_flux_fit_200)Jystat.fit;phot.fluxDOUBLEprincipale_Fintfit200Error on fitted 200MHz integrated flux density (err_int_flux_fit_200)Jystat.errorDOUBLEprincipalgalah_dr4Studying galaxy evolution through galactic archaeologygalah_dr4.vac3dnltelitableGALAH DR4 VAC 3D-NLTE Lithium Version 240705tmass_id2MASS identifiermeta.id.crossVARCHARprincipalsobject_idGALAH identifiermeta.idBIGINTprincipalteffSpectroscopic effective temperature (used for fitting)phys.temperature.effectiveREALprincipale_teffUncertainty teffstat.error;phys.temperature.effectiveREALprincipalloggSurface gravity adjusted via parallax informationphys.gravityREALprincipale_loggUncertainty logg_plxstat.error;phys.gravityREALprincipalfe_hAbundance of Fe and all other elements not fitted in GALAH (Fe: 1D-NLTE)phys.abund.FeREALprincipale_fe_hUncertainty fe_hstat.error;phys.abund.FeREALprincipalEWEquivalent width of LiI 6708 line regionspect.line.eqWidthREALprincipale_EW_lowLower uncertainty limit of ew_listat.error;spect.line.eqWidthREALprincipale_EW_uppUpper uncertainty limit of ew_listat.error;spect.line.eqWidthREALprincipale_EW_norrisNorris uncertainty limit of ew_listat.error;spect.line.eqWidthREALprincipalALiAbsolute Lithium abundancephys.abundREALprincipalALi_upp_limUpper limit of a_listat.error;phys.abundREALprincipale_ALi_lowLower uncertainty of a_listat.error;phys.abundREALprincipale_ALi_uppUpper uncertainty of a_listat.error;phys.abundREALprincipale_ALi_teffTeff-correlated uncertainty of a_listat.error;phys.abundREALprincipalminchisqA_Li fitting minimum chi2stat.fit.chi2REALprincipalflag_spMajor spectroscopic quality bitmask flagmeta.code.qual,stat.fitINTEGERprincipalflag_fe_hQuality flag fe_hmeta.code.qual,stat.fitINTEGERprincipalflag_ALiQuality bitmask flag of a_limeta.code.qual,stat.fitINTEGERprincipalfwhm_liFWHM of LiI 6708 line fitspect.line.width;stat.fwhmREALprincipalrvRadial velocity used for orbit estimationarith.factor;spect.dopplerVelocREALprincipalsnrSNR of LiI 6708 line fitstat.snrREALprincipalCN1CN1 of LiI 6708 line fitspect.line.eqWidthREALprincipalFeFe of LiI 6708 line fitspect.line.eqWidthREALprincipalCN2CN2 of LiI 6708 line fitspect.line.eqWidthREALprincipalV/CeV/Ce of LiI 6708 line fitspect.line.eqWidthREALprincipalQuest1?1 of LiI 6708 line fitspect.line.eqWidthREALprincipalQuest2?2 of LiI 6708 line fitspect.line.eqWidthREALprincipalgalah_dr4.vacdynamicstableGALAH DR4 VAC Dynamics Version 240705omega_RRadial orbit frequencysrc.orbitalREALprincipalsobject_idGALAH identifiermeta.idBIGINTprincipaltmass_id2MASS identifiermeta.id.crossVARCHARprincipalgaiadr3_source_idGaia DR3 source_idmeta.id.crossBIGINTprincipalraGaia DR3 Right ascensionpos.eq.ra;meta.mainREALindexedprincipaldecGaia DR3 Declinationpos.eq.dec;meta.mainREALindexedprincipalr_medMedian Distance used for calculating logg(plx)pos.distanceREALprincipalpmraGaia DR3 Proper motion in right ascension directionpos.pm;pos.eq.raREALprincipalpmdecGaia DR3 Proper motion in declination directionpos.pm;pos.eq.decREALprincipalrvRadial velocity used for orbit estimationarith.factor;spect.dopplerVelocREALprincipalX_XYZBest-value heliocentric Galactic rectangular x-coordinatepos.cartesian.x;pos.heliocentricREALprincipalY_XYZBest-value heliocentric Galactic rectangular y-coordinatepos.cartesian.y;pos.heliocentricREALprincipalZ_XYZBest-value heliocentric Galactic rectangular z-coordinatepos.cartesian.z;pos.heliocentricREALprincipalU_UVWBest-value heliocentric Galactic rectangular x-velocityphys.vel.orbital;pos.heliocentricREALprincipalV_UVWBest-value heliocentric Galactic rectangular y-velocityphys.vel.orbital;pos.heliocentricREALprincipalW_UVWBest-value heliocentric Galactic rectangular z-velocityphys.vel.orbital;pos.heliocentricREALprincipalR_RzphiBest-value Galactocentric Radiuspos.galactocentricREALprincipalphi_RzphiBest-value Galactocentric azimuthpos.galactocentricREALprincipalz_RzphiBest-value Galactocentric heightpos.galactocentricREALprincipalvR_RzphiBest-value Galactocentric radial velocityphys.vel.orbital;pos.galactocentricREALprincipalvT_RzphiBest-value Galactocentric tangential velocityphys.vel.orbital;pos.galactocentricREALprincipalvz_RzphiBest-value Galactocentric vertical velocityphys.vel.orbital;pos.galactocentricREALprincipalJ_RBest-value radial actionsrc.orbitalREALprincipalL_ZBest-value azimuthal action / angular momentumsrc.orbital;phys.angMomentumREALprincipalJ_ZBest-value vertical actionsrc.orbitalREALprincipalomega_phiAzimuthal orbit frequencysrc.orbitalREALprincipalomega_zVertical orbit frequencysrc.orbitalREALprincipalangle_RRadial orbit anglesrc.orbitalREALprincipalangle_phiAzimuthal orbit anglesrc.orbitalREALprincipalangle_zVertical orbit anglesrc.orbitalREALprincipaleccBest-value orbit eccentricitysrc.orbital.eccentricityREALprincipalzmaxBest-value maximum Galactocentric heightsrc.orbitalREALprincipalR_periBest-value Galactocentric pericenter radiussrc.orbitalREALprincipalR_apBest-value Galactocentric apocenter radiussrc.orbitalREALprincipalEnergyBest-value orbit energysrc.orbital;phys.energyREALprincipalgalah_dr4.vacxmatchtableGALAH DR4 VAC X-Match to Gaia DR3, 2MASS, WISE Version 240705sobject_idGALAH identifiermeta.idBIGINTprincipaltmass_id2MASS identifiermeta.id.crossVARCHARprincipaltmass_ph_qual2MASS Photometric quality flag. Three character flag, one character per bameta.code.qual;photVARCHARprincipalraj20002MASS J2000 right ascension with respect to the ICRSpos.eq.ra;meta.mainREALindexedprincipaldej20002MASS J2000 declination with respect to the ICRSpos.eq.dec;meta.mainREALindexedprincipalj_m2MASS J-band magnitudephot.mag;em.IR.JREALprincipalj_msigcom2MASS Uncertainty of j_mstat.error;phot.mag;em.IR.JREALprincipalh_m2MASS H-band magnitudephot.mag;em.IR.HREALprincipalh_msigcom2MASS Uncertainty of h_mstat.error;phot.mag;em.IR.HREALprincipalks_m2MASS Ks-band magnitudephot.mag;em.IR.KREALprincipalks_msigcom2MASS Uncertainty of ks_mstat.error;phot.mag;em.IR.KREALprincipalwise_idAllWISE Sexagesimal, equatorial position-based source name in the form:?hhmmmeta.id.crossVARCHARprincipalW1magAllWISE W1 magnitude measured with profile-fitting photometry, or the magnitphot.mag;em.IR.3-4umREALprincipale_W1magAllWISE W1 profile-fit photometric measurement uncertainty in mag units. Thistat.error;phot.magREALprincipalW2magAllWISE W2-band magnitudephot.mag;em.IR.4-8umREALprincipale_W2magAllWISE uncertainty of W2magstat.error;phot.magREALprincipalW3magAllWISE W3 magnitude measured with profile-fitting photometry, or the magnitphot.mag;em.IR.8-15umREALprincipale_W3magAllWISE W3 profile-fit photometric measurement uncertainty in mag units. Thistat.error;phot.magREALprincipalW4magAllWISE W4 magnitude measured with profile-fitting photometry, or the magnitphot.mag;em.IR.15-30umREALprincipale_W4magAllWISE W4 profile-fit photometric measurement uncertainty in mag units. Thistat.error;phot.magREALprincipalwise_ph_qualAllWISE Photometric quality flag. ?Four character flag, one character per bmeta.code.qual;photVARCHARprincipalr_med_geoBailer-Jones+ (2021) The median of the geometric distance posterior. The geometric distanpos.distanceREALprincipalr_lo_geoBailer-Jones+ (2021) The 16th percentile of the geometric distance posterior. The lower 1pos.distance;stat.minREALprincipalr_hi_geoBailer-Jones+ (2021) The 84th percentile of the geometric distance posterior. The upper 1pos.distance;stat.maxREALprincipalr_med_photogeoBailer-Jones+ (2021) The median of the photogeometric distance posterior. The photogeometpos.distanceREALprincipalr_lo_photogeoBailer-Jones+ (2021) The 16th percentile of the photogeometric distance posterior. The lopos.distance;stat.minREALprincipalr_hi_photogeoBailer-Jones+ (2021) The 84th percentile of the photogeometric distance posterior. The uppos.distance;stat.maxREALprincipalcalj_flagBailer-Jones+ (2021) Additional information on the solution. Do not use for filtering (semeta.codeVARCHARprincipalsolution_idGaia DR3 Solution Identifiermeta.versionBIGINTprincipaldesignationGaia DR3 Unique source designation (unique across all Data Releases)meta.id;meta.mainVARCHARindexedprincipalsource_idGaia DR3 Unique source identifier (unique within a particular Data Release)meta.idBIGINTprincipalrandom_indexGaia DR3 Random index for use when selecting subsetsmeta.codeBIGINTprincipalref_epochGaia DR3 Reference epochmeta.ref;time.epochREALprincipalraGaia DR3 Right ascensionpos.eq.ra;meta.mainREALindexedprincipalra_errorGaia DR3 Standard error of right ascensionstat.error;pos.eq.raREALprincipaldecGaia DR3 Declinationpos.eq.dec;meta.mainREALindexedprincipaldec_errorGaia DR3 Standard error of declinationstat.error;pos.eq.decREALprincipalparallaxAstrometric parallax used for GALAH DR4pos.parallax.trigREALprincipalparallax_errorGaia DR3 Standard error of parallaxstat.error;pos.parallax.trigREALprincipalparallax_over_errorGaia DR3 Parallax divided by its standard errorstat.snr;pos.parallax.trigREALprincipalpmGaia DR3 Total proper motionpos.pm;pos.eqREALprincipalpmraGaia DR3 Proper motion in right ascension directionpos.pm;pos.eq.raREALprincipalpmra_errorGaia DR3 Standard error of proper motion in right ascension directionstat.error;pos.pm;pos.eq.raREALprincipalpmdecGaia DR3 Proper motion in declination directionpos.pm;pos.eq.decREALprincipalpmdec_errorGaia DR3 Standard error of proper motion in declination directionstat.error;pos.pm;pos.eq.decREALprincipalra_dec_corrGaia DR3 Correlation between right ascension and declinationstat.correlationREALprincipalra_parallax_corrGaia DR3 Correlation between right ascension and parallaxstat.correlationREALprincipalra_pmra_corrGaia DR3 Correlation between right ascension and proper motion in right ascenstat.correlationREALprincipalra_pmdec_corrGaia DR3 Correlation between right ascension and proper motion in declinationstat.correlationREALprincipaldec_parallax_corrGaia DR3 Correlation between declination and parallaxstat.correlationREALprincipaldec_pmra_corrGaia DR3 Correlation between declination and proper motion in right ascensionstat.correlationREALprincipaldec_pmdec_corrGaia DR3 Correlation between declination and proper motion in declinationstat.correlationREALprincipalparallax_pmra_corrGaia DR3 Correlation between parallax and proper motion in right ascensionstat.correlationREALprincipalparallax_pmdec_corrGaia DR3 Correlation between parallax and proper motion in declinationstat.correlationREALprincipalpmra_pmdec_corrGaia DR3 Correlation between proper motion in right ascension and proper motistat.correlationREALprincipalastrometric_n_obs_alGaia DR3 Total number of observations in the along-scan (AL) directionmeta.numberINTEGERprincipalastrometric_n_obs_acGaia DR3 Total number of observations in the across-scan (AC) directionmeta.numberINTEGERprincipalastrometric_n_good_obs_alGaia DR3 Number of good observations in the along-scan (AL) directionmeta.numberINTEGERprincipalastrometric_n_bad_obs_alGaia DR3 Number of bad observations in the along-scan (AL) directionmeta.numberINTEGERprincipalastrometric_gof_alGaia DR3 Goodness of fit statistic of model wrt along-scan observationsstat.fit.goodnessREALprincipalastrometric_chi2_alGaia DR3 AL chi-square valuestat.fit.chi2REALprincipalastrometric_excess_noiseGaia DR3 Excess noise of the sourcestat.valueREALprincipalastrometric_excess_noise_sigGaia DR3 Significance of excess noisestat.valueREALprincipalastrometric_params_solvedGaia DR3 Which parameters have been solved for?meta.numberINTEGERprincipalastrometric_primary_flagGaia DR3 Primary or secondaymeta.codeBOOLEANprincipalnu_eff_used_in_astrometryGaia DR3 Effective wavenumber of the source used in the astrometric solutionem.wavenumberREALprincipalpseudocolourGaia DR3 Astrometrically estimated pseudocolour of the sourceem.wavenumberREALprincipalpseudocolour_errorGaia DR3 Standard error of the pseudocolour of the sourcestat.error;em.wavenumberREALprincipalra_pseudocolour_corrGaia DR3 Correlation between right ascension and pseudocolourstat.correlation;em.wavenumber;pos.eq.raREALprincipaldec_pseudocolour_corrGaia DR3 Correlation between declination and pseudocolourstat.correlation;em.wavenumber;pos.eq.decREALprincipalparallax_pseudocolour_corrGaia DR3 Correlation between parallax and pseudocolourstat.correlation;em.wavenumber;pos.parallaxREALprincipalpmra_pseudocolour_corrGaia DR3 Correlation between proper motion in right asension and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.raREALprincipalpmdec_pseudocolour_corrGaia DR3 Correlation between proper motion in declination and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.decREALprincipalastrometric_matched_transitsGaia DR3 Matched FOV transits used in the AGIS solutionmeta.numberINTEGERprincipalvisibility_periods_usedGaia DR3 Number of visibility periods used in Astrometric solutionmeta.numberINTEGERprincipalastrometric_sigma5d_maxGaia DR3 The longest semi-major axis of the 5-d error ellipsoidstat;pos.errorEllipseREALprincipalmatched_transitsGaia DR3 The number of transits matched to this sourcemeta.numberINTEGERprincipalnew_matched_transitsGaia DR3 The number of transits newly incorporated into an existing source inmeta.numberINTEGERprincipalmatched_transits_removedGaia DR3 The number of transits removed from an existing source in the currenmeta.numberINTEGERprincipalipd_gof_harmonic_amplitudeGaia DR3 Amplitude of the IPD GoF versus position angle of scanstat.valueREALprincipalipd_gof_harmonic_phaseGaia DR3 Phase of the IPD GoF versus position angle of scanpos.posAng;stat.valueREALprincipalipd_frac_multi_peakGaia DR3 Percent of successful-IPD windows with more than one peakstat.valueINTEGERprincipalipd_frac_odd_winGaia DR3 Percent of transits with truncated windows or multiple gatestat.valueINTEGERprincipalruweGaia DR3 Renormalised unit weight errorstat.errorREALprincipalscan_direction_strength_k1Gaia DR3 Degree of concentration of scan directions across the sourcestat.valueREALprincipalscan_direction_strength_k2Gaia DR3 Degree of concentration of scan directions across the sourcestat.valueREALprincipalscan_direction_strength_k3Gaia DR3 Degree of concentration of scan directions across the sourcestat.valueREALprincipalscan_direction_strength_k4Gaia DR3 Degree of concentration of scan directions across the sourcestat.valueREALprincipalscan_direction_mean_k1Gaia DR3 Mean position angle of scan directions across the sourcepos.posAng;stat.meanREALprincipalscan_direction_mean_k2Gaia DR3 Mean position angle of scan directions across the sourcepos.posAng;stat.meanREALprincipalscan_direction_mean_k3Gaia DR3 Mean position angle of scan directions across the sourcepos.posAng;stat.meanREALprincipalscan_direction_mean_k4Gaia DR3 Mean position angle of scan directions across the sourcepos.posAng;stat.meanREALprincipalduplicated_sourceGaia DR3 Source with multiple source identifiersmeta.code.statusBOOLEANprincipalphot_g_n_obsGaia DR3 Number of observations contributing to G photometrymeta.numberINTEGERprincipalphot_g_mean_fluxGaia DR3 G-band mean fluxphot.flux;em.optREALprincipalphot_g_mean_flux_errorGaia DR3 Error on G-band mean fluxstat.error;phot.flux;em.optREALprincipalphot_g_mean_flux_over_errorGaia DR3 G-band mean flux divided by its errorstat.snr;phot.flux;em.optREALprincipalphot_g_mean_magGaia DR3 G-band mean magnitudephot.mag;em.optREALprincipalphot_bp_n_obsGaia DR3 Number of observations contributing to BP photometrymeta.numberINTEGERprincipalphot_bp_mean_fluxGaia DR3 Integrated BP mean fluxphot.flux;em.opt.BREALprincipalphot_bp_mean_flux_errorGaia DR3 Error on the integrated BP mean fluxstat.error;phot.flux;em.opt.BREALprincipalphot_bp_mean_flux_over_errorGaia DR3 Integrated BP mean flux divided by its errorstat.snr;phot.flux;em.opt.BREALprincipalphot_bp_mean_magGaia DR3 Integrated BP mean magnitudephot.mag;em.opt.BREALprincipalphot_rp_n_obsGaia DR3 Number of observations contributing to RP photometrymeta.numberINTEGERprincipalphot_rp_mean_fluxGaia DR3 Integrated RP mean fluxphot.flux;em.opt.RREALprincipalphot_rp_mean_flux_errorGaia DR3 Error on the integrated RP mean fluxstat.error;phot.flux;em.opt.RREALprincipalphot_rp_mean_flux_over_errorGaia DR3 Integrated RP mean flux divided by its errorstat.snr;phot.flux;em.opt.RREALprincipalphot_rp_mean_magGaia DR3 Integrated RP mean magnitudephot.mag;em.opt.RREALprincipalphot_bp_rp_excess_factorGaia DR3 BP/RP excess factorarith.factor;phot.flux;em.optREALprincipalphot_bp_n_contaminated_transitsGaia DR3 Number of BP contaminated transitsmeta.numberINTEGERprincipalphot_bp_n_blended_transitsGaia DR3 Number of BP blended transitsmeta.numberINTEGERprincipalphot_rp_n_contaminated_transitsGaia DR3 Number of RP contaminated transitsmeta.numberINTEGERprincipalphot_rp_n_blended_transitsGaia DR3 Number of RP blended transitsmeta.numberINTEGERprincipalphot_proc_modeGaia DR3 Photometry processing modemeta.codeINTEGERprincipalbp_rpGaia DR3 BP - RP colourphot.color;em.opt.B;em.opt.RREALprincipalbp_gGaia DR3 BP - G colourphot.color;em.opt.B;em.optREALprincipalg_rpGaia DR3 G - RP colourphot.color;em.opt;em.opt.RREALprincipalradial_velocityGaia DR3 Radial velocityspect.dopplerVeloc.opt;em.opt.IREALprincipalradial_velocity_errorGaia DR3 Radial velocity errorstat.error;spect.dopplerVeloc.opt;em.opt.IREALprincipalrv_method_usedGaia DR3 Method used to obtain the radial velocitymeta.code.classINTEGERprincipalrv_nb_transitsGaia DR3 Number of transits used to compute the radial velocitymeta.numberINTEGERprincipalrv_nb_deblended_transitsGaia DR3 Number of valid transits that have undergone deblendingmeta.numberINTEGERprincipalrv_visibility_periods_usedGaia DR3 Number of visibility periods used to estimate the radial velocitymeta.numberINTEGERprincipalrv_expected_sig_to_noiseGaia DR3 Expected signal to noise ratio in the combination of the spectra usestat.snrREALprincipalrv_renormalised_gofGaia DR3 Radial velocity renormalised goodness of fitstat.fit.goodnessREALprincipalrv_chisq_pvalueGaia DR3 P-value for constancy based on a chi-squared criterionstat.fit.paramREALprincipalrv_time_durationGaia DR3 Time coverage of the radial velocity time seriestime.durationREALprincipalrv_amplitude_robustGaia DR3 Total amplitude in the radial velocity time series after outlier remstat.error;spect.dopplerVeloc.opt;em.opt.IREALprincipalrv_template_teffGaia DR3 Teff of the template used to compute the radial velocitystat.fit.paramREALprincipalrv_template_loggGaia DR3 Logg of the template used to compute the radial velocitystat.fit.paramREALprincipalrv_template_fe_hGaia DR3 [Fe/H] of the template used to compute the radial velocityystat.fit.paramREALprincipalrv_atm_param_originGaia DR3 Origin of the atmospheric parameters associated to the templatemeta.code.classINTEGERprincipalvbroadGaia DR3 Spectral line broadening parameterspect.dopplerVeloc.opt;em.opt.IREALprincipalvbroad_errorGaia DR3 Uncertainty on the spectral line broadeningstat.error;spect.dopplerVeloc.opt;em.opt.IREALprincipalvbroad_nb_transitsGaia DR3 Number of transits used to compute vbroadmeta.numberINTEGERprincipalgrvs_magGaia DR3 Integrated Grvs magnitudephot.mag;em.optREALprincipalgrvs_mag_errorGaia DR3 Grvs magnitude uncertaintystat.error;phot.mag;em.optREALprincipalgrvs_mag_nb_transitsGaia DR3 Number of transits used to compute Grvsmeta.numberINTEGERprincipalrvs_spec_sig_to_noiseGaia DR3 Signal to noise ratio in the mean RVS spectrumstat.snrREALprincipalphot_variable_flagGaia DR3 Photometric variability flagmeta.code;src.varVARCHARprincipallGaia DR3 Galactic longitudepos.galactic.lonREALprincipalbGaia DR3 Galactic latitudepos.galactic.latREALprincipalecl_lonGaia DR3 Ecliptic longitudepos.ecliptic.lonREALprincipalecl_latGaia DR3 Ecliptic latitudepos.ecliptic.latREALprincipalin_qso_candidatesGaia DR3 Flag indicating the availability of additional information in the QSmeta.code.statusBOOLEANprincipalin_galaxy_candidatesGaia DR3 Flag indicating the availability of additional information in the gameta.code.statusBOOLEANprincipalnon_single_starGaia DR3 Flag indicating the availability of additional information in the vameta.code.statusINTEGERprincipalhas_xp_continuousGaia DR3 Flag indicating the availability of mean BP/RP spectrum in continuoumeta.code.statusBOOLEANprincipalhas_xp_sampledGaia DR3 Flag indicating the availability of mean BP/RP spectrum in sampled fmeta.code.statusBOOLEANprincipalhas_rvsGaia DR3 Flag indicating the availability of mean RVS spectrum for this sourcmeta.code.statusBOOLEANprincipalhas_epoch_photometryGaia DR3 Flag indicating the availability of epoch photometry for this sourcemeta.code.statusBOOLEANprincipalhas_epoch_rvGaia DR3 Flag indicating the availability of epoch radial velocity for this smeta.code.statusBOOLEANprincipalhas_mcmc_gspphotGaia DR3 Flag indicating the availability of GSP-Phot MCMC samples for this smeta.code.statusBOOLEANprincipalhas_mcmc_mscGaia DR3 Flag indicating the availability of MSC MCMC samples for this sourcemeta.code.statusBOOLEANprincipalin_andromeda_surveyGaia DR3 Flag indicating that the source is present in the Gaia Andromeda Phometa.code.statusBOOLEANprincipalclassprob_dsc_combmod_quasarGaia DR3 Probability from DSC-Combmod of being a quasar (data used: BP/RP spestat.probabilityREALprincipalclassprob_dsc_combmod_galaxyGaia DR3 Probability from DSC-Combmod of being a galaxy (data used: BP/RP spestat.probabilityREALprincipalclassprob_dsc_combmod_starGaia DR3 Probability from DSC-Combmod of being a single star (but not a whitestat.probabilityREALprincipalteff_gspphotGaia DR3 Effective temperature from GSP-Phot Aeneas best library using BP/RPphys.temperature.effectiveREALprincipalteff_gspphot_lowerGaia DR3 Lower confidence level (16%) of effective temperature from GSP-Photphys.temperature.effective;stat.minREALprincipalteff_gspphot_upperGaia DR3 Upper confidence level (84%) of effective temperature from GSP-Photphys.temperature.effective;stat.maxREALprincipallogg_gspphotGaia DR3 Surface gravity from GSP-Phot Aeneas best library using BP/RP spectrphys.gravityREALprincipallogg_gspphot_lowerGaia DR3 Lower confidence level (16%) of surface gravity from GSP-Phot Aeneasphys.gravity;stat.minREALprincipallogg_gspphot_upperGaia DR3 Upper confidence level (84%) of surface gravity from GSP-Phot Aeneasphys.gravity;stat.maxREALprincipalmh_gspphotGaia DR3 Iron abundance from GSP-Phot Aeneas best library using BP/RP spectraphys.abund.ZREALprincipalmh_gspphot_lowerGaia DR3 Lower confidence level (16%) of iron abundance from GSP-Phot Aeneasphys.abund.Z;stat.minREALprincipalmh_gspphot_upperGaia DR3 Upper confidence level (84%) of iron abundance from GSP-Phot Aeneasphys.abund.Z;stat.maxREALprincipaldistance_gspphotGaia DR3 Distance from GSP-Phot Aeneas best library using BP/RP spectrapos.distance;pos.eqREALprincipaldistance_gspphot_lowerGaia DR3 Lower confidence level (16%) of distance from GSP-Phot Aeneas best lpos.distance;pos.eqREALprincipaldistance_gspphot_upperGaia DR3 Upper confidence level (84%) of distance from GSP-Phot Aeneas best lpos.distance;pos.eqREALprincipalazero_gspphotGaia DR3 Monochromatic extinction $A_0$ at 547.7nm from GSP-Phot Aeneas bestphys.absorption;em.optREALprincipalazero_gspphot_lowerGaia DR3 Lower confidence level (16%) of monochromatic extinction $A_0$ at 54phys.absorption;em.optREALprincipalazero_gspphot_upperGaia DR3 Upper confidence level (84%) of monochromatic extinction $A_0$ at 54phys.absorption;em.optREALprincipalag_gspphotGaia DR3 Extinction in G band from GSP-Phot Aeneas best library using BP/RP sphys.absorption;em.optREALprincipalag_gspphot_lowerGaia DR3 Lower confidence level (16%) of extinction in G band from GSP-Phot Aphys.absorption;em.optREALprincipalag_gspphot_upperGaia DR3 Upper confidence level (84%) of extinction in G band from GSP-Phot Aphys.absorption;em.optREALprincipalebpminrp_gspphotGaia DR3 Reddening $E(G_{\rm BP} - G_{\rm RP})$ from GSP-Phot Aeneas best libphot.color.excessREALprincipalebpminrp_gspphot_lowerGaia DR3 Lower confidence level (16%) of reddening $E(G_{\rm BP} - G_{\rm RPphot.color.excess;stat.minREALprincipalebpminrp_gspphot_upperGaia DR3 Upper confidence level (84%) of reddening $E(G_{\rm BP} - G_{\rm RPphot.color.excess;stat.maxREALprincipallibname_gspphotGaia DR3 Name of library that achieves the highest mean log-posterior in MCMCmeta.noteVARCHARprincipalebvExtinction E(B-V)phys.absorption.galREALprincipalphot_g_mean_mag_errorGaia DR3 G-band mean magnitude errorstat.error;phot.mag;em.optREALprincipalphot_bp_mean_mag_errorIntegrated BP mean magnitude errorstat.error;phot.mag;em.opt.BREALprincipalphot_rp_mean_mag_errorIntegrated RP mean magnitude errorstat.error;phot.mag;em.opt.RREALprincipalplx_zpt_corrLindegren+ (2021) Gaia DR3 parallax zeropoint correctionstat.errorREALprincipalparallax_rawGaia DR3 Raw Parallax (before plx_zpt_corr)pos.parallax.trigREALprincipalparallax_error_rawGaia DR3 Raw Parallax (before plx_zpt_corr)stat.error;pos.parallax.trigREALprincipalgalah_dr4.mainspectableGALAH DR4 Main Allspec Version 240705sobject_idGALAH identifiermeta.idBIGINTprincipaltmass_id2MASS identifiermeta.id.crossVARCHARprincipalgaiadr3_source_idGaia DR3 source_idmeta.id.crossBIGINTprincipalsurvey_nameHERMES-2dF Survey/Program/Pointing (other if not available)meta.idVARCHARprincipalfield_idGALAH Field ID (-1 if not available)meta.numberINTEGERprincipalsetupAnalysis setup: single/binary/coaddsmeta.versionVARCHARprincipalmjdModified Julian Datetime.epochREALprincipalraGaia DR3 Right ascensionpos.eq.ra;meta.mainREALindexedprincipaldecGaia DR3 Declinationpos.eq.dec;meta.mainREALindexedprincipalflag_spMajor spectroscopic quality bitmask flagmeta.code.qual,stat.fitINTEGERprincipalflag_sp_fitMajor spectroscopic fitting quality bitmask flagmeta.code.qual,stat.fitINTEGERprincipalopt_loopNr of optimisation loops used for fittingmeta.modelledINTEGERprincipalflag_redQuality bitmask flag of reduction pipelinemeta.code.qual,stat.fitINTEGERprincipalsnr_px_ccd1Average signal-to-noise ratio (per pixel) of CCD1stat.snrREALprincipalsnr_px_ccd2Average signal-to-noise ratio (per pixel) of CCD2stat.snrREALprincipalsnr_px_ccd3Average signal-to-noise ratio (per pixel) of CCD3stat.snrREALprincipalsnr_px_ccd4Average signal-to-noise ratio (per pixel) of CCD4stat.snrREALprincipalchi2_spChi2 value of spectroscopic fittingstat.fit.chi2REALprincipalpx_used_percPercentage of spectrum used for spectroscopic fitfit.paramINTEGERprincipalmodel_nameNeural network model used for creating synthetic spectrameta.modelledVARCHARprincipalclosest_modelNeural network model closest for Teff/logg/[Fe/H] combinationmeta.modelledVARCHARprincipalcomp_timeComputation time spent on spectrummeta.numberREALprincipalrv_comp_nrNumber of peaks in RV cross-correlation function (CCF)meta.numberINTEGERprincipalrv_comp_1Radial velocity of primary sourcespect.dopplerVeloc.optREALprincipale_rv_comp_1Uncertainty of rv_comp_1stat.error;spect.dopplerVeloc.optREALprincipalrv_comp_1_pProminence of rv_comp_1 in CCFstat.paramREALprincipalrv_comp_2Radial velocity of potential secondary sourcespect.dopplerVeloc.optREALprincipalrv_comp_2_hHeight of rv_comp_1 in CCFstat.paramREALprincipalrv_comp_2_pProminence of rv_comp_1 in CCFstat.paramREALprincipalrv_gaia_dr3Radial velocity in Gaia DR3spect.dopplerVeloc.optREALprincipale_rv_gaia_dr3Uncertainty of rv_gaia_dr3stat.error;spect.dopplerVeloc.optREALprincipalv_bary_effBarycentric velocity applied to reduced spectraarith.factor;phys.velocREALprincipalteffSpectroscopic effective temperature (used for fitting)phys.temperature.effectiveREALprincipale_teffUncertainty teffstat.error;phys.temperature.effectiveREALprincipalloggSurface gravity adjusted via parallax informationphys.gravityREALprincipale_loggUncertainty logg_plxstat.error;phys.gravityREALprincipalfe_hAbundance of Fe and all other elements not fitted in GALAH (Fe: 1D-NLTE)phys.abund.FeREALprincipale_fe_hUncertainty fe_hstat.error;phys.abund.FeREALprincipalflag_fe_hQuality flag fe_hmeta.code.qual,stat.fitINTEGERprincipalvmicMicroturbulence velocity (fitted)phys.veloc.microTurbREALprincipale_vmicUncertainty vmicstat.error;phys.veloc.microTurbREALprincipalvsiniBroadening velocity (fitted sme.vsini with sme.vmac=0)phys.veloc.rotatREALprincipale_vsiniUncertainty of vsinistat.error;phys.veloc.rotatREALprincipalli_feElemental abundance for [Li/Fe]phys.abundREALprincipale_li_feUncertainty Li_festat.error;phys.abundREALprincipalflag_li_feQuality bitmask flag of Li_femeta.code.qual,stat.fitINTEGERprincipalc_feElemental abundance for [C/Fe]phys.abundREALprincipale_c_feUncertainty C_festat.error;phys.abundREALprincipalflag_c_feQuality bitmask flag of C_femeta.code.qual,stat.fitINTEGERprincipaln_feElemental abundance for [N/Fe]phys.abundREALprincipale_n_feUncertainty N_festat.error;phys.abundREALprincipalflag_n_feQuality bitmask flag of N_femeta.code.qual,stat.fitINTEGERprincipalo_feElemental abundance for [O/Fe]phys.abundREALprincipale_o_feUncertainty O_festat.error;phys.abundREALprincipalflag_o_feQuality bitmask flag of O_femeta.code.qual,stat.fitINTEGERprincipalna_feElemental abundance for [Na/Fe]phys.abundREALprincipale_na_feUncertainty Na_festat.error;phys.abundREALprincipalflag_na_feQuality bitmask flag of Na_femeta.code.qual,stat.fitINTEGERprincipalmg_feElemental abundance for [Mg/Fe]phys.abundREALprincipale_mg_feUncertainty Mg_festat.error;phys.abundREALprincipalflag_mg_feQuality bitmask flag of Mg_femeta.code.qual,stat.fitINTEGERprincipalal_feElemental abundance for [Al/Fe]phys.abundREALprincipale_al_feUncertainty Al_festat.error;phys.abundREALprincipalflag_al_feQuality bitmask flag of Al_femeta.code.qual,stat.fitINTEGERprincipalsi_feElemental abundance for [Si/Fe]phys.abundREALprincipale_si_feUncertainty Si_festat.error;phys.abundREALprincipalflag_si_feQuality bitmask flag of Si_femeta.code.qual,stat.fitINTEGERprincipalk_feElemental abundance for [K/Fe]phys.abundREALprincipale_k_feUncertainty K_festat.error;phys.abundREALprincipalflag_k_feQuality bitmask flag of K_femeta.code.qual,stat.fitINTEGERprincipalca_feElemental abundance for [Ca/Fe]phys.abundREALprincipale_ca_feUncertainty Ca_festat.error;phys.abundREALprincipalflag_ca_feQuality bitmask flag of Ca_femeta.code.qual,stat.fitINTEGERprincipalsc_feElemental abundance for [Sc/Fe]phys.abundREALprincipale_sc_feUncertainty Sc_festat.error;phys.abundREALprincipalflag_sc_feQuality bitmask flag of Sc_femeta.code.qual,stat.fitINTEGERprincipalti_feElemental abundance for [Ti/Fe]phys.abundREALprincipale_ti_feUncertainty Ti_festat.error;phys.abundREALprincipalflag_ti_feQuality bitmask flag of Ti_femeta.code.qual,stat.fitINTEGERprincipalv_feElemental abundance for [V/Fe]phys.abundREALprincipale_v_feUncertainty V_festat.error;phys.abundREALprincipalflag_v_feQuality bitmask flag of V_femeta.code.qual,stat.fitINTEGERprincipalcr_feElemental abundance for [Cr/Fe]phys.abundREALprincipale_cr_feUncertainty Cr_festat.error;phys.abundREALprincipalflag_cr_feQuality bitmask flag of Cr_femeta.code.qual,stat.fitINTEGERprincipalmn_feElemental abundance for [Mn/Fe]phys.abundREALprincipale_mn_feUncertainty Mn_festat.error;phys.abundREALprincipalflag_mn_feQuality bitmask flag of Mn_femeta.code.qual,stat.fitINTEGERprincipalco_feElemental abundance for [Co/Fe]phys.abundREALprincipale_co_feUncertainty Co_festat.error;phys.abundREALprincipalflag_co_feQuality bitmask flag of Co_femeta.code.qual,stat.fitINTEGERprincipalni_feElemental abundance for [Ni/Fe]phys.abundREALprincipale_ni_feUncertainty Ni_festat.error;phys.abundREALprincipalflag_ni_feQuality bitmask flag of Ni_femeta.code.qual,stat.fitINTEGERprincipalcu_feElemental abundance for [Cu/Fe]phys.abundREALprincipale_cu_feUncertainty Cu_festat.error;phys.abundREALprincipalflag_cu_feQuality bitmask flag of Cu_femeta.code.qual,stat.fitINTEGERprincipalzn_feElemental abundance for [Zn/Fe]phys.abundREALprincipale_zn_feUncertainty Zn_festat.error;phys.abundREALprincipalflag_zn_feQuality bitmask flag of Zn_femeta.code.qual,stat.fitINTEGERprincipalrb_feElemental abundance for [Rb/Fe]phys.abundREALprincipale_rb_feUncertainty Rb_festat.error;phys.abundREALprincipalflag_rb_feQuality bitmask flag of Rb_femeta.code.qual,stat.fitINTEGERprincipalsr_feElemental abundance for [Sr/Fe]phys.abundREALprincipale_sr_feUncertainty Sr_festat.error;phys.abundREALprincipalflag_sr_feQuality bitmask flag of Sr_femeta.code.qual,stat.fitINTEGERprincipaly_feElemental abundance for [Y/Fe]phys.abundREALprincipale_y_feUncertainty Y_festat.error;phys.abundREALprincipalflag_y_feQuality bitmask flag of Y_femeta.code.qual,stat.fitINTEGERprincipalzr_feElemental abundance for [Zr/Fe]phys.abundREALprincipale_zr_feUncertainty Zr_festat.error;phys.abundREALprincipalflag_zr_feQuality bitmask flag of Zr_femeta.code.qual,stat.fitINTEGERprincipalmo_feElemental abundance for [Mo/Fe]phys.abundREALprincipale_mo_feUncertainty Mo_festat.error;phys.abundREALprincipalflag_mo_feQuality bitmask flag of Mo_femeta.code.qual,stat.fitINTEGERprincipalru_feElemental abundance for [Ru/Fe]phys.abundREALprincipale_ru_feUncertainty Ru_festat.error;phys.abundREALprincipalflag_ru_feQuality bitmask flag of Ru_femeta.code.qual,stat.fitINTEGERprincipalba_feElemental abundance for [Ba/Fe]phys.abundREALprincipale_ba_feUncertainty Ba_festat.error;phys.abundREALprincipalflag_ba_feQuality bitmask flag of Ba_femeta.code.qual,stat.fitINTEGERprincipalla_feElemental abundance for [La/Fe]phys.abundREALprincipale_la_feUncertainty La_festat.error;phys.abundREALprincipalflag_la_feQuality bitmask flag of La_femeta.code.qual,stat.fitINTEGERprincipalce_feElemental abundance for [Ce/Fe]phys.abundREALprincipale_ce_feUncertainty Ce_festat.error;phys.abundREALprincipalflag_ce_feQuality bitmask flag of Ce_femeta.code.qual,stat.fitINTEGERprincipalnd_feElemental abundance for [Nd/Fe]phys.abundREALprincipale_nd_feUncertainty Nd_festat.error;phys.abundREALprincipalflag_nd_feQuality bitmask flag of Nd_femeta.code.qual,stat.fitINTEGERprincipalsm_feElemental abundance for [Sm/Fe]phys.abundREALprincipale_sm_feUncertainty Sm_festat.error;phys.abundREALprincipalflag_sm_feQuality bitmask flag of Sm_femeta.code.qual,stat.fitINTEGERprincipaleu_feElemental abundance for [Eu/Fe]phys.abundREALprincipale_eu_feUncertainty Eu_festat.error;phys.abundREALprincipalflag_eu_feQuality bitmask flag of Eu_femeta.code.qual,stat.fitINTEGERprincipalsb2_rv_1616th perc. radial velocity of fit to syn-obs residualsstat.error;spect.dopplerVeloc.optREALprincipalsb2_rv_5050th perc. radial velocity of fit to syn-obs residualsspect.dopplerVeloc.optREALprincipalsb2_rv_8484th perc. radial velocity of fit to syn-obs residualsstat.error;spect.dopplerVeloc.optREALprincipalew_h_betaEquivalent Width of observed Hbeta corefit.param;spect.line.eqWidthREALprincipalew_h_alphaEquivalent Width of observed Halpha corefit.param;spect.line.eqWidthREALprincipalres_h_betaResidual Equivalent Width of syn-obs residuals at Hbeta corefit.param;spect.line.eqWidthREALprincipalres_h_alphaResidual Equivalent Width of syn-obs residuals at Halpha corefit.param;spect.line.eqWidthREALprincipalew_k_isEquivalent Width of fit for K7699 Interstellar Linefit.param;spect.line.eqWidthREALprincipalsigma_k_isSigma auf Gaussian fit for K7699 Interstellar Linefit.paramREALprincipalrv_k_isRadial velocity of fit to syn-obs residuals around K7699 linefit.param;spect.dopplerVeloc.optREALprincipalew_dib5780Equivalent Width of fit for 5780 Diffiuse Interstellar Bandfit.param;spect.line.eqWidthREALprincipalsigma_dib5780Sigma auf Gaussian fit for 5780 DIBfit.paramREALprincipalrv_dib5780Radial velocity of fit to syn-obs residuals around 5780 DIBfit.param;spect.dopplerVeloc.optREALprincipalew_dib5797Equivalent Width of fit for 5797 Diffiuse Interstellar Bandfit.param;spect.line.eqWidthREALprincipalsigma_dib5797Sigma auf Gaussian fit for 5797 DIBfit.paramREALprincipalrv_dib5797Radial velocity of fit to syn-obs residuals around 5797 DIBfit.param;spect.dopplerVeloc.optREALprincipalew_dib6613Equivalent Width of fit for 6613 Diffiuse Interstellar Bandfit.param;spect.line.eqWidthREALprincipalsigma_dib6613Sigma auf Gaussian fit for 6613 DIBfit.paramREALprincipalrv_dib6613Radial velocity of fit to syn-obs residuals around 6613 DIBfit.param;spect.dopplerVeloc.optREALprincipallogg_specSpectroscopic surface gravity (used for fitting)phys.gravityREALprincipale_logg_specUncertainty logg_specstat.error;phys.gravityREALprincipalphot_g_mean_magGaia DR3 G-band mean magnitudephot.mag;em.optREALprincipalphot_bp_mean_magGaia DR3 Integrated BP mean magnitudephot.mag;em.opt.BREALprincipalbp_rpGaia DR3 BP - RP colourphot.color;em.opt.B;em.opt.RREALprincipalh_m2MASS H-band magnitudephot.mag;em.IR.HREALprincipalh_msigcom2MASS Uncertainty of h_mstat.error;phot.mag;em.IR.HREALprincipalks_m2MASS Ks-band magnitudephot.mag;em.IR.KREALprincipalks_msigcom2MASS Uncertainty of ks_mstat.error;phot.mag;em.IR.KREALprincipalebvExtinction E(B-V)phys.absorption.galREALprincipalW2magAllWISE W2-band magnitudephot.mag;em.IR.4-8umREALprincipale_W2magAllWISE uncertainty of W2magstat.error;phot.magREALprincipalparallaxAstrometric parallax used for GALAH DR4pos.parallax.trigREALprincipale_parallaxUncertainty of astrometric parallax used for GALAH DR4stat.error;pos.parallax.trigREALprincipalparallax_gaia_edr3Parallax reported with corrections by Gaia EDR3pos.parallax.trigREALprincipale_parallax_gaia_edr3Uncertainty of parallax reported with corrections by Gaia EDR3stat.error;pos.parallax.trigREALprincipalruweGaia DR3 Renormalised unit weight errorstat.errorREALprincipalr_medMedian Distance used for calculating logg(plx)pos.distanceREALprincipalr_loLower Limit Distance used for calculating logg(plx)stat.error;stat.min;pos.distanceREALprincipalr_hiHigher Limit Distance used for calculating logg(plx)stat.error;stat.max;pos.distanceREALprincipala_ksAttenuation in Ks-band A(Ks) used for calculating logg(plx)phys.absorption.galREALprincipalmassMass used for calculating logg(plx)fit.param;phys.massREALprincipalageAge estimated when calculating massfit.param;time.ageREALprincipalbc_ksBolometric Correction of Ks, BC(Ks), used for calculating logg(plx)phot.mag.bc;em.IR.KREALprincipallbolBolometric Luminosity used for calculating logg(plx)fit.param;phys.luminosityREALprincipalgalah_dr4.mainstartableGALAH DR4 Main Allstar Version 240705raGaia DR3 Right ascensionpos.eq.ra;meta.mainREALindexedprincipalsobject_idGALAH identifiermeta.idBIGINTprincipaltmass_id2MASS identifiermeta.id.crossVARCHARprincipalgaiadr3_source_idGaia DR3 source_idmeta.id.crossBIGINTprincipalsurvey_nameHERMES-2dF Survey/Program/Pointing (other if not available)meta.idVARCHARprincipalfield_idGALAH Field ID (-1 if not available)meta.numberINTEGERprincipalsetupAnalysis setup: single/binary/coaddsmeta.versionVARCHARprincipalmjdModified Julian Datetime.epochREALprincipaldecGaia DR3 Declinationpos.eq.dec;meta.mainREALindexedprincipalflag_spMajor spectroscopic quality bitmask flagmeta.code.qual,stat.fitINTEGERprincipalflag_sp_fitMajor spectroscopic fitting quality bitmask flagmeta.code.qual,stat.fitINTEGERprincipalopt_loopNr of optimisation loops used for fittingmeta.modelledINTEGERprincipalflag_redQuality bitmask flag of reduction pipelinemeta.code.qual,stat.fitINTEGERprincipalsnr_px_ccd1Average signal-to-noise ratio (per pixel) of CCD1stat.snrREALprincipalsnr_px_ccd2Average signal-to-noise ratio (per pixel) of CCD2stat.snrREALprincipalsnr_px_ccd3Average signal-to-noise ratio (per pixel) of CCD3stat.snrREALprincipalsnr_px_ccd4Average signal-to-noise ratio (per pixel) of CCD4stat.snrREALprincipalchi2_spChi2 value of spectroscopic fittingstat.fit.chi2REALprincipalpx_used_percPercentage of spectrum used for spectroscopic fitfit.paramINTEGERprincipalmodel_nameNeural network model used for creating synthetic spectrameta.modelledVARCHARprincipalclosest_modelNeural network model closest for Teff/logg/[Fe/H] combinationmeta.modelledVARCHARprincipalcomp_timeComputation time spent on spectrummeta.numberREALprincipalfit_global_rvAre spectra coadded (without RV shifts) and then a global RV fitted?meta.modelledBOOLEANprincipalrv_comp_1Radial velocity of primary sourcespect.dopplerVeloc.optREALprincipale_rv_comp_1Uncertainty of rv_comp_1stat.error;spect.dopplerVeloc.optREALprincipalrv_comp_2Radial velocity of potential secondary sourcespect.dopplerVeloc.optREALprincipale_rv_comp_2Uncertainty of rv_comp_1stat.error;spect.dopplerVeloc.optREALprincipalrv_gaia_dr3Radial velocity in Gaia DR3spect.dopplerVeloc.optREALprincipale_rv_gaia_dr3Uncertainty of rv_gaia_dr3stat.error;spect.dopplerVeloc.optREALprincipalv_bary_effBarycentric velocity applied to reduced spectraarith.factor;phys.velocREALprincipalteffSpectroscopic effective temperature (used for fitting)phys.temperature.effectiveREALprincipale_teffUncertainty teffstat.error;phys.temperature.effectiveREALprincipalloggSurface gravity adjusted via parallax informationphys.gravityREALprincipale_loggUncertainty logg_plxstat.error;phys.gravityREALprincipalfe_hAbundance of Fe and all other elements not fitted in GALAH (Fe: 1D-NLTE)phys.abund.FeREALprincipale_fe_hUncertainty fe_hstat.error;phys.abund.FeREALprincipalflag_fe_hQuality flag fe_hmeta.code.qual,stat.fitINTEGERprincipalvmicMicroturbulence velocity (fitted)phys.veloc.microTurbREALprincipale_vmicUncertainty vmicstat.error;phys.veloc.microTurbREALprincipalvsiniBroadening velocity (fitted sme.vsini with sme.vmac=0)phys.veloc.rotatREALprincipale_vsiniUncertainty of vsinistat.error;phys.veloc.rotatREALprincipalnn_li_feNeural Network Elemental abundance for [Li/Fe]phys.abundREALprincipalnn_e_li_feUncertainty nn_li_fephys.abundREALprincipalnn_flag_li_feQuality bitmask flag of nn_li_fephys.abundINTEGERprincipalc_feElemental abundance for [C/Fe]phys.abundREALprincipale_c_feUncertainty C_festat.error;phys.abundREALprincipalflag_c_feQuality bitmask flag of C_femeta.code.qual,stat.fitINTEGERprincipaln_feElemental abundance for [N/Fe]phys.abundREALprincipale_n_feUncertainty N_festat.error;phys.abundREALprincipalflag_n_feQuality bitmask flag of N_femeta.code.qual,stat.fitINTEGERprincipalo_feElemental abundance for [O/Fe]phys.abundREALprincipale_o_feUncertainty O_festat.error;phys.abundREALprincipalflag_o_feQuality bitmask flag of O_femeta.code.qual,stat.fitINTEGERprincipalna_feElemental abundance for [Na/Fe]phys.abundREALprincipale_na_feUncertainty Na_festat.error;phys.abundREALprincipalflag_na_feQuality bitmask flag of Na_femeta.code.qual,stat.fitINTEGERprincipalmg_feElemental abundance for [Mg/Fe]phys.abundREALprincipale_mg_feUncertainty Mg_festat.error;phys.abundREALprincipalflag_mg_feQuality bitmask flag of Mg_femeta.code.qual,stat.fitINTEGERprincipalal_feElemental abundance for [Al/Fe]phys.abundREALprincipale_al_feUncertainty Al_festat.error;phys.abundREALprincipalflag_al_feQuality bitmask flag of Al_femeta.code.qual,stat.fitINTEGERprincipalsi_feElemental abundance for [Si/Fe]phys.abundREALprincipale_si_feUncertainty Si_festat.error;phys.abundREALprincipalflag_si_feQuality bitmask flag of Si_femeta.code.qual,stat.fitINTEGERprincipalk_feElemental abundance for [K/Fe]phys.abundREALprincipale_k_feUncertainty K_festat.error;phys.abundREALprincipalflag_k_feQuality bitmask flag of K_femeta.code.qual,stat.fitINTEGERprincipalca_feElemental abundance for [Ca/Fe]phys.abundREALprincipale_ca_feUncertainty Ca_festat.error;phys.abundREALprincipalflag_ca_feQuality bitmask flag of Ca_femeta.code.qual,stat.fitINTEGERprincipalsc_feElemental abundance for [Sc/Fe]phys.abundREALprincipale_sc_feUncertainty Sc_festat.error;phys.abundREALprincipalflag_sc_feQuality bitmask flag of Sc_femeta.code.qual,stat.fitINTEGERprincipalti_feElemental abundance for [Ti/Fe]phys.abundREALprincipale_ti_feUncertainty Ti_festat.error;phys.abundREALprincipalflag_ti_feQuality bitmask flag of Ti_femeta.code.qual,stat.fitINTEGERprincipalv_feElemental abundance for [V/Fe]phys.abundREALprincipale_v_feUncertainty V_festat.error;phys.abundREALprincipalflag_v_feQuality bitmask flag of V_femeta.code.qual,stat.fitINTEGERprincipalcr_feElemental abundance for [Cr/Fe]phys.abundREALprincipale_cr_feUncertainty Cr_festat.error;phys.abundREALprincipalflag_cr_feQuality bitmask flag of Cr_femeta.code.qual,stat.fitINTEGERprincipalmn_feElemental abundance for [Mn/Fe]phys.abundREALprincipale_mn_feUncertainty Mn_festat.error;phys.abundREALprincipalflag_mn_feQuality bitmask flag of Mn_femeta.code.qual,stat.fitINTEGERprincipalco_feElemental abundance for [Co/Fe]phys.abundREALprincipale_co_feUncertainty Co_festat.error;phys.abundREALprincipalflag_co_feQuality bitmask flag of Co_femeta.code.qual,stat.fitINTEGERprincipalni_feElemental abundance for [Ni/Fe]phys.abundREALprincipale_ni_feUncertainty Ni_festat.error;phys.abundREALprincipalflag_ni_feQuality bitmask flag of Ni_femeta.code.qual,stat.fitINTEGERprincipalcu_feElemental abundance for [Cu/Fe]phys.abundREALprincipale_cu_feUncertainty Cu_festat.error;phys.abundREALprincipalflag_cu_feQuality bitmask flag of Cu_femeta.code.qual,stat.fitINTEGERprincipalzn_feElemental abundance for [Zn/Fe]phys.abundREALprincipale_zn_feUncertainty Zn_festat.error;phys.abundREALprincipalflag_zn_feQuality bitmask flag of Zn_femeta.code.qual,stat.fitINTEGERprincipalrb_feElemental abundance for [Rb/Fe]phys.abundREALprincipale_rb_feUncertainty Rb_festat.error;phys.abundREALprincipalflag_rb_feQuality bitmask flag of Rb_femeta.code.qual,stat.fitINTEGERprincipalsr_feElemental abundance for [Sr/Fe]phys.abundREALprincipale_sr_feUncertainty Sr_festat.error;phys.abundREALprincipalflag_sr_feQuality bitmask flag of Sr_femeta.code.qual,stat.fitINTEGERprincipaly_feElemental abundance for [Y/Fe]phys.abundREALprincipale_y_feUncertainty Y_festat.error;phys.abundREALprincipalflag_y_feQuality bitmask flag of Y_femeta.code.qual,stat.fitINTEGERprincipalzr_feElemental abundance for [Zr/Fe]phys.abundREALprincipale_zr_feUncertainty Zr_festat.error;phys.abundREALprincipalflag_zr_feQuality bitmask flag of Zr_femeta.code.qual,stat.fitINTEGERprincipalmo_feElemental abundance for [Mo/Fe]phys.abundREALprincipale_mo_feUncertainty Mo_festat.error;phys.abundREALprincipalflag_mo_feQuality bitmask flag of Mo_femeta.code.qual,stat.fitINTEGERprincipalru_feElemental abundance for [Ru/Fe]phys.abundREALprincipale_ru_feUncertainty Ru_festat.error;phys.abundREALprincipalflag_ru_feQuality bitmask flag of Ru_femeta.code.qual,stat.fitINTEGERprincipalba_feElemental abundance for [Ba/Fe]phys.abundREALprincipale_ba_feUncertainty Ba_festat.error;phys.abundREALprincipalflag_ba_feQuality bitmask flag of Ba_femeta.code.qual,stat.fitINTEGERprincipalla_feElemental abundance for [La/Fe]phys.abundREALprincipale_la_feUncertainty La_festat.error;phys.abundREALprincipalflag_la_feQuality bitmask flag of La_femeta.code.qual,stat.fitINTEGERprincipalce_feElemental abundance for [Ce/Fe]phys.abundREALprincipale_ce_feUncertainty Ce_festat.error;phys.abundREALprincipalflag_ce_feQuality bitmask flag of Ce_femeta.code.qual,stat.fitINTEGERprincipalnd_feElemental abundance for [Nd/Fe]phys.abundREALprincipale_nd_feUncertainty Nd_festat.error;phys.abundREALprincipalflag_nd_feQuality bitmask flag of Nd_femeta.code.qual,stat.fitINTEGERprincipalsm_feElemental abundance for [Sm/Fe]phys.abundREALprincipale_sm_feUncertainty Sm_festat.error;phys.abundREALprincipalflag_sm_feQuality bitmask flag of Sm_femeta.code.qual,stat.fitINTEGERprincipaleu_feElemental abundance for [Eu/Fe]phys.abundREALprincipale_eu_feUncertainty Eu_festat.error;phys.abundREALprincipalflag_eu_feQuality bitmask flag of Eu_femeta.code.qual,stat.fitINTEGERprincipalmassMass used for calculating logg(plx)fit.param;phys.massREALprincipalageAge estimated when calculating massfit.param;time.ageREALprincipalbc_ksBolometric Correction of Ks, BC(Ks), used for calculating logg(plx)phot.mag.bc;em.IR.KREALprincipala_ksAttenuation in Ks-band A(Ks) used for calculating logg(plx)phys.absorption.galREALprincipallbolBolometric Luminosity used for calculating logg(plx)fit.param;phys.luminosityREALprincipalr_medMedian Distance used for calculating logg(plx)pos.distanceREALprincipalr_loLower Limit Distance used for calculating logg(plx)stat.error;stat.min;pos.distanceREALprincipalr_hiHigher Limit Distance used for calculating logg(plx)stat.error;stat.max;pos.distanceREALprincipalsb2_rv_1616th perc. radial velocity of fit to syn-obs residualsstat.error;spect.dopplerVeloc.optREALprincipalsb2_rv_5050th perc. radial velocity of fit to syn-obs residualsspect.dopplerVeloc.optREALprincipalsb2_rv_8484th perc. radial velocity of fit to syn-obs residualsstat.error;spect.dopplerVeloc.optREALprincipalew_h_betaEquivalent Width of observed Hbeta corefit.param;spect.line.eqWidthREALprincipalew_h_alphaEquivalent Width of observed Halpha corefit.param;spect.line.eqWidthREALprincipalres_h_betaResidual Equivalent Width of syn-obs residuals at Hbeta corefit.param;spect.line.eqWidthREALprincipalres_h_alphaResidual Equivalent Width of syn-obs residuals at Halpha corefit.param;spect.line.eqWidthREALprincipalew_k_isEquivalent Width of fit for K7699 Interstellar Linefit.param;spect.line.eqWidthREALprincipalsigma_k_isSigma auf Gaussian fit for K7699 Interstellar Linefit.paramREALprincipalrv_k_isRadial velocity of fit to syn-obs residuals around K7699 linefit.param;spect.dopplerVeloc.optREALprincipalew_dib5780Equivalent Width of fit for 5780 Diffiuse Interstellar Bandfit.param;spect.line.eqWidthREALprincipalsigma_dib5780Sigma auf Gaussian fit for 5780 DIBfit.paramREALprincipalrv_dib5780Radial velocity of fit to syn-obs residuals around 5780 DIBfit.param;spect.dopplerVeloc.optREALprincipalew_dib5797Equivalent Width of fit for 5797 Diffiuse Interstellar Bandfit.param;spect.line.eqWidthREALprincipalsigma_dib5797Sigma auf Gaussian fit for 5797 DIBfit.paramREALprincipalrv_dib5797Radial velocity of fit to syn-obs residuals around 5797 DIBfit.param;spect.dopplerVeloc.optREALprincipalew_dib6613Equivalent Width of fit for 6613 Diffiuse Interstellar Bandfit.param;spect.line.eqWidthREALprincipalsigma_dib6613Sigma auf Gaussian fit for 6613 DIBfit.paramREALprincipalrv_dib6613Radial velocity of fit to syn-obs residuals around 6613 DIBfit.param;spect.dopplerVeloc.optREALprincipalebvExtinction E(B-V)phys.absorption.galREALprincipalphot_g_mean_magGaia DR3 G-band mean magnitudephot.mag;em.optREALprincipalbp_rpGaia DR3 BP - RP colourphot.color;em.opt.B;em.opt.RREALprincipalj_m2MASS J-band magnitudephot.mag;em.IR.JREALprincipalj_msigcom2MASS Uncertainty of j_mstat.error;phot.mag;em.IR.JREALprincipalh_m2MASS H-band magnitudephot.mag;em.IR.HREALprincipalh_msigcom2MASS Uncertainty of h_mstat.error;phot.mag;em.IR.HREALprincipalks_m2MASS Ks-band magnitudephot.mag;em.IR.KREALprincipalks_msigcom2MASS Uncertainty of ks_mstat.error;phot.mag;em.IR.KREALprincipalW2magAllWISE W2-band magnitudephot.mag;em.IR.4-8umREALprincipale_W2magAllWISE uncertainty of W2magstat.error;phot.magREALprincipalruweGaia DR3 Renormalised unit weight errorstat.errorREALprincipalparallaxAstrometric parallax used for GALAH DR4pos.parallax.trigREALprincipalparallax_errorGaia DR3 Standard error of parallaxstat.error;pos.parallax.trigREALprincipalew_liEquivalent width of LiI 6708 line regionspect.line.eqWidthREALprincipale_ew_li_lowLower uncertainty limit of ew_listat.error;spect.line.eqWidthREALprincipale_ew_li_uppUpper uncertainty limit of ew_listat.error;spect.line.eqWidthREALprincipala_liAbsolute Lithium abundancephys.abundREALprincipala_li_upp_limUpper limit of a_listat.error;phys.abundREALprincipale_a_li_lowLower uncertainty of a_listat.error;phys.abundREALprincipale_a_li_uppUpper uncertainty of a_listat.error;phys.abundREALprincipale_a_li_teffTeff-correlated uncertainty of a_listat.error;phys.abundREALprincipalflag_a_liQuality bitmask flag of a_limeta.code.qual,stat.fitINTEGERprincipalsami_dr1<div id="project_overview_text"><p>The SAMI Galaxy Survey is a spatially resolved spectroscopic survey of a large sample of nearby (z<0.1) galaxies, conducted with the Sydney – Australian Astronomical Observatory Multi-Object Integral Field Spectrograph (SAMI). SAMI is mounted on the 3.9 meter Anglo-Australian Telescope at Siding Spring Observatory. Survey observations began in March 2013 and were completed in May 2018. At the completion of survey observing, just over 3000 total galaxies were observed.</p><p>The key science goals of the SAMI Survey are to answer the following questions:</p><ul><li>What is the physical role of environment in galaxy evolution?</li><li>What is the relationship between stellar mass growth and angular momentum development in galaxies?</li><li>How does gas get into and out of galaxies, and how does this drive star formation?</li></ul></div>sami_dr1.InputCatalogThis is the SAMI Input Catalog for the data release 1.mag_r_band_auto-VARCHARprincipalmag_r_band_petrosian-VARCHARprincipalposition_angle_r_band-VARCHARprincipalpriority_class-VARCHARprincipalr_band_effective_radius-VARCHARprincipalredshift_flowcorrected-VARCHARprincipalredshift_heliocentric-VARCHARprincipalstellar_mass-VARCHARprincipalsurface_brightness_1r_e-VARCHARprincipalsurface_brightness_1r_e_avg-VARCHARprincipalsurface_brightness_2r_e-VARCHARprincipalabsolute_mag_r_band_auto-VARCHARprincipalbad_class-VARCHARprincipalcatalog_coordinate_dec-VARCHARindexedprincipalcatalog_coordinate_ra-VARCHARindexedprincipalcolour_auto_g_i-VARCHARprincipalellipticity_r_band-VARCHARprincipalgalactic_extinction_g_band-VARCHARprincipaliau_identifier-VARCHARprincipalid-VARCHARindexedprincipallobes_dr1The goal of LoBES is to improve the sky-catalogue used by the Murchison Widefield Array (MWA) Epoch of Reionisation (EoR) group for both data calibration and foreground source removal. This survey consists of multi-frequency observations of the main MWA EoR fields and their eight neighbouring fields using the MWA Phase II extended array. LoBES covers roughly 6000 square degrees of the Southern Sky and includes nearly 160--thousand sources. The resulting catalogue contains 16 separate spectral measurements between 100 and 230 MHz for each source, and Bayesian spectral modelling for 80% of these sources. Additionally, we include gaussian models for the structure of each source in the catalogue. The survey surpasses all previous low-frequency surveys covering the MWA EoR fields in regards to sensitivity and completeness.lobes_dr1.LoBESEoR0SrcThis table contains source positions, overall gaussian structure, and spectral information for sources located in the MWA EoR0 field (R.A. = 0 hours; Decl. = -27 degrees), or one of the four neighbouring fields.UNQ_SOURCE_IDUnique identification number associated with each source.stat.valueVARCHARprincipalNAMEUnique name for each source.meta.id.parentVARCHARindexedprincipalRARight ascension for source.degpos.eq.raVARCHARindexedprincipalERR_RAUncertainty in measured right ascension.degpos.eq.ra;stat.error.sysVARCHARprincipalDECDeclination for source.degpos.eq.decVARCHARindexedprincipalERR_DECUncertainty in measured declination.degpos.eq.dec;stat.error.sysVARCHARprincipalMAJOR_DCDeconvolved major axis of gaussian for overall source structure.degphys.angSize.smajAxisVARCHARprincipalMINOR_DCDeconvolved minor axis of gaussian for overall source structure.degphys.angSize.sminAxisVARCHARprincipalPA_DCDeconvolved position angle of gaussian for overall source structure.degpos.posAngVARCHARprincipalINT_FLX107Source integrated flux density in 107 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX107Uncertainty in source integrated flux density in 107 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX115Source integrated flux density in 115 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX115Uncertainty in source integrated flux density in 115 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX122Source integrated flux density in 122 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX122Uncertainty in source integrated flux density in 122 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX130Source integrated flux density in 130 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX130Uncertainty in source integrated flux density in 130 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX143Source integrated flux density in 143 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX143Uncertainty in source integrated flux density in 143 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX151Source integrated flux density in 151 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX151Uncertainty in source integrated flux density in 151 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX158Source integrated flux density in 158 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX158Uncertainty in source integrated flux density in 158 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX166Source integrated flux density in 166 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX166Uncertainty in source integrated flux density in 166 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX174Source integrated flux density in 174 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX174Uncertainty in source integrated flux density in 174 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX181Source integrated flux density in 181 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX181Uncertainty in source integrated flux density in 181 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX189Source integrated flux density in 189 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX189Uncertainty in source integrated flux density in 189 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX197Source integrated flux density in 197 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX197Uncertainty in source integrated flux density in 197 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX204Source integrated flux density in 204 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX204Uncertainty in source integrated flux density in 204 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX212Source integrated flux density in 212 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX212Uncertainty in source integrated flux density in 212 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX220Source integrated flux density in 220 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX220Uncertainty in source integrated flux density in 220 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX227Source integrated flux density in 227 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX227Uncertainty in source integrated flux density in 227 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalMOD_TYPEModel type that best fits the spectral measurements. 'pl' indicates power-law; 'cpl' indicates curved power-law; 'nan' no best-fit model.meta.idVARCHARprincipalNORM_PLAmplitude for power-law model (reference frequency 160 MHz).Jymeta.modelled;stat.valueVARCHARprincipalALPHA_PLSpectral-index for power-law model.meta.modelled;spec.indexVARCHARprincipalLOGZ_PLNatural log of Bayesian evidence value for power-law model.meta.modelled;stat.valueVARCHARprincipalNORM_CPLAmplitude for curved power-law model (reference frequency 160 MHz).Jymeta.modelled;stat.valueVARCHARprincipalALPHA_CPLSpectral-index for curved power-law model.meta.modelled;stat.valueVARCHARprincipalCURVE_CPLSpectral curvature value (q) for curved power-law model.meta.modelled;stat.valueVARCHARprincipalLOGZ_CPLNatural log of Bayesian evidence value for curved power-law model.meta.modelled;stat.valueVARCHARprincipallobes_dr1.LoBESEoR0CompThis table contains information about the individual gaussian components that make up the total source model for each of the sources located in the MWA EoR0 field (R.A. = 0 hours; Decl. = -27 degrees), or one of the four neighbouring fields. This includes component positions, gaussian structure, and spectral information (both modelled and measured).LOBES_FLDLoBES field the source is located within.meta.idVARCHARprincipalP_FLX107Source peak flux in 107 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX107Uncertainty in component peak flux in 107 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX107Source integrated flux density in 107 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX107Uncertainty in component integrated flux density in 107 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS107Local rms of 107 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX115Source peak flux in 115 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX115Uncertainty in component peak flux in 115 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX115Source integrated flux density in 115 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX115Uncertainty in component integrated flux density in 115 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS115Local rms of 115 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX122Source peak flux in 122 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX122Uncertainty in component peak flux in 122 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX122Source integrated flux density in 122 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX122Uncertainty in component integrated flux density in 122 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS122Local rms of 122 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX130Source peak flux in 130 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX130Uncertainty in component peak flux in 130 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX130Source integrated flux density in 130 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX130Uncertainty in component integrated flux density in 130 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS130Local rms of 130 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX143Source peak flux in 143 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX143Uncertainty in component peak flux in 143 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX143Source integrated flux density in 143 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX143Uncertainty in component integrated flux density in 143 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS143Local rms of 143 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX151Source peak flux in 151 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX151Uncertainty in component peak flux in 151 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX151Source integrated flux density in 151 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX151Uncertainty in component integrated flux density in 151 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS151Local rms of 151 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX158Source peak flux in 158 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX158Uncertainty in component peak flux in 158 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX158Source integrated flux density in 158 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX158Uncertainty in component integrated flux density in 158 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS158Local rms of 158 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX166Source peak flux in 166 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX166Uncertainty in component peak flux in 166 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalUNQ_SOURCE_IDUnique identification number associated with each source.stat.valueVARCHARprincipalNAMEUnique name for each source.meta.id.parentVARCHARprincipalRARight ascension for component.degpos.eq.raVARCHARprincipalERR_RAUncertainty in measured right ascension.degpos.eq.ra;stat.error.sysVARCHARprincipalDECDeclination for component.degpos.eq.decVARCHARprincipalERR_DECUncertainty in measured declination.degpos.eq.dec;stat.error.sysVARCHARprincipalMAJOR_DCDeconvolved major axis of gaussian component.degphys.angSize.smajAxisVARCHARprincipalMINOR_DCDeconvolved minor axis of gaussian component.degphys.angSize.sminAxisVARCHARprincipalPA_DCDeconvolved position angle of gaussian component.degpos.posAngVARCHARprincipalINT_WIDEIntegrated flux density measured in the wide-band image (central frequency of 200 MHz).Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_WIDEUncertainty in integrated flux density in wide-band image (central frequency 0f 200 MHz).Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalPEAK_WIDEPeak flux measure for the component in the wide-band image (central frequency of 200 MHz).Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_PEAK_WIDEUncertainty of the component peak flux in the wide-band image (central frequency of 200 MHz).Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS_WIDELocal rms of wide-band image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalINT_FLX166Source integrated flux density in 166 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX166Uncertainty in component integrated flux density in 166 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS166Local rms of 166 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX174Source peak flux in 174 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX174Uncertainty in component peak flux in 174 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX174Source integrated flux density in 174 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX174Uncertainty in component integrated flux density in 174 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS174Local rms of 174 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX181Source peak flux in 181 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX181Uncertainty in component peak flux in 181 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX181Source integrated flux density in 181 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX181Uncertainty in component integrated flux density in 181 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS181Local rms of 181 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX189Source peak flux in 189 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX189Uncertainty in component peak flux in 189 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX189Source integrated flux density in 189 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX189Uncertainty in component integrated flux density in 189 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS189Local rms of 189 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX197Source peak flux in 197 MHz image.Jy/beamphot.flux.density.sb;em.radio.100-200MHzVARCHARprincipalERR_P_FLX197Uncertainty in component peak flux in 197 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.100-200MHzVARCHARprincipalINT_FLX197Source integrated flux density in 197 MHz image.Jyphot.flux.density;em.radio.100-200MHzVARCHARprincipalERR_INT_FLX197Uncertainty in component integrated flux density in 197 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.100-200MHzVARCHARprincipalRMS197Local rms of 197 MHz image at the location of the component.Jy/beamstat.rms;em.radio.100-200MHzVARCHARprincipalP_FLX204Source peak flux in 204 MHz image.Jy/beamphot.flux.density.sb;em.radio.200-400MHzVARCHARprincipalERR_P_FLX204Uncertainty in component peak flux in 204 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX204Source integrated flux density in 204 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX204Uncertainty in component integrated flux density in 204 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalRMS204Local rms of 204 MHz image at the location of the component.Jy/beamstat.rms;em.radio.200-400MHzVARCHARprincipalP_FLX212Source peak flux in 212 MHz image.Jy/beamphot.flux.density.sb;em.radio.200-400MHzVARCHARprincipalERR_P_FLX212Uncertainty in component peak flux in 212 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX212Source integrated flux density in 212 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX212Uncertainty in component integrated flux density in 212 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalRMS212Local rms of 212 MHz image at the location of the component.Jy/beamstat.rms;em.radio.200-400MHzVARCHARprincipalP_FLX220Source peak flux in 220 MHz image.Jy/beamphot.flux.density.sb;em.radio.200-400MHzVARCHARprincipalERR_P_FLX220Uncertainty in component peak flux in 220 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX220Source integrated flux density in 220 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX220Uncertainty in component integrated flux density in 220 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalRMS220Local rms of 220 MHz image at the location of the component.Jy/beamstat.rms;em.radio.200-400MHzVARCHARprincipalP_FLX227Source peak flux in 227 MHz image.Jy/beamphot.flux.density.sb;em.radio.200-400MHzVARCHARprincipalERR_P_FLX227Uncertainty in component peak flux in 227 MHz image.Jy/beamphot.flux.density.sb;stat.error.sys;em.radio.200-400MHzVARCHARprincipalINT_FLX227Source integrated flux density in 227 MHz image.Jyphot.flux.density;em.radio.200-400MHzVARCHARprincipalERR_INT_FLX227Uncertainty in component integrated flux density in 227 MHz image.Jyphot.flux.density;stat.error.sys;em.radio.200-400MHzVARCHARprincipalRMS227Local rms of 227 MHz image at the location of the component.Jy/beamstat.rms;em.radio.200-400MHzVARCHARprincipalMOD_TYPEModel type that best fits the spectral measurements. 'pl' indicates power-law; 'cpl' indicates curved power-law; 'nan' no best-fit model.meta.idVARCHARprincipalNORM_PLAmplitude for power-law model (reference frequency 160 MHz).Jymeta.modelled;stat.valueVARCHARprincipalALPHA_PLSpectral-index for power-law model.meta.modelled;spec.indexVARCHARprincipalLOGZ_PLNatural log of Bayesian evidence value for power-law model.meta.modelled;stat.valueVARCHARprincipalNORM_CPLAmplitude for curved power-law model (reference frequency 160 MHz).Jymeta.modelled;stat.valueVARCHARprincipalALPHA_CPLSpectral-index for curved power-law model.meta.modelled;stat.valueVARCHARprincipalCURVE_CPLSpectral curvature value (q) for curved power-law model.meta.modelled;stat.valueVARCHARprincipalLOGZ_CPLNatural log of Bayesian evidence value for curved power-law model.meta.modelled;stat.valueVARCHARprincipals5_dr1The Southern Stellar Stream Spectroscopic Survey (S⁵) is a spectroscopic survey of stars in the stellar streams of the Southern sky, with the aim of mapping their kinematics and chemistry. The streams represent material tidally striped from dwarf galaxies and globular clusters, and are essential dynamical probes of the dark matter distribution of the Milky Way, as well as providing a detailed snapshot of its accretion history.s5_dr1.s5This table contains all columns from S5 DR1vel1Radial velocity (RV) statistics from rvspecfit. 1th percentile of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel99Radial velocity (RV) statistics from rvspecfit. 99th percentile of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel50Radial velocity (RV) statistics from rvspecfit. 50th percentile (median) of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel16Radial velocity (RV) statistics from rvspecfit. 16th percentile of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel84Radial velocity (RV) statistics from rvspecfit. 84th percentile of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel_stdRadial velocity (RV) statistics from rvspecfit. Standard deviation of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel_skewRadial velocity (RV) statistics from rvspecfit. Skewness of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel_kurtRadial velocity (RV) statistics from rvspecfit. Kurtosis of the RV posterior distributionkmsspect.dopplerVeloc;meta.modelledVARCHARprincipalfeh1Metallicity ([Fe/H]) measurement from rvspecfit. 1th percentile of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh99Metallicity ([Fe/H]) measurement from rvspecfit. 99th percentile of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh50Metallicity ([Fe/H]) measurement from rvspecfit. 50th percentile (median) of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh16Metallicity ([Fe/H]) measurement from rvspecfit. 16th percentile of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh84Metallicity ([Fe/H]) measurement from rvspecfit. 84th percentile of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh_stdMetallicity ([Fe/H]) measurement from rvspecfit. Standard deviation of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh_skewMetallicity ([Fe/H]) measurement from rvspecfit. Skewness of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipalfeh_kurtMetallicity ([Fe/H]) measurement from rvspecfit. Kurtosis of the posterior distribution.dexphys.abund.Z;meta.modelledVARCHARprincipallogg1Surface gravity (logg) measurement from rvspecfit. 1th percentile of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg99Surface gravity (logg) measurement from rvspecfit. 99th percentile of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg50Surface gravity (logg) measurement from rvspecfit. 50th percentile (median) of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg16Surface gravity (logg) measurement from rvspecfit. 16th percentile of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg84Surface gravity (logg) measurement from rvspecfit. 84th percentile of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg_stdSurface gravity (logg) measurement from rvspecfit. Standard deviation of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg_skewSurface gravity (logg) measurement from rvspecfit. Skewness of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipallogg_kurtSurface gravity (logg) measurement from rvspecfit. Kurtosis of the posterior distribution.dexphys.gravity;meta.modelledVARCHARprincipalteff1Effective temperature statistics from rvspecfit. 1th percentile of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff99Effective temperature statistics from rvspecfit. 99th percentile of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff50Effective temperature statistics from rvspecfit. 50th percentile (median) of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff16Effective temperature statistics from rvspecfit. 16th percentile of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff84Effective temperature statistics from rvspecfit. 84th percentile of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff_stdEffective temperature statistics from rvspecfit. Standard deviation of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff_skewEffective temperature statistics from rvspecfit. Skewness of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalteff_kurtEffective temperature statistics from rvspecfit. Kurtosis of the posterior distribution.Kphys.temperature.effective;meta.modelledVARCHARprincipalvel_calibRadial velocity calibrated to have no zeropoint offset. Offset is determined by cross-matching with APOGEE data. See details in Section 4.1 of Li et al. (2019).kmsspect.dopplerVeloc;meta.modelledVARCHARprincipalvel_calib_stdCalibrated radial velocity uncertainty using repeated observations.kmsspect.dopplerVeloc;stat.error;meta.modelledVARCHARprincipalfeh_calib_stdCalibrated [Fe/H] uncertainty using repeated observations.dexphys.abund.Z;stat.error;meta.modelledVARCHARprincipalredchisq_1700dReduced chi square from the best fit template model from rvspecfitstat.fit.chi2;meta.modelledVARCHARprincipalchisq_1700dChi square from the best fit template model from rvspecfitstat.fit.chi2;meta.modelledVARCHARprincipalabsdev_1700dMedian absolute deviation from the best fit template model from rvspecfit, defined as Median(Data-Model)/Median(Model)arith.diff;stat.median;meta.modelledVARCHARprincipalraRight ascension of the objectdegpos.eq.ra;meta.mainVARCHARindexedprincipaldecDeclination of the objectdegpos.eq.dec;meta.mainVARCHARindexedprincipalnameObject name used for AAT observation. For stellar targets, name is usually source_id from Gaia DR2, for galaxy targets (S5-lowz), the name is usually object_id from DES DR1. Some observations prior S5 were also included and for those, names could follow different conventions.meta.idVARCHARprincipalfieldName of the stream fields, corresponding to field name in Table 2 of Li et al. (2019)meta.idVARCHARprincipalfileinfoFilename of the reduced AAT spectra from each field.meta.fileVARCHARprincipalutmjdUTMJD of the observationtime.epochVARCHARprincipalsn_1700dMedian Signal-to-Noise ratio of the 1700d spectra. For DR1, we decide to only release objects with sn_1700d > 3 to ensure the high quality of this dataset.stat.snr;stat.medianVARCHARprincipalmoon_distMoon distancedegpos.distanceVARCHARprincipalmoon_phaseMoon phase in percents (0-100 fraction of surface illumination). 0% corresponds to new moon and 100% corresponds to full moontime.phaseVARCHARprincipalmoon_altMoon altitudedegpos.bodyrc.altVARCHARprincipalqso_flag_wise0 or 1. 1 = Likely QSO objects based on WISE photometry. 0 = not a QSO See details in Section 4.4 of Li et al. (2019)meta.code.classVARCHARprincipalpriorityInitial target selection priorities. Integer 1 to 9 is used. 9 is highest and 1 is lowest. 7-9 are stream targets; 3-6 are halo star targets; 1-2 are galaxy targets and therefore the parameters derived here with rvspecfit should not be used. For details, please refer to Section 2 of Li et al. (2019).meta.codeVARCHARprincipalprimaryFor some objects, multiple observations were taken. Primary = True if this is the observation with the highest S/N. For objects that only one observation was taken, Primary is always True. This column is useful if you want to get only one measurement per target to remove duplicates.meta.code.statusVARCHARprincipalgood_star_pbGood star probability based on random forest trained on the following parameters as features: chi-squared values of the fit, radial velocity error, radial velocity posterior skewness and kurtosis, effective temperature, median signal to noise in the spectrum and median absolute deviation from the best fit template model. See details in Section 4.5 of Li et al. (2019).meta.code.qual;stat.probabilityVARCHARprincipalgood_starA flag to select stellar spectra with good fitting quality. good_star = 0 if it meets one of the 3 following criteria: 1. good_star_pb < 0.5 2. priority < = 2 3. qso_flag_wise == 1. It is recommended to only use the stellar parameters and radial velocities for object with good_star = 1. See details in Section 4.5 of Li et al. (2019). For DR1, we decide to only release objects with good_star = 1 to ensure the high quality of this dataset.meta.code.qualVARCHARprincipalebvE(B-V) from Schlegel et al (1998).magphot.color;arith.diffVARCHARprincipalgaia_source_idGaia source id from Gaia eDR3meta.idVARCHARprincipalparallaxparallax Measurement from Gaia eDR3maspos.parallax.photVARCHARprincipalparallax_errorparallax_error Measurement from Gaia eDR3maspos.parallax.phot;stat.errorVARCHARprincipalpmrapmra Measurement from Gaia eDR3masyrpos.eq.raVARCHARprincipalpmdecpmdec Measurement from Gaia eDR3masyrpos.eq.decVARCHARprincipalpmra_errorpmra_error Measurement from Gaia eDR3masyrpos.eq.raVARCHARprincipalpmdec_errorpmdec_error Measurement from Gaia eDR3masyrpos.eq.raVARCHARprincipalphot_g_mean_magphot_g_mean_mag Measurement from Gaia eDR3magphot.magVARCHARprincipalphot_bp_mean_magphot_bp_mean_mag Measurement from Gaia eDR3magphot.magVARCHARprincipalphot_rp_mean_magphot_rp_mean_mag Measurement from Gaia eDR3magphot.magVARCHARprincipalphot_bp_rp_excess_factorphot_bp_rp_excess_factor Measurement from Gaia eDR3phot.magVARCHARprincipaldecam_gDECam photometry in g (without reddening correction) from DES DR1, DECaLS DR9 or NSC DR2. If the object is in multiple catalogs, then DES is first considered, then DECaLS and finally NSC. See decam_phot_src_bits for the source of the photometrymagphot.magVARCHARprincipaldecam_rDECam photometry in r (without reddening correction) from DES DR1, DECaLS DR9 or NSC DR2. If the object is in multiple catalogs, then DES is first considered, then DECaLS and finally NSC. See decam_phot_src_bits for the source of the photometrymagphot.magVARCHARprincipaldecam_iDECam photometry in i (without reddening correction) from DES DR1, DECaLS DR9 or NSC DR2. If the object is in multiple catalogs, then DES is first considered, then DECaLS and finally NSC. See decam_phot_src_bits for the source of the photometrymagphot.magVARCHARprincipaldecam_zDECam photometry in z (without reddening correction) from DES DR1, DECaLS DR9 or NSC DR2. If the object is in multiple catalogs, then DES is first considered, then DECaLS and finally NSC. See decam_phot_src_bits for the source of the photometrymagphot.magVARCHARprincipaldecam_phot_src_bitsThe source of the decam photometry. It is a 12 bit integer ABC DEF GHI JKL where ABC bits describe the source of g photometry, DEF bits the source of r photometry, etc. The value of 1 corresponds to DES DR2, 2 to DECALS, 3 to NSC. For example, decam_phot_src_bits = 585 corresponds to 001001001001, which means that griz photometry all comes from DES DR2; decam_phot_src_bits = 83 corresponds to 000 001 010 011, which means that the griz photometry comes from NONE, DES, DECALS, NSC.meta.codeVARCHARprincipalflux_w1unWISE flux in filter w1 from Schlafly+2019 fluxes in vega nano-maggies, i.e. to convert into mags one need to do 22.5-2.5*log_10(f)phot.fluxVARCHARprincipalflux_w2unWISE flux in filter w2 from Schlafly+2019 fluxes in vega nano-maggies, i.e. to convert into mags one need to do 22.5-2.5*log_10(f)phot.fluxVARCHARprincipaldflux_w1unWISE flux uncertainty in filter w1 from Schlafly+2019 fluxes in vega nano-maggiesphot.flux;stat.errorVARCHARprincipaldflux_w2unWISE flux uncertainty in filter w2 from Schlafly+2019 fluxes in vega nano-maggiesphot.flux;stat.errorVARCHARprincipalu_skmSkymapper DR2 photometry; u bandmagphot.magVARCHARprincipalg_skmSkymapper DR2 photometry; g bandmagphot.magVARCHARprincipalr_skmSkymapper DR2 photometry; r bandmagphot.magVARCHARprincipali_skmSkymapper DR2 photometry; i bandmagphot.magVARCHARprincipalz_skmSkymapper DR2 photometry; z bandmagphot.magVARCHARprincipalstarhorse_dist05Starhorse distances at 5th percentile from Queiroz et al+2018kpcpos.distance;meta.modelledVARCHARprincipalstarhorse_dist16Starhorse distances at 16th percentile from Queiroz et al+2018kpcpos.distance;meta.modelledVARCHARprincipalstarhorse_dist50Starhorse distances at 50th percentile from Queiroz et al+2018kpcpos.distance;meta.modelledVARCHARprincipalstarhorse_dist84Starhorse distances at 84th percentile from Queiroz et al+2018kpcpos.distance;meta.modelledVARCHARprincipalstarhorse_dist95Starhorse distances at 95th percentile from Queiroz et al+2018kpcpos.distance;meta.modelledVARCHARprincipaldc_idUnique ID for S5 DR1 (generated by Data Centralmeta.id;meta.mainVARCHARindexedprincipalozdes_dr2Over six observing seasons, OzDES used the 2dF fibre positioner and AAOmega spectrograph on the 3.9-metre Anglo-Australian Telescope to monitor 771 AGN, classify hundreds of transients, and obtain redshifts for thousands of galaxies within the 10 deep fields of the Dark Energy Survey. OzDES is a survey that samples the time domain, and some targets have been observed dozens of times. In addition to the co-added spectra and redshifts, the second data release contains the individual spectra that went into the coadds. In total, there are over 300,000 spectra and 30,000 redshfts. The second data release supercedes the first data release, which contained 15,000 redshifts. For more detailed information on OzDES click on the doc and website tabs above.ozdes_dr2.RedshiftCatalogueRedshifts of objects within the 10 deep fields of the Dark Energy Survey. Column names and descriptions are below. Only quality 3, 4, and 6 redshifts should be used for science.OzDES_IDOzDES IDmeta.id;meta.mainVARCHARindexedprincipalAlpha_J2000Right ascension (Equinox J2000)degpos.eq.ra;meta.mainREALindexedprincipalDelta_J2000Declination (Equinox J2000)degpos.eq.dec;meta.mainREALindexedprincipalrmagAB magnitude in a 2 arc second aperturephot.magREALprincipalObject_typesObject types separated by commasmeta.code.classVARCHARprincipalzredshiftsrc.redshiftREALprincipalqopredshift quality flagmeta.code.qualINTEGERprincipalTransient_typeTransient type (e.g. SN Ia, SN II). Set to None if not applicablemeta.code.classVARCHARprincipalCommentCommentmeta.noteVARCHARprincipalozdes_dr1Over six observing seasons, OzDES used the 2dF fibre positioner and AAOmega spectrograph on the 3.9-metre Anglo-Australian Telescope to monitor 771 AGN, classify hundreds of transients, and obtain redshifts for thousands of galaxies within the 10 deep fields of the Dark Energy Survey. OzDES is a survey that samples the time domain, and some targets have been observed dozens of times. In addition to the co-added spectra and redshifts, the second data release contains the individual spectra that went into the coadds. In total, there are over 300,000 spectra and 30,000 redshfts. The second data release supercedes the first data release, which contained 15,000 redshifts. For more detailed information on OzDES click on the doc and website tabs above.ozdes_dr1.CatalogueRedshifts of objects within the 10 deep fields of the Dark Energy SurveyDECDeclination (Equinox J2000)degpos.eq.dec;meta.mainREALindexedprincipalOzDES_IDOzDES IDmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (Equinox J2000)degpos.eq.ra;meta.mainREALindexedprincipalflagredshift quality flagmeta.code.classVARCHARprincipaltypesMain object typemeta.code.classVARCHARprincipalzredshiftsrc.redshiftREALprincipalgalahtess_dr1The GALAH-TESS catalog contains 47,000+ stars that have been observed by both the second data release of GALAH, GALAH DR2, and/will be observed by NASA's planet-finding mission, TESS. This catalog contains the physical, chemical and dervied parameters for these stars, assisting in the characterisation of the exoplanets they might host. It includes, but is not limited to, the stellar mass, radius, age, habitable zones, effective temperature, surface gravity, elemental abundances and molar ratios for these selected stars. More information about the catalog can be found here: https://doi.org/10.1093/mnras/stab1052galahtess_dr1.galahtessThis is the table containing the GALAH-TESS catalogGAIADR2GAIA DR2 Identifiermeta.idBIGINTprincipalpriorityTIC DR8 Priorityphot.flux.density;em.IR.8-15umREALprincipalraGAIA DR2 Right Ascension (RA)degpos.eq.ra;meta.mainREALindexedprincipale_raGAIA DR2 Right Ascension (RA) Errordegstat.error;pos.eq.raREALprincipaldecGAIA DR2 Declination (Dec)degpos.eq.dec;meta.mainREALindexedprincipale_decGAIA DR2 Declination (Dec) Errordegstat.error;pos.eq.decREALprincipalteffGALAH DR2 Effective Temperature (Teff)Kphys.temperature.effectiveINTEGERprincipale_teffGALAH DR2 Effective Temperature (Teff) ErrorKstat.error;phys.temperature.effectiveINTEGERprincipalloggGALAH DR2 Surface Gravity (logg)cgsphys.gravityREALprincipale_loggGALAH DR2 Surface Gravity (logg) Errorcgsstat.error;phys.gravityREALprincipalm_hOverall Metalicity ([M/H])dexphys.abund.ZREALprincipale_mhOverall Metalicity ([M/H]) Errordexstat.error;phys.abund.ZREALprincipalalpha_feAlpha Abundance ([alpha/Fe])dexphys.abundREALprincipale_alpha_feAlpha Abundance ([alpha/Fe]) Errordexstat.error;phys.abundREALprincipalVmagTIC DR8 Vmagmagphot.mag;em.opt.VREALprincipale_VmagTIC DR8 Vmag Errormagstat.error;phot.mag;em.opt.VREALprincipalTmagTIC DR8 Tmagmagphot.mag;em.optREALprincipale_TmagTIC DR8 Tmag Errormagstat.error;phot.mag;em.optREALprincipalJmag2MASS Jmagmagphot.mag;em.IR.JREALprincipale_Jmag2MASS Jmag Errormagstat.error;phot.mag;em.IR.JREALprincipalHmag2MASS Hmagmagphot.mag;em.IR.HREALprincipale_Hmag2MASS Hmag Errormagstat.error;phot.mag;em.IR.HREALprincipalKmag2MASS Kmagmagphot.mag;em.IR.KREALprincipale_Kmag2MASS Kmag Errormagstat.error;phot.mag;em.IR.KREALprincipalGmagGAIA DR2 Gmagmagphot.mag;em.opt.GREALprincipale_GmagGAIA DR2 Gmag Errormagstat.error;phot.mag;em.opt.GREALprincipalGRPmagGAIA DR2 GRPmagmagphot.mag;em.opt.RREALprincipale_GRPmagGAIA DR2 GRPmag Errormagstat.error;phot.mag;em.opt.RREALprincipalGBPmagGAIA DR2 GBPmagmagphot.mag;em.opt.BREALprincipale_GBPmagGAIA DR2 GBPmag Errormagstat.error;phot.mag;em.opt.BREALprincipalplxGAIA DR2 Parallaxmaspos.parallaxREALprincipale_plxGAIA DR2 Parallax Errormasstat.error;pos.parallaxREALprincipaldistTIC DR8 Distancepcpos.distanceREALprincipale_distTIC DR8 Distance Errorpcstat.error;pos.distanceREALprincipalradiusStellar RadiusRsunphys.size.radiusREALprincipale_radiusStellar Radius ErrorRsunstat.error;phys.size.radiusREALprincipalmassStellar MassMsunphys.massREALprincipale_massStellar Mass ErrorMsunstat.error;phys.massREALprincipalrhoStellar Densitygcm-3phys.densityREALprincipale_rhoStellar Density Errorgcm-3stat.error;phys.densityREALprincipallumStellar LuminosityLsunphys.luminosityREALprincipale_lumStellar Luminosity ErrorLsunstat.error;phys.luminosityREALprincipalageStellar AgeGyrtime.ageREALprincipale_ageStellar Age ErrorGyrstat.error;time.ageREALprincipaleepMIST Equivalent Evolutionary Phase (EEP)arithINTEGERprincipale_eepMIST Equivalent Evolutionary Phase (EEP) Errorstat.error;arithINTEGERprincipalrvGALAH DR2 Radial Velocitykms-1spect.dopplerVeloc.optREALprincipalTIC_IDTIC Identifiermeta.id;meta.mainINTEGERindexedprincipalTWOMASS2MASS Identifiermeta.idVARCHARprincipale_rvGALAH DR2 Radial Velocity Errorkms-1stat.error;spect.dopplerVeloc.optREALprincipalvsiniGALAH DR2 Rotational Velocity (vsini)kms-1phys.veloc.rotatREALprincipale_vsiniGALAH DR2 Rotational Velocity (vsini) Errorkms-1stat.error;phys.veloc.rotatREALprincipalvmicGALAH DR2 Microturbulence Velocity (vmic)kms-1phys.veloc.microTurbREALprincipale_vmicGALAH DR2 Microturbulence Velocity (vmic) Errorkms-1stat.error;phys.veloc.microTurbREALprincipalhzRecVenRecent Venus Habitable Zoneaupos.distance;src.orbitalREALprincipalhzRunGrnRunaway Greenhouse Habitable Zoneaupos.distance;src.orbitalREALprincipalhzMoiGrnMoist Greenhouse Habitable Zoneaupos.distance;src.orbitalREALprincipalhzMaxGrnMaximum Greenhouse Habitable Zoneaupos.distance;src.orbitalREALprincipalhzEarMarEarly Mars Habitable Zoneaupos.distance;src.orbitalREALprincipalli_hLithium Abundance ([Li/H])dexphys.abundREALprincipale_li_hLithium Abundance ([Li/H]) Errordexstat.error;phys.abundREALprincipalc_hCarbon Abundance ([C/H])dexphys.abundREALprincipale_c_hCarbon Abundance ([C/H]) Errordexstat.error;phys.abundREALprincipalo_hOxygen Abundance ([O/H])dexphys.abundREALprincipale_o_hOxygen Abundance ([O/H]) Errordexstat.error;phys.abundREALprincipalna_hSodium Abundance ([Na/H])dexphys.abundREALprincipale_na_hSodium Abundance ([Na/H]) Errordexstat.error;phys.abundREALprincipalmg_hMagnesium Abundance ([Mg/H])dexphys.abundREALprincipale_mg_hMagnesium Abundance ([Mg/H]) Errordexstat.error;phys.abundREALprincipalal_hAluminum Abundance ([Al/H])dexphys.abundREALprincipale_al_hAluminum Abundance ([Al/H]) Errordexstat.error;phys.abundREALprincipalsi_hSilicon Abundance ([Si/H])dexphys.abundREALprincipale_si_hSilicon Abundance ([Si/H]) Errordexstat.error;phys.abundREALprincipalk_hPotassium Abundance ([K/H])dexphys.abundREALprincipale_k_hPotassium Abundance ([K/H]) Errordexstat.error;phys.abundREALprincipalca_hCalcium Abundance ([Ca/H])dexphys.abundREALprincipale_ca_hCalcium Abundance ([Ca/H]) Errordexstat.error;phys.abundREALprincipalsc_hScandium Abundance ([Sc/H])dexphys.abundREALprincipale_sc_hScandium Abundance ([Sc/H]) Errordexstat.error;phys.abundREALprincipalti_hTitanium Abundance ([Ti/H])dexphys.abundREALprincipale_ti_hTitanium Abundance ([Ti/H]) Errordexstat.error;phys.abundREALprincipalv_hVanadium Abundance ([V/H])dexphys.abundREALprincipale_v_hVanadium Abundance ([V/H]) Errordexstat.error;phys.abundREALprincipalcr_hChromium Abundance ([Cr/H])dexphys.abundREALprincipale_cr_hChromium Abundance ([Cr/H]) Errordexstat.error;phys.abundREALprincipalmn_hManganese Abundance ([Mn/H])dexphys.abundREALprincipale_mn_hManganese Abundance ([Mn/H]) Errordexstat.error;phys.abundREALprincipalfe_hIron Abundance ([Fe/H])dexphys.abund;phys.abund.FeREALprincipale_fe_hIron Abundance ([Fe/H]) Errordexstat.error;phys.abund.Fe;phys.abundREALprincipalco_hCobalt Abundance ([Co/H])dexphys.abundREALprincipale_co_hCobalt Abundance ([Co/H]) Errordexstat.error;phys.abundREALprincipalni_hNickel Abundance ([Ni/H])dexphys.abundREALprincipale_ni_hNickel Abundance ([Ni/H]) Errordexstat.error;phys.abundREALprincipalcu_hCopper Abundance ([Cu/H])dexphys.abundREALprincipale_cu_hCopper Abundance ([Cu/H]) Errordexstat.error;phys.abundREALprincipalzn_hZinc Abundance ([Zn/H])dexphys.abundREALprincipale_zn_hZinc Abundance ([Zn/H]) Errordexstat.error;phys.abundREALprincipaly_hYttrium Abundance ([Y/H])dexphys.abundREALprincipale_y_hYttrium Abundance ([Y/H]) Errordexstat.error;phys.abundREALprincipalba_hBarium Abundance ([Ba/H])dexphys.abundREALprincipale_ba_hBarium Abundance ([Ba/H]) Errordexstat.error;phys.abundREALprincipalla_hLanthanum Abundance ([La/H])dexphys.abundREALprincipale_la_hLanthanum Abundance ([La/H]) Errordexstat.error;phys.abundREALprincipaleu_hEuropium Abundance ([Eu/H])dexarith.ratio;phys.abundREALprincipale_eu_hEuropium Abundance ([Eu/H]) Errordexstat.error;arith.ratio;phys.abundREALprincipalc_oStellar C/O Molar Ratioarith.ratio;phys.abundREALprincipale_c_oStellar C/O Molar Ratiostat.error;arith.ratio;phys.abundREALprincipalmg_siStellar Mg/Si Molar Ratioarith.ratio;phys.abundREALprincipale_mg_siStellar Mg/Si Molar Ratiostat.error;arith.ratio;phys.abundREALprincipalfe_mgStellar Fe/Mg Molar Ratioarith.ratio;phys.abundREALprincipale_fe_mgStellar Fe/Mg Molar Ratiostat.error;arith.ratio;phys.abundREALprincipalfe_siStellar Fe/Si Molar Ratioarith.ratio;phys.abundREALprincipale_fe_siStellar Fe/Si Molar Ratiostat.error;arith.ratio;phys.abundREALprincipalgama_pdr4v2<p>GAMA is a project to exploit the latest generation of ground-based and space-borne survey facilities to study cosmology and galaxy formation and evolution. </p> <p>At the heart of this project lies the GAMA spectroscopic survey of ~300,000 galaxies down to r&nbsp;&lt;&nbsp;19.8&nbsp;mag over ~286&nbsp;deg<sup>2</sup>, carried out using the <a href="http://www.aao.gov.au/AAO/2df/aaomega/aaomega.html">AAOmega</a> multi-object spectrograph on the <a href="http://www.aao.gov.au/">Anglo-Australian Telescope (AAT)</a> by the GAMA team</a>. This project was awarded 210 nights over 7 years (2008–2014) and the observations are now completed. This survey builds on, and is augmented by, previous spectroscopic surveys such as the <a href="http://www.sdss.org/">Sloan Digital Sky Survey (SDSS)</a>, the <a href="http://www.mso.anu.edu.au/2dFGRS/">2dF Galaxy Redshift Survey(2dFGRS)</a> and the <a href="http://www.eso.org/~jliske/mgc/">Millennium Galaxy Catalogue (MGC)</a>.</p>gama_pdr4v2.AATRunzResultsv27All spectra collected for GAMA at the AAT were redshifted using thecode runz. This table contains the complete redshifting results.Note that many spectra were redshifted more than once and thiscatalogue contains all duplications.Z_FINFinal selected redshiftsrc.redshiftVARCHARprincipalRUNZRESIDID of runz outputmeta.id;meta.mainVARCHARindexedprincipalSPECIDID of GAMA AAT spectrummeta.id;spectVARCHARprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalUSERRedshiftermeta.idVARCHARprincipalDATE_ZDate of runz runtime.processingVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalOBJECTObject nameVARCHARprincipalRAHRA hours of spectrum (J2000)hVARCHARprincipalRAMRA minutesmVARCHARprincipalRASRA secondssVARCHARprincipalDECDDEC degree of spectrum (J2000)degVARCHARprincipalDECMDEC minutesmVARCHARprincipalDECSDEC secondssVARCHARprincipalRMAGExtinction corrected SDSS r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalNEBNumber of matching emission lines at best emission line redshiftmeta.numberVARCHARprincipalNEGTotal number of detected potential emission linesmeta.numberVARCHARprincipalZEMEmission line redshiftsrc.redshiftVARCHARprincipalZEM_ERREmission line redshift errorstat.error;src.redshiftVARCHARprincipalQEMEmission line redshift qualitymeta.code.qual;src.redshiftVARCHARprincipalTEMPCross-correlation templateVARCHARprincipalXCORCross-correlation peak heightVARCHARprincipalZXCross-correlation redshiftsrc.redshiftVARCHARprincipalZX_ERRCross-correlation redshift errorstat.error;src.redshiftVARCHARprincipalQXCross-correlation redshift qualitymeta.code.qual;src.redshiftVARCHARprincipalZ_FIN_ERRError of final selected redshiftstat.error;src.redshiftVARCHARprincipalQAAutomatic quality of final selected redshiftmeta.code.qual;src.redshiftVARCHARprincipalQOPUser assigned quality of final selected redshiftmeta.code.qual;src.redshiftVARCHARprincipalFFlag indicating whether Z_FIN is different from automatic redshifts: 0 = equal to best auto redshift; 1 = not equal to best auto redshift; 2 = not equal to either auto redshiftsmeta.codeVARCHARprincipalFLDUnusedVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalCCDCCD numbermeta.id;instrVARCHARprincipalPLATEPlate numbermeta.id;instrVARCHARprincipalX_POSNFibre x position on plateVARCHARprincipalY_POSNFibre y position on plateVARCHARprincipalS_NS/N of spectrumstat.snrVARCHARprincipalSPMAGUnusedmagVARCHARprincipalVSPApproximate V-band fibre mag with zeropoint 32magVARCHARprincipalRSPApproximate R-band fibre mag with zeropoint 32.3magVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCOMMENT_FLAGFlag encoding the user commentmeta.codeVARCHARprincipalCOMMENTFree format user comment on this spectrummeta.noteVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.AATSpecAllv27This is a table of all GAMA AAT spectra. Many targets were observedmore than once by GAMA, and these duplications are retained here.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalZ_RUNZHeliocentric redshift as determined by runz (incl re-redshifting)src.redshiftVARCHARprincipalNQ_RUNZNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROB_RUNZProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalCOMBIDCombined spectrum this spectrum contributes tometa.idVARCHARprincipalCOMBNOFirst, second or third spectrum in the combination?meta.idVARCHARprincipalZ_COMBHeliocentric redshift of the combined spectrumsrc.redshiftVARCHARprincipalNQ_COMBNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROB_COMBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalS_NS/N of spectrumstat.snrVARCHARprincipalWARNING_FLAGWarnings raised for this spectrummeta.code.qualVARCHARprincipalCOMMENTS_FLAGFlag encoding all user comments on this spectrummeta.codeVARCHARprincipalPLATEPlate numbermeta.id;instrVARCHARprincipalX_POSNFibre x position on platepos.cartesian.x;instrVARCHARprincipalY_POSNFibre y position on platepos.cartesian.y;instrVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTGAMA AAT spectrum with best redshift for this object?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.AATSpecAllzAllv27Many GAMA AAT spectra were redshifted more than once using the coderunz. This table contains one line per spectrum summarising all ofthe redshifting results for this spectrum, as well as listing theresults of the analysis to determine the best redshift based on thereliabilities of the redshifters.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalN_OPNumber of opinions for this spectrummeta.numberVARCHARprincipalN_OPQGNumber of opinions with Q >= 2meta.numberVARCHARprincipalN_OPQBNumber of opinions with Q < 2meta.numberVARCHARprincipalN_ZNumber of different redshiftsmeta.numberVARCHARprincipalBEST_PROBProbability that the most probable possibility is correctstat.probability;src.redshiftVARCHARprincipalBEST_ZRedshift of the most probable possibilitysrc.redshiftVARCHARprincipalBEST_Z_NQNormalised Q of the most probable possibilitymeta.code.qual;src.redshiftVARCHARprincipalBEST_Z_NNumber of opinions supporting the most probable possibilitymeta.numberVARCHARprincipalBEST_Z_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q1Number of supporting Q=1 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q0Number of supporting Q=0 opinionsmeta.numberVARCHARprincipalZ1_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ1_ZPossible redshiftsrc.redshiftVARCHARprincipalZ1_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ1_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ1_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ1_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ1_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ2_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ2_ZPossible redshiftsrc.redshiftVARCHARprincipalZ2_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ2_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ2_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ2_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ2_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ3_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ3_ZPossible redshiftsrc.redshiftVARCHARprincipalZ3_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ3_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ3_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ3_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ3_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ4_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ4_ZPossible redshiftsrc.redshiftVARCHARprincipalZ4_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ4_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ4_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ4_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ4_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ5_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ5_ZPossible redshiftsrc.redshiftVARCHARprincipalZ5_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ5_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ5_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ5_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ5_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalBEST_IDXIndex of best possibility in the above listVARCHARprincipalQ1_PROBProbability that no redshift can be found (i.e. that Q=1 is correct)stat.probabilityVARCHARprincipalQ1_N_Q1Number of supporting Q=1 opinionsmeta.numberVARCHARprincipalQ1_N_Q0Number of supporting Q=0 opinionsmeta.numberVARCHARprincipalCOMP_PROBProbability that none of the offered possibilities are correctstat.probabilityVARCHARprincipalCOMMENTS_FLAGFlag encoding all user comments on this spectrummeta.codeVARCHARprincipalOP1_RUNZRESIDID of original runz result in AATRunzResultsmeta.idVARCHARprincipalOP1_RSOriginal redshiftermeta.idVARCHARprincipalOP1_QOriginal Qmeta.code.qual;src.redshiftVARCHARprincipalOP1_ZOriginal redshiftsrc.redshiftVARCHARprincipalOP1_CFFlag encoding original user comment on this spectrummeta.codeVARCHARprincipalOP1_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP2_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP2_RSRedshiftermeta.idVARCHARprincipalOP2_QQmeta.code.qual;src.redshiftVARCHARprincipalOP2_ZRedshiftsrc.redshiftVARCHARprincipalOP2_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP2_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP3_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP3_RSRedshiftermeta.idVARCHARprincipalOP3_QQmeta.code.qual;src.redshiftVARCHARprincipalOP3_ZRedshiftsrc.redshiftVARCHARprincipalOP3_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP3_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP4_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP4_RSRedshiftermeta.idVARCHARprincipalOP4_QQmeta.code.qual;src.redshiftVARCHARprincipalOP4_ZRedshiftsrc.redshiftVARCHARprincipalOP4_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP4_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP5_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP5_RSRedshiftermeta.idVARCHARprincipalOP5_QQmeta.code.qual;src.redshiftVARCHARprincipalOP5_ZRedshiftsrc.redshiftVARCHARprincipalOP5_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP5_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP6_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP6_RSRedshiftermeta.idVARCHARprincipalOP6_QQmeta.code.qual;src.redshiftVARCHARprincipalOP6_ZRedshiftsrc.redshiftVARCHARprincipalOP6_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP6_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP7_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP7_RSRedshiftermeta.idVARCHARprincipalOP7_QQmeta.code.qual;src.redshiftVARCHARprincipalOP7_ZRedshiftsrc.redshiftVARCHARprincipalOP7_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP7_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.AATSpecAutozAllv27This table provides a fully automated redshift estimate for eachGAMA AAT spectrum. These redshifts are completely independent fromthe ones derived by runz, and are considered more reliable.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.idVARCHARprincipalCOUNT_BADPIXELNumber of bad pixels masked in spectrummeta.numberVARCHARprincipalCOUNT_HIGHVALNumber of high values in the high-passed spectrummeta.numberVARCHARprincipalCOUNT_LOWVALNumber of low values in the high-passed spectrummeta.numberVARCHARprincipalRMS_MAD_RATIORMS divided by mean absolute deviation for the HP spectrumstat.valueVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalCC_SIGMACross-correlation peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATETemplate ID; 0-22 for stars, 40-47 for galaxiesmeta.idVARCHARprincipalZ2Heliocentric redshift of second peaksrc.redshiftVARCHARprincipalCC_SIGMA2Cross-correlation 2nd peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATE2Template ID for second peakmeta.idVARCHARprincipalCC_SIGMA3Cross-correlation 3rd peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA4Cross-correlation 4th peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA1TO234Peak value divided by RMS of 2nd-4th peak valuesstat.valueVARCHARprincipalCC_FOMFigure of merit for primary redshift confidencestat.valueVARCHARprincipalPROBEstimated probability of redshift successstat.valueVARCHARprincipalVEL_ERRUncertainty in redshift, given as a velocity, delta c ln(1+z)km/sstat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.TilingExtrav02Science targets in the GAMA II equatorial survey regions not foundin InputCatAv06. These are mainly FIRST-SDSS targets, but also sometargets just North of -1 deg in G09 where a different reduction wasused between GAMA I and GAMA II.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFLAGSSee SDSS photoobj tablemeta.code.qual;photVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalFIBERMAG_RSDSS DR7 r band fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalPETROMAG_RSDSS DR7 r band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalMODELMAG_RSDSS DR7 r band model magnitudemagphot.mag;em.opt.RVARCHARprincipalEXTINCTION_RGalactic extinction in r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalPSFMAG_ISDSS DR7 iband PSF magnitude, not entered for somemagphot.mag;em.opt.IVARCHARprincipalMODELMAG_ISDSS magnitudemagphot.mag;em.opt.IVARCHARprincipalEXTINCTION_IGalactic extinction in i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalSECTARGETSecondary target flag from SDSSmeta.code.classVARCHARprincipalPSFMAG_GSDSS DR7 g band PSF magnitude, not entered for somemagphot.mag;em.optVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.ApMatchedCatv06This table contains r-band defined aperture matched photometry andother Source Extractor outputs for all objects in the GAMA IIequatorial survey regions.CATAIDUnique GAMA IDmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinate from TilingCatdegpos.eq.raVARCHARprincipalDECJ2000 coordinate from TilingCatdegpos.eq.decVARCHARprincipalXx coordinate of aperture centre in r band cutoutpixelposVARCHARprincipalYy coordinate of aperture centre in r band cutoutpixelposVARCHARprincipalALPHA_J2000J2000 RA from SExtractor (r band)degpos.eq.ra;em.opt.RVARCHARprincipalDELTA_J2000J2000 Dec from SExtractor (r band)degpos.eq.dec;em.opt.RVARCHARprincipalA_IMAGEProfile RMS along major axis (r band)pixelphys.angSize;em.opt.RVARCHARprincipalB_IMAGEProfile RMS along minor axis (r band)pixelphys.angSize;em.opt.RVARCHARprincipalERRA_IMAGEMajor axis profile RMS error (r band)pixelstat.error;phys.angSize;em.opt.RVARCHARprincipalERRB_IMAGEMinor axis profile RMS error (r band)pixelstat.error;phys.angSize;em.opt.RVARCHARprincipalKRON_RADIUSKron radius (r band)pixelphys.size.radius;em.opt.RVARCHARprincipalPETRO_RADIUSPetrosian radius (r band)pixelphys.size.radius;em.opt.RVARCHARprincipalTHETA_IMAGEPosition angle on image (counterclockwise, r band)degpos.posAng;em.opt.RVARCHARprincipalTHETA_J2000Position angle on sky (east of north, r band)degpos.posAng;em.opt.RVARCHARprincipalERRTHETA_J2000J2000 position angle error (r band)degstat.error;pos.posAng;em.opt.RVARCHARprincipalTHRESHOLDDetection threshold above background (r band)countsinstr.sensitivity;phot.count;em.opt.RVARCHARprincipalMU_THRESHOLDDetection threshold above background (r band)mag/arcsec^2instr.sensitivity;phot.mag.sb;em.opt.RVARCHARprincipalISOAREAF_IMAGEIsophotal area (filtered) (r band)pixelphys.angArea;em.opt.RVARCHARprincipalFLUX_AUTO_uKron flux (u band)countsphot.flux;em.opt.UVARCHARprincipalFLUXERR_AUTO_uKron flux error (u band)countsstat.error;phot.flux;em.opt.UVARCHARprincipalMAG_AUTO_uKron magnitude (u band)magphot.mag;em.opt.UVARCHARprincipalMAGERR_AUTO_uKron magnitude error (u band)magstat.error;phot.mag;em.opt.UVARCHARprincipalFLUX_PETRO_uPetrosian flux (u band)countsphot.flux;em.opt.UVARCHARprincipalFLUXERR_PETRO_uPetrosian flux error (u band)countsstat.error;phot.flux;em.opt.UVARCHARprincipalMAG_PETRO_uPetrosian magnitude (u band)magphot.mag;em.opt.UVARCHARprincipalMAGERR_PETRO_uPetrosian magnitude error (u band)magstat.error;phot.mag;em.opt.UVARCHARprincipalBACKGROUND_uBackground at centroid (u band)countsinstr.background;phot.count;em.opt.UVARCHARprincipalFLUX_MAX_uPeak flux (u band)countsphot.flux;stat.max;em.opt.UVARCHARprincipalISOAREA_IMAGE_uIsophotal area (u band)pixelphys.angArea;em.opt.UVARCHARprincipalMU_MAX_uPeak surface brightness (u band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.UVARCHARprincipalFWHM_IMAGE_uFWHM assuming a Gaussian core (u band)pixelspect.line.width;obs.image;em.opt.UVARCHARprincipalFLAGS_uSource Extractor flags (u band)meta.code.qual;em.opt.UVARCHARprincipalFLUX_AUTO_gKron flux (g band)countsphot.flux;em.opt.GVARCHARprincipalFLUXERR_AUTO_gKron flux error (g band)countsstat.error;phot.flux;em.opt.GVARCHARprincipalMAG_AUTO_gKron magnitude (g band)magphot.mag;em.opt.GVARCHARprincipalMAGERR_AUTO_gKron magnitude error (g band)magstat.error;phot.mag;em.opt.GVARCHARprincipalFLUX_PETRO_gPetrosian flux (g band)countsphot.flux;em.opt.GVARCHARprincipalFLUXERR_PETRO_gPetrosian flux error (g band)countsstat.error;phot.flux;em.opt.GVARCHARprincipalMAG_PETRO_gPetrosian magnitude (g band)magphot.mag;em.opt.GVARCHARprincipalMAGERR_PETRO_gPetrosian magnitude error (g band)magstat.error;phot.mag;em.opt.GVARCHARprincipalBACKGROUND_gBackground at centroid (g band)countsinstr.background;phot.count;em.opt.GVARCHARprincipalFLUX_MAX_gPeak flux (g band)countsphot.flux;stat.max;em.opt.GVARCHARprincipalISOAREA_IMAGE_gIsophotal area (g band)pixelphys.angArea;em.opt.GVARCHARprincipalMU_MAX_gPeak surface brightness (g band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.GVARCHARprincipalFWHM_IMAGE_gFWHM assuming a Gaussian core (g band)pixelspect.line.width;obs.image;em.opt.GVARCHARprincipalFLAGS_gSource Extractor flags (g band)meta.code.qual;em.opt.GVARCHARprincipalFLUX_AUTO_rKron flux (r band)countsphot.flux;em.opt.RVARCHARprincipalFLUXERR_AUTO_rKron flux error (r band)countsstat.error;phot.flux;em.opt.RVARCHARprincipalMAG_AUTO_rKron magnitude (r band)magphot.mag;em.opt.RVARCHARprincipalMAGERR_AUTO_rKron magnitude error (r band)magstat.error;phot.mag;em.opt.RVARCHARprincipalFLUX_PETRO_rPetrosian flux (r band)countsphot.flux;em.opt.RVARCHARprincipalFLUXERR_PETRO_rPetrosian flux error (r band)countsstat.error;phot.flux;em.opt.RVARCHARprincipalMAG_PETRO_rPetrosian magnitude (r band)magphot.mag;em.opt.RVARCHARprincipalMAGERR_PETRO_rPetrosian magnitude error (r band)magstat.error;phot.mag;em.opt.RVARCHARprincipalBACKGROUND_rBackground at centroid (r band)countsinstr.background;phot.count;em.opt.RVARCHARprincipalFLUX_MAX_rPeak flux (r band)countsphot.flux;stat.max;em.opt.RVARCHARprincipalISOAREA_IMAGE_rIsophotal area (r band)pixelphys.angArea;em.opt.RVARCHARprincipalMU_MAX_rPeak surface brightness (r band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.RVARCHARprincipalFWHM_IMAGE_rFWHM assuming a Gaussian core (r band)pixelspect.line.width;obs.image;em.opt.RVARCHARprincipalFLAGS_rSource Extractor flags (r band)meta.code.qual;em.opt.RVARCHARprincipalFLUX_AUTO_iKron flux (i band)countsphot.flux;em.opt.IVARCHARprincipalFLUXERR_AUTO_iKron flux error (i band)countsstat.error;phot.flux;em.opt.IVARCHARprincipalMAG_AUTO_iKron magntiude (i band)magphot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_iKron magnitude error (i band)magstat.error;phot.mag;em.opt.IVARCHARprincipalFLUX_PETRO_iPetrosian flux (i band)countsphot.flux;em.opt.IVARCHARprincipalFLUXERR_PETRO_iPetrosian flux error (i band)countsstat.error;phot.flux;em.opt.IVARCHARprincipalMAG_PETRO_iPetrosian magnitude (i band)magphot.mag;em.opt.IVARCHARprincipalMAGERR_PETRO_iPetrosian magnitude error (i band)magstat.error;phot.mag;em.opt.IVARCHARprincipalBACKGROUND_iBackground at centroid (i band)countsinstr.background;phot.count;em.opt.IVARCHARprincipalFLUX_MAX_iPeak flux (i band)countsphot.flux;stat.max;em.opt.IVARCHARprincipalISOAREA_IMAGE_iIsophotal area (i band)pixelphys.angArea;em.opt.IVARCHARprincipalMU_MAX_iPeak surface brightness (i band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.IVARCHARprincipalFWHM_IMAGE_iFWHM assuming a Gaussian core (i band)pixelspect.line.width;obs.image;em.opt.IVARCHARprincipalFLAGS_iSource Extractor flags (i band)meta.code.qual;em.opt.IVARCHARprincipalFLUX_AUTO_zKron flux (SDSS z band)countsphot.flux;em.opt.ZVARCHARprincipalFLUXERR_AUTO_zKron flux error (SDSS z band)countsstat.error;phot.flux;em.opt.ZVARCHARprincipalMAG_AUTO_zKron magnitude (SDSS z band)magphot.mag.em.opt.ZVARCHARprincipalMAGERR_AUTO_zKron magnitude error (SDSS z band)magstat.error;phot.mag;em.opt.ZVARCHARprincipalFLUX_PETRO_zPetrosian flux (SDSS z band)countsphot.flux;em.opt.ZVARCHARprincipalFLUXERR_PETRO_zPetrosian flux error (SDSS z band)countsstat.error;phot.flux;em.opt.ZVARCHARprincipalMAG_PETRO_zPetrosian magnitude (SDSS z band)magphot.mag;em.opt.ZVARCHARprincipalMAGERR_PETRO_zPetrosian magnitude error (SDSS z band)magstat.error;phot.mag;em.opt.ZVARCHARprincipalBACKGROUND_zBackground at centroid (SDSS z band)countsinstr.background;phot.count;em.opt.ZVARCHARprincipalFLUX_MAX_zPeak flux (SDSS z band)countsphot.flux;stat.max;em.opt.ZVARCHARprincipalISOAREA_IMAGE_zIsophotal area (SDSS z band)pixelphys.angArea;em.opt.ZVARCHARprincipalMU_MAX_zPeak surface brightness (SDSS z band)mag/arcsec^2phot.mag.sb;statm.ax;em.opt.ZVARCHARprincipalFWHM_IMAGE_zFWHM assuming a Gaussian core (SDSS z band)pixelspect.line.width;obs.image;em.opt.ZVARCHARprincipalFLAGS_zSource Extractor flags (SDSS z band)meta.code.qual;em.opt.ZVARCHARprincipalFLUX_AUTO_XKron flux (VIKING Z band)countsphot.flux;em.IR.ZVARCHARprincipalFLUXERR_AUTO_XKron flux error (VIKING Z band)countsstat.error;phot.flux;em.IR.ZVARCHARprincipalMAG_AUTO_XKron magnitude (VIKING Z band)magphot.mag;em.IR.ZVARCHARprincipalMAGERR_AUTO_XKron magnitude error (VIKING Z band)magstat.error;phot.mag;em.IR.ZVARCHARprincipalFLUX_PETRO_XPetrosian flux (VIKING Z band)countsphot.flux;em.IR.ZVARCHARprincipalFLUXERR_PETRO_XPetrosian flux error (VIKING Z band)countsstat.error;phot.flux;em.IR.ZVARCHARprincipalMAG_PETRO_XPetrosian magnitude (VIKING Z band)magphot.mag;em.IR.ZVARCHARprincipalMAGERR_PETRO_XPetrosian magnitude error (VIKING Z band)magstat.error;phot.mag;em.IR.ZVARCHARprincipalBACKGROUND_XBackground at centroid (VIKING Z band)countsinstr.background;phot.count;em.IR.ZVARCHARprincipalFLUX_MAX_XPeak flux (VIKING Z band)countsphot.flux;stat.max;em.IR.ZVARCHARprincipalISOAREA_IMAGE_XIsophotal area (VIKING Z band)pixelphys.angArea;em.IR.ZVARCHARprincipalMU_MAX_XPeak surface brightness (VIKING Z band)mag/arcsec^2phot.mag.sb;statm.ax;em.IR.ZVARCHARprincipalFWHM_IMAGE_XFWHM assuming a Gaussian core (VIKING Z band)pixelspect.line.width;obs.image;em.IR.ZVARCHARprincipalFLAGS_XSource Extractor flags (VIKING Z band)meta.code.qual;em.IR.ZVARCHARprincipalFLUX_AUTO_YKron flux (Y band)countsphot.flux;em.IR.YVARCHARprincipalFLUXERR_AUTO_YKron flux error (Y band)countsstat.error;phot.flux;em.IR.YVARCHARprincipalMAG_AUTO_YKron magnitude (Y band)magphot.mag;em.IR.YVARCHARprincipalMAGERR_AUTO_YKron magnitude error (Y band)magstat.error;phot.mag;em.IR.YVARCHARprincipalFLUX_PETRO_YPetrosian flux (Y band)countsphot.flux;em.IR.YVARCHARprincipalFLUXERR_PETRO_YPetrosian flux error (Y band)countsstat.error;phot.flux;em.IR.YVARCHARprincipalMAG_PETRO_YPetrosian magnitude (Y band)magphot.mag;em.IR.YVARCHARprincipalMAGERR_PETRO_YPetrosian magnitude error (Y band)magstat.error;phot.mag;em.IR.YVARCHARprincipalBACKGROUND_YBackground at centroid (Y band)countsinstr.background;phot.count;em.IR.YVARCHARprincipalFLUX_MAX_YPeak flux (Y band)countsphot.flux;stat.max;em.IR.YVARCHARprincipalISOAREA_IMAGE_YIsophotal area (Y band)pixelphys.angArea;em.IR.YVARCHARprincipalMU_MAX_YPeak surface brightness (Y band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.YVARCHARprincipalFWHM_IMAGE_YFWHM assuming a Gaussian core (Y band)pixelspect.line.width;obs.image;em.IR.YVARCHARprincipalFLAGS_YSource Extractor flags (Y band)meta.code.qual;em.IR.YVARCHARprincipalFLUX_AUTO_JKron flux (J band)countsphot.flux;em.IR.JVARCHARprincipalFLUXERR_AUTO_JKron flux error (J band)countsstat.error;phot.flux;em.IR.JVARCHARprincipalMAG_AUTO_JKron magnitude (J band)magphot.mag;em.IR.JVARCHARprincipalMAGERR_AUTO_JKron magnitude error (J band)magstat.error;phot.mag;em.IR.JVARCHARprincipalFLUX_PETRO_JPetrosian flux (J band)countsphot.flux;em.IR.JVARCHARprincipalFLUXERR_PETRO_JPetrosian flux error (J band)countsstat.error;phot.flux;em.IR.JVARCHARprincipalMAG_PETRO_JPetrosian magnitude (J band)magphot.mag;em.IR.JVARCHARprincipalMAGERR_PETRO_JPetrosian magnitude error (J band)magstat.error;phot.mag;em.IR.JVARCHARprincipalBACKGROUND_JBackground at centroid (J band)countsinstr.background;phot.count;em.IR.JVARCHARprincipalFLUX_MAX_JPeak flux (J band)countsphot.flux;stat.max;em.IR.JVARCHARprincipalISOAREA_IMAGE_JIsophotal area (J band)pixelphys.angArea;em.IR.JVARCHARprincipalMU_MAX_JPeak surface brightness (J band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.JVARCHARprincipalFWHM_IMAGE_JFWHM assuming a Gaussian core (J band)pixelspect.line.width;obs.image;em.IR.JVARCHARprincipalFLAGS_JSource Extractor flags (J band)meta.code.qual;em.IR.JVARCHARprincipalFLUX_AUTO_HKron flux (H band)countsphot.flux;em.IR.HVARCHARprincipalFLUXERR_AUTO_HKron flux error (H band)countsstat.error;phot.flux;em.IR.HVARCHARprincipalMAG_AUTO_HKron magnitude (H band)magphot.mag;em.IR.HVARCHARprincipalMAGERR_AUTO_HKron magnitude error (H band)magstat.error;phot.mag;em.IR.HVARCHARprincipalFLUX_PETRO_HPetrosian flux (H band)countsphot.flux;em.IR.HVARCHARprincipalFLUXERR_PETRO_HPetrosian flux error (H band)countsstat.error;phot.flux;em.IR.HVARCHARprincipalMAG_PETRO_HPetrosian magnitude (H band)magphot.mag;em.IR.HVARCHARprincipalMAGERR_PETRO_HPetrosian magnitude error (H band)magstat.error;phot.mag;em.IR.HVARCHARprincipalBACKGROUND_HBackground at centroid (H band)countsinstr.background;phot.count;em.IR.HVARCHARprincipalFLUX_MAX_HPeak flux (H band)countsphot.flux;stat.max;em.IR.HVARCHARprincipalISOAREA_IMAGE_HIsophotal area (H band)pixelphys.angArea;em.IR.HVARCHARprincipalMU_MAX_HPeak surface brightness (H band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.HVARCHARprincipalFWHM_IMAGE_HFWHM assuming a Gaussian core (H band)pixelspect.line.width;obs.image;em.IR.HVARCHARprincipalFLAGS_HSource Extractor flags (H band)meta.code.qual;em.IR.HVARCHARprincipalFLUX_AUTO_KKron flux (K band)countsphot.flux;em.IR.KVARCHARprincipalFLUXERR_AUTO_KKron flux error (K band)countsstat.error;phot.flux;em.IR.KVARCHARprincipalMAG_AUTO_KKron magnitude (K band)magphot.mag;em.IR.KVARCHARprincipalMAGERR_AUTO_KKron magnitude error (K band)magstat.error;phot.mag;em.IR.KVARCHARprincipalFLUX_PETRO_KPetrosian flux (K band)countsphot.flux;em.IR.KVARCHARprincipalFLUXERR_PETRO_KPetrosian flux error (K band)countsstat.error;phot.flux;em.IR.KVARCHARprincipalMAG_PETRO_KPetrosian magnitude (K band)magphot.mag;em.IR.KVARCHARprincipalMAGERR_PETRO_KPetrosian magnitude error (K band)magstat.error;phot.mag;em.IR.KVARCHARprincipalBACKGROUND_KBackground at centroid (K band)countsinstr.background;phot.count;em.IR.KVARCHARprincipalFLUX_MAX_KPeak flux (K band)countsphot.flux;stat.max;em.IR.KVARCHARprincipalISOAREA_IMAGE_KIsophotal area (K band)pixelphys.angArea;em.IR.KVARCHARprincipalMU_MAX_KPeak surface brightness (K band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.KVARCHARprincipalFWHM_IMAGE_KFWHM assuming a Gaussian core (K band)pixelspect.line.width;obs.image;em.IR.KVARCHARprincipalFLAGS_KSource Extractor flags (K band)mag.code.qual;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.EnvironmentMeasuresv06This catalogue provides three different environment measures for allGAMA II galaxies with 0.002 < z < 0.18: a surface density, thenumber of galaxies within a cylinder, and the adaptive Gaussianenvironment parameter.CATAIDUnique GAMA IDmeta.idVARCHARprincipalRAJ2000degpos.eq.raVARCHARprincipalDECJ2000degpos.eq.decVARCHARprincipalZ_TONRYHeliocentric redshift corrected for the effects of peculiar velocitysrc.redshiftVARCHARprincipalnQRedshift quality flagmeta.code.qual;src.redshiftVARCHARprincipalMExtinction and k-corrected absolute r-band (G02-G15) or i-band (G23) magnitude, see notesmagphys.magAbsVARCHARprincipalDistanceToEdgeDistance to nearest angular survey edge in co-moving unitsMpcpos.distanceVARCHARprincipalCompletenessValue used to correct environment measures for local survey incompleteness, see notesarith.factorVARCHARprincipalDistanceTo5nnDistance to 5th nearest neighbour in co-moving unitsMpcpos.distanceVARCHARprincipalSurfaceDensitySurface density based on the distance to the 5th nearest neighbourMpc^-2src.densityVARCHARprincipalSurfaceDensityErrSurface density uncertaintyMpc^-2stat.error;src.densityVARCHARprincipalSurfaceDensityFlagFlag indicating problems with surface density measurement, see notesmeta.code.error;src.densityVARCHARprincipalCountInCylNumber of (other) galaxies within cylinder of radius 1 co-moving Mpcmeta.numberVARCHARprincipalCountInCylErrPoisson error on number of galaxies in cylinderstat.error;meta.numberVARCHARprincipalCountInCylFlagFlag indicating problems with CountInCyl, see notesmeta.code.error;meta.numberVARCHARprincipalAGEDenParAdaptive Gaussian environment parameterMpc^-1src.densityVARCHARprincipalAGEErrPoisson error on the number of galaxies used to calculate AGEDenParstat.error;meta.numberVARCHARprincipalAGEScaleAdaptive scaling factor used for the adaptive Gaussian ellipsoidarith.factorVARCHARprincipalAGEDenParFlagFlag indicating problems with AGEDenPar, see notesmeta.code.error;src.densityVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.ExternalSpecAllv07This table lists all spectra that are available from previousspectroscopic surveys (such as the SDSS) in the GAMA II surveyregions, including duplicate observations. Every spectrum listed inthis table is available in the GAMA database.SPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in originating survey?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.XXLClusterCatv01This catalogue provides the x-ray properties and cluster redshiftsof XXL clusters that were matched to GAMA objects (i.e. those thatappear in the table XXLClusterAssoc). This catalogue is one of theoutputs of the GAMA/XXL Matching Group. It was produced by TatyanaSadibekova and was not modified in any way.CLUSTERIDUnique ID of a combination of XXL source and cluster redshiftmeta.id;meta.mainVARCHARindexedprincipalXIDXXL ID of clustermeta.idVARCHARprincipalXNAMEXXL name of clustermeta.idVARCHARprincipalRARA of XXL clusterdegpos.eq.raVARCHARprincipalDECDec of XXL clusterdegpos.eq.decVARCHARprincipalFLUXSOFTPipeline flux in 0.5-2 keV band, see notes10^(-14)erg/s/cm^2VARCHARprincipalEXTSOFTPipeline extension, see notesarcsecVARCHARprincipalFLUX60Flux measured within r=60" aperture in 0.5-2 keV band, see notes10^(-14)erg/s/cm^2VARCHARprincipalTX60Temperature measured from x-ray spectrum within 60" aperture, see noteskeVVARCHARprincipalZ_CLSpectroscopic redshift used for the correlation within 2 MpcVARCHARprincipalR_2MPCMatching radius corresponding to 2 Mpcarcminpos.angDistanceVARCHARprincipalN_GALNumber of GAMA objects matched within 2 MpcVARCHARprincipalMULTMultiplicity of XXL source (number of projected optical clusters), see notesVARCHARprincipalgama_pdr4v2.GalacticExtinctionv03This table provides the Galactic foreground extinction in all GALEX,SDSS (= KiDS), UKIDSS and VIKING bands for all objects in the GAMA IIequatorial survey regions, i.e. for every object in InputCatA,TilingExtra and SpStandards.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_B_MGCGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_uGalactic extinction in SDSS and KiDS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_gGalactic extinction in SDSS and KiDS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_rGalactic extinction in SDSS and KiDS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_iGalactic extinction in SDSS and KiDS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_zGalactic extinction in SDSS and KiDS z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_UKIDSSGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_UKIDSSGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_UKIDSSGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_UKIDSSGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_Z_VIKINGGalactic extinction in VIKING Z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_VIKINGGalactic extinction in VIKING Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_VIKINGGalactic extinction in VIKING J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_VIKINGGalactic extinction in VIKING H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_VIKINGGalactic extinction in VIKING K bandmagphys.absorption.gal;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalaxyPartMatchesv12This table can be used to match a vis_class=3 object (deblended partof a galaxy) to a vis_class=0 or 1 object (chosen main part of agalaxy). Each galaxy should only have one main part but some haveseveral deblended parts.CATAID_VC3CATAID of vis_class=3 objectmeta.idVARCHARprincipalCATAID_MAINCATAID of main partmeta.idVARCHARprincipalgama_pdr4v2.GamaIToGamaIIv01This table contains a match between all GAMA I and GAMA II objects,i.e. between all objects in InputCatAv05 and InputCatAv06. Itprovides flags to easily identify objects that are (only) in GAMA I,(only) in GAMA II, or in both. It also provides the CATAIDtranslation for those objects in both that have a different CATAIDin GAMA I and GAMA II.PairIDUnique GAMA I-II pair IDmeta.idVARCHARprincipalCATAID_IGAMA I ID (as in InputCatAv05)meta.idVARCHARprincipalOBJID_ISDSS DR6 objidmeta.idVARCHARprincipalRA_IJ2000 coordinate (DR6)degpos.eq.raVARCHARprincipalDEC_IJ2000 coordinate (DR6)degpos.eq.decVARCHARprincipalCATAID_IIGAMA II ID (as in InputCatAv06)meta.idVARCHARprincipalOBJID_IISDSS DR7 objidmeta.idVARCHARprincipalRA_IIJ2000 coordinate (DR7)degpos.eq.raVARCHARprincipalDEC_IIJ2000 coordinate (DR7)degpos.eq.decVARCHARprincipalInIFlag indicating that the object is in GAMA I (InputCatAv05)meta.codeVARCHARprincipalInIIFlag indicating that the object is in GAMA II (InputCatAv06)meta.codeVARCHARprincipalOnlyInIFlag indicating that the object is in GAMA I but not in GAMA IImeta.codeVARCHARprincipalOnlyInIIFlag indicating that the object is in GAMA II but not in GAMA Imeta.codeVARCHARprincipalInBothFlag indicating that the object is in both GAMA I and IImeta.codeVARCHARprincipalInBothDifferentIDFlag indicating that the object is in both GAMA I and II but with different CATAIDsmeta.codeVARCHARprincipalSeparationDistance between matched objects along a great circlearcsecpos.angDistanceVARCHARprincipalgama_pdr4v2.GuideStarsv03Guide stars selected from SDSS DR7 for the GAMA II equatorial surveyregions.RAJ2000 positiondegpos.eq.raVARCHARprincipalDECJ2000 positiondegpos.eq.decVARCHARprincipalRAERRError in positiondegstat.error;pos.eq.raVARCHARprincipalDECERRError in positiondegstat.error;pos.eq.decVARCHARprincipalPSFMAG_GSDSS DR7 g band PSF magnitudemagphot.mag;em.optVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalPSFMAG_ISDSS DR7 i band PSF magnitudemagphot.mag;em.opt.IVARCHARprincipalPROPERMOTIONFrom USNO-B matchmas/yrpos.pmVARCHARprincipalAREA_FLAG2=GAMA I 4x12 areas, 1=extended GAMA II areasmeta.codeVARCHARprincipalVIS_CLASS0=unchecked, 1=okay, 2=not goodmeta.code.qualVARCHARprincipalVIS_CLASS_USERInitials of classifiermeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalCATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.InputCatAv07This is the GAMA II master input catalogue for the GAMA IIequatorial survey regions. It provides SDSS DR7 data for an enlargedarea of 14x6.5 deg^2 covering the GAMA II equatorial regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFLAGSSee SDSS photoobj tablemeta.code.qual;photVARCHARprincipalPRIMTARGETSee SDSS photoobj tablemeta.code.classVARCHARprincipalTYPESDSS photo type (3=galaxy, 6=star, 8=sky)src.classVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalFIBERMAG_RSDSS DR7 r band 3-arcsec fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalFLAGS_RSee SDSS photoobj tablemeta.code.qual;phot;em.opt.RVARCHARprincipalEXTINCTION_RGalactic extinction in r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalPETRORAD_RPetrosian radius in r bandarcsecphys.angSize;em.opt.RVARCHARprincipalPETROR90_RRadius containing 90% of Petrosian fluxarcsecphys.angSize;em.opt.RVARCHARprincipalPETROR50_RRadius containing 50% of Petrosian fluxarcsecphys.angSize;em.opt.RVARCHARprincipalPETROMAG_GSDSS DR7 g band Petrosian magnitudemagphot.mag;em.optVARCHARprincipalPETROMAG_RSDSS DR7 r band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalPETROMAG_ISDSS DR7 i band Petrosian magnitudemagphot.mag;em.opt.IVARCHARprincipalMODELMAG_USDSS DR7 u band model magnitudemagphot.mag;em.opt.UVARCHARprincipalMODELMAG_GSDSS DR7 g band model magnitudemagphot.mag;em.optVARCHARprincipalMODELMAG_RSDSS DR7 r band model magnitudemagphot.mag;em.opt.RVARCHARprincipalMODELMAG_ISDSS DR7 i band model magnitudemagphot.mag;em.opt.IVARCHARprincipalMODELMAG_ZSDSS DR7 z band model magnitudemagphot.mag;em.optVARCHARprincipalSTATUSSee SDSS photoobj tablemeta.code.statusVARCHARprincipalRUNSDSS run numberobs.paramVARCHARprincipalMASK_IC_10Mask value 0.0 to 1.0 around V<10 stars, see notesmeta.codeVARCHARprincipalMASK_IC_12Mask value 0.0 to 1.0 around V<12 stars, see notesmeta.codeVARCHARprincipalMASK_SATURSaturation class from FLAGS and FLAGS_R, see notesmeta.codeVARCHARprincipalEXCEPTION_FLAGExceptions to mask criteria, targets to includemeta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.StellarMassesv24_LambdarCatv01catidCATAID from LambdarCatv01VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_pdr4v2.SpStandardsv09Standard stars from SDSS for the GAMA II equatorial survey regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR7 r band fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalPSFMAG_GSDSS DR7 g band PSF magnitudemagphot.mag;em.opt.BVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalPSFMAG_ISDSS DR7 i band PSF magnitudemagphot.mag;em.opt.IVARCHARprincipalSECTARGET2^1 for REDDEN_STD, 2^5 for SPECTROPHOTO_STDmeta.code.classVARCHARprincipalSTATUSSDSS status flag related to primary secondarymeta.code.statusVARCHARprincipalRUNSDSS run numberobs.paramVARCHARprincipalAREA_FLAG2 for GAMA I regions, 1 otherwisemeta.codeVARCHARprincipalPRIORITY_CLASSSee notesmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.TilingCatv46Science targets in the GAMA II equatorial survey regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR7 r band fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 r band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalU_MODELExtinction-corrected SDSS DR7 u band model magnitudemagphot.mag;em.opt.UVARCHARprincipalG_MODELExtinction-corrected SDSS DR7 g band model magnitudemagphot.mag;em.opt.BVARCHARprincipalR_MODELExtinction-corrected SDSS DR7 r band model magnitudemagphot.mag;em.opt.RVARCHARprincipalI_MODELExtinction-corrected SDSS DR7 i band model magnitudemagphot.mag;em.opt.IVARCHARprincipalZ_MODELExtinction-corrected SDSS DR7 z band model magnitudemagphot.mag;em.opt.IVARCHARprincipalSURVEY_CODESurvey code for redshift source, see notesmeta.code;meta.datasetVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalNQ2_FLAGTests of NQ=2 redshifts, see notesmeta.code.qual;src.redshiftVARCHARprincipalSPECIDID of spectrum from SpecAll tablemeta.id.cross;spectVARCHARprincipalVEL_ERRRedshift uncertainty, c delta ln(1+z), see noteskm/ssrc.redshift;stat.errorVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra within 1 arcsecmeta.number;spectVARCHARprincipalR_SBSDSS Petro half-light surface brightnessmag/arcsec^2phot.mag.sb;em.opt.RVARCHARprincipalSG_SEPr_psf - r_model star-galaxy separation parametermagsrc.class.starGalaxyVARCHARprincipalSG_SEP_JKJ - K - f_locus star-galaxy separation parametermagsrc.class.starGalaxyVARCHARprincipalK_AUTOExtinction-corrected r-defined auto AB magmagphot.mag;em.IR.KVARCHARprincipalRADIO_FLUXFlux from FIRST-SDSS matchingmJyphot.flux.density;em.radioVARCHARprincipalHATLAS_FLAG1 for match to H-ATLAS SDSS possible IDmeta.codeVARCHARprincipalAREA_FLAG1-deg strip, 2 for GAMA I regionsmeta.codeVARCHARprincipalTARGET_FLAGSBitwise target criteria, see notesmeta.codeVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalPRIORITY_CLASSPriorities for targeting, see notesmeta.code.classVARCHARprincipalNEIGHBOUR_CLASSNumber of survey_class>=3 targets within 40 arcsecmeta.code.classVARCHARprincipalTC_V11_IDCATAID of object in TilingCatv11, see notesmeta.code.crossVARCHARprincipalMASK_IC_10Mask value 0.0 to 1.0 around V<10 starsmeta.codeVARCHARprincipalMASK_IC_12Mask value 0.0 to 1.0 around V<12 starsmeta.codeVARCHARprincipalVIS_CLASSVisual classification, see notesmata.code.qualVARCHARprincipalVIS_CLASS_USERInitials of classifiers, xxx for nonemeta.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LambdarSPIRE500v01This catalogue contains the complete LAMBDAR output for the Herschel SPIRE 500 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarVIKINGHv01This catalogue contains the complete LAMBDAR output for the VIKING H band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarVIKINGJv01This catalogue contains the complete LAMBDAR output for the VIKING J band.DFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarVIKINGKv01This catalogue contains the complete LAMBDAR output for the VIKING K band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.ExternalzAllv07This table lists a few redshifts in the GAMA II survey regions takenfrom the literature. The spectra from which these redshifts weremeasured are NOT available in the GAMA database.SPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.FilBranchesv02Table of all branches in filaments.LengthLength of all links in the branchMpc/hphys.sizeVARCHARprincipalBranchIDUnique ID of branchmeta.idVARCHARprincipalFilIDID of filament that the branch is inmeta.idVARCHARprincipalBranchOrderBranch ordermeta.codeVARCHARprincipalNgroupNumber of groups in the branchmeta.numberVARCHARprincipalCutNumber of groups in the branch near survey edgemeta.numberVARCHARprincipalgama_pdr4v2.FilGalsv02Table of all galaxies near filaments.CATAIDUnique ID of galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipaldOrthogonal distance to nearest filamentMpc/hpos.distanceVARCHARprincipalGroupIDID of group galaxy belongs to (0 if ungrouped)meta.idVARCHARprincipalBranchIDID of branch galaxy is closest tometa.idVARCHARprincipalFilIDID of filamentmeta.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.FilGroupsv02Table of all groups in filaments.GroupIDUnique ID of groupmeta.idVARCHARprincipalRAGroup centre RA (IterCenRA)degpos.eq.raVARCHARprincipalDecGroup centre Dec (IterCenDEC)degpos.eq.decVARCHARprincipalZfofGroup median redshiftsrc.redshiftVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipalBranchIDID of the branch the group is inmeta.idVARCHARprincipalBranchOrderOrder of branchmeta.codeVARCHARprincipalFilIDFilament the group is inmeta.idVARCHARprincipalCutIndicates if the group is near survey edgemeta.numberVARCHARprincipalgama_pdr4v2.FilLinksv02Table of links between groups.LinkIDUnique ID of linkmeta.idVARCHARprincipalGroupID1GroupID of link startmeta.idVARCHARprincipalGroupID2GroupID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_pdr4v2.Filamentsv02Table of all filaments composed of groups of galaxies.FilIDUnique ID of filamentmeta.idVARCHARprincipalNbranchNumber of branches in filamentmeta.numberVARCHARprincipalNgroupNumber of groups in filamentmeta.numberVARCHARprincipalLengthTotal length of all links in filamentMpc/hphys.sizeVARCHARprincipalBBlengthTotal length of all links in the backboneMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the filament near survey edgemeta.numberVARCHARprincipalgama_pdr4v2.MockFilBranchesv01Table of all branches in mock filaments.BranchIDUnique ID of mock branchmeta.idVARCHARprincipalFilIDID of filament that the branch is inmeta.idVARCHARprincipalBranchOrderBranch ordermeta.codeVARCHARprincipalNgroupNumber of groups in the branchmeta.numberVARCHARprincipalLengthLength of all links in the branchMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the branch near survey edgemeta.numberVARCHARprincipalgama_pdr4v2.MockFilGalsv01Table of all mock galaxies near filaments.GalIDUnique ID of mock galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipaldOrthogonal distance to nearest filamentMpc/hpos.distanceVARCHARprincipalGroupIDID of group galaxy belongs to (0 if ungrouped)meta.idVARCHARprincipalBranchIDID of branch galaxy is closest tometa.idVARCHARprincipalFilIDID of filamentmeta.idVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_pdr4v2.MockFilGroupsv01Table of all mock groups in filaments.GroupIDUnique ID of mock groupmeta.idVARCHARprincipalRAGroup centre RA (IterCenRA)degpos.eq.raVARCHARprincipalDecGroup centre Dec (IterCenDEC)degpos.eq.decVARCHARprincipalZfofGroup median redshiftsrc.redshiftVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipalBranchIDID of the branch the group is inmeta.idVARCHARprincipalBranchOrderOrder of branchmeta.codeVARCHARprincipalFilIDFilament the group is inmeta.idVARCHARprincipalCutIndicates if the group is near survey edgemeta.numberVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_pdr4v2.MockFilLinksv01Table of links between mock groups.LinkIDUnique ID of linkmeta.idVARCHARprincipalGroupID1GroupID of link startmeta.idVARCHARprincipalGroupID2GroupID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_pdr4v2.MockFilamentsv01Table of all filaments composed of groups of mock galaxies.FilIDUnique ID of mock filamentmeta.idVARCHARprincipalNbranchNumber of branches in filamentmeta.numberVARCHARprincipalNgroupNumber of groups in filamentmeta.numberVARCHARprincipalLengthTotal length of all links in filamentMpc/hphys.sizeVARCHARprincipalBBlengthTotal length of all links in the backboneMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the filament near survey edgemeta.numberVARCHARprincipalgama_pdr4v2.MockTendrilGalsv01Table of all mock galaxies in tendrils.GalIDUnique ID of mock galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinatesMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinatesMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinatesMpc/hpos.cartesian.zVARCHARprincipalTendrilIDID of tendril galaxy belongs tometa.idVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_pdr4v2.MockTendrilLinksv01Table of links between mock galaxies in tendrils.LinkIDUnique ID of linkmeta.idVARCHARprincipalGalID1GalID of link startmeta.idVARCHARprincipalGalID2GalID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_pdr4v2.MockTendrilsv01Table of mock galaxy tendrils.TendrilIDUnique ID of mock tendrilmeta.idVARCHARprincipalNgalNumber of galaxies in tendrilmeta.numberVARCHARprincipalLengthTotal length of all links in tendrilMpc/hphys.sizeVARCHARprincipalgama_pdr4v2.MockVoidGalsv01Table of all mock galaxies in voids, i.e. of all mock galaxies notgrouped in filaments or tendrils.GalIDUnique ID of mock galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_pdr4v2.TendrilGalsv02Table of all galaxies in tendrils.CATAIDUnique ID of galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinatesMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinatesMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinatesMpc/hpos.cartesian.zVARCHARprincipalTendrilIDID of tendril galaxy belongs tometa.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.TendrilLinksv02Table of links between galaxies in tendrils.LinkIDUnique ID of linkmeta.idVARCHARprincipalCATAID1CATAID of link startmeta.idVARCHARprincipalCATAID2CATAID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_pdr4v2.Tendrilsv02Table of galaxy tendrils.TendrilIDUnique iD of tendrilmeta.idVARCHARprincipalNgalNumber of galaxies in tendrilmeta.numberVARCHARprincipalLengthTotal length of all links in tendrilMpc/hphys.sizeVARCHARprincipalgama_pdr4v2.VoidGalsv02Table of all galaxies in voids, i.e. of all galaxies not grouped infilaments or tendrils.CATAIDUnique ID of galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02CFHTLSInputCatv04CFHTLS W1 input catalogue and photometry for the G02 survey region.ELLIPTICITY1-B/Asrc.ellipticityVARCHARprincipalMAG_APER06_R6-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_APER12_R12-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_APER18_R18-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_APER24_R24-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_UKron-like elliptical aperture magnitudemagphot.mag;em.opt.UVARCHARprincipalMAG_AUTO_GKron-like elliptical aperture magnitudemagphot.mag;em.opt.BVARCHARprincipalMAG_AUTO_RKron-like elliptical aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_IKron-like elliptical aperture magnitudemagphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_ZKron-like elliptical aperture magnitudemagphot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_UAperture magnitude errormagphot.mag;em.opt.UVARCHARprincipalMAGERR_AUTO_GAperture magnitude errormagphot.mag;em.opt.BVARCHARprincipalMAGERR_AUTO_RAperture magnitude errormagphot.mag;em.opt.RVARCHARprincipalMAGERR_AUTO_IAperture magnitude errormagphot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_ZAperture magnitude errormagphot.mag;em.opt.IVARCHARprincipalEXTINCTION_Uu-band Galactic extinctionmagphys.absorption.gal;em.opt.UVARCHARprincipalEXTINCTION_Gg-band Galactic extinctionmagphys.absorption.gal;em.opt.BVARCHARprincipalEXTINCTION_Rr-band Galactic extinctionmagphys.absorption.gal;em.opt.RVARCHARprincipalEXTINCTION_Ii-band Galactic extinctionmagphys.absorption.gal;em.opt.IVARCHARprincipalEXTINCTION_Zz-band Galactic extinctionmagphys.absorption.gal;em.opt.IVARCHARprincipalCOBJIDUnique ID from field number and sequence numbermeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.raVARCHARprincipalCLASS_STARStar-galaxy classifier outputsrc.classVARCHARprincipalKRON_RADIUSKron radius, unsure of unitsphys.angSizeVARCHARprincipalAProfile RMS along major axispixelphys.angSize.smajAxisVARCHARprincipalBProfile RMS along minor axispixelphys.angSize.sminAxisVARCHARprincipalMASKMask information from CFHTLenSmeta.code.qualVARCHARprincipalgama_pdr4v2.LambdarVIKINGYv01This catalogue contains the complete LAMBDAR output for the VIKING Y band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarVIKINGZv01This catalogue contains the complete LAMBDAR output for the VIKING Z band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarWISEW1v01This catalogue contains the complete LAMBDAR output for the WISE W1 band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarWISEW2v01This catalogue contains the complete LAMBDAR output for the WISE W2 band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.G02GalacticExtinctionv01This table provides the Galactic foreground extinction in all GALEX,SDSS (= KiDS), UKIDSS and VIKING bands for every object inG02TilingCatv06, G02TilingExtrav03 and G02SpStandardsv01.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_B_MGCGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_uGalactic extinction in SDSS and KiDS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_gGalactic extinction in SDSS and KiDS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_rGalactic extinction in SDSS and KiDS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_iGalactic extinction in SDSS and KiDS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_zGalactic extinction in SDSS and KiDS z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_UKIDSSGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_UKIDSSGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_UKIDSSGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_UKIDSSGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_Z_VIKINGGalactic extinction in VIKING Z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_VIKINGGalactic extinction in VIKING Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_VIKINGGalactic extinction in VIKING J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_VIKINGGalactic extinction in VIKING H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_VIKINGGalactic extinction in VIKING K bandmagphys.absorption.gal;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02GalaxyPartMatchesv02This table can be used to match a vis_class=3 object (deblended partof a galaxy) to a vis_class=1 object (chosen main part of agalaxy). Each galaxy should only have one main part but some haveseveral deblended parts.CATAID_VC3CATAID of vis_class=3 objectmeta.idVARCHARprincipalCATAID_MAINCATAID of main partmeta.idVARCHARprincipalgama_pdr4v2.G02GuideStarsv01Guide stars for the G02 survey region.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR8 r band magnitude in 3 arcsec diameter fibermagphot.mag;em.opt.RVARCHARprincipalPSFMAG_RSDSS DR8 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02SDSSInputCatv01SDSS DR8 input catalogue and photometry for the G02 survey region.OBJIDUnique SDSS identifiermeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalflagsPhoto object attribute flagsmeta.code.qualVARCHARprincipalflags_rr band photo object attribute flagsmeta.code.qualVARCHARprincipaltypeMorphological type classificationmeta.code.classVARCHARprincipalrowcRow centre positionpixelpos.cartesian.yVARCHARprincipalcolcColumn centre positionpixelpos.cartesian.xVARCHARprincipalfiberMag_rr band magnitude in 3 arcsec diameter fiber radiusmagphot.magVARCHARprincipalpsfMag_uu band PSF magnitudemagphot.magVARCHARprincipalpsfMag_gg band PSF magnitudemagphot.magVARCHARprincipalpsfMag_rr band PSF magnitudemagphot.magVARCHARprincipalpsfMag_ii band PSF magnitudemagphot.magVARCHARprincipalpsfMag_zz band PSF magnitudemagphot.magVARCHARprincipalpsfMagErr_uu band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_gg band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_rr band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_ii band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_zz band PSF magnitude errormagphot.magVARCHARprincipalpetroMag_uu band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_gg band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_rr band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_ii band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_zz band Petrosian magnitudemagphot.magVARCHARprincipalpetroMagErr_uu band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_gg band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_rr band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_ii band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_zz band Petrosian magnitude errormagphot.magVARCHARprincipalmodelMag_uu band model magnitudemagphot.magVARCHARprincipalmodelMag_gg band model magnitude fitmagphot.magVARCHARprincipalmodelMag_rr band model magnitude fitmagphot.magVARCHARprincipalmodelMag_ii band model magnitude fitmagphot.magVARCHARprincipalmodelMag_zz band model magnitude fitmagphot.magVARCHARprincipalmodelMagErr_uu band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_gg band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_rr band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_ii band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_zz band model magnitude fit errormagphot.magVARCHARprincipalextinction_uu band extinctionmagphys.absorption.gal;em.opt.UVARCHARprincipalextinction_gg band extinctionmagphys.absorption.gal;em.opt.BVARCHARprincipalextinction_rr band extinctionmagphys.absorption.gal;em.opt.VVARCHARprincipalextinction_ii band extinctionmagphys.absorption.gal;em.opt.RVARCHARprincipalextinction_zz band extinctionmagphys.absorption.gal;em.opt.IVARCHARprincipalgama_pdr4v2.G02SpStandardsv01Standard stars from SDSS for the G02 survey regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR8 r band magnitude in 3 arcsec diameter fibermagphot.mag;em.opt.RVARCHARprincipalPSFMAG_RSDSS DR8 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalPRIORITY_CLASSSpectroscopic prioritymeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02TilingCatv07Science targets in the G02 survey region.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objid, -1 for no matchmeta.idVARCHARprincipalCOBJIDG02CFHTLSInputCat ID, xxx for no matchmeta.idVARCHARprincipalRAJ2000 coordinate, from G02CFHTLSInputCat if matchdegpos.eq.raVARCHARprincipalDECJ2000 coordinate, from G02CFHTLSInputCat if matchdegpos.eq.decVARCHARprincipalDIST_SDSSAngular distance between RA and DEC in this table and SDSS match, 9.99 for no matcharcsecpos.angDistanceVARCHARprincipalPRIORITY_CLASSPriorities for last targeting run, 9 high, 0 not a targetmeta.code.classVARCHARprincipalSURVEY_CLASS6=selected with SDSS and CFHTLenS; 5=selected with SDSS only; 4=selected with CFHTLenS only; 2=fillermeta.code.classVARCHARprincipalAREA_FLAG1 for DEC < -6, 2 for DEC > -6 = high-priority regionmeta.codeVARCHARprincipalFLAGS_SELECTSum of flags, 1 if mask=0, 2 if class_star<0.7 from CFHTLenS, 4 if passed SDSS star-galaxy separationmeta.code.memberVARCHARprincipalR_PETROExtinction-corrected r band SDSS Petrosian magnitude, 0 for no matchmagphot.mag;em.opt.RVARCHARprincipalR_AUTOExtinction-corrected r band CFHTLenS AUTO magnitude, 0 for no matchmagphot.mag;em.opt.RVARCHARprincipalR_MAGExtinction-corrected r bnd SDSS Petrosian or CFHTLenS AUTO magnitudemagphot.mag;em.opt.RVARCHARprincipalFIBERMAG_Rr band SDSS fibermag or CFHTLenS mag_aper12magphot.mag;em.opt.RVARCHARprincipalSURVEY_CODESurvey code for redshift source, see SpecCat notesmeta.code;meta.datasetVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalSPECIDID of spectrum from SpecCat tablemeta.id.cross;spectVARCHARprincipalVEL_ERRRedshift uncertainty, c delta ln(1+z)km/ssrc.redshift;stat.errorVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra within 1 arcsecmeta.numberVARCHARprincipalVIS_CLASSVisual classification, see notesmeta.code.qualVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02TilingExtrav03This is a table of extra galaxy targets in the G02 survey region.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalCOBJIDG02CFHTLSInputCat IDmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalXXL_FLAG1 if X-ray AGN target selected by Antonis Georgakakismeta.codeVARCHARprincipalR_MAGExtinction-corrected r band SDSS Petrosian or CFHTLenS AUTO magnitude, 22.5 for unknownmagphot.mag;em.opt.RVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23GalacticExtinctionv01This table provides the Galactic foreground extinction in all GALEX,SDSS (= KiDS), UKIDSS and VIKING bands for every object inG23InputCatAv01.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_B_MGCGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_uGalactic extinction in SDSS and KiDS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_gGalactic extinction in SDSS and KiDS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_rGalactic extinction in SDSS and KiDS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_iGalactic extinction in SDSS and KiDS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_zGalactic extinction in SDSS and KiDS z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_UKIDSSGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_UKIDSSGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_UKIDSSGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_UKIDSSGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_Z_VIKINGGalactic extinction in VIKING Z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_VIKINGGalactic extinction in VIKING Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_VIKINGGalactic extinction in VIKING J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_VIKINGGalactic extinction in VIKING H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_VIKINGGalactic extinction in VIKING K bandmagphys.absorption.gal;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23GuideStarsv01Guide stars for the G23 survey region.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalRA_SEPRA offset between GAMA object and matched ATLAS object (GAMA-ATLAS)arcsecpos.angDistanceVARCHARprincipalDEC_SEPDEC offset between GAMA object and matched ATLAS object (GAMA-ATLAS)arcsecpos.angDistanceVARCHARprincipalMAG_PETRO_Rr band Petrosian magnitude from ATLAS, not corrected for extinctionmagphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_Ii band Kron magnitude, not extinction correctedmagphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_ZZ band Kron magnitude, not extinction correctedmagphot.mag;em.optVARCHARprincipalMAG_AUTO_YY band Kron magnitude, not extinction correctedmagphot.mag;em.IR.NIRVARCHARprincipalMAG_AUTO_JJ band Kron magnitude, not extinction correctedmagphot.mag;em.IR.JVARCHARprincipalMAG_AUTO_HH band Kron magnitude, not extinction correctedmagphot.mag;em.IR.HVARCHARprincipalMAG_AUTO_KK band Kron magnitude, not extinction correctedmagphot.mag;em.IR.KVARCHARprincipalCLASS_STAR_Ii band stellaricitysrc.classVARCHARprincipalTYPEType of object: 1=galaxy, 2=star, 3=unknown, 4=artifactsrc.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23InputCatv06This is the GAMA II master input catalogue for the G23 survey regionbased on KiDS and VIKING data.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalNPIXMASKNumber of masked pixels in i-band detected objectmeta.code.qualVARCHARprincipalMAG_AUTO_Ii band Kron magnitude, not extinction correctedmagphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_ZZ band Kron magnitude, not extinction correctedmagphot.mag;em.optVARCHARprincipalMAG_AUTO_YY band Kron magnitude, not extinction correctedmagphot.mag;em.IR.NIRVARCHARprincipalMAG_AUTO_JJ band Kron magnitude, not extinction correctedmagphot.mag;em.IR.JVARCHARprincipalMAG_AUTO_HH band Kron magnitude, not extinction correctedmagphot.mag;em.opt.HVARCHARprincipalMAG_AUTO_KK band Kron magnitude, not extinction correctedmagphot.mag;em.IR.KVARCHARprincipalAPMAG_ZZ band 2 arcsec aperture magnitude, not extinction correctedmagphot.mag;em.optVARCHARprincipalMU_E_Ii band effective surface brightness, not extinction correctedmag/arcsec^2phot.mag.sb;em.opt.IVARCHARprincipalFLUX_RADIUS_Ii band half-light radiusarcsecphys.angSize;em.opt.IVARCHARprincipalMAG_NUVNUV magnitude from LAMBDAR, not extinction correctedmagphot.mag;em.UV.200-300nmVARCHARprincipalEXTINCTION_IGalactic extinction in i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalEXTINCTION_YGalactic extinction in Y bandmagphys.absorption.gal;em.optVARCHARprincipalEXTINCTION_ZGalactic extinction in Z bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalEXTINCTION_JGalactic extinction in J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalEXTINCTION_HGalactic extinction in H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalEXTINCTION_KGalactic extinction in K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalEXTINCTION_NUVGalactic extinction in NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalCLASS_STAR_Ii band stellaricitysrc.class;em.opt.IVARCHARprincipalCLASS_STAR_ZZ band stellaricitysrc.class;em.optVARCHARprincipalCLASS_STAR_YY band stellaricitysrc.class;em.IR.NIRVARCHARprincipalCLASS_STAR_JJ band stellaricitysrc.class;em.IR.JVARCHARprincipalCLASS_STAR_HH band stellaricitysrc.class;em.IR.HVARCHARprincipalCLASS_STAR_KK band stellaricitysrc.class;em.IR.KVARCHARprincipalMASK_IC_14Bright star masking flag (stars i < 14)src.classVARCHARprincipalMASK_IC_13Bright star masking flag (stars i < 13)src.classVARCHARprincipalMASK_IC_12Bright star masking flag (stars i < 12)src.classVARCHARprincipalMASK_IC_THBright star masking flag (Hipparcos/Tycho stars)src.classVARCHARprincipalSGSEP_JKOffset from J-K stellar locusmagVARCHARprincipalTYPEType of object: 1=galaxy, 2=star, 3=unknown, 4=artifactsrc.classVARCHARprincipalVIS_CLASSVisual classification, see notessrc.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LambdarWISEW3v01This catalogue contains the complete LAMBDAR output for the WISE W3 band.QuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.G23SpStandardsv01Standard stars from KiDS and VIKING data for the G23 survey region.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalMAG_AUTO_IKiDS auto i band magnitudemagphot.mag;em.opt.IVARCHARprincipalRMSDIFFDeviation of colours from fiducial point in RMS unitsmagphot.magVARCHARprincipalPRIORITY_CLASS2 or 3 depending on RMSDIFFmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23TilingCatv11Science targets in the G23 survey region.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalI_AUTOi band Kron magnitude, extinction correctedmagphot.mag;em.opt.IVARCHARprincipalZ_AUTOZ band Kron magnitude, extinction correctedmagphot.mag;em.optVARCHARprincipalY_AUTOY band Kron magnitude, extinction correctedmagphot.mag;em.IR.NIRVARCHARprincipalJ_AUTOJ band Kron magnitude, extinction correctedmagphot.mag;em.IR.JVARCHARprincipalH_AUTOH band Kron magnitude, extinction correctedmagphot.mag;em.IR.HVARCHARprincipalK_AUTOK band Kron magnitude, extinction correctedmagphot.mag;em.IR.KVARCHARprincipalAPMAG_ZZ band 2 arcsec aperture magnitudemagphot.mag;em.optVARCHARprincipalNUV_AUTONUV magnitude, extinction correctedmagphot.mag;em.UV.200-300nmVARCHARprincipalSURVEY_CODESurvey code for redshift source, see SpecCat DMUmeta.code;meta.datasetVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalSPECIDID of spectrum from SpecAll tablemeta.id.cross;spectVARCHARprincipalVEL_ERRRedshift uncertainty, c delta ln(1+z)km/ssrc.redshift;stat.errorVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra within 1 arcsecmeta.number;spectVARCHARprincipalTYPEType of object: 1=galaxy, 2=star, 3=unknown, 4=artifactmeta.numberVARCHARprincipalVIS_CLASSVisual classification, see notesmata.code.qualVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalPRIORITY_CLASSPriorities for targeting, see notesmeta.code.classVARCHARprincipalNEIGHBOUR_CLASSNumber of SURVEY_CLASS >= 3 targets within 40 arcsecmeta.code.classVARCHARprincipalAREA_FLAGSet to 1 for 2014 target region, 0 otherwisemeta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23TilingExtrav01Table of galaxy targets in G23 that are not (or no longer) mainsurvey targets.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalMAGMagnitude from the config filemagphot.magVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalexAdvancedMatchv02This catalogue contains the result of an advanced match betweenInputCatAv06 and GalexPhot. The matching procedure takes intoaccount the possibility of multiple matches between GALEX and GAMAobjects and seeks to reconstruct the original UV flux of a givenGAMA object. GAMA objects without a GALEX match are not included inthis catalogue.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalNMATCHUVNumber of GALEX objects involved in the matchingmeta.numberVARCHARprincipalNMATCHOPTNumber of GAMA objects involved in the matchingmeta.numberVARCHARprincipalUVIDXLISTID list of GALEX object used in the flux redistribution calculation using NAME from GalexPhot; string always ends with a commaVARCHARprincipalOPTIDXLISTID list of GAMA objects used in the flux redistribution calculation using SDSS OBJID; string always ends with a commaVARCHARprincipalNUVFLAGCombination of the NUV artifact flags of all GALEX objects involved in the matchingmeta.code;em.UV.200-300nmVARCHARprincipalFUVFLAGCombination of the FUV artifact flags of all GALEX objects involved in the matchingmeta.code;em.UV.100-200nmVARCHARprincipalFLUXTOT_NUVTotal NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXTOTERR_NUVTotal NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAGTOT_NUVTotal NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.200-300nmVARCHARprincipalMAGTOTERR_NUVTotal NUV AB magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXSPLIT_NUVRedistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXSPLITERR_NUVRedistributed NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAGSPLIT_NUVRedistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nmVARCHARprincipalMAGSPLITERR_NUVRedistributed NUV AB magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXTOT_FUVTotal FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXTOTERR_FUVTotal FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAGTOT_FUVTotal FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.100-200nmVARCHARprincipalMAGTOTERR_FUVTotal FUV AB magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXSPLIT_FUVRedistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXSPLITERR_FUVRedistributed FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAGSPLIT_FUVRedistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nmVARCHARprincipalMAGSPLITERR_FUVRedistributed FUV AB magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalexCoGPhotv02This catalogue provides GALEX NUV and FUV curve-of-growth photometryfor all objects in SersicCatv07 (covering only the GAMA I surveyregions).CATAID_IUnique GAMA I ID of GAMA object (see notes)meta.idVARCHARprincipalCATAIDUnique GAMA II ID of GAMA object (see notes)meta.idVARCHARprincipalCPS_NUVNUV counts per secondcounts/sphot.count;em.UV.200-300nmVARCHARprincipalCPSERR_NUVNUV counts per second errorcounts/sphot.count;em.UV.200-300nm;stat.errorVARCHARprincipalFLUX_NUVNUV fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXERR_NUVNUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_NUVNUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalMAGERR_NUVNUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalRE_CRIT_NUVNUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalHP_RAD_NUVNUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCONFSOURCE_NUVNUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCPS_FUVFUV counts per secondcounts/sphot.count;em.UV.100-200nmVARCHARprincipalCPSERR_FUVFUV counts per second errorcounts/sphot.count;em.UV.100-200nm;stat.errorVARCHARprincipalFLUX_FUVFUV fluxmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXERR_FUVFUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAG_FUVFUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalMAGERR_FUVFUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalRE_CRIT_FUVFUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalHP_RAD_FUVFUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCONFSOURCE_FUVFUV flag indicating whether masking occurredmeta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalexObsInfov02This catalogue provides basic GALEX observational information,i.e. exposure times, background levels and detection limits, for allobjects in InputCatAv06.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalBKGRND_FLUX_NUVNUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.200-300nm;src.netVARCHARprincipalBKGRND_FLUX_FUVFUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.100-200nm;src.netVARCHARprincipalNUVFLUXLIMIT2p5S/N=2.5 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalFUVFLUXLIMIT2p5S/N=2.5 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalNUVMAGLIMIT2p5S/N=2.5 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalFUVMAGLIMIT2p5S/N=2.5 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalNUVFLUXLIMIT5S/N=5 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalFUVFLUXLIMIT5S/N=5 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalNUVMAGLIMIT5S/N=5 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalFUVMAGLIMIT5S/N=5 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalNUVFLUXLIMIT10S/N=10 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalFUVFLUXLIMIT10S/N=10 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalNUVMAGLIMIT10S/N=10 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalFUVMAGLIMIT10S/N=10 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalexPhotv02This catalogue provides GALEX NUV and FUV photometry for primarysources with S/N_NUV >= 2.5 in the GAMA II equatorial surveyregions. This photometry was derived using the GALEXSExtractor-based pipeline.GGOIDGALEX Global Object IDmeta.idVARCHARprincipalNUMBER_MCATRunning object number from GALEX MCAT filemeta.idVARCHARprincipalNAMEObject IAU format namemeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalGLONGalactic longitudedegpos.galactic.lonVARCHARprincipalGLATGalactic latitudedegpos.galactic.latVARCHARprincipalPOSERRPosition errorarcsecstat.errorVARCHARprincipalTILENUMGALEX tile numbermeta.numberVARCHARprincipalTILEGALEX tile namemeta.idVARCHARprincipalFOV_RADIUSDistance of object from centre of FoVdegpos.angDistanceVARCHARprincipalHP_PIXELHEALPix pixel on sky coverage maps on GALEX-GAMA web site (nside = 16384; nested)VARCHARprincipalEXPTIME_NUVNUV exposure time of tilesobs.exposure;em.UV.200-300nmVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEXPTIME_FUVFUV exposure time of tilesobs.exposure;em.UV.100-200nmVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalFLUX_NUVNUV calibrated fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXERR_NUVNUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_NUVNUV calibrated AB Kron magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalMAGERR_NUVNUV calibrated AB Kron magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalS2N_NUVNUV signal-to-noise from flux valuestat.snr;em.UV.200-300nmVARCHARprincipalARTIFACT_NUVNUV artifact flag (see notes)meta.code;em.UV.200-300nmVARCHARprincipalBKGRND_FLUX_NUVNUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.200-300nm;src.netVARCHARprincipalBKGRND_MAG_NUVNUV sky background surface brightnessmag/arcsec^2phot.mag;em.UV.200-300nm;src.netVARCHARprincipalFLUX_FUVFUV calibrated flux using NUV aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXERR_FUVFUV flux error using NUV aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAG_FUVFUV calibrated AB Kron magnitude using NUV aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAGERR_FUVFUV calibrated AB Kron magnitude error using NUV aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalS2N_FUVFUV signal-to-noise from flux value (NB: can become negative for negative flux)stat.snr;em.UV.100-200nmVARCHARprincipalARTIFACT_FUVFUV artifact flag (see notes)meta.code;em.UV.100-200nmVARCHARprincipalBKGRND_FLUX_FUVFUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.100-200nm;src.netVARCHARprincipalBKGRND_MAG_FUVFUV sky background surface brightnessmag/arcsec^2phot.mag;em.UV.100-200nm;src.netVARCHARprincipalFLUX_D3p0_NUVNUV flux in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D4p5_NUVNUV flux in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D7p5_NUVNUV flux in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D12p0_NUVNUV flux in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D18p0_NUVNUV flux in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D25p5_NUVNUV flux in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D34p5_NUVNUV flux in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXERR_D3p0_NUVNUV flux error in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D4p5_NUVNUV flux error in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D7p5_NUVNUV flux error in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D12p0_NUVNUV flux error in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D18p0_NUVNUV flux error in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D25p5_NUVNUV flux error in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D34p5_NUVNUV flux error in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_D3p0_NUVNUV AB magnitude in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D4p5_NUVNUV AB magnitude in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D7p5_NUVNUV AB magnitude in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D12p0_NUVNUV AB magnitude in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D18p0_NUVNUV AB magnitude in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D25p5_NUVNUV AB magnitude in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D34p5_NUVNUV AB magnitude in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAGERR_D3p0_NUVNUV AB magnitude error in 3.0 arcsec (2 pixel)diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D4p5_NUVNUV AB magnitude error in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D7p5_NUVNUV AB magnitude error in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D12p0_NUVNUV AB magnitude error in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D18p0_NUVNUV AB magnitude error in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D25p5_NUVNUV AB magnitude error in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D34p5_NUVNUV AB magnitude error in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalFLUX20_RADIUS_NUVNUV 20 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX50_RADIUS_NUVNUV 50 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX80_RADIUS_NUVNUV 80 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX90_RADIUS_NUVNUV 90 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX95_RADIUS_NUVNUV 95 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX_MAX_NUVNUV peak flux above backgroundmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalX_IMAGEObject pixel position on intensity mapspixelVARCHARprincipalY_IMAGEObject pixel position on intensity mapspixelVARCHARprincipalXPEAK_IMAGEPixel position of the brightest NUV pixel on intensity mapspixelVARCHARprincipalYPEAK_IMAGEPixel position of the brightest NUV pixel on intensity mapspixelVARCHARprincipalSEMIMAJORSemimajor axisarcsecphys.size.radiusVARCHARprincipalSEMIMINORSemiminor axisarcsecphys.size.radiusVARCHARprincipalSEMIMAJORERRSemimajor axis errorarcsecphys.size.radius;stat.errorVARCHARprincipalSEMIMINORERRSemiminor axis errorarcsecphys.size.radius;stat.errorVARCHARprincipalPOSANGPosition angle (east of north)degpos.posAngVARCHARprincipalPOSANGERRPosition angle errordegpos.posAng;stat.errorVARCHARprincipalFWHM_NUVNUV FWHM assuming a gaussian corearcsecphys.size;em.UV.200-300nmVARCHARprincipalFLAGS_NUVNUV Sextraxtor extraction flagsmeta.code;em.UV.200-300nmVARCHARprincipalCLASS_STARNUV Sextractor star/galaxy classifier outputmeta.code;em.UV.200-300nmVARCHARprincipalFLUX_D3p0_FUVFUV flux in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D4p5_FUVFUV flux in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D7p5_FUVFUV flux in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D12p0_FUVFUV flux in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D18p0_FUVFUV flux in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D25p5_FUVFUV flux in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D34p5_FUVFUV flux in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXERR_D3p0_FUVFUV flux error in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D4p5_FUVFUV flux error in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D7p5_FUVFUV flux error in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D12p0_FUVFUV flux error in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D18p0_FUVFUV flux error in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D25p5_FUVFUV flux error in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D34p5_FUVFUV flux error in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAG_D3p0_FUVFUV AB magnitude in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D4p5_FUVFUV AB magnitude in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D7p5_FUVFUV AB magnitude in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D12p0_FUVFUV AB magnitude in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D18p0_FUVFUV AB magnitude in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D25p5_FUVFUV AB magnitude in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D34p5_FUVFUV AB magnitude in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAGERR_D3p0_FUVFUV AB magnitude error in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D4p5_FUVFUV AB magnitude error in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D7p5_FUVFUV AB magnitude error in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D12p0_FUVFUV AB magnitude error in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D18p0_FUVFUV AB magnitude error in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D25p5_FUVFUV AB magnitude error in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D34p5_FUVFUV AB magnitude error in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalFLUX20_RADIUS_FUVFUV 20 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX50_RADIUS_FUVFUV 50 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX80_RADIUS_FUVFUV 80 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX90_RADIUS_FUVFUV 90 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX95_RADIUS_FUVFUV 95 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX_MAX_FUVFUV peak flux above backgroundmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFWHM_FUVFUV FWHM assuming a gaussian corearcsecphys.size;em.UV.100-200nmVARCHARprincipalFLAGS_FUVFUV Sextraxtor extraction flagsmeta.code;em.UV.100-200nmVARCHARprincipalgama_pdr4v2.LambdarWISEW4v01This catalogue contains the complete LAMBDAR output for the WISE W4 band.NumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.GalexSimpleMatchv02This catalogue contains the result of a simple nearest neighbourmatch between InputCatAv06 and GalexPhot. GAMA objects without aGALEX nearest neighbour within a distance of 4 arcsec are consideredunmatched and are not included in this catalogue.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objid of GAMA objectmeta.idVARCHARprincipalGGOIDGlobal Object ID of nearest neighbour GALEX objectmeta.idVARCHARprincipalFUVMATCHFlag indicating whether matched GALEX source has FUV flux with S/N >=2.5 (-1=no FUV data)meta.code;em.UV.100-200nmVARCHARprincipalNN_DISTDistance between GAMA object and nearest neighbour GALEX objectarcsecpos.angDistanceVARCHARprincipalNMATCH4Number of GALEX objects found within 4 arcsec of GAMA objectmeta.numberVARCHARprincipalMANY2ONENumber of GAMA objects the GALEX object is matched tometa.numberVARCHARprincipalGNEIGHBOR_DISTString list of distances to all GALEX sources within 20 arcsecVARCHARprincipalGNEIGHBOR_NAMEString list of names of all GALEX sources within 20 arcsecVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalexMainv02This is the main catalogue of the GalexPhotometry DMU. It reproducesthe most important information from the other catalogues in this DMUand provides a best estimate of the NUV and FUV fluxes of all GAMAobjects in the GAMA II equatorial survey regions that were detectedby GALEX.The following columns contain the output of the advanced matching procedureThe following columns contain the result of our CoG photometryThe following columns refer to the GAMA object's nearest neighbour GALEX objectCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRARight Ascension of GAMA object (J2000)degpos.eq.raVARCHARprincipalDECDeclination of GAMA object (J2000)degpos.eq.decVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalBEST_FLUX_NUVBest estimate of the GAMA object's NUV fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalBEST_FLUXERR_NUVBest estimate NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalBEST_MAG_NUVBest estimate of the GAMA object's NUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalBEST_MAGERR_NUVBest estimate NUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalBEST_FLUX_FUVBest estimate of the GAMA object's FUV fluxmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalBEST_FLUXERR_FUVBest estimate FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalBEST_MAG_FUVBest estimate of the GAMA object's FUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalBEST_MAGERR_FUVBest estimate FUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalBEST_METHODMethod used for the best flux estimates (AdvancedMatch or CoG)meta.codeVARCHARprincipalNMATCHUVNumber of GALEX objects involved in advanced matching proceduremeta.numberVARCHARprincipalNMATCHOPTNumber of GAMA objects involved in advanced matching proceduremeta.numberVARCHARprincipalNUVFLAGCombination of the NUV artifact flags of all GALEX objects involved in advanced matching proceduremeta.code;em.UV.200-300nmVARCHARprincipalFUVFLAGCombination of the FUV artifact flags of all GALEX objects involved in advanced matching proceduremeta.code;em.UV.100-200nmVARCHARprincipalTOT_FLUX_NUVTotal NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.200-300nmVARCHARprincipalTOT_FLUXERR_NUVError on the total NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalTOT_MAG_NUVTotal NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.200-300nmVARCHARprincipalTOT_MAGERR_NUVError on total NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalTOT_FLUX_FUVTotal FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.100-200nmVARCHARprincipalTOT_FLUXERR_FUVError on total FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalTOT_MAG_FUVTotal FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.100-200nmVARCHARprincipalTOT_MAGERR_FUVError on total FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalSPLIT_FLUX_NUVRedistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalSPLIT_FLUXERR_NUVError on redistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalSPLIT_MAG_NUVRedistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nmVARCHARprincipalSPLIT_MAGERR_NUVError on redistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalSPLIT_FLUX_FUVRedistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalSPLIT_FLUXERR_FUVError on redistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalSPLIT_MAG_FUVRedistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nmVARCHARprincipalSPLIT_MAGERR_FUVError on redistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_FLUX_NUVCoG NUV flux at the position of the GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalCOG_FLUXERR_NUVCoG NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalCOG_MAG_NUVCoG NUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalCOG_MAGERR_NUVCoG NUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalCOG_FLUX_FUVCoG FUV flux at the position of the GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalCOG_FLUXERR_FUVCoG FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_MAG_FUVCoG FUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalCOG_MAGERR_FUVCoG FUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_RE_CRIT_NUVCoG NUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCOG_HP_RAD_NUVCoG NUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCOG_RE_CRIT_FUVCoG FUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCOG_HP_RAD_FUVCoG FUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCOG_CONFSOURCE_NUVCoG NUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCOG_CONFSOURCE_FUVCoG FUV flag indicating whether masking occurredmeta.codeVARCHARprincipalNN_GGOIDGlobal Object ID of nearest neighbour GALEX objectmeta.idVARCHARprincipalNN_RA_GALEXRight Ascension of nearest neighbour GALEX object (J2000)degpos.eq.raVARCHARprincipalNN_DEC_GALEXDeclination of nearest neighbour GALEX object (J2000)degpos.eq.decVARCHARprincipalNN_DISTDistance between GAMA object and nearest neighbour GALEX objectarcsecpos.angDistanceVARCHARprincipalNN_NMATCH4Number of GALEX objects found within 4 arcsec of GAMA objectmeta.numberVARCHARprincipalNN_MANY2ONENumber of GAMA objects the nearest neighbour GALEX object is matched tometa.numberVARCHARprincipalNN_FLUX_NUVNUV flux of nearest neighbour GALEX objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalNN_FLUXERR_NUVNUV flux error of nearest neighbour GALEX objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalNN_MAG_NUVNUV AB Kron magnitude of nearest neighbour GALEX objectmagphot.mag;em.UV.200-300nmVARCHARprincipalNN_MAGERR_NUVNUV AB Kron magnitude error of nearest neighbour GALEX objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalNN_FLUX_FUVFUV flux of nearest neighbour GALEX object using NUV aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalNN_FLUXERR_FUVFUV flux error of nearest neighbour GALEX object using NUV aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalNN_MAG_FUVFUV AB Kron magnitude of nearest neighbour GALEX object using NUV aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalNN_MAGERR_FUVFUV AB Kron magnitude error of nearest neighbour GALEX object using NUV aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalNN_ARTIFACT_NUVNUV artifact flag of nearest neighbour GALEX object (see GalexPhot notes)meta.code;em.UV.200-300nmVARCHARprincipalNN_ARTIFACT_FUVFUV artifact flag of nearest neighbour GALEX object (see GalexPhot notes)meta.code;em.UV.100-200nmVARCHARprincipalNN_SFLAGS_NUVNUV Sextraxtor extraction flags of nearest neighbour GALEX objectmeta.code;em.UV.200-300nmVARCHARprincipalNN_SFLAGS_FUVFUV Sextraxtor extraction flags of nearest neighbour GALEX objectmeta.code;em.UV.100-200nmVARCHARprincipalNN_FLUX50_RADIUS_NUVNUV 50 percent fraction-of-light radius of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_FLUX50_RADIUS_FUVFUV 50 percent fraction-of-light radius of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalNN_SEMIMAJOR_NUVNUV semimajor axis of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_SEMIMINOR_NUVNUV semiminor axis of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_SEMIMAJORERR_NUVNUV semimajor axis error of nearest neighbour GALEX objectarcsecphys.size.radius;stat.errorVARCHARprincipalNN_SEMIMINORERR_NUVNUV semiminor axis error of nearest neighbour GALEX objectarcsecphys.size.radius;stat.errorVARCHARprincipalNN_POSANG_NUVNUV position angle (east of north) of nearest neighbour GALEX objectdegpos.posAngVARCHARprincipalNN_POSANGERR_NUVNUV position angle error of nearest neighbour GALEX objectdegpos.posAng;stat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GalaxiesClassifiedv01This table classifies the geometric environment of galaxies aseither a void, sheet, filament or knot.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARA of galaxy (J2000)degpos.eq.raVARCHARprincipalDECDEC of galaxy (J2000)degpos.eq.decVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQRedshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalGeoS4Geometric environment of galaxy computed with 4 Mpc/h smoothingmeta.code.classVARCHARprincipalGeoS10Geometric environment of galaxy computed with 10 Mpc/h smoothingmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GeometricGridv01This table lists the geometric environment classification of eachcell of a cartesian mesh on the GAMA II equatorial survey regions.CellIDUnique cell IDmeta.idVARCHARprincipalRARA of the centre of the mesh celldegpos.eq.raVARCHARprincipalDECDEC of the centre of the mesh celldegpos.eq.decVARCHARprincipalZRedshift of the centre of the mesh cellsrc.redshiftVARCHARprincipalGeoS4Geometric environment classification of cell computed with 4 Mpc/h smoothingmeta.code.classVARCHARprincipalGeoS10Geometric environment classification of cell computed with 10 Mpc/h smoothingmeta.code.classVARCHARprincipalgama_pdr4v2.GroupsClassifiedv01This table classifies the geometric environment of groups as eithera void, sheet, filament or knot.GroupIDUnique group IDmeta.idVARCHARprincipalRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalDECDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalZRedshift of the iterative central galaxysrc.redshiftVARCHARprincipalGeoS4Geometric environment of group computed with 4 Mpc/h smoothingmeta.code.classVARCHARprincipalGeoS10Geometric environment of group computed with 10 Mpc/h smoothingmeta.code.classVARCHARprincipalgama_pdr4v2.G3CFoFGroupv10This is a catalogue of the galaxy group properties in the GAMA IIequatorial and G02 survey regions.GroupIDUnique group ID, as listed in the associated G3CGal linksmeta.id;meta.mainVARCHARindexedprincipalNfofGroup multiplicityVARCHARprincipalIterCenCATAIDReference ID of the iterative central galaxy (preferred position of the group centre)meta.idVARCHARprincipalIterCenRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalIterCenDecDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalIterCenZRedshift of the iterative central galaxysrc.redshiftVARCHARprincipalZfofMedian redshift of the groupsrc.redshiftVARCHARprincipalRad50Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenIDMpc/hphys.size.radiusVARCHARprincipalRad1SigGroup radius defined by the 68th percentile group member, based on the projected distance away from IterCenIDMpc/hphys.size.radiusVARCHARprincipalRad100Group radius defined by the most distant group member, based on the projected distance away from IterCenIDMpc/hphys.size.radiusVARCHARprincipalRelDenRelative galaxy space density (w.r.t. prediction based on the random catalogues) within a cylinder of radius 1.5Mpc/h and offset 18Mpc/h (i.e. diameter 3.0Mpc/h and total length 36Mpc/h) centred on IterCenIDVARCHARprincipalZcompAverage redshift completeness of the group: for each group member the redshift completeness within a projected 1.5Mpc/h radius (at the position of the galaxy) is estimated and then averaged over all group members to provide ZCompVARCHARprincipalGroupEdgeFraction of the group within the survey volume, as estimated from IterCen and Rad100VARCHARprincipalVelDispGroup velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRawkm/sphys.velocVARCHARprincipalVelDispRawRaw group velocity dispersionkm/sphys.velocVARCHARprincipalVelErrTotal group velocity errorkm/sphys.velocVARCHARprincipalTotRmagr-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its membersmag-5log(h)phys.magAbsVARCHARprincipalTotFluxProxyProxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on the total observed r-band flux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift; value listed corresponds to B=1 in Eq. 22 of Robotham et al. (2011)VARCHARprincipalMassProxyProxy for dynamical group mass estimated via M \propto Rad50 * VelDisp^2; value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)VARCHARprincipalBCGCATAIDGAMA ID of BCGmeta.idVARCHARprincipalBCGRARA of BCG (J2000)degpos.eq.raVARCHARprincipalBCGDecDec of BCG (J2000)degpos.eq.decVARCHARprincipalRgapApparent r-band magnitude gap between BCG and second brightest group membermagphot.magVARCHARprincipalCenRARA of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.raVARCHARprincipalCenDecDec of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.decVARCHARprincipalRadKurtUnbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCenVARCHARprincipalAxAngAngle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1980) algorithm (0<=AxAng<=180, requires 3 or more members, so -999 otherwise)degpos.posAngVARCHARprincipalAxRatAxial ratio of the minor and major axes of the group using the Carter & Metcalfe (1980) algorithm (0<=AxRat<=1, requires 3 or more members, so -999 otherwise)phys.size.axisRatioVARCHARprincipalSymKSKS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)VARCHARprincipalVelSkewUnbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)VARCHARprincipalVelKurtUnbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)VARCHARprincipalModalityModality of the system: (1+VelSkew^2)/(3+VelKurt^2); this will be 1/3 for a normal distribution and 0.555 for a uniform oneVARCHARprincipalLinkTotTotal number of FoF links in the systemVARCHARprincipalLinkStrenProjLink strength in projection, 1 minus the average projected FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenProj<=1), i.e. larger values mean a stronger linkVARCHARprincipalLinkStrenRadLink strength radially, 1 minus the average radial FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenZ<=1), i.e. larger values mean a stronger linkVARCHARprincipalLinkStrenCombLink strength combined, the average of LinkStrenProj*LinkStrenZ for all the links in the group (0<=LinkStrenComb<=1), i.e. larger values mean a stronger linkVARCHARprincipalMassAMass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)Msun/hphys.massVARCHARprincipalMassAfuncMass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)Msun/hphys.massVARCHARprincipalLumBTotFluxProxy times the global B factor required to get a median unbaised r-band luminosity estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)Lsun/h^2phys.luminosityVARCHARprincipalLumBfuncTotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)Lsun/h^2phys.luminosityVARCHARprincipald3vol3D convex hull volume in comoving units (only for Nfof>=4, -999 otherwise)(Mpc/h)^3VARCHARprincipald3areaSurface area of the 3D convex hull in comoving units (only for Nfof>=4, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipald2radecProjected area of the hull in the ra dec plane in comoving units (only for Nfof>=3, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipald2razProjected area of the hull in the ra redshift plane in comoving units (only for Nfof>=3, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipald2deczProjected area of the hull in the dec rdshift plane in comoving Mpc units (only for Nfof>=3, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipaldistortcircReflects how non-circular the group projection appears to be, see notes, (only for Nfof>=3, -999 otherwise)VARCHARprincipaldistortellipReflects how non-elliptical the group appears to be, see notes, (only for Nfof>=4, -999 otherwise)VARCHARprincipaldistortsphReflects how non-spherical the system appears to be, see notes, (only for Nfof>=4, -999 otherwise)VARCHARprincipalURL_IMGURL of the group's imagemeta.ref.url;meta.fileVARCHARprincipalgama_pdr4v2.G3CGalPairv10Catalogue of all galaxy pairs with a projected physical separationof 100 kpc/h and a velocity separation of 1000 km/s.PairIDUnique pair IDmeta.id;meta.mainVARCHARindexedprincipalCATAID1CATAID of galaxy 1 in G3CGalmeta.idVARCHARprincipalCATAID2CATAID of galaxy 2 in G3CGalmeta.idVARCHARprincipalSepProjAngPhysical projected separation between galaxy 1 and galaxy 2kpc/hpos.distanceVARCHARprincipalSepVelVelocity separation of galaxy 1 and galaxy 2km/sphys.velocVARCHARprincipalRAbarRA of the r-band (petro) flux weighted centre-of-light of the pairdegpos.eq.raVARCHARprincipalDecbarDec of the r-band (petro) flux weighted centre-of-light of the pairdegpos.eq.decVARCHARprincipalZbarRedshift of the r-band (petro) flux weighted centre-of-light of the pairsrc.redshiftVARCHARprincipalMagSumTotal r-band (petro) apparent magnitude of the pairmagphot.magVARCHARprincipalgama_pdr4v2.G3CGalv10Catalogue of all GAMA galaxies used in the G3C GroupFinding DMU.CATAIDGAMA CATAIDmeta.id;meta.mainVARCHARindexedprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDecDeclination (J2000)degpos.eq.decVARCHARprincipalZRedshift in CMB framesrc.redshiftVARCHARprincipalRpetroPetrosian apparent r-band magnitude (AB, extinction corrected) [GAMA selection magnitude]magphot.magVARCHARprincipalDM_100_25_75Distance modulus using H0=100km/s/Mpc, Omega_m=0.25 and Omega_L=0.75magphot.mag.distModVARCHARprincipalSURVEY_CODESource for redshift: 1=SDSS, 2=2dFGRS, 3=MGC, 4=2SLAQ-LRG, 5=GAMA, 6=6dFGS, 7=UZC, 8=2QZ, 9=2SLAQ-QSO, 10=NED, 11=GAMA-LT, 12=WiggleZVARCHARprincipalSigErrVelocity uncertainty (on redshift): assumed to be 30km/s for SDSS, 50km/s for GAMA and 80km/s for 2dFGRSkm/sphys.velocVARCHARprincipalGroupIDGroupID for this galaxy in G3CFoFGroup, 0 is un-groupedmeta.idVARCHARprincipalRankIterCenRelative rank of the galaxy to the RA and Dec of the group 'IterCen' coordinates, where 1 indicates closest and 2 second closest etcVARCHARprincipalSepIterCenProjected angular separation of the galaxy to the RA and Dec of the group 'IterCen' coordinatesarcsecphys.angSizeVARCHARprincipalCoSepIterCenProjected comoving distance separation of the galaxy to the RA and Dec of the group 'IterCen' coordinatesMpc/hphys.size.radiusVARCHARprincipalAngSepIterCenProjected angular size distance (comoving/(1+z)) separation of the galaxy to the RA and Dec of the group 'IterCen' coordinatesMpc/hphys.size.radiusVARCHARprincipalRankBCGRelative rank of the galaxy to the RA and Dec of the group 'BCG' coordinates, where 1 indicates closest and 2 second closest etcVARCHARprincipalSepBCGProjected angular separation of the galaxy to the RA and Dec of the group 'BCG' coordinatesarcsecphys.angSizeVARCHARprincipalCoSepBCGProjected comoving distance separation of the galaxy to the RA and Dec of the group 'BCG' coordinatesMpc/hphys.size.radiusVARCHARprincipalAngSepBCGProjected angular size distance (comoving/(1+z)) separation of the galaxy to the RA and Dec of the group 'BCG' coordinatesMpc/hphys.size.radiusVARCHARprincipalRankCenRelative rank of the galaxy to the RA and Dec of the group 'Cen' coordinates, where 1 indicates closest and 2 second closest etcVARCHARprincipalSepCenProjected angular separation of the galaxy to the RA and Dec of the group 'Cen' coordinatesarcsecphys.angSizeVARCHARprincipalCoSepCenProjected comoving distance separation of the galaxy to the RA and Dec of the group 'Cen' coordinatesMpc/hphys.size.radiusVARCHARprincipalAngSepCenProjected angular size distance (comoving/(1+z)) separation of the galaxy to the RA and Dec of the group 'Cen' coordinatesMpc/hphys.size.radiusVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G3CLinkv10Catalogue that gives linking between all GAMA galaxies that share acommon group in G3CFoFGroup.LinkIDUnique linking IDmeta.id;meta.mainVARCHARindexedprincipalGal1CATAIDCATAID of galaxy 1 in G3CGalmeta.idVARCHARprincipalGal2CATAIDCATAID of galaxy 2 in G3CGalmeta.idVARCHARprincipalSepProjCoProjected separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hpos.distanceVARCHARprincipalLimProjCoMaximum allowed projected separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimProjCo>=SepProjCo)kpc/hpos.distanceVARCHARprincipalSepRadCoRadial separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hpos.distanceVARCHARprincipalLimRadCoMaximum allowed radial separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimRadCo>=SepRadCo)kpc/hpos.distanceVARCHARprincipalgama_pdr4v2.HATLASCatv03This catalogue provides Herschel SPIRE and PACS photometry ofHerschel sources matched to GAMA objects in the GAMA II equatorialsurvey regions.EXTINCTION_RSDSS r band extinctionVARCHARprincipalU_KRONextinction-corrected gama kron u magVARCHARprincipalG_KRONextinction-corrected gama kron g magVARCHARprincipalR_KRONextinction-corrected gama kron r magVARCHARprincipalI_KRONextinction-corrected gama kron i magVARCHARprincipalZ_KRONextinction-corrected gama kron z magVARCHARprincipalY_KRONextinction-corrected gama kron y magVARCHARprincipalJ_KRONextinction-corrected gama kron j magVARCHARprincipalH_KRONextinction-corrected gama kron h magVARCHARprincipalK_KRONextinction-corrected gama kron k magVARCHARprincipalU_KRON_ERRgama kron u mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalG_KRON_ERRgama kron g mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalR_KRON_ERRgama kron r mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalI_KRON_ERRgama kron i mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalZ_KRON_ERRgama kron z mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalY_KRON_ERRgama kron y mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalJ_KRON_ERRgama kron j mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalH_KRON_ERRgama kron h mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalK_KRON_ERRgama kron k mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalUKIDSS_LAS_IDSource ID for UKIDSS LAS detections in YJHKVARCHARprincipalCATAIDGAMA catalogue indexVARCHARprincipalHATLAS_IAU_IDHATLAS IAU identifier from the 250 micron positionVARCHARprincipalSOURCE_IDGAMA catalogue identifier. The * indicates which field a source lies inVARCHARprincipalRA_J2000RA (J2000), determined from the 250 micron data (degrees)VARCHARprincipalDEC_J2000Declination (J2000), determined from the 250 micron data (degrees)VARCHARprincipalF250_PPoint source 250 micron flux (Jy)VARCHARprincipalF350_PPoint source 350 micron flux (Jy)VARCHARprincipalF500_PPoint source 500 micron flux (Jy)VARCHARprincipalE250_PPoint source 250 micron 1 sigma error (Jy)VARCHARprincipalE350_PPoint source 350 micron 1 sigma error (Jy)VARCHARprincipalE500_PPoint source 500 micron 1 sigma error (Jy)VARCHARprincipalF250_BESTBest 250 micron flux, either point source or aperture value (Jy) (see README for more information)VARCHARprincipalF350_BESTBest 350 micron flux, either point source or aperture value (Jy) (see README for more information)VARCHARprincipalF500_BESTBest 500 micron flux, either point source or aperture value (Jy) (see README for more information)VARCHARprincipalE250_BESTBest 250 micron 1 sigma flux error (Jy)VARCHARprincipalE350_BESTBest 350 micron 1 sigma flux error (Jy)VARCHARprincipalE500_BESTBest 500 micron 1 sigma flux error (Jy)VARCHARprincipalAP_F250Aperture radius used for aperture flux in F250_BEST if source is extended (arcsec). A value of -99 indicates F250_BEST = F250_PVARCHARprincipalAP_F350Aperture radius used for aperture flux in F350_BEST if source is extended (arcsec). A value of -99 indicates F350_BEST = F350_PVARCHARprincipalAP_F500Aperture radius used for aperture flux in F500_BEST if source is extended (arcsec). A value of -99 indicates F500_BEST = F500_PVARCHARprincipalFLAGIf FLAG = 1 the aperture flux value was measured by hand. See extended_apertures.dat for details of ellipticity if a non-circular aperture was usedVARCHARprincipalF100_BESTBest 100 micron flux, either point or aperture value (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalF160_BESTBest 160 micron flux, either point or aperture value (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalE100_BESTBest 100 micron 1 sigma error (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalE160_BESTBest 160 micron 1 sigma error (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalAP_F100Aperture radius used for PACS flux in F100_BEST (arcsec)VARCHARprincipalAP_F160Aperture radius used for PACS flux in F160_BEST (arcsec)VARCHARprincipalSDSS_OBJIDSDSS DR7 OBJIDVARCHARprincipalSDSS_RASDSS DR7 Right Ascension (J2000, double precision)VARCHARprincipalSDSS_DECSDSS DR7 Declination (J2000, double precision)VARCHARprincipalSDSS_RMODELMAGSDSS DR7 r band model magVARCHARprincipalSDSS_RMODELMAG_ERRSDSS DR7 r band model mag errorVARCHARprincipalSDSS_ISOASDSS DR7 isophotal major axis, used for extended source SPIRE/PACS aperture fluxesVARCHARprincipalSDSS_SEPSeparation between 250um and SDSS DR7 positionsVARCHARprincipalLRLikelihood ratioVARCHARprincipalRELIABILITYReliability (R>=0.8 is to be treated as reliable)VARCHARprincipalID_FLAGFlag indicating if reliability has been changed or if other warnings are required (m=merger,r=resolved source,s=affected by star or SSGEP changed)VARCHARprincipalSGSEPStar/Gal separation (0 = Gal, 1=unresolved)VARCHARprincipalPHOTOZPhotometric redshifts from ANNz by Dave Bonfield (Smith et al., 2011, arXiv:1007.5260)VARCHARprincipalPHOTOZERRError on photometric redshift from ANNz (Smith et al., 2011, arXiv:1007.5260)VARCHARprincipalPHOTOZBANDS_STRINGString containing the bands used to derive the photozVARCHARprincipalPHOTOZBANDS_INTInteger showing which bands are present for deriving photozVARCHARprincipalPHOTOZBANDS_COUNTNumber of bands used in deriving photozVARCHARprincipalZ_SPECThe spectroscopic redshiftVARCHARprincipalZ_QUALThe z_spec quality flag (only use z_qual >= 3, as these have at least 90% reliability)VARCHARprincipalZFLAGFlag indicating the source of the redshift (1=SDSS, 5=GAMA)VARCHARprincipalGAMA_IAU_IDGAMA IAU IDVARCHARprincipalGAMA_RAGAMA RA (J2000)VARCHARprincipalGAMA_DECGAMA Dec (J2000)VARCHARprincipalR_PETROPetrosian r band mag from GAMAVARCHARprincipalBEST_MAG_NUV_EXCORExtinction-corrected Best estimate NUV magnitudeVARCHARprincipalBEST_MAGERR_NUVBest estimate NUV magnitude errorVARCHARprincipalBEST_MAG_FUV_EXCORExtinction-corrected Best estimate FUV magnitudeVARCHARprincipalBEST_MAGERR_FUVBest estimate FUV magnitude errorVARCHARprincipalEBVE(B-V)VARCHARprincipalNUVMAGLIMIT5_EXCORGALEX NUV 5-sigma detection limit for a circular source with default radius 3.4", or radius GAL_RE_R if greaterVARCHARprincipalFUVMAGLIMIT5_EXCORGALEX FUV 5-sigma detection limit for a circular source with default radius 3.4", or radius GAL_RE_R if greaterVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LTRedshiftsv01Liverpool Telescope FrodoSpec redshifts of a small number of veryfibre-bright targets. There should normally be no need to use thistable.SPECIDID made from LTF and date and timemeta.id;meta.mainVARCHARindexedprincipalCATAIDCATAIDmeta.id.cross;srcVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalTEMPLATESDSS template number see notesmeta.codeVARCHARprincipalCC_SIGMACross-correlation sigma see notesVARCHARprincipalQUALITYRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LambdarCatv01This is the main catalogue of the LambdarPhotometry DMU. It containsthe final 21-band fluxes and uncertainties, measured using theLAMBDAR program, in the three GAMA II equatorial survey regions. Thefluxes for each object are aperture-matched and deblended, and thevariations of the PSF and pixel scale across the various bands arecorrectly accounted for.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight Ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalFUV_fluxExtinction corrected GALEX FUV fluxJyphot.flux.density;em.UV.100-200nmVARCHARprincipalFUV_fluxerrError in extinction corrected GALEX FUV fluxJyphot.flux.density;em.UV.100-200nm;stat.errorVARCHARprincipalNUV_fluxExinction corrected GALEX NUV fluxJyphot.flux.density;em.UV.200-300nmVARCHARprincipalNUV_fluxerrError in extinction corrected GALEX NUV fluxJyphot.flux.density;em.UV.200-300nm;stat.errorVARCHARprincipalu_fluxExtinction corrected SDSS u band fluxJyphot.flux.density;em.opt.UVARCHARprincipalu_fluxerrError in extinction corrected SDSS u band fluxJyphot.flux.density;em.opt.U;stat.errorVARCHARprincipalg_fluxExtinction corrected SDSS g band fluxJyphot.flux.density;em.opt.GVARCHARprincipalg_fluxerrError in extinction corrected SDSS g band fluxJyphot.flux.density;em.opt.G;stat.errorVARCHARprincipalr_fluxExtinction corrected SDSS r band fluxJyphot.flux.density;em.opt.RVARCHARprincipalr_fluxerrError in extinction corrected SDSS r band fluxJyphot.flux.density;em.opt.R;stat.errorVARCHARprincipali_fluxExtinction corrected SDSS i band fluxJyphot.flux.density;em.opt.IVARCHARprincipali_fluxerrError in extinction corrected SDSS i band fluxJyphot.flux.density;em.opt.I;stat.errorVARCHARprincipalz_fluxExtinction corrected SDSS z band fluxJyphot.flux.density;em.opt.ZVARCHARprincipalz_fluxerrError in extinction corrected SDSS z band fluxJyphot.flux.density;em.opt.Z;stat.errorVARCHARprincipalX_fluxExtinction correctd VISTA Z band fluxJyphot.flux.density;em.opt.ZVARCHARprincipalX_fluxerrError in extinction corrected VISTA Z band fluxJyphot.flux.density;em.opt.Z;stat.errorVARCHARprincipalY_fluxExtinction corrected VISTA Y band fluxJyphot.flux.density;em.IR.YVARCHARprincipalY_fluxerrError in extinction corrected VISTA Y band fluxJyphot.flux.density;em.IR.Y;stat.errorVARCHARprincipalJ_fluxExtinction corrected VISTA J band fluxJyphot.flux.density;em.IR.JVARCHARprincipalJ_fluxerrError in extinction corrected VISTA J band fluxJyphot.flux.density;em.IR.J;stat.errorVARCHARprincipalH_fluxExtinction corrected VISTA H band fluxJyphot.flux.density;em.IR.HVARCHARprincipalH_fluxerrError in extinction corrected VISTA H band fluxJyphot.flux.density;em.IR.H;stat.errorVARCHARprincipalK_fluxExtinction corrected VISTA K band fluxJyphot.flux.density;em.IR.KVARCHARprincipalK_fluxerrError in extinction corrected VISTA K band fluxJyphot.flux.density;em.IR.K;stat.errorVARCHARprincipalW1_fluxWISE W1 band fluxJyphot.flux.density;em.IR.3-4umVARCHARprincipalW1_fluxerrError in WISE W1 band fluxJyphot.flux.density;em.IR.3-4um;stat.errorVARCHARprincipalW2_fluxWISE W2 band fluxJyphot.flux.density;em.IR.4-8umVARCHARprincipalW2_fluxerrError in WISE W2 band fluxJyphot.flux.density;em.IR.4-8um;stat.errorVARCHARprincipalW3_fluxWISE W3 band fluxJyphot.flux.density;em.IR.8-15umVARCHARprincipalW3_fluxerrError in WISE W3 band fluxJyphot.flux.density;em.IR.8-15um;stat.errorVARCHARprincipalW4_fluxWISE W4 band fluxJyphot.flux.density;em.IR.15-30umVARCHARprincipalW4_fluxerrError in WISE W4 band fluxJyphot.flux.density;em.IR.15-30um;stat.errorVARCHARprincipalP100_fluxHerschel PACS 100 micron fluxJyphot.flux.density;em.mm.1500-3000GHzVARCHARprincipalP100_fluxerrError in Herschel PACS 100 micron fluxJyphot.flux.density;em.mm.1500-3000GHz;stat.errorVARCHARprincipalP160_fluxHerschel PACS 160 micron fluxJyphot.flux.density;em.mm.1500-3000GHzVARCHARprincipalP160_fluxerrError in Herschel PACS 160 micron fluxJyphot.flux.density;em.mm.1500-3000GHz;stat.errorVARCHARprincipalS250_fluxHerschel SPIRE 250 micron fluxJyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalS250_fluxerrError in Herschel SPIRE 250 micron fluxJyphot.flux.density;em.mm.750-1500GHz;stat.errorVARCHARprincipalS350_fluxHerschel SPIRE 350 micron fluxJyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalS350_fluxerrError in Herschel SPIRE 350 micron fluxJyphot.flux.density;em.mm.750-1500GHz;stat.errorVARCHARprincipalS500_fluxHerschel SPIRE 500 micron fluxJyphot.flux.density;em.mm.400-750GHzVARCHARprincipalS500_fluxerrError in Herschel SPIRE 500 micron fluxJyphot.flux.density;em.mm.400-750GHz;stat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LambdarGALEXFUVv01This catalogue contains the complete LAMBDAR output for the GALEX FUV band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarGALEXNUVv01This catalogue contains the complete LAMBDAR output for the GALEX NUV band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarInputCatFIRv01This table contains the input catalogue of apertures used formeasuring the fluxes and uncertainties in the WISE W3 - SPIRE 500 µmbands using the LAMBDAR program in the three GAMA II equatorialsurvey regions.DECDeclinationdegpos.eq.decVARCHARprincipalROTN2EAperture orientation angledegpos.posAngVARCHARprincipalRADMAJAperture semimajor axis lengtharcsecphys.angSize.smajAxisVARCHARprincipalRADMINAperture semiminor axis lengtharcsecphys.angSize.sminAxisVARCHARprincipalAP_ORIGINOrigin of the object aperturemeta.noteVARCHARprincipalCONTAMContaminant flag; T=contaminantmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARight ascensiondegpos.eq.raVARCHARprincipalgama_pdr4v2.LambdarInputCatMIRv01This table contains the input catalogue of apertures used formeasuring the fluxes and uncertainties in the WISE W1 - WISE W2bands using the LAMBDAR program in the three GAMA II equatorialsurvey regions.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARight ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalROTN2EAperture orientation angledegpos.posAngVARCHARprincipalRADMAJAperture semimajor axis lengtharcsecphys.angSize.smajAxisVARCHARprincipalRADMINAperture semiminor axis lengtharcsecphys.angSize.sminAxisVARCHARprincipalAP_ORIGINOrigin of the object aperturemeta.noteVARCHARprincipalCONTAMContaminant flag; T=contaminantmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.StellarMassesv24_GAMAKidsVikingv02uberIDuberID from GAMAKidsVikingv02VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_pdr4v2.LambdarInputCatUVOptNIRv01This table contains the input catalogue of apertures used formeasuring the fluxes and uncertainties in the GALEX FUV - VIKING Kbands using the LAMBDAR program in the three GAMA II equatorialsurvey regions.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARight ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalROTN2EAperture orientation angledegpos.posAngVARCHARprincipalRADMAJAperture semimajor axis lengtharcsecphys.angSize.smajAxisVARCHARprincipalRADMINAperture semiminor axis lengtharcsecphys.angSize.sminAxisVARCHARprincipalAP_ORIGINOrigin of the object aperturemeta.noteVARCHARprincipalCONTAMContaminant flag; T=contaminantmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LambdarPACS100v01This catalogue contains the complete LAMBDAR output for the Herschel PACS 100 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarPACS160v01This catalogue contains the complete LAMBDAR output for the Herschel PACS 160 µm band.DFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSDSSgv01This catalogue contains the complete LAMBDAR output for the SDSS g band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSDSSiv01This catalogue contains the complete LAMBDAR output for the SDSS i band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSDSSrv01This catalogue contains the complete LAMBDAR output for the SDSS r band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSDSSuv01This catalogue contains the complete LAMBDAR output for the SDSS u band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSDSSzv01This catalogue contains the complete LAMBDAR output for the SDSS z band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSPIRE250v01This catalogue contains the complete LAMBDAR output for the Herschel SPIRE 250 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.LambdarSPIRE350v01This catalogue contains the complete LAMBDAR output for the Herschel SPIRE 350 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_pdr4v2.DistancesFramesv14This table provides redshifts in various reference frames,flow-corrected redshifts, and distance moduli for all GAMA IIobjects with redshifts.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalZ_HELIOHeliocentric redshiftsrc.redshiftVARCHARprincipalZ_LGLocal Group frame redshiftsrc.redshiftVARCHARprincipalZ_CMBCMB frame redshiftsrc.redshiftVARCHARprincipalZ_TONRYFlow-corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalZ_TONRY_HIGHRecomputed after adjusting z_helio by +180 km/ssrc.redshiftVARCHARprincipalZ_TONRY_LOWRecomputed after adjusting z_helio by -180 km/ssrc.redshiftVARCHARprincipalDM_70_30_70Distance modulus for 737 cosmologymagphot.mag.distModVARCHARprincipalDM_100_30_70Distance modulus for H0=100, om_m=0.30, om_L=0.70magphot.mag.distModVARCHARprincipalDM_70_25_75Distance modulus for H0=70, om_m=0.25, om_L=0.75magphot.mag.distModVARCHARprincipalDM_100_25_75Distance modulus for H0=100, om_m=0.25, om_L=0.75magphot.mag.distModVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.MagPhysv06This table provides physical stellar population and ISM parametersfor galaxies in the GAMA II equatorial survey regions, derived byrunning the SED-fitting code MAGPHYS on LambdarCatv01.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalZSpectroscopic redshiftsrc.redshiftVARCHARprincipalf_mu_SFH_best_fitBest fit fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile2_52.5th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile1616th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile50Median fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile8484th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile97_597.5th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_best_fitBest fit fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile2_52.5th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile1616th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile50Median fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile8484th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile97_597.5th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_best_fitBest fit fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile2_52.5th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile1616th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile50Median fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile8484th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile97_597.5th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_best_fitBest fit total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile2_52.5th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile1616th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile50Median total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile8484th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile97_597.5th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipalsSFR_0_1Gyr_best_fitBest fit specific star formation rateyr^-1phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile2_52.5th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile1616th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile50Median of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile8484th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile97_597.5th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalmass_stellar_best_fitBest fit total mass of stars ever formed; integral of the star formation rateMsunphys.massVARCHARprincipalmass_stellar_percentile2_52.5th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile1616th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile50Median total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile8484th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile97_597.5th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalL_dust_best_fitBest fit total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)Lsunphys.luminosityVARCHARprincipalL_dust_percentile2_52.5th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile1616th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile50Median total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile8484th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile97_597.5th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalT_C_ISM_best_fitBest fit equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile2_52.5th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile1616th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile50Median equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile8484th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile97_597.5th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_best_fitBest fit equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile2_52.5th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile1616th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile50Median equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile8484th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile97_597.5th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalxi_C_tot_best_fitBest fit fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile2_52.5th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile1616th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile50Median fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile8484th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile97_597.5th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_PAH_tot_best_fitBest fit fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile2_52.5th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile1616th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile50Median fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile8484th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile97_597.5th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_best_fitBest fit fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile2_52.5th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile1616th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile50Median fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile8484th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile97_597.5th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_best_fitBest fit fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile2_52.5th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile1616th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile50Median fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile8484th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile97_597.5th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipaltau_V_ISM_best_fitBest fit total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile2_52.5th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile1616th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile50Median total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile8484th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile97_597.5th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmass_dust_best_fitBest fit total mass of dustMsunphys.massVARCHARprincipalmass_dust_percentile2_52.5th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile1616th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile50Median total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile8484th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile97_597.5th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalSFR_0_1Gyr_best_fitBest fit star formation rateMsun/yrphys.SFRVARCHARprincipalSFR_0_1Gyr_percentile2_52.5th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile1616th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile50Median star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile8484th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile97_597.5th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalmetalicity_Z_Zo_percentile2_52.5th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile1616th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile50Median metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile8484th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile97_597.5th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipaltform_percentile2_52.5th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile1616th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile50Median age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile8484th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile97_597.5th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipalgamma_percentile2_52.5th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile1616th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile50Median star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile8484th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile97_597.5th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipaltlastb_percentile2_52.5th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile1616th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile50Median time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile8484th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile97_597.5th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipalagem_percentile2_52.5th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile1616th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile50Median mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile8484th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile97_597.5th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalager_percentile2_52.5th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile1616th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile50Median r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile8484th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile97_597.5th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalsfr16_percentile2_52.5th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile1616th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile50Median star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile8484th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile97_597.5th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile2_52.5th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile1616th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile50Median star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile8484th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile97_597.5th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile2_52.5th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile1616th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile50Median star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile8484th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile97_597.5th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile2_52.5th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile1616th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile50Median star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile8484th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile97_597.5th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile2_52.5th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile1616th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile50Median star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile8484th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile97_597.5th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalfb16_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile50Median fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb17_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile50Median fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb18_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile50Median fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb19_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile50Median fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb29_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile1616th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile50Median fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile8484th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalURL_SEDURL of MAGPHYS output file containing the best-fit spectrummeta.ref.url;meta.fileVARCHARprincipalURL_FITURL of MAGPHYS output file containing individual parameter PDFsmeta.ref.url;meta.fileVARCHARprincipalURL_PNGURL of plot of the best-fit spectrum and input photometrymeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.MegaMorphCatv01This table provides the results of fitting both a single Sersiccomponent model as well as a two-component bulge-disk model to the2D surface brightness distributions of galaxies in the GAMA I G09survey region using the MegaMorph multi-band fitting method. In thismethod the ugriz (from SDSS) and YJHK (from UKIDSS-LAS) surfacebrightness distributions of a galaxy are fit simultaneously whileimposing some constraints on how some of the model parameters areallowed to vary with wavelength.CATAIDGAMA object IDmeta.idVARCHARprincipalRAJ2000 coordinate of the GAMA objectdegpos.eq.raVARCHARprincipalDECJ2000 coordinate of the GAMA objectdegpos.eq.decVARCHARprincipalALPHA_J2000J2000 coordinate of the MegaMorph fitdegpos.eq.raVARCHARprincipalDELTA_J2000J2000 coordinate of the MegaMorph fitdegpos.eq.decVARCHARprincipalTHETA_IMAGEPosition angle on the image, counterclockwise, 0 is the NAXIS1 image axisdegpos.posAngVARCHARprincipalELLIPTICITYAxial ratio of galaxy, b/asrc.ellipticityVARCHARprincipalBACKGROUNDLocal backgroundcountsphot.fluxVARCHARprincipalFLUX_BESTFlux estimatecountsphot.flux;em.optVARCHARprincipalFLUXERR_BESTFlux errorcountsphot.flux;stat.errorVARCHARprincipalMAG_BESTMagnitude estimatemagphot.magVARCHARprincipalMAGERR_BESTMagnitude estimate errormagphot.mag;stat.errorVARCHARprincipalFLUX_RADIUSHalflight radiusarcsecphys.angSizeVARCHARprincipalISOAREA_IMAGEObject area; number of pixels above analysis thresholdpixelphys.areaVARCHARprincipalFWHM_IMAGEImage FWHMpixelphys.size.diameter;instr.det.psfVARCHARprincipalFLAGSSExtractor flagsmeta.codeVARCHARprincipalCLASS_STARStar/galaxy classifiersrc.class.starGalaxyVARCHARprincipalRE_GALFIT_CHEB_0Chebyshev coefficients of effective radiusstat.fit.param;meta.modelledVARCHARprincipalRE_GALFIT_CHEB_1Chebyshev coefficients of effective radiusstat.fit.param;meta.modelledVARCHARprincipalRE_GALFIT_CHEB_2Chebyshev coefficients of effective radiusstat.fit.param;meta.modelledVARCHARprincipalREERR_GALFIT_CHEB_0Error on Chebyshev coefficients of effective radiusstat.fit.param;stat.error;meta.modelledVARCHARprincipalREERR_GALFIT_CHEB_1Error on Chebyshev coefficients of effective radiusstat.fit.param;stat.error;meta.modelledVARCHARprincipalREERR_GALFIT_CHEB_2Error on Chebyshev coefficients of effective radiusstat.fit.param;stat.error;meta.modelledVARCHARprincipalN_GALFIT_CHEB_0Chebyshev coefficients of Sersic indexstat.fit.param;meta.modelledVARCHARprincipalN_GALFIT_CHEB_1Chebyshev coefficients of Sersic indexstat.fit.param;meta.modelledVARCHARprincipalN_GALFIT_CHEB_2Chebyshev coefficients of Sersic indexstat.fit.param;meta.modelledVARCHARprincipalNERR_GALFIT_CHEB_0Error on Chebyshev coefficients of Sersic indexstat.fit.param;stat.error;meta.modelledVARCHARprincipalNERR_GALFIT_CHEB_1Error on Chebyshev coefficients of Sersic indexstat.fit.param;stat.error;meta.modelledVARCHARprincipalNERR_GALFIT_CHEB_2Error on Chebyshev coefficients of Sersic indexstat.fit.param;stat.error;meta.modelledVARCHARprincipalMAG_GALFIT_BAND_uApparent magnitudemagphot.mag;meta.modelled;em.opt.UVARCHARprincipalMAG_GALFIT_BAND_gApparent magnitudemagphot.mag;meta.modelled;em.opt.GVARCHARprincipalMAG_GALFIT_BAND_rApparent magnitudemagphot.mag;meta.modelled;em.opt.RVARCHARprincipalMAG_GALFIT_BAND_iApparent magnitudemagphot.mag;meta.modelled;em.opt.IVARCHARprincipalMAG_GALFIT_BAND_zApparent magnitudemagphot.mag;meta.modelled;em.opt.ZVARCHARprincipalMAG_GALFIT_BAND_YApparent magnitudemagphot.mag;meta.modelled;em.IR.YVARCHARprincipalMAG_GALFIT_BAND_JApparent magnitudemagphot.mag;meta.modelled;em.IR.JVARCHARprincipalMAG_GALFIT_BAND_HApparent magnitudemagphot.mag;meta.modelled;em.IR.HVARCHARprincipalMAG_GALFIT_BAND_KApparent magnitudemagphot.mag;meta.modelled;em.IR.KVARCHARprincipalMAGERR_GALFIT_BAND_uError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.UVARCHARprincipalMAGERR_GALFIT_BAND_gError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.GVARCHARprincipalMAGERR_GALFIT_BAND_rError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.RVARCHARprincipalMAGERR_GALFIT_BAND_iError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.IVARCHARprincipalMAGERR_GALFIT_BAND_zError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.ZVARCHARprincipalMAGERR_GALFIT_BAND_YError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalMAGERR_GALFIT_BAND_JError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalMAGERR_GALFIT_BAND_HError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalMAGERR_GALFIT_BAND_KError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalRE_GALFIT_BAND_uEffective radiusarcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalRE_GALFIT_BAND_gEffective radiusarcsecphys.angSize;meta.modelled;em.opt.GVARCHARprincipalRE_GALFIT_BAND_rEffective radiusarcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalRE_GALFIT_BAND_iEffective radiusarcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalRE_GALFIT_BAND_zEffective radiusarcsecphys.angSize;meta.modelled;em.opt.ZVARCHARprincipalRE_GALFIT_BAND_YEffective radiusarcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalRE_GALFIT_BAND_JEffective radiusarcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalRE_GALFIT_BAND_HEffective radiusarcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalRE_GALFIT_BAND_KEffective radiusarcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalREERR_GALFIT_BAND_uError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.UVARCHARprincipalREERR_GALFIT_BAND_gError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.GVARCHARprincipalREERR_GALFIT_BAND_rError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.RVARCHARprincipalREERR_GALFIT_BAND_iError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.IVARCHARprincipalREERR_GALFIT_BAND_zError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.ZVARCHARprincipalREERR_GALFIT_BAND_YError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalREERR_GALFIT_BAND_JError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalREERR_GALFIT_BAND_HError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalREERR_GALFIT_BAND_KError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalN_GALFIT_BAND_uSersic indexphys.angSize;meta.modelled;em.opt.UVARCHARprincipalN_GALFIT_BAND_gSersic indexphys.angSize;meta.modelled;em.opt.GVARCHARprincipalN_GALFIT_BAND_rSersic indexphys.angSize;meta.modelled;em.opt.RVARCHARprincipalN_GALFIT_BAND_iSersic indexphys.angSize;meta.modelled;em.opt.IVARCHARprincipalN_GALFIT_BAND_zSersic indexphys.angSize;meta.modelled;em.opt.ZVARCHARprincipalN_GALFIT_BAND_YSersic indexphys.angSize;meta.modelled;em.IR.YVARCHARprincipalN_GALFIT_BAND_JSersic indexphys.angSize;meta.modelled;em.IR.JVARCHARprincipalN_GALFIT_BAND_HSersic indexphys.angSize;meta.modelled;em.IR.HVARCHARprincipalN_GALFIT_BAND_KSersic indexphys.angSize;meta.modelled;em.IR.KVARCHARprincipalNERR_GALFIT_BAND_uError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.UVARCHARprincipalNERR_GALFIT_BAND_gError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.GVARCHARprincipalNERR_GALFIT_BAND_rError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.RVARCHARprincipalNERR_GALFIT_BAND_iError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.IVARCHARprincipalNERR_GALFIT_BAND_zError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.ZVARCHARprincipalNERR_GALFIT_BAND_YError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalNERR_GALFIT_BAND_JError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalNERR_GALFIT_BAND_HError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalNERR_GALFIT_BAND_KError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalQ_GALFIT_BANDAxial ratiosrc.ellipticity;meta.modelledVARCHARprincipalQERR_GALFIT_BANDError on axial ratiosrc.ellipticity;stat.error;meta.modelledVARCHARprincipalPA_GALFIT_BANDPosition angle on sky, counterclockwise, 0 is Northdegpos.posAng;meta.modelledVARCHARprincipalPAERR_GALFIT_BANDError on position angle on skydegpos.posAng;stat.error;meta.modelledVARCHARprincipalSKY_GALFIT_BAND_uSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.UVARCHARprincipalSKY_GALFIT_BAND_gSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.GVARCHARprincipalSKY_GALFIT_BAND_rSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.RVARCHARprincipalSKY_GALFIT_BAND_iSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.IVARCHARprincipalSKY_GALFIT_BAND_zSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.ZVARCHARprincipalSKY_GALFIT_BAND_YSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.YVARCHARprincipalSKY_GALFIT_BAND_JSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.JVARCHARprincipalSKY_GALFIT_BAND_HSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.HVARCHARprincipalSKY_GALFIT_BAND_KSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.KVARCHARprincipalMAG_GALFIT_BAND_D_uApparent magnitude of discmagphot.mag;meta.modelled;em.opt.UVARCHARprincipalMAG_GALFIT_BAND_D_gApparent magnitude of discmagphot.mag;meta.modelled;em.opt.GVARCHARprincipalMAG_GALFIT_BAND_D_rApparent magnitude of discmagphot.mag;meta.modelled;em.opt.RVARCHARprincipalMAG_GALFIT_BAND_D_iApparent magnitude of discmagphot.mag;meta.modelled;em.opt.IVARCHARprincipalMAG_GALFIT_BAND_D_zApparent magnitude of discmagphot.mag;meta.modelled;em.opt.ZVARCHARprincipalMAG_GALFIT_BAND_D_YApparent magnitude of discmagphot.mag;meta.modelled;em.IR.YVARCHARprincipalMAG_GALFIT_BAND_D_JApparent magnitude of discmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalMAG_GALFIT_BAND_D_HApparent magnitude of discmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalMAG_GALFIT_BAND_D_KApparent magnitude of discmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalMAGERR_GALFIT_BAND_D_uError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.UVARCHARprincipalMAGERR_GALFIT_BAND_D_gError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.GVARCHARprincipalMAGERR_GALFIT_BAND_D_rError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.RVARCHARprincipalMAGERR_GALFIT_BAND_D_iError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.IVARCHARprincipalMAGERR_GALFIT_BAND_D_zError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.ZVARCHARprincipalMAGERR_GALFIT_BAND_D_YError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalMAGERR_GALFIT_BAND_D_JError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalMAGERR_GALFIT_BAND_D_HError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalMAGERR_GALFIT_BAND_D_KError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalMAG_GALFIT_BAND_B_uApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.UVARCHARprincipalMAG_GALFIT_BAND_B_gApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.GVARCHARprincipalMAG_GALFIT_BAND_B_rApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.RVARCHARprincipalMAG_GALFIT_BAND_B_iApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.IVARCHARprincipalMAG_GALFIT_BAND_B_zApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.ZVARCHARprincipalMAG_GALFIT_BAND_B_YApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.YVARCHARprincipalMAG_GALFIT_BAND_B_JApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.JVARCHARprincipalMAG_GALFIT_BAND_B_HApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.HVARCHARprincipalMAG_GALFIT_BAND_B_KApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.KVARCHARprincipalMAGERR_GALFIT_BAND_B_uError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.UVARCHARprincipalMAGERR_GALFIT_BAND_B_gError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.GVARCHARprincipalMAGERR_GALFIT_BAND_B_rError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.RVARCHARprincipalMAGERR_GALFIT_BAND_B_iError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.IVARCHARprincipalMAGERR_GALFIT_BAND_B_zError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.ZVARCHARprincipalMAGERR_GALFIT_BAND_B_YError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalMAGERR_GALFIT_BAND_B_JError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalMAGERR_GALFIT_BAND_B_HError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalMAGERR_GALFIT_BAND_B_KError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalRE_GALFIT_BAND_DEffective radius of discarcsecphys.angSize;meta.modelledVARCHARprincipalREERR_GALFIT_BAND_DError on effective radius of discarcsecphys.angSize;stat.error;meta.modelledVARCHARprincipalRE_GALFIT_BAND_BEffective radius of bulgearcsecphys.angSize;meta.modelledVARCHARprincipalREERR_GALFIT_BAND_BError on effective radius of bulgearcsecphys.angSize;stat.error;meta.modelledVARCHARprincipalN_GALFIT_BAND_DSersic index of discphys.angSize;meta.modelledVARCHARprincipalN_GALFIT_BAND_BSersic index of bulgephys.angSize;meta.modelledVARCHARprincipalNERR_GALFIT_BAND_BError on Sersic index of bulgephys.angSize;stat.error;meta.modelledVARCHARprincipalQ_GALFIT_BAND_DAxial ratio of discsrc.ellipticity;meta.modelledVARCHARprincipalQERR_GALFIT_BAND_DError on axial ratio of discsrc.ellipticity;stat.error;meta.modelledVARCHARprincipalQ_GALFIT_BAND_BAxial ratio of bulgesrc.ellipticity;meta.modelledVARCHARprincipalQERR_GALFIT_BAND_BError on axial ratio of bulgesrc.ellipticity;stat.error;meta.modelledVARCHARprincipalPA_GALFIT_BAND_DPosition angle of disc on sky, counterclockwise, 0 is Northdegpos.posAng;meta.modelledVARCHARprincipalPAERR_GALFIT_BAND_DError on position angle of disc on skydegpos.posAng;stat.error;meta.modelledVARCHARprincipalPA_GALFIT_BAND_BPosition angle of bulge on sky, counterclockwise, 0 is Northdegpos.posAng;meta.modelledVARCHARprincipalPAERR_GALFIT_BAND_BError on position angle of bulge on skydegpos.posAng;stat.error;meta.modelledVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.21BandPhotomv03This table combines available flux measurements from theGalexPhotometry, ApMatchedPhotom and WISEPhotometry DMUs withbespoke flux measurements in the Herschel PACS and SPIRE bands byKate Rowlands and Nathan Bourne for all objects in the GAMA IIequatorial survey regions. The data are presented in the formrequired by MAGPHYS.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalZHeliocentric redshift of objectsrc.redshiftVARCHARprincipalFUV_fluxExtinction corrected GALEX FUV fluxJyphot.mag;em.UV.100-200nmVARCHARprincipalFUV_fluxerrError in extinction corrected GALEX FUV fluxJyphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalNUV_fluxExinction corrected GALEX NUV fluxJyphot.mag;em.UV.200-300nmVARCHARprincipalNUV_fluxerrError in extinction corrected GALEX NUV fluxJyphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalu_fluxExtinction corrected SDSS u band fluxJyphot.mag;em.opt.UVARCHARprincipalu_fluxerrError in extinction corrected SDSS u band fluxJyphot.mag;em.opt.U;stat.errorVARCHARprincipalg_fluxExtinction corrected SDSS g band fluxJyphot.mag;em.opt.GVARCHARprincipalg_fluxerrError in extinction corrected SDSS g band fluxJyphot.mag;em.opt.G;stat.errorVARCHARprincipalr_fluxExtinction corrected SDSS r band fluxJyphot.mag;em.opt.RVARCHARprincipalr_fluxerrError in extinction corrected SDSS r band fluxJyphot.mag;em.opt.R;stat.errorVARCHARprincipali_fluxExtinction corrected SDSS i band fluxJyphot.mag;em.opt.IVARCHARprincipali_fluxerrError in extinction corrected SDSS i band fluxJyphot.mag;em.opt.I;stat.errorVARCHARprincipalz_fluxExtinction corrected SDSS z band fluxJyphot.mag;em.opt.ZVARCHARprincipalz_fluxerrError in extinction corrected SDSS z band fluxJyphot.mag;em.opt.Z;stat.errorVARCHARprincipalX_fluxExtinction correctd VISTA Z band fluxJyphot.mag;em.opt.ZVARCHARprincipalX_fluxerrError in extinction corrected VISTA Z band fluxJyphot.mag;em.opt.Z;stat.errorVARCHARprincipalY_fluxExtinction corrected VISTA Y band fluxJyphot.mag;em.IR.YVARCHARprincipalY_fluxerrError in extinction corrected VISTA Y band fluxJyphot.mag;em.IR.Y;stat.errorVARCHARprincipalJ_fluxExtinction corrected VISTA J band fluxJyphot.mag;em.IR.JVARCHARprincipalJ_fluxerrError in extinction corrected VISTA J band fluxJyphot.mag;em.IR.J;stat.errorVARCHARprincipalH_fluxExtinction corrected VISTA H band fluxJyphot.mag;em.IR.HVARCHARprincipalH_fluxerrError in extinction corrected VISTA H band fluxJyphot.mag;em.IR.H;stat.errorVARCHARprincipalK_fluxExtinction corrected VISTA Ks band fluxJyphot.mag;em.IR.KVARCHARprincipalK_fluxerrError in extinction corrected VISTA Ks band fluxJyphot.mag;em.IR.K;stat.errorVARCHARprincipalW1_fluxWISE band 1 fluxJyphot.mag;em.IR.3-4umVARCHARprincipalW1_fluxerrError in WISE band 1 fluxJyphot.mag;em.IR.3-4um;stat.errorVARCHARprincipalW2_fluxWISE band 2 fluxJyphot.mag;em.IR.4-8umVARCHARprincipalW2_fluxerrError in WISE band 2 fluxJyphot.mag;em.IR.4-8um;stat.errorVARCHARprincipalW3_fluxWISE band 3 fluxJyphot.mag;em.IR.8-15umVARCHARprincipalW3_fluxerrError in WISE band 3 fluxJyphot.mag;em.IR.8-15um;stat.errorVARCHARprincipalW4_fluxWISE band 4 fluxJyphot.mag;em.IR.15-30umVARCHARprincipalW4_fluxerrError in WISE band 4 fluxJyphot.mag;em.IR.15-30um;stat.errorVARCHARprincipal100_fluxHerschel PACS 100 micron fluxJyphot.mag;em.mm.1500-3000GHzVARCHARprincipal100_fluxerrError in Herschel PACS 100 micron fluxJyphot.mag;em.mm.1500-3000GHz;stat.errorVARCHARprincipal160_fluxHerschel PACS 160 micron fluxJyphot.mag;em.mm.1500-3000GHzVARCHARprincipal160_fluxerrError in Herschel PACS 160 micron fluxJyphot.mag;em.mm.1500-3000GHz;stat.errorVARCHARprincipal250_fluxHerschel SPIRE 250 micron fluxJyphot.mag;em.mm.750-1500GHzVARCHARprincipal250_fluxerrError in Herschel SPIRE 250 micron fluxJyphot.mag;em.mm.750-1500GHz;stat.errorVARCHARprincipal350_fluxHerschel SPIRE 350 micron fluxJyphot.mag;em.mm.750-1500GHzVARCHARprincipal350_fluxerrError in Herschel SPIRE 350 micron fluxJyphot.mag;em.mm.750-1500GHz;stat.errorVARCHARprincipal450_fluxHerschel SPIRE 450 micron fluxJyphot.mag;em.mm.400-750GHzVARCHARprincipal450_fluxerrError in Herschel SPIRE 450 micron fluxJyphot.mag;em.mm.400-750GHz;stat.errorVARCHARprincipalURL_PNGURL of SED summary plotmeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.RadialDensityv01This table provides the radial density variation of galaxies in theGAMA II equatorial survey regions.ZBinIDID of the redshift binmeta.id;meta.mainVARCHARindexedprincipalZRedshift of bin centresrc.redshiftVARCHARprincipaldelta_G09Multiplicative overdensity in G09src.densityVARCHARprincipaldelta_G12Multiplicative overdensity in G12src.densityVARCHARprincipaldelta_G15Multiplicative overdensity in G15src.densityVARCHARprincipaldelta_AVMultiplicative overdensity averaged over all equatorial regionssrc.densityVARCHARprincipalgama_pdr4v2.RandomsUnwindowedv02This table provides a set of randomly distributed points with thesame selection function as the galaxies in the GAMA II equatorialsurvey regions. Each point is a clone of a real GAMA galaxy,identified by its CATAID, which can be used to assign properties tothe random points. The redshifts of randoms are NOT restricted to aGaussian window around the redshift of the real galaxy being cloned.RANDIDUnique random IDmeta.id;meta.mainVARCHARindexedprincipalCATAIDGAMA galaxy IDmeta.idVARCHARprincipalRARight Ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalZRedshiftsrc.redshiftVARCHARprincipalR_PETRO_ABSAbsolute r-band Petrosian magnitudemagphys.magAbs;em.opt.RVARCHARprincipalR_PETROApparent r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalRAND_NUMA random number in the range (0,1] to select subsetsstat.valueVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Randomsv02This table provides a set of randomly distributed points with thesame selection function as the galaxies in the GAMA II equatorialsurvey regions. Each point is a clone of a real GAMA galaxy,identified by its CATAID, which can be used to assign properties tothe random points. The redshifts of randoms are restricted to aGaussian window around the redshift of the real galaxy being cloned.RANDIDUnique random IDmeta.id;meta.mainVARCHARindexedprincipalCATAIDGAMA galaxy IDmeta.idVARCHARprincipalRARight Ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalZRedshiftsrc.redshiftVARCHARprincipalR_PETRO_ABSAbsolute r-band Petrosian magnitudemagphys.magAbs;em.opt.RVARCHARprincipalR_PETROApparent r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalRAND_NUMA random number in the range (0,1] to select subsetsstat.valueVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.SersicCatSDSSv09This table provides the results of a single-Sersic-component fit tothe 2D surface brightness distribution of every object in theGAMA II equatorial survey regions in the SDSS ugriz bands.CATAIDGAMA Object IDmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalCENFLUX_uCentral pixel flux value prior to background estimationcountsphot.count;em.opt.uVARCHARprincipalBACKFLUX_uSEx subtracted background at object positioncountsphot.count;em.opt.uVARCHARprincipalPSFNUM_uPSFEx number of stars usedmeta.number;em.opt.uVARCHARprincipalPSFCHI2_uPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.uVARCHARprincipalPSFFWHM_uPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.uVARCHARprincipalNSEC_uSEx number of secondary components detectedmeta.number;em.opt.uVARCHARprincipalGALXCEN_uGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.uVARCHARprincipalGALYCEN_uGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.uVARCHARprincipalGALMAG_uGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.uVARCHARprincipalGALRE_uGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.uVARCHARprincipalGALINDEX_uGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.uVARCHARprincipalGALELLIP_uGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.uVARCHARprincipalGALPA_uGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.uVARCHARprincipalGALXCENERR_uGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALYCENERR_uGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALMAGERR_uGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALREERR_uGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALINDEXERR_uGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALELLIPERR_uGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALPAERR_uGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALRA_uGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.uVARCHARprincipalGALDEC_uGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.uVARCHARprincipalGALMAG10RE_uGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.uVARCHARprincipalGALMU0_uGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.uVARCHARprincipalGALMUE_uGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.uVARCHARprincipalGALMUEAVG_uGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.uVARCHARprincipalGALR90_uGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.uVARCHARprincipalGALCHI2FULL_uGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.uVARCHARprincipalGALNDOF_uGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.uVARCHARprincipalGALCHI2_uGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.uVARCHARprincipalGALPLAN_uSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.uVARCHARprincipalPRICHI2FULL_uPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalPRINFP_uPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalPRINDOF_uPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalPRICHI2_uPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalCENFLUX_gCentral pixel flux value prior to background estimationcountsphot.count;em.opt.gVARCHARprincipalBACKFLUX_gSEx subtracted background at object positioncountsphot.count;em.opt.gVARCHARprincipalPSFNUM_gPSFEx number of stars usedmeta.number;em.opt.gVARCHARprincipalPSFCHI2_gPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.gVARCHARprincipalPSFFWHM_gPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.gVARCHARprincipalNSEC_gSEx number of secondary components detectedmeta.number;em.opt.gVARCHARprincipalGALXCEN_gGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.gVARCHARprincipalGALYCEN_gGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.gVARCHARprincipalGALMAG_gGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.gVARCHARprincipalGALRE_gGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.gVARCHARprincipalGALINDEX_gGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.gVARCHARprincipalGALELLIP_gGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.gVARCHARprincipalGALPA_gGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.gVARCHARprincipalGALXCENERR_gGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALYCENERR_gGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALMAGERR_gGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALREERR_gGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALINDEXERR_gGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALELLIPERR_gGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALPAERR_gGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALRA_gGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.gVARCHARprincipalGALDEC_gGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.gVARCHARprincipalGALMAG10RE_gGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.gVARCHARprincipalGALMU0_gGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.gVARCHARprincipalGALMUE_gGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.gVARCHARprincipalGALMUEAVG_gGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.gVARCHARprincipalCENFLUX_iCentral pixel flux value prior to background estimationcountsphot.count;em.opt.iVARCHARprincipalGALR90_gGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.gVARCHARprincipalGALCHI2FULL_gGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.gVARCHARprincipalGALNDOF_gGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.gVARCHARprincipalGALCHI2_gGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.gVARCHARprincipalGALPLAN_gSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.gVARCHARprincipalPRICHI2FULL_gPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalPRINFP_gPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalPRINDOF_gPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalPRICHI2_gPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalCENFLUX_rCentral pixel flux value prior to background estimationcountsphot.count;em.opt.rVARCHARprincipalBACKFLUX_rSEx subtracted background at object positioncountsphot.count;em.opt.rVARCHARprincipalPSFNUM_rPSFEx number of stars usedmeta.number;em.opt.rVARCHARprincipalPSFCHI2_rPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.rVARCHARprincipalPSFFWHM_rPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.rVARCHARprincipalNSEC_rSEx number of secondary components detectedmeta.number;em.opt.rVARCHARprincipalGALXCEN_rGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.rVARCHARprincipalGALYCEN_rGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.rVARCHARprincipalGALMAG_rGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.rVARCHARprincipalGALRE_rGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.rVARCHARprincipalGALINDEX_rGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.rVARCHARprincipalGALELLIP_rGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.rVARCHARprincipalGALPA_rGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.rVARCHARprincipalGALXCENERR_rGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALYCENERR_rGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALMAGERR_rGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALREERR_rGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALINDEXERR_rGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALELLIPERR_rGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALPAERR_rGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALRA_rGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.rVARCHARprincipalGALDEC_rGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.rVARCHARprincipalGALMAG10RE_rGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.rVARCHARprincipalGALMU0_rGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.rVARCHARprincipalGALMUE_rGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.rVARCHARprincipalGALMUEAVG_rGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.rVARCHARprincipalGALR90_rGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.rVARCHARprincipalGALCHI2FULL_rGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.rVARCHARprincipalGALNDOF_rGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.rVARCHARprincipalGALCHI2_rGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.rVARCHARprincipalGALPLAN_rSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.rVARCHARprincipalPRICHI2FULL_rPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalPRINFP_rPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalPRINDOF_rPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalPRICHI2_rPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalBACKFLUX_iSEx subtracted background at object positioncountsphot.count;em.opt.iVARCHARprincipalPSFNUM_iPSFEx number of stars usedmeta.number;em.opt.iVARCHARprincipalPSFCHI2_iPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.iVARCHARprincipalPSFFWHM_iPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.iVARCHARprincipalNSEC_iSEx number of secondary components detectedmeta.number;em.opt.iVARCHARprincipalGALXCEN_iGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.iVARCHARprincipalGALYCEN_iGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.iVARCHARprincipalGALMAG_iGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.iVARCHARprincipalGALRE_iGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.iVARCHARprincipalGALINDEX_iGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.iVARCHARprincipalGALELLIP_iGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.iVARCHARprincipalGALPA_iGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.iVARCHARprincipalGALXCENERR_iGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALYCENERR_iGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALMAGERR_iGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALREERR_iGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALINDEXERR_iGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALELLIPERR_iGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALPAERR_iGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALRA_iGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.iVARCHARprincipalGALDEC_iGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.iVARCHARprincipalGALMAG10RE_iGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.iVARCHARprincipalGALMU0_iGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.iVARCHARprincipalGALMUE_iGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.iVARCHARprincipalGALMUEAVG_iGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.iVARCHARprincipalGALR90_iGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.iVARCHARprincipalGALCHI2FULL_iGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.iVARCHARprincipalGALNDOF_iGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.iVARCHARprincipalGALCHI2_iGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.iVARCHARprincipalGALPLAN_iSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.iVARCHARprincipalPRICHI2FULL_iPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalPRINFP_iPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalPRINDOF_iPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalPRICHI2_iPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalCENFLUX_zCentral pixel flux value prior to background estimationcountsphot.count;em.opt.zVARCHARprincipalBACKFLUX_zSEx subtracted background at object positioncountsphot.count;em.opt.zVARCHARprincipalPSFNUM_zPSFEx number of stars usedmeta.number;em.opt.zVARCHARprincipalPSFCHI2_zPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.zVARCHARprincipalPSFFWHM_zPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.zVARCHARprincipalNSEC_zSEx number of secondary components detectedmeta.number;em.opt.zVARCHARprincipalGALXCEN_zGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.zVARCHARprincipalGALYCEN_zGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.zVARCHARprincipalGALMAG_zGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.zVARCHARprincipalGALRE_zGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.zVARCHARprincipalGALINDEX_zGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.zVARCHARprincipalGALELLIP_zGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.zVARCHARprincipalGALPA_zGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.zVARCHARprincipalGALXCENERR_zGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALYCENERR_zGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALMAGERR_zGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALREERR_zGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALINDEXERR_zGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALELLIPERR_zGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALPAERR_zGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALRA_zGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.zVARCHARprincipalGALDEC_zGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.zVARCHARprincipalGALMAG10RE_zGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.zVARCHARprincipalGALMU0_zGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.zVARCHARprincipalGALMUE_zGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.zVARCHARprincipalGALMUEAVG_zGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.zVARCHARprincipalGALR90_zGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.zVARCHARprincipalGALCHI2FULL_zGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.zVARCHARprincipalGALNDOF_zGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.zVARCHARprincipalGALCHI2_zGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.zVARCHARprincipalGALPLAN_zSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.zVARCHARprincipalPRICHI2FULL_zPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.zVARCHARprincipalPRINFP_zPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.zVARCHARprincipalPRINDOF_zPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.zVARCHARprincipalPRICHI2_zPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.zVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.SersicCatUKIDSSv09This table provides the results of a single-Sersic-component fit tothe 2D surface brightness distribution of every object in theGAMA II equatorial survey regions in the UKIDSS-LAS YJHK bands.CATAIDGAMA Object IDmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalCENFLUX_YCentral pixel flux value prior to background estimationcountsphot.count;em.IR.YVARCHARprincipalBACKFLUX_YSEx subtracted background at object positioncountsphot.count;em.IR.YVARCHARprincipalPSFNUM_YPSFEx number of stars usedmeta.number;em.IR.YVARCHARprincipalPSFCHI2_YPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.YVARCHARprincipalPSFFWHM_YPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.YVARCHARprincipalNSEC_YSEx number of secondary components detectedmeta.number;em.IR.YVARCHARprincipalGALXCEN_YGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.YVARCHARprincipalGALYCEN_YGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.YVARCHARprincipalGALMAG_YGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALRE_YGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALINDEX_YGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.YVARCHARprincipalGALELLIP_YGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.YVARCHARprincipalGALPA_YGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.YVARCHARprincipalGALXCENERR_YGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALYCENERR_YGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALMAGERR_YGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALREERR_YGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALINDEXERR_YGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALELLIPERR_YGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALPAERR_YGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALRA_YGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.YVARCHARprincipalGALDEC_YGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.YVARCHARprincipalGALMAG10RE_YGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALMU0_YGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUE_YGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUEAVG_YGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALR90_YGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALCHI2FULL_YGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALNDOF_YGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALCHI2_YGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALPLAN_YSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2FULL_YPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINFP_YPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINDOF_YPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2_YPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalCENFLUX_JCentral pixel flux value prior to background estimationcountsphot.count;em.IR.JVARCHARprincipalBACKFLUX_JSEx subtracted background at object positioncountsphot.count;em.IR.JVARCHARprincipalPSFNUM_JPSFEx number of stars usedmeta.number;em.IR.JVARCHARprincipalPSFCHI2_JPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.JVARCHARprincipalPSFFWHM_JPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.JVARCHARprincipalNSEC_JSEx number of secondary components detectedmeta.number;em.IR.JVARCHARprincipalGALXCEN_JGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.JVARCHARprincipalGALYCEN_JGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.JVARCHARprincipalGALMAG_JGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALRE_JGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALINDEX_JGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.JVARCHARprincipalGALELLIP_JGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.JVARCHARprincipalGALPA_JGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.JVARCHARprincipalGALXCENERR_JGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALYCENERR_JGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALMAGERR_JGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALREERR_JGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALINDEXERR_JGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALELLIPERR_JGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALPAERR_JGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALRA_JGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.JVARCHARprincipalGALDEC_JGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.JVARCHARprincipalGALMAG10RE_JGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALMU0_JGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUE_JGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUEAVG_JGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALR90_JGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALCHI2FULL_JGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALNDOF_JGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALCHI2_JGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALPLAN_JSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2FULL_JPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINFP_JPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINDOF_JPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2_JPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalCENFLUX_HCentral pixel flux value prior to background estimationcountsphot.count;em.IR.HVARCHARprincipalBACKFLUX_HSEx subtracted background at object positioncountsphot.count;em.IR.HVARCHARprincipalPSFNUM_HPSFEx number of stars usedmeta.number;em.IR.HVARCHARprincipalPSFCHI2_HPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.HVARCHARprincipalPSFFWHM_HPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.HVARCHARprincipalNSEC_HSEx number of secondary components detectedmeta.number;em.IR.HVARCHARprincipalGALXCEN_HGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.HVARCHARprincipalGALYCEN_HGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.HVARCHARprincipalGALMAG_HGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALRE_HGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALINDEX_HGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.HVARCHARprincipalGALELLIP_HGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.HVARCHARprincipalGALPA_HGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.HVARCHARprincipalGALXCENERR_HGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALYCENERR_HGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALMAGERR_HGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALREERR_HGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALINDEXERR_HGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALELLIPERR_HGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALPAERR_HGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALRA_HGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.HVARCHARprincipalGALDEC_HGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.HVARCHARprincipalGALMAG10RE_HGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALMU0_HGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUE_HGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUEAVG_HGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALR90_HGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALCHI2FULL_HGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALNDOF_HGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALCHI2_HGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALPLAN_HSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2FULL_HPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINFP_HPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINDOF_HPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2_HPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalCENFLUX_KCentral pixel flux value prior to background estimationcountsphot.count;em.IR.KVARCHARprincipalBACKFLUX_KSEx subtracted background at object positioncountsphot.count;em.IR.KVARCHARprincipalPSFNUM_KPSFEx number of stars usedmeta.number;em.IR.KVARCHARprincipalPSFCHI2_KPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.KVARCHARprincipalPSFFWHM_KPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.KVARCHARprincipalNSEC_KSEx number of secondary components detectedmeta.number;em.IR.KVARCHARprincipalGALXCEN_KGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.KVARCHARprincipalGALYCEN_KGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.KVARCHARprincipalGALMAG_KGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALRE_KGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALINDEX_KGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.KVARCHARprincipalGALELLIP_KGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.KVARCHARprincipalGALPA_KGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.KVARCHARprincipalGALXCENERR_KGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALYCENERR_KGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALMAGERR_KGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALREERR_KGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALINDEXERR_KGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALELLIPERR_KGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALPAERR_KGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALRA_KGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.KVARCHARprincipalGALDEC_KGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.KVARCHARprincipalGALMAG10RE_KGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALMU0_KGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUE_KGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUEAVG_KGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALR90_KGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALCHI2FULL_KGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALNDOF_KGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALCHI2_KGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALPLAN_KSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2FULL_KPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINFP_KPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINDOF_KPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2_KPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.SersicCatVIKINGv09This table provides the results of a single-Sersic-component fit tothe 2D surface brightness distribution of every object in theGAMA II equatorial survey regions in the VIKING ZYJHK bands.CATAIDGAMA Object IDmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalCENFLUX_ZCentral pixel flux value prior to background estimationcountsphot.count;em.IR.ZVARCHARprincipalBACKFLUX_ZSEx subtracted background at object positioncountsphot.count;em.IR.ZVARCHARprincipalPSFNUM_ZPSFEx number of stars usedmeta.number;em.IR.ZVARCHARprincipalPSFCHI2_ZPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.ZVARCHARprincipalPSFFWHM_ZPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.ZVARCHARprincipalNSEC_ZSEx number of secondary components detectedmeta.number;em.IR.ZVARCHARprincipalGALXCEN_ZGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.ZVARCHARprincipalGALYCEN_ZGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.ZVARCHARprincipalGALMAG_ZGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.ZVARCHARprincipalGALRE_ZGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.ZVARCHARprincipalGALINDEX_ZGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.ZVARCHARprincipalGALELLIP_ZGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.ZVARCHARprincipalGALPA_ZGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.ZVARCHARprincipalGALXCENERR_ZGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALYCENERR_ZGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALMAGERR_ZGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALREERR_ZGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALINDEXERR_ZGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALELLIPERR_ZGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALPAERR_ZGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALRA_ZGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.ZVARCHARprincipalGALDEC_ZGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.ZVARCHARprincipalGALMAG10RE_ZGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.ZVARCHARprincipalGALMU0_ZGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.ZVARCHARprincipalGALMUE_ZGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.ZVARCHARprincipalGALMUEAVG_ZGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.ZVARCHARprincipalGALR90_ZGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.ZVARCHARprincipalGALCHI2FULL_ZGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.ZVARCHARprincipalGALNDOF_ZGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.ZVARCHARprincipalGALCHI2_ZGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.ZVARCHARprincipalGALPLAN_ZSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.ZVARCHARprincipalPRICHI2FULL_ZPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalPRINFP_ZPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalPRINDOF_ZPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalPRICHI2_ZPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalCENFLUX_YCentral pixel flux value prior to background estimationcountsphot.count;em.IR.YVARCHARprincipalBACKFLUX_YSEx subtracted background at object positioncountsphot.count;em.IR.YVARCHARprincipalPSFNUM_YPSFEx number of stars usedmeta.number;em.IR.YVARCHARprincipalPSFCHI2_YPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.YVARCHARprincipalPSFFWHM_YPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.YVARCHARprincipalNSEC_YSEx number of secondary components detectedmeta.number;em.IR.YVARCHARprincipalGALXCEN_YGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.YVARCHARprincipalGALYCEN_YGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.YVARCHARprincipalGALMAG_YGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALRE_YGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALINDEX_YGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.YVARCHARprincipalGALELLIP_YGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.YVARCHARprincipalGALPA_YGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.YVARCHARprincipalGALXCENERR_YGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALYCENERR_YGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALMAGERR_YGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALREERR_YGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALINDEXERR_YGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALELLIPERR_YGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALPAERR_YGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALRA_YGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.YVARCHARprincipalGALDEC_YGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.YVARCHARprincipalGALMAG10RE_YGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALMU0_YGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUE_YGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUEAVG_YGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALR90_YGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALCHI2FULL_YGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALNDOF_YGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALCHI2_YGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALPLAN_YSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2FULL_YPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINFP_YPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINDOF_YPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2_YPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalCENFLUX_JCentral pixel flux value prior to background estimationcountsphot.count;em.IR.JVARCHARprincipalBACKFLUX_JSEx subtracted background at object positioncountsphot.count;em.IR.JVARCHARprincipalPSFNUM_JPSFEx number of stars usedmeta.number;em.IR.JVARCHARprincipalPSFCHI2_JPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.JVARCHARprincipalPSFFWHM_JPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.JVARCHARprincipalNSEC_JSEx number of secondary components detectedmeta.number;em.IR.JVARCHARprincipalGALXCEN_JGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.JVARCHARprincipalGALYCEN_JGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.JVARCHARprincipalGALMAG_JGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALRE_JGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALINDEX_JGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.JVARCHARprincipalGALELLIP_JGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.JVARCHARprincipalGALPA_JGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.JVARCHARprincipalGALXCENERR_JGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALYCENERR_JGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALMAGERR_JGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALREERR_JGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALINDEXERR_JGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALELLIPERR_JGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALPAERR_JGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALRA_JGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.JVARCHARprincipalGALDEC_JGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.JVARCHARprincipalGALMAG10RE_JGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALMU0_JGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUE_JGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUEAVG_JGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALR90_JGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALCHI2FULL_JGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALNDOF_JGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALCHI2_JGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALPLAN_JSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2FULL_JPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINFP_JPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINDOF_JPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2_JPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalCENFLUX_HCentral pixel flux value prior to background estimationcountsphot.count;em.IR.HVARCHARprincipalBACKFLUX_HSEx subtracted background at object positioncountsphot.count;em.IR.HVARCHARprincipalPSFNUM_HPSFEx number of stars usedmeta.number;em.IR.HVARCHARprincipalPSFCHI2_HPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.HVARCHARprincipalPSFFWHM_HPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.HVARCHARprincipalNSEC_HSEx number of secondary components detectedmeta.number;em.IR.HVARCHARprincipalGALXCEN_HGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.HVARCHARprincipalGALYCEN_HGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.HVARCHARprincipalGALMAG_HGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALRE_HGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALINDEX_HGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.HVARCHARprincipalGALELLIP_HGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.HVARCHARprincipalGALPA_HGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.HVARCHARprincipalGALXCENERR_HGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALYCENERR_HGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALMAGERR_HGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALREERR_HGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALINDEXERR_HGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALELLIPERR_HGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALPAERR_HGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALRA_HGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.HVARCHARprincipalGALDEC_HGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.HVARCHARprincipalGALMAG10RE_HGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALMU0_HGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUE_HGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUEAVG_HGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALR90_HGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALCHI2FULL_HGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALNDOF_HGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALCHI2_HGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALPLAN_HSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2FULL_HPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINFP_HPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINDOF_HPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2_HPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalCENFLUX_KCentral pixel flux value prior to background estimationcountsphot.count;em.IR.KVARCHARprincipalBACKFLUX_KSEx subtracted background at object positioncountsphot.count;em.IR.KVARCHARprincipalPSFNUM_KPSFEx number of stars usedmeta.number;em.IR.KVARCHARprincipalPSFCHI2_KPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.KVARCHARprincipalPSFFWHM_KPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.KVARCHARprincipalNSEC_KSEx number of secondary components detectedmeta.number;em.IR.KVARCHARprincipalGALXCEN_KGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.KVARCHARprincipalGALYCEN_KGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.KVARCHARprincipalGALMAG_KGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALRE_KGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALINDEX_KGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.KVARCHARprincipalGALELLIP_KGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.KVARCHARprincipalGALPA_KGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.KVARCHARprincipalGALXCENERR_KGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALYCENERR_KGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALMAGERR_KGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALREERR_KGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALINDEXERR_KGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALELLIPERR_KGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALPAERR_KGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALRA_KGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.KVARCHARprincipalGALDEC_KGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.KVARCHARprincipalGALMAG10RE_KGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALMU0_KGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUE_KGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUEAVG_KGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALR90_KGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALCHI2FULL_KGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALNDOF_KGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALCHI2_KGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALPLAN_KSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2FULL_KPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINFP_KPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINDOF_KPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2_KPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.AATFibreAllv27This table contains all fibre information for all GAMA AATobservations in AATFields from the fibre fits extension ofthe final reduced 2d data files.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalNAMEName of target in config filemeta.id;srcVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalXFibre x position on platepos.cartesian.xVARCHARprincipalYFibre y position on platepos.cartesian.yVARCHARprincipalXERRError on Xstat.error;pos.cartesian.xVARCHARprincipalYERRError on Ystat.error;pos.cartesian.yVARCHARprincipalTHETAAngle of fibre on field platepos.posAngVARCHARprincipalTYPEFibre type: F=guide, N=broken, P=program, S=sky, U=unusedmeta.code.classVARCHARprincipalPIVOT2dF fibre pivot numbermeta.id;instrVARCHARprincipalMAGNITUDEMagnitude of target from config filephot.magVARCHARprincipalPIDProgram IDmeta.idVARCHARprincipalRETRACTOR2dF retractor numbermeta.id;instrVARCHARprincipalWLENUnknownmeta.crypticVARCHARprincipalCOMMENTComment from the config filemeta.noteVARCHARprincipalgama_pdr4v2.AATFieldsv27This is a table of all AAT 2dF/AAOmega fields observed for GAMA.FIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalRARA of field centre (J2000)degpos.eq.ra;obs.fieldVARCHARprincipalDECDEC of field centre (J2000)degpos.eq.dec;obs.fieldVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalUTMJDMean MJD of start of exposurestime.epoch;obs.exposureVARCHARprincipalUTSTARTUT of start of first exposuretime.start;obs.exposureVARCHARprincipalUTENDUT of end of last exposuretime.end;obs.exposureVARCHARprincipalZDSTARTZenith distance at start of first exposuredegpos.az.zd;time.startVARCHARprincipalZDENDZenith distance at end of last exposuredegpos.az.zd;time.rndVARCHARprincipalHASTARTHour angle at start of first exposuredegpos.eq.ha;time.startVARCHARprincipalHAENDHour angle at end of last exposuredegpos.eq.ha;time.endVARCHARprincipalN_EXPNumber of exposuresmeta.number;obs.exposureVARCHARprincipalN_NIGHTSNumber of nights over which exposures were spreadmeta.numberVARCHARprincipalT_EXPTotal exposure timestime.duration;obs.exposureVARCHARprincipalMEAN_SNMean S/N of spectrastat.snr;spectVARCHARprincipalPLATE2dF plate numbermeta.id;instrVARCHARprincipalCONFIG_FILEName of configuration filemeta.id;meta.file;instr.setupVARCHARprincipalTDFDRVERVersion of 2dfdr data reduction softwaremeta.version;meta.softwareVARCHARprincipalUSEROriginal redshifter of this fieldmeta.idVARCHARprincipalDATE_ZDate of original redshifting runtime.processingVARCHARprincipalCRCORVERRunz version used for original redshifting runmeta.version;meta.softwareVARCHARprincipalHEL_VCHeliocentric velocity correctionkm/sphys.velocity;pos.heliocentricVARCHARprincipalN_SPECNumber of spectra observedmeta.number;spectVARCHARprincipalN_GALNumber of galaxy targets observedmeta.number;srcVARCHARprincipalN_STARNumber of calibration stars observedmeta.number;src.calibVARCHARprincipalN_GOODNumber of spectra with a good quality redshift, i.e. nQ >= 3meta.number;spectVARCHARprincipalN_GAL_GOODNumber of galaxy target spectra with a good quality redshift, i.e. nQ >= 3meta.number;srcVARCHARprincipalCOMPLRedshift success ratearith.ratio;meta.number;spectVARCHARprincipalGAL_COMPLRedshift success rate among galaxy targetsarith.ratio;meta.number;srcVARCHARprincipalFILENAMEFull path and filename of the field's FITS filemeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the field's FITS filemeta.ref.url;meta.file;meta.fitsVARCHARprincipalgama_pdr4v2.AATSpecAutozCombv27This table provides a fully automated redshift estimate forcombinations of two or three GAMA AAT spectra of the same target.COMBIDID for spectral coaddmeta.id;meta.mainVARCHARindexedprincipalSPECID1ID of GAMA AAT spectrummeta.idVARCHARprincipalSPECID2ID of GAMA AAT spectrummeta.idVARCHARprincipalSPECID3ID of GAMA AAT spectrum, set to xxx if only two spectra are combinedmeta.idVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.idVARCHARprincipalRMS_MAD_RATIORMS divided by mean absolute deviation for the HP spectrumstat.valueVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalCC_SIGMACross-correlation peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATETemplate ID; 0-22 for stars, 40-47 for galaxiesmeta.idVARCHARprincipalZ2Heliocentric redshift of second peaksrc.redshiftVARCHARprincipalCC_SIGMA2Cross-correlation 2nd peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATE2Template ID for second peakmeta.idVARCHARprincipalCC_SIGMA3Cross-correlation 3rd peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA4Cross-correlation 4th peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA1TO234Peak value divided by RMS of 2nd-4th peak valuesstat.valueVARCHARprincipalCC_FOMFigure of merit for primary redshift confidencestat.valueVARCHARprincipalPROBEstimated probability of redshift successstat.valueVARCHARprincipalVEL_ERRUncertainty in redshift, given as a velocity, delta c ln(1+z)km/sstat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.DoublezCandidatesv01This table provides a list of GAMA AAT spectra that probably includethe light from two galaxies and thus show two redshifts.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.idVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalCC_SIGMACross-correlation peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATETemplate ID; 0-22 for stars, 40-47 for galaxiesmeta.idVARCHARprincipalZ2Heliocentric redshift of second peaksrc.redshiftVARCHARprincipalCC_SIGMA2Cross-correlation 2nd peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATE2Template ID for second peakmeta.idVARCHARprincipalCC_SIGMA2TO342nd peak value divided by RMS of 3rd and 4th peak valuesstat.valueVARCHARprincipalCC_SIGMA2TO34_OLDOld value of CC_SIGMA2TO34, using templates 23-28 for galaxiesstat.valueVARCHARprincipalIS_DBESTSpectrum of object with highest CC_SIGMA2TO34 value?meta.codeVARCHARprincipalSPECTYPESpectral classification: PG=templates 40-42, ELG=43-47, lowest redshift firstmeta.codeVARCHARprincipalVISUALTYPEPreliminary visual classfication by Benne Holwerdameta.codeVARCHARprincipalCOMMENTComments by Benne Holwerda on visual classificationmeta.noteVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.LTSpecAllv03This table lists a small number of spectra of fibre-bright targetscollected by the GAMA team at the Liverpool Telescope (LT).SPECIDID of GAMA LT spectrummeta.id;meta.mainVARCHARindexedprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTGAMA LT spectrum with best redshift for this object?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.SpecAllv27This table lists all spectra that are available in the GAMA surveyregions, including GAMA spectra and those from previousspectroscopic surveys (such as the SDSS). Duplicate observations ofthe same object are retained in this table (but a flag is providedto mark the spectrum that provided the best available redshift of agiven object). Every spectrum listed in this table is available inthe GAMA DR4 database.SPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalSURVEY_CODENumerical code for originating surveymeta.code;meta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in originating survey?meta.codeVARCHARprincipalIS_BESTSpectrum with best redshift for this object?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.SpecObjv27This table lists each observed target and the spectrum thatprovides its best redshift (from GAMA or otherwise).CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalIC_FLAGCatalogue source(s) of GAMA objectmeta.code.memberVARCHARprincipalN_SPECNumber of spectra available for this objectmeta.number;spectVARCHARprincipalN_GAMA_SPECNumber of GAMA spectra available for this objectmeta.number;spectVARCHARprincipalDISTDistance between GAMA object and best matched spectrumarcsecpos.angDistanceVARCHARprincipalSPECIDID of best matched spectrummeta.id.cross;spectVARCHARprincipalSURVEYSurvey best matched spectrum originated frommeta.datasetVARCHARprincipalSURVEY_CODENumerical code for originating surveymeta.code;meta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.DirectSummationv05This table provides direct summation line measurements for allspectra of those objects that have a best redshift with nQ > 1and 0.002 < z < 1.35.SPECIDUnique spectrum IDVARCHARprincipalCATAIDUnique GAMA object IDVARCHARprincipalRAJ2000degVARCHARprincipalDECJ2000degVARCHARprincipalZRedshift with heliocentric correction removedVARCHARprincipalNQRedshift qualityVARCHARprincipalSURVEYSurvey spectrum originated fromVARCHARprincipalSURVEY_CODENumerical code for originating surveyVARCHARprincipalIS_BESTSpectrum with best redshift for this object?VARCHARprincipalIS_SBESTSpectrum with best redshift for originating survey?VARCHARprincipalSNS/N ratio per pixel in the 6383 - 6536 A window in the galaxy frameVARCHARprincipalD4000N4000 A break strength (see notes for description)VARCHARprincipalD4000N_ERRUncertainty on the 4000 A break strengthVARCHARprincipalBH_NAD_CONTBH_NAD continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_NAD_EW_ERRBH_NAD equivalent width uncertaintymagVARCHARprincipalBH_NAD_EWBH_NAD line equivalent widthmagVARCHARprincipalBH_NAD_FLUX_ERRBH_NAD flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_NAD_FLUXBH_NAD line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_FC_CONTBH_FC continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_FC_EW_ERRBH_FC equivalent width uncertaintymagVARCHARprincipalBH_FC_EWBH_FC line equivalent widthmagVARCHARprincipalBH_FC_FLUX_ERRBH_FC flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_FC_FLUXBH_FC line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MH_CONTBH_MH continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_MH_EW_ERRBH_MH equivalent width uncertaintymagVARCHARprincipalBH_MH_EWBH_MH line equivalent widthmagVARCHARprincipalBH_MH_FLUX_ERRBH_MH flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MH_FLUXBH_MH line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MGG_CONTBH_MGG continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_MGG_EW_ERRBH_MGG equivalent width uncertaintymagVARCHARprincipalBH_MGG_EWBH_MGG line equivalent widthmagVARCHARprincipalBH_MGG_FLUX_ERRBH_MGG flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MGG_FLUXBH_MGG line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HB_CONTBH_HB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_HB_EW_ERRBH_HB equivalent width uncertaintymagVARCHARprincipalBH_HB_EWBH_HB line equivalent widthmagVARCHARprincipalBH_HB_FLUX_ERRBH_HB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HB_FLUXBH_HB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_G_CONTBH_G continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_G_EW_ERRBH_G equivalent width uncertaintymagVARCHARprincipalBH_G_EWBH_G line equivalent widthmagVARCHARprincipalBH_G_FLUX_ERRBH_G flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_G_FLUXBH_G line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CAI_CONTBH_CAI continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_CAI_EW_ERRBH_CAI equivalent width uncertaintymagVARCHARprincipalBH_CAI_EWBH_CAI line equivalent widthmagVARCHARprincipalBH_CAI_FLUX_ERRBH_CAI flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CAI_FLUXBH_CAI line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HK_CONTBH_HK continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_HK_EW_ERRBH_HK equivalent width uncertaintymagVARCHARprincipalBH_HK_EWBH_HK line equivalent widthmagVARCHARprincipalBH_HK_FLUX_ERRBH_HK flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HK_FLUXBH_HK line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CNB_CONTBH_CNB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_CNB_EW_ERRBH_CNB equivalent width uncertaintymagVARCHARprincipalBH_CNB_EWBH_CNB line equivalent widthmagVARCHARprincipalBH_CNB_FLUX_ERRBH_CNB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CNB_FLUXBH_CNB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_CONTSIIR continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSIIR_EW_ERRSIIR equivalent width uncertaintyAVARCHARprincipalSIIR_EWSIIR line equivalent widthAVARCHARprincipalSIIR_FLUX_ERRSIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_FLUXSIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_CONTSIIB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSIIB_EW_ERRSIIB equivalent width uncertaintyAVARCHARprincipalSIIB_EWSIIB line equivalent widthAVARCHARprincipalSIIB_FLUX_ERRSIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_FLUXSIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_CONTNIIR continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNIIR_EW_ERRNIIR equivalent width uncertaintyAVARCHARprincipalNIIR_EWNIIR line equivalent widthAVARCHARprincipalNIIR_FLUX_ERRNIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_FLUXNIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_CONTNIIB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNIIB_EW_ERRNIIB equivalent width uncertaintyAVARCHARprincipalNIIB_EWNIIB line equivalent widthAVARCHARprincipalNIIB_FLUX_ERRNIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_FLUXNIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_CONTHA continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_EW_ERRHA equivalent width uncertaintyAVARCHARprincipalHA_EWHA line equivalent widthAVARCHARprincipalHA_FLUX_ERRHA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_FLUXHA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6364_CONTOI6364 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI6364_EW_ERROI6364 equivalent width uncertaintyAVARCHARprincipalOI6364_EWOI6364 line equivalent widthAVARCHARprincipalOI6364_FLUX_ERROI6364 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6364_FLUXOI6364 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIII6312_CONTSIII6312 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSIII6312_EW_ERRSIII6312 equivalent width uncertaintyAVARCHARprincipalSIII6312_EWSIII6312 line equivalent widthAVARCHARprincipalSIII6312_FLUX_ERRSIII6312 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIII6312_FLUXSIII6312 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6300_CONTOI6300 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI6300_EW_ERROI6300 equivalent width uncertaintyAVARCHARprincipalOI6300_EWOI6300 line equivalent widthAVARCHARprincipalOI6300_FLUX_ERROI6300 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6300_FLUXOI6300 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO2_CONTTIO2 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalTIO2_EW_ERRTIO2 equivalent width uncertaintymagVARCHARprincipalTIO2_EWTIO2 line equivalent widthmagVARCHARprincipalTIO2_FLUX_ERRTIO2 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO2_FLUXTIO2 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO1_CONTTIO1 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalTIO1_EW_ERRTIO1 equivalent width uncertaintymagVARCHARprincipalTIO1_EWTIO1 line equivalent widthmagVARCHARprincipalTIO1_FLUX_ERRTIO1 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO1_FLUXTIO1 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNA5895_CONTNA5895 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNA5895_EW_ERRNA5895 equivalent width uncertaintyAVARCHARprincipalNA5895_EWNA5895 line equivalent widthAVARCHARprincipalNA5895_FLUX_ERRNA5895 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNA5895_FLUXNA5895 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNII5755_CONTNII5755 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNII5755_EW_ERRNII5755 equivalent width uncertaintyAVARCHARprincipalNII5755_EWNII5755 line equivalent widthAVARCHARprincipalNII5755_FLUX_ERRNII5755 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNII5755_FLUXNII5755 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5782_CONTFE5782 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5782_EW_ERRFE5782 equivalent width uncertaintyAVARCHARprincipalFE5782_EWFE5782 line equivalent widthAVARCHARprincipalFE5782_FLUX_ERRFE5782 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5782_FLUXFE5782 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5709_CONTFE5709 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5709_EW_ERRFE5709 equivalent width uncertaintyAVARCHARprincipalFE5709_EWFE5709 line equivalent widthAVARCHARprincipalFE5709_FLUX_ERRFE5709 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5709_FLUXFE5709 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5406_CONTFE5406 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5406_EW_ERRFE5406 equivalent width uncertaintyAVARCHARprincipalFE5406_EWFE5406 line equivalent widthAVARCHARprincipalFE5406_FLUX_ERRFE5406 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5406_FLUXFE5406 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5335_CONTFE5335 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5335_EW_ERRFE5335 equivalent width uncertaintyAVARCHARprincipalFE5335_EWFE5335 line equivalent widthAVARCHARprincipalFE5335_FLUX_ERRFE5335 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5335_FLUXFE5335 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5270_CONTFE5270 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5270_EW_ERRFE5270 equivalent width uncertaintyAVARCHARprincipalFE5270_EWFE5270 line equivalent widthAVARCHARprincipalFE5270_FLUX_ERRFE5270 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5270_FLUXFE5270 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMGB5177_CONTMGB5177 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalMGB5177_EW_ERRMGB5177 equivalent width uncertaintyAVARCHARprincipalMGB5177_EWMGB5177 line equivalent widthAVARCHARprincipalMGB5177_FLUX_ERRMGB5177 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMGB5177_FLUXMGB5177 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG2_CONTMG2 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalMG2_EW_ERRMG2 equivalent width uncertaintymagVARCHARprincipalMG2_EWMG2 line equivalent widthmagVARCHARprincipalMG2_FLUX_ERRMG2 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG2_FLUXMG2 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG1_CONTMG1 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalMG1_EW_ERRMG1 equivalent width uncertaintymagVARCHARprincipalMG1_EWMG1 line equivalent widthmagVARCHARprincipalMG1_FLUX_ERRMG1 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG1_FLUXMG1 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5015_CONTFE5015 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5015_EW_ERRFE5015 equivalent width uncertaintyAVARCHARprincipalFE5015_EWFE5015 line equivalent widthAVARCHARprincipalFE5015_FLUX_ERRFE5015 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5015_FLUXFE5015 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_CONTOIIIR continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOIIIR_EW_ERROIIIR equivalent width uncertaintyAVARCHARprincipalOIIIR_EWOIIIR line equivalent widthAVARCHARprincipalOIIIR_FLUX_ERROIIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_FLUXOIIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_CONTOIIIB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOIIIB_EW_ERROIIIB equivalent width uncertaintyAVARCHARprincipalOIIIB_EWOIIIB line equivalent widthAVARCHARprincipalOIIIB_FLUX_ERROIIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_FLUXOIIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_P_CONTHB_P continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_P_EW_ERRHB_P equivalent width uncertaintyAVARCHARprincipalHB_P_EWHB_P line equivalent widthAVARCHARprincipalHB_P_FLUX_ERRHB_P flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_P_FLUXHB_P line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_CONTHB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_EW_ERRHB equivalent width uncertaintyAVARCHARprincipalHB_EWHB line equivalent widthAVARCHARprincipalHB_FLUX_ERRHB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_FLUXHB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4668_CONTFE4668 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE4668_EW_ERRFE4668 equivalent width uncertaintyAVARCHARprincipalFE4668_EWFE4668 line equivalent widthAVARCHARprincipalFE4668_FLUX_ERRFE4668 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4668_FLUXFE4668 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4531_CONTFE4531 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE4531_EW_ERRFE4531 equivalent width uncertaintyAVARCHARprincipalFE4531_EWFE4531 line equivalent widthAVARCHARprincipalFE4531_FLUX_ERRFE4531 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4531_FLUXFE4531 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4455_CONTCA4455 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCA4455_EW_ERRCA4455 equivalent width uncertaintyAVARCHARprincipalCA4455_EWCA4455 line equivalent widthAVARCHARprincipalCA4455_FLUX_ERRCA4455 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4455_FLUXCA4455 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4383_CONTFE4383 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE4383_EW_ERRFE4383 equivalent width uncertaintyAVARCHARprincipalFE4383_EWFE4383 line equivalent widthAVARCHARprincipalFE4383_FLUX_ERRFE4383 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4383_FLUXFE4383 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIII4363_CONTOIII4363 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOIII4363_EW_ERROIII4363 equivalent width uncertaintyAVARCHARprincipalOIII4363_EWOIII4363 line equivalent widthAVARCHARprincipalOIII4363_FLUX_ERROIII4363 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIII4363_FLUXOIII4363 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA275_CONTHGVA275 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGVA275_EW_ERRHGVA275 equivalent width uncertaintymagVARCHARprincipalHGVA275_EWHGVA275 line equivalent widthmagVARCHARprincipalHGVA275_FLUX_ERRHGVA275 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA275_FLUXHGVA275 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA200_CONTHGVA200 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGVA200_EW_ERRHGVA200 equivalent width uncertaintymagVARCHARprincipalHGVA200_EWHGVA200 line equivalent widthmagVARCHARprincipalHGVA200_FLUX_ERRHGVA200 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA200_FLUXHGVA200 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA125_CONTHGVA125 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGVA125_EW_ERRHGVA125 equivalent width uncertaintymagVARCHARprincipalHGVA125_EWHGVA125 line equivalent widthmagVARCHARprincipalHGVA125_FLUX_ERRHGVA125 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA125_FLUXHGVA125 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGF_CONTHGF continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGF_EW_ERRHGF equivalent width uncertaintyAVARCHARprincipalHGF_EWHGF line equivalent widthAVARCHARprincipalHGF_FLUX_ERRHGF flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGF_FLUXHGF line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGA_CONTHGA continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGA_EW_ERRHGA equivalent width uncertaintyAVARCHARprincipalHGA_EWHGA line equivalent widthAVARCHARprincipalHGA_FLUX_ERRHGA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGA_FLUXHGA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalG4300_CONTG4300 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalG4300_EW_ERRG4300 equivalent width uncertaintyAVARCHARprincipalG4300_EWG4300 line equivalent widthAVARCHARprincipalG4300_FLUX_ERRG4300 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalG4300_FLUXG4300 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4227_CONTCA4227 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCA4227_EW_ERRCA4227 equivalent width uncertaintyAVARCHARprincipalCA4227_EWCA4227 line equivalent widthAVARCHARprincipalCA4227_FLUX_ERRCA4227 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4227_FLUXCA4227 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN2_CONTCN2 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCN2_EW_ERRCN2 equivalent width uncertaintymagVARCHARprincipalCN2_EWCN2 line equivalent widthmagVARCHARprincipalCN2_FLUX_ERRCN2 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN2_FLUXCN2 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN1_CONTCN1 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCN1_EW_ERRCN1 equivalent width uncertaintymagVARCHARprincipalCN1_EWCN1 line equivalent widthmagVARCHARprincipalCN1_FLUX_ERRCN1 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN1_FLUXCN1 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDF_CONTHDF continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHDF_EW_ERRHDF equivalent width uncertaintyAVARCHARprincipalHDF_EWHDF line equivalent widthAVARCHARprincipalHDF_FLUX_ERRHDF flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDF_FLUXHDF line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDA_CONTHDA continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHDA_EW_ERRHDA equivalent width uncertaintyAVARCHARprincipalHDA_EWHDA line equivalent widthAVARCHARprincipalHDA_FLUX_ERRHDA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDA_FLUXHDA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOII_CONTOII continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_EW_ERROII equivalent width uncertaintyAVARCHARprincipalOII_EWOII line equivalent widthAVARCHARprincipalOII_FLUX_ERROII flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOII_FLUXOII line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GaussFitComplexv05This table provides emission line measurements from more complicatedGaussian fits to the OIII/Hbeta and NII/Halpha regions for allspectra of those objects that have a best redshift with nQ > 1and 0.002 < z < 1.35.SPECIDUnique spectrum IDVARCHARprincipalCATAIDUnique GAMA object IDVARCHARprincipalHB_CONTHB/OIIIB/OIIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_CONT_ERRHB/OIIIB/OIIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRADHB/OIIIB/OIIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRAD_ERRHB continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_REDCHI_EMBReduced chisquared for the continuum+narrow+broad emission line fitVARCHARprincipalHB_REDCHI_EMABSReduced chisquared for the continuum+narrow+absorption emission line fitVARCHARprincipalHB_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalHB_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHB_MODSEL_EMB_EMModel selection score for the continuum and Narrow+Broad emission-line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHB_MODSEL_NABS_NModel selection score for the continuum and Narrow emission plus absorption line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHB_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHB_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHB_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHB_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HBHB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_ERRHB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HBHB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_ERRHB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HBHB line sigma from Gaussian fitAVARCHARprincipalSIG_HB_ERRUncertainty on the HB line sigma from the Gaussian fitAVARCHARprincipalHB_FLUXHB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_FLUX_ERRHB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_EWHB line equivalent widthAVARCHARprincipalHB_EW_ERRHB equivalent width uncertaintyAVARCHARprincipalAMP_HB_ABSHB_ABS line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_ABS_ERRHB_ABS uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HB_ABSHB_ABS line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_ABS_ERRHB_ABS uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HB_ABSHB_ABS line sigma from Gaussian fitAVARCHARprincipalSIG_HB_ABS_ERRUncertainty on the HB_ABS line sigma from the Gaussian fitAVARCHARprincipalHB_ABS_FLUXHB_ABS line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_ABS_FLUX_ERRHB_ABS flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_ABS_EWHB_ABS line equivalent widthAVARCHARprincipalHB_ABS_EW_ERRHB_ABS equivalent width uncertaintyAVARCHARprincipalHB_ABS_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalAMP_HB_BHB_B line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_B_ERRHB_B uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HB_BHB_B line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_B_ERRHB_B uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HB_BHB_B line sigma from Gaussian fitAVARCHARprincipalSIG_HB_B_ERRUncertainty on the HB_B line sigma from the Gaussian fitAVARCHARprincipalHB_B_FLUXHB_B line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_B_FLUX_ERRHB_B flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_B_EWHB_B line equivalent widthAVARCHARprincipalHB_B_EW_ERRHB_B equivalent width uncertaintyAVARCHARprincipalHB_B_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalAMP_OIIIBOIIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIB_ERROIIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIBOIIIB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIB_ERROIIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIBOIIIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIB_ERRUncertainty on the OIIIB line sigma from the Gaussian fitAVARCHARprincipalOIIIB_FLUXOIIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_FLUX_ERROIIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_EWOIIIB line equivalent widthAVARCHARprincipalOIIIB_EW_ERROIIIB equivalent width uncertaintyAVARCHARprincipalAMP_OIIIROIIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIR_ERROIIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIROIIIR line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIR_ERROIIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIROIIIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIR_ERRUncertainty on the OIIIR line sigma from the Gaussian fitAVARCHARprincipalOIIIR_FLUXOIIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_FLUX_ERROIIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_EWOIIIR line equivalent widthAVARCHARprincipalOIIIR_EW_ERROIIIR equivalent width uncertaintyAVARCHARprincipalOIIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIRVARCHARprincipalOIIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIBVARCHARprincipalHA_CONTNIIB/HA/NIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_CONT_ERRNIIB/HA/NIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRADNIIB/HA/NIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRAD_ERRHA continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_REDCHI_EMBReduced chisquared for the continuum+narrow+broad emission line fitVARCHARprincipalHA_REDCHI_EMABSReduced chisquared for the continuum+narrow+absorption emission line fitVARCHARprincipalHA_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHA_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalHA_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHA_MODSEL_EMB_EMModel selection score for the continuum and Narrow+Broad emission-line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHA_MODSEL_NABS_NModel selection score for the continuum and Narrow emission plus absorption line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHA_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHA_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHA_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHA_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HAHA line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_ERRHA uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HAHA line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_ERRHA uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HAHA line sigma from Gaussian fitAVARCHARprincipalSIG_HA_ERRUncertainty on the HA line sigma from the Gaussian fitAVARCHARprincipalHA_FLUXHA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_FLUX_ERRHA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_EWHA line equivalent widthAVARCHARprincipalHA_EW_ERRHA equivalent width uncertaintyAVARCHARprincipalAMP_HA_ABSHA_ABS line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_ABS_ERRHA_ABS uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HA_ABSHA_ABS line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_ABS_ERRHA_ABS uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HA_ABSHA_ABS line sigma from Gaussian fitAVARCHARprincipalSIG_HA_ABS_ERRUncertainty on the HA_ABS line sigma from the Gaussian fitAVARCHARprincipalHA_ABS_FLUXHA_ABS line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_ABS_FLUX_ERRHA_ABS flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_ABS_EWHA_ABS line equivalent widthAVARCHARprincipalHA_ABS_EW_ERRHA_ABS equivalent width uncertaintyAVARCHARprincipalHA_ABS_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalAMP_HA_BHA_B line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_B_ERRHA_B uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HA_BHA_B line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_B_ERRHA_B uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HA_BHA_B line sigma from Gaussian fitAVARCHARprincipalSIG_HA_B_ERRUncertainty on the HA_B line sigma from the Gaussian fitAVARCHARprincipalHA_B_FLUXHA_B line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_B_FLUX_ERRHA_B flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_B_EWHA_B line equivalent widthAVARCHARprincipalHA_B_EW_ERRHA_B equivalent width uncertaintyAVARCHARprincipalHA_B_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalAMP_NIIBNIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIB_ERRNIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIBNIIB line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIB_ERRNIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIBNIIB line sigma from Gaussian fitAVARCHARprincipalSIG_NIIB_ERRUncertainty on the NIIB line sigma from the Gaussian fitAVARCHARprincipalNIIB_FLUXNIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_FLUX_ERRNIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_EWNIIB line equivalent widthAVARCHARprincipalNIIB_EW_ERRNIIB equivalent width uncertaintyAVARCHARprincipalAMP_NIIRNIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIR_ERRNIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIRNIIR line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIR_ERRNIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIRNIIR line sigma from Gaussian fitAVARCHARprincipalSIG_NIIR_ERRUncertainty on the NIIR line sigma from the Gaussian fitAVARCHARprincipalNIIR_FLUXNIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_FLUX_ERRNIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_EWNIIR line equivalent widthAVARCHARprincipalNIIR_EW_ERRNIIR equivalent width uncertaintyAVARCHARprincipalNIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIBVARCHARprincipalNIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIRVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.GaussFitSimplev05This table provides emission line measurements from simple Gaussianfits for all spectra of those objects that have a best redshift withnQ > 1 and 0.002 < z < 1.35.NQRedshift qualityVARCHARprincipalZRedshift with heliocentric correction removedVARCHARprincipalSPECIDUnique spectrum IDVARCHARprincipalCATAIDUnique GAMA object IDVARCHARprincipalRAJ2000degVARCHARprincipalDECJ2000degVARCHARprincipalSURVEYSurvey spectrum originated fromVARCHARprincipalSURVEY_CODENumerical code for originating surveyVARCHARprincipalIS_BESTSpectrum with best redshift for this object?VARCHARprincipalIS_SBESTSpectrum with best redshift for originating survey?VARCHARprincipalSNS/N ratio per pixel in the 6383 - 6536 A window in the galaxy frameVARCHARprincipalMEAN_CONTSigma clipped mean continuum level used for S in S/NVARCHARprincipalSIGMA_CONTScatter around continuum used for N in S/NVARCHARprincipalFSCALEFor SDSS spectra, the flux is scaled by this value to approximate the scaling used for AAOmega spectraVARCHARprincipalD4000N4000 A break strength (see notes for description)VARCHARprincipalD4000N_ERRUncertainty on the 4000 A break strengthVARCHARprincipalOII_CONTOII continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_CONT_ERROII continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_GRADOII continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_GRAD_ERROII continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalOII_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalOII_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalOII_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalOII_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalOII_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalOII_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalOII_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_OIIROIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIR_ERROIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIROIIR line position from Gaussian fit measured relative to OII_CENAVARCHARprincipalPOS_OIIR_ERROIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIROIIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIIR_ERRUncertainty on the OIIR line sigma from the Gaussian fitAVARCHARprincipalOIIR_FLUXOIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIR_FLUX_ERROIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIR_EWOIIR line equivalent widthAVARCHARprincipalOIIR_EW_ERROIIR equivalent width uncertaintyAVARCHARprincipalAMP_OIIBOIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIB_ERROIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIBOIIB line position from Gaussian fit measured relative to OII_CENAVARCHARprincipalPOS_OIIB_ERROIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIBOIIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIIB_ERRUncertainty on the OIIB line sigma from the Gaussian fitAVARCHARprincipalOIIB_FLUXOIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIB_FLUX_ERROIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIB_EWOIIB line equivalent widthAVARCHARprincipalOIIB_EW_ERROIIB equivalent width uncertaintyAVARCHARprincipalOIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIBVARCHARprincipalOIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIRVARCHARprincipalHB_CONTHB/OIIIB/OIIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_CONT_ERRHB/OIIIB/OIIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRADHB/OIIIB/OIIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRAD_ERRHB continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalHB_REDCHI_ABSReduced chisquared for the continuum plus absorption line fitVARCHARprincipalHB_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalHB_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHB_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHB_MODSEL_ABS_LINEModel selection score for the continuum-plus-absorption-line fit compared to the straight-line continuum fitVARCHARprincipalHB_MODSEL_EM_ABSModel selection score for the continuum-plus-emission-line fit compared to the continuum-plus-absorption-line fitVARCHARprincipalHB_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHB_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHB_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHB_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HBHB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_ERRHB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HBHB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_ERRHB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HBHB line sigma from Gaussian fitAVARCHARprincipalSIG_HB_ERRUncertainty on the HB line sigma from the Gaussian fitAVARCHARprincipalHB_FLUXHB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_FLUX_ERRHB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_EWHB line equivalent widthAVARCHARprincipalHB_EW_ERRHB equivalent width uncertaintyAVARCHARprincipalHB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalAMP_OIIIBOIIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIB_ERROIIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIBOIIIB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIB_ERROIIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIBOIIIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIB_ERRUncertainty on the OIIIB line sigma from the Gaussian fitAVARCHARprincipalOIIIB_FLUXOIIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_FLUX_ERROIIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_EWOIIIB line equivalent widthAVARCHARprincipalOIIIB_EW_ERROIIIB equivalent width uncertaintyAVARCHARprincipalAMP_OIIIROIIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIR_ERROIIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIROIIIR line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIR_ERROIIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIROIIIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIR_ERRUncertainty on the OIIIR line sigma from the Gaussian fitAVARCHARprincipalOIIIR_FLUXOIIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_FLUX_ERROIIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_EWOIIIR line equivalent widthAVARCHARprincipalOIIIR_EW_ERROIIIR equivalent width uncertaintyAVARCHARprincipalOIIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIBVARCHARprincipalOIIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIRVARCHARprincipalHA_CONTNIIB/HA/NIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_CONT_ERRNIIB/HA/NIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRADNIIB/HA/NIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRAD_ERRHA continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalHA_REDCHI_ABSReduced chisquared for the continuum plus absorption line fitVARCHARprincipalHA_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalHA_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHA_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHA_MODSEL_ABS_LINEModel selection score for the continuum-plus-absorption-line fit compared to the straight-line continuum fitVARCHARprincipalHA_MODSEL_EM_ABSModel selection score for the continuum-plus-emission-line fit compared to the continuum-plus-absorption-line fitVARCHARprincipalHA_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHA_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHA_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHA_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HAHA line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_ERRHA uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HAHA line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_ERRHA uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HAHA line sigma from Gaussian fitAVARCHARprincipalSIG_HA_ERRUncertainty on the HA line sigma from the Gaussian fitAVARCHARprincipalHA_FLUXHA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_FLUX_ERRHA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_EWHA line equivalent widthAVARCHARprincipalHA_EW_ERRHA equivalent width uncertaintyAVARCHARprincipalHA_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalAMP_NIIBNIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIB_ERRNIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIBNIIB line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIB_ERRNIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIBNIIB line sigma from Gaussian fitAVARCHARprincipalSIG_NIIB_ERRUncertainty on the NIIB line sigma from the Gaussian fitAVARCHARprincipalNIIB_FLUXNIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_FLUX_ERRNIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_EWNIIB line equivalent widthAVARCHARprincipalNIIB_EW_ERRNIIB equivalent width uncertaintyAVARCHARprincipalAMP_NIIRNIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIR_ERRNIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIRNIIR line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIR_ERRNIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIRNIIR line sigma from Gaussian fitAVARCHARprincipalSIG_NIIR_ERRUncertainty on the NIIR line sigma from the Gaussian fitAVARCHARprincipalNIIR_FLUXNIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_FLUX_ERRNIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_EWNIIR line equivalent widthAVARCHARprincipalNIIR_EW_ERRNIIR equivalent width uncertaintyAVARCHARprincipalNIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIBVARCHARprincipalNIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIRVARCHARprincipalSII_CONTSII continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_CONT_ERRSII continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_GRADSII continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_GRAD_ERRSII continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalSII_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalSII_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalSII_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalSII_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalSII_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalSII_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalSII_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_SIIBSIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_SIIB_ERRSIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_SIIBSIIB line position from Gaussian fit measured relative to SII_CENAVARCHARprincipalPOS_SIIB_ERRSIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_SIIBSIIB line sigma from Gaussian fitAVARCHARprincipalSIG_SIIB_ERRUncertainty on the SIIB line sigma from the Gaussian fitAVARCHARprincipalSIIB_FLUXSIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_FLUX_ERRSIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_EWSIIB line equivalent widthAVARCHARprincipalSIIB_EW_ERRSIIB equivalent width uncertaintyAVARCHARprincipalAMP_SIIRSIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_SIIR_ERRSIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_SIIRSIIR line position from Gaussian fit measured relative to SII_CENAVARCHARprincipalPOS_SIIR_ERRSIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_SIIRSIIR line sigma from Gaussian fitAVARCHARprincipalSIG_SIIR_ERRUncertainty on the SIIR line sigma from the Gaussian fitAVARCHARprincipalSIIR_FLUXSIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_FLUX_ERRSIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_EWSIIR line equivalent widthAVARCHARprincipalSIIR_EW_ERRSIIR equivalent width uncertaintyAVARCHARprincipalSIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to SIIBVARCHARprincipalSIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to SIIRVARCHARprincipalOI_CONTOI continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_CONT_ERROI continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_GRADOI continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_GRAD_ERROI continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalOI_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalOI_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalOI_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalOI_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalOI_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalOI_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalOI_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_OIBOIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIB_ERROIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIBOIB line position from Gaussian fit measured relative to OI_CENAVARCHARprincipalPOS_OIB_ERROIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIBOIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIB_ERRUncertainty on the OIB line sigma from the Gaussian fitAVARCHARprincipalOIB_FLUXOIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIB_FLUX_ERROIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIB_EWOIB line equivalent widthAVARCHARprincipalOIB_EW_ERROIB equivalent width uncertaintyAVARCHARprincipalAMP_OIROIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIR_ERROIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIROIR line position from Gaussian fit measured relative to OI_CENAVARCHARprincipalPOS_OIR_ERROIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIROIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIR_ERRUncertainty on the OIR line sigma from the Gaussian fitAVARCHARprincipalOIR_FLUXOIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIR_FLUX_ERROIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIR_EWOIR line equivalent widthAVARCHARprincipalOIR_EW_ERROIR equivalent width uncertaintyAVARCHARprincipalOIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIBVARCHARprincipalOIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIRVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.StellarMassesv24_21BandPhotomv03catidCATAID from 21BandPhotomv03VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_pdr4v2.StellarMassesv24_G02CFHTLSInputCatv04catidCATAID from G02TilingCatv07.fitsVARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_zz-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_zstatistical uncertainty in absmag_zVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_z_starsintrinsic stellar z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_z_starsstatistical uncertainty in absmag_z_starsVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_zobservers frame z-band flux from SPS fitVARCHARprincipaldelfitflux_zstatistical uncertainty in fitflux_zVARCHARprincipalgama_pdr4v2.StellarMassesv24_G02SDSSInputCatv01catidCATAID from G02TilingCatv07.fitsVARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_zz-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_zstatistical uncertainty in absmag_zVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_z_starsintrinsic stellar z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_z_starsstatistical uncertainty in absmag_z_starsVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_zobservers frame z-band flux from SPS fitVARCHARprincipaldelfitflux_zstatistical uncertainty in fitflux_zVARCHARprincipalgama_pdr4v2.StellarMassesv24_GAMAKidsVikingv01catidCATAID from GAMAKidsVikingv01VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_pdr4v2.VisualMorphologyv03This table provides a number of visual morphological classificationsperformed by various people for various samples of GAMA II galaxiesin the equatorial survey regions.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalELLIPTICALSimon`s and Stephen`s visual classificationmeta.code.classVARCHARprincipalELLIPTICAL_CODENumerical code for ELLIPTICAL, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPE_SPDSimon`s and Stephen`s visual Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_SPD_CODENumerical code for HUBBLE_TYPE_SPD, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPE_LSKLee`s and Uros` visual Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_LSK_CODENumerical code for HUBBLE_TYPE_LSK, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPE_ASGRAaron`s and Rebecca`s visual Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_ASGR_CODENumerical code for HUBBLE_TYPE_ASGR, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPEFinal Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_CODENumerical code for HUBBLE_TYPE, see notesmeta.code.classVARCHARprincipalASGR_DISTURBEDRenormalised votes that galaxy is disturbed, see notesmeta.code.classVARCHARprincipalASGR_NORMALRenormalised votes that galaxy is undisturbed, see notesmeta.code.classVARCHARprincipalASGR_UNSURERenormalised votes that classification in unclearmeta.code.classVARCHARprincipalASGR_CLASSIFIERSTotal number of classifiers (renormalised)meta.code.classVARCHARprincipalASGR_PROBDISTProbability galaxy is disturbed (ASGR_DISTURBED/ASGR_CLASSIFIERS)meta.code.classVARCHARprincipalP_ELFraction of Galaxy Zoo votes for Elliptical (biased)meta.code.classVARCHARprincipalP_CSFraction of Galaxy Zoo votes for NotElliptical (biased)meta.code.classVARCHARprincipalP_EL_DEBIASEDFraction of Galaxy Zoo votes for Elliptical (debiased)meta.code.classVARCHARprincipalP_CS_DEBIASEDFraction of Galaxy Zoo votes for NotElliptical (debiased)meta.code.classVARCHARprincipalURL_IMGURL of SDSS/UKIDSS-LAS/VIKING giH postage stampmeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.WISECatv02This table provides mid-IR photometry from WISE for all objects inthe GAMA II equatorial survey regions detected by WISE.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalDESIG_ALLWISEDesignation of matched WISE source from AllWISE Cataloguemeta.id.crossVARCHARprincipalDESIG_ALLSKYDesignation of matched WISE source from All-Sky Cataloguemeta.id.crossVARCHARprincipalRARight ascension (J2000) of matched WISE sourcedegpos.eq.raVARCHARprincipalDECDeclination (J2000) of matched WISE sourcedegpos.eq.decVARCHARprincipalSEPARATIONDistance between GAMA object and matched WISE sourcearcsecpos.angDistanceVARCHARprincipalW1MNumber of individual W1 exposures on which profile-fit was possibleVARCHARprincipalW2MNumber of individual W2 exposures on which profile-fit was possibleVARCHARprincipalW3MNumber of individual W3 exposures on which profile-fit was possibleVARCHARprincipalW4MNumber of individual W4 exposures on which profile-fit was possibleVARCHARprincipalW1COVMean pixel coverage in W1VARCHARprincipalW2COVMean pixel coverage in W2VARCHARprincipalW3COVMean pixel coverage in W3VARCHARprincipalW4COVMean pixel coverage in W4VARCHARprincipalMAG_W1Recommended W1 magnitudemagphot.mag;em.IR.3-4umVARCHARprincipalMAGERR_W1Recommended W1 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W1Recommended W1 photometry flag: 1=profile-fit, 2=isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W1Radius of aperture measurement in W1arcsecphys.angSizeVARCHARprincipalMAGPRO_W1Profile-fit W1 magnitudemagphot.mag;em.IR.3-4umVARCHARprincipalMAGPROERR_W1Profile-fit W1 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W1Reduced chi^2 of profile-fit W1 measurementstat.fit.chi2VARCHARprincipalFLUX_W1Raw W1 source flux measured in profile-fit photometrymJyphot.flux;em.IR.3-4umVARCHARprincipalFLUXERR_W1Uncertainty in the raw W1 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W1Standard aperture magnitude for W1magphot.mag;em.IR.3-4umVARCHARprincipalMAGSTDAPERR_W1Standard aperture magnitude error for W1magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W1Standard aperture magnitude flag for W1meta.codeVARCHARprincipalRADIUS_ISO_W1Isophotal radius in W1arcsecphys.angSizeVARCHARprincipalMAGISO_W1Isophotal W1 magnitudemagphot.mag;em.IR.3-4umVARCHARprincipalMAGISOERR_W1Isophotal W1 magnitude errormagstat.error;phot.magVARCHARprincipalMAG_W2Recommended W2 magnitudemagphot.mag;em.IR.4-8umVARCHARprincipalMAGERR_W2Recommended W2 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W2Recommended W2 photometry flag: 1=profile-fit, 2=derived from isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W2Radius of aperture measurement in W2arcsecphys.angSizeVARCHARprincipalMAGPRO_W2Profile-fit W2 magnitudemagphot.mag;em.IR.4-8umVARCHARprincipalMAGPROERR_W2Profile-fit W2 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W2Reduced chi^2 of profile-fit W2 measurementstat.fit.chi2VARCHARprincipalFLUX_W2Raw W2 source flux measured in profile-fit photometrymJyphot.flux;em.IR.4-8umVARCHARprincipalFLUXERR_W2Uncertainty in the raw W2 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W2Standard aperture magnitude for W2magphot.mag;em.IR.4-8umVARCHARprincipalMAGSTDAPERR_W2Standard aperture magnitude error for W2magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W2Standard aperture magnitude flag for W2meta.codeVARCHARprincipalRADIUS_ISO_W2Isophotal radius in W2arcsecphys.angSizeVARCHARprincipalMAGISO_W2Isophotal W2 magnitudemagphot.mag;em.IR.4-8umVARCHARprincipalMAGISOERR_W2Isophotal W2 magnitude errormagstat.error;phot.magVARCHARprincipalMAGDER_W2Derived W2 magnitude (from MAGISO_W1 and W1-W2 colour)magphot.mag;em.IR.4-8umVARCHARprincipalMAGDERERR_W2Derived W2 magnitude errormagstat.error;phot.magVARCHARprincipalMAG_W3Recommended W3 magnitudemagphot.mag;em.IR.8-15umVARCHARprincipalMAGERR_W3Recommended W3 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W3Recommended W3 photometry flag: 1=profile-fit, 2=isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W3Radius of aperture measurement in W3arcsecphys.angSizeVARCHARprincipalMAGPRO_W3Profile-fit W3 magnitudemagphot.mag;em.IR.8-15umVARCHARprincipalMAGPROERR_W3Profile-fit W3 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W3Reduced chi^2 of profile-fit W3 measurementstat.fit.chi2VARCHARprincipalFLUX_W3Raw W3 source flux measured in profile-fit photometrymJyphot.flux;em.IR.8-15umVARCHARprincipalFLUXERR_W3Uncertainty in the raw W3 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W3Standard aperture magnitude for W3magphot.mag;em.IR.8-15umVARCHARprincipalMAGSTDAPERR_W3Standard aperture magnitude error for W3magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W3Standard aperture magnitude flag for W3meta.codeVARCHARprincipalRADIUS_ISO_W3Isophotal radius in W3arcsecphys.angSizeVARCHARprincipalMAGISO_W3Isophotal W3 magnitudemagphot.mag;em.IR.8-15umVARCHARprincipalMAGISOERR_W3Isophotal W3 magnitude errormagstat.error;phot.magVARCHARprincipalMAG_W4Recommended W4 magnitudemagphot.mag;em.IR.15-30umVARCHARprincipalMAGERR_W4Recommended W4 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W4Recommended W4 photometry flag: 1=profile-fit, 2=derived from isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W4Radius of aperture measurement in W4arcsecphys.angSizeVARCHARprincipalMAGPRO_W4Profile-fit W4 magnitudemagphot.mag;em.IR.15-30umVARCHARprincipalMAGPROERR_W4Profile-fit W4 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W4Reduced chi^2 of profile-fit W4 measurementstat.fit.chi2VARCHARprincipalFLUX_W4Raw W4 source flux measured in profile-fit photometrymJyphot.flux;em.IR.15-30umVARCHARprincipalFLUXERR_W4Uncertainty in the raw W4 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W4Standard aperture magnitude for W4magphot.mag;em.IR.15-30umVARCHARprincipalMAGSTDAPERR_W4Standard aperture magnitude error for W4magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W4Standard aperture magnitude flag for W4meta.codeVARCHARprincipalRADIUS_ISO_W4Isophotal radius in W4arcsecphys.angSizeVARCHARprincipalMAGISO_W4Isophotal W4 magnitudemagphot.mag;em.IR.15-30umVARCHARprincipalMAGISOERR_W4Isophotal W4 magnitude errormagstat.error;phot.magVARCHARprincipalMAGDER_W4Derived W4 magnitude (from MAGISO_W3 and W3-W4 colour)magphot.mag;em.IR.15-30umVARCHARprincipalMAGDERERR_W4Derived W4 magnitude errormagstat.error;phot.magVARCHARprincipalXSCPROXDistance between WISE source and nearest 2MASS XSC sourcearcsecpos.angDistanceVARCHARprincipalBA_ISOAxis ratio of the isophotal ellipse in W1phys.size.axisRatioVARCHARprincipalPA_ISOPosition angle (E of N) of the isophotal ellipse in W1degpos.posAngVARCHARprincipalRFUZZYMeasure of resolvedness of WISE source, see notesarcsecVARCHARprincipalNAActive deblend flagmeta.codeVARCHARprincipalNBNumber of deblended componentsmeta.numberVARCHARprincipalCC_FLAGSContamination and confusion flag, see notesmeta.codeVARCHARprincipalDeblendedFractionLAMBDAR deblended fraction, see notesarith.ratioVARCHARprincipalSApFlagStandard Aperture Deblend Flag, see notesmeta.codeVARCHARprincipalNnearSApNumber of intersecting Standard Apertures, see notesmeta.numberVARCHARprincipalGApFlagGAMA Aperture Deblend Flag, see notesmeta.codeVARCHARprincipalNnearGApNumber of intersecting GAMA objects, see notesmeta.numberVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.XXLClusterAssocv01This catalogue provides the result of matching GAMA objects to XXLclusters in the G02 survey region. Both the x-ray sources and theGAMA objects in this catalogue may appear multiple times. Thiscatalogue is one of the outputs of the GAMA/XXL Matching Group. Itwas produced by Tatyana Sadibekova and was not modified in any way.MATCHIDUnique ID of association between XXL cluster and GAMA objectmeta.id;meta.mainVARCHARindexedprincipalXIDXXL ID of matched clustermeta.idVARCHARprincipalXNAMEXXL name of matched clustermeta.idVARCHARprincipalSEPLinear separation between the XXL cluster and the GAMA objectMpcpos.distanceVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalSPECIDUnique ID of GAMA spectrummeta.idVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDec of spectrum (J2000)degpos.eq.decVARCHARprincipalN_SPECNumber of spectra available for a GAMA positionVARCHARprincipalZ_GAMARedshift from GAMAsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalSYSNOIndex for optical system (can be >1 if there is more than one counterpart)VARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.XXLPointSourceAssocv01This catalogue provides the result of matching XXL point sourceswith GAMA objects. It contains the properties of the associationbetween an XXL point source and a GAMA object in the G02 surveyregion. Both the x-ray sources and the GAMA objects in thiscatalogue may appear multiple times. This catalogue is one of theoutputs of the GAMA/XXL Matching Group. It was produced by AngelaBongiorno and was not modified in any way.MATCHIDUnique ID of association between XXL point source and GAMA objectmeta.id;meta.mainVARCHARindexedprincipalXIDXXL IDmeta.idVARCHARprincipalXNAMEName of XXL sourcemeta.idVARCHARprincipalDISTDistance between XXL source and GAMA objectarcsecpos.angDistanceVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalZ_FLAG_ASSOCQuality of the match: 3=secure, 2=unsecure, 0=unsure, -1=no association, see notesmeta.code.qualVARCHARprincipalSECURE_ASSOCFlag indicating matches with Z_FLAG_ASSOC=3VARCHARprincipalUNSECURE_ASSOCFlag indicating matches with Z_FLAG_ASSOC=2VARCHARprincipalUNSURE_ASSOCFlag indicating matches with Z_FLAG_ASSOC=0VARCHARprincipalNO_ASSOCFlag indicating matches with Z_FLAG_ASSOC=-1VARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.XXLPointSourceCatv01This catalogue provides XXL photometry of XMM detected point sourcesin the G02 survey region. Specifically, it contains the x-rayproperties of those XMM point source detections that have a matchamong GAMA spectra (i.e. those that appear in the tableXXLPointSourceAssoc). This catalogue is one of the outputs of theGAMA/XXL Matching Group. It was produced by Angela Bongiorno and wasnot modified in any way.XIDXXL identifiermeta.id;meta.mainVARCHARindexedprincipalXNAMEXXL namemeta.idVARCHARprincipalRARA of x-ray source (J2000)degpos.eq.raVARCHARprincipalDECDec of x-ray source (J2000)degpos.eq.decVARCHARprincipalCOUNTS_SOFTCounts in the 0.5-2.0 keV bandVARCHARprincipalCOUNTS_HARDCounts in the 2-10 keV bandVARCHARprincipalFLUX_SOFTAveraged flux in the 0.5-2.0 keV banderg/s/cm^2VARCHARprincipalFLUX_HARDAveraged flux in the 2-10 keV banderg/s/cm^2VARCHARprincipalgama_pdr4v2.XXLPointSourceProbsv01For several different reasons (see notes), 33 x-ray sources werematched manually to GAMA objects. These were visually inspected andthe results recorded in this table. Some of the objects in thiscatalogue also appear in XXLPointSourceAssoc. This catalogue is oneof the outputs of the GAMA/XXL Matching Group. It was produced byAngela Bongiorno and was not modified in any way.XIDXXL identifiermeta.id;meta.mainVARCHARindexedprincipalXNAMEXXL namemeta.idVARCHARprincipalRARA of x-ray source (J200)degpos.eq.raVARCHARprincipalDECDec of x-ray source (J2000)degpos.eq.decVARCHARprincipalCOUNTS_SOFTCounts in the 0.5-2.0 keV bandVARCHARprincipalCOUNTS_HARDCounts in the 2-10 keV bandVARCHARprincipalDISTDistance between XXL source and GAMA objectarcsecpos.angDistanceVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalCOMMENTComment from visual inspectionVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Eqkcorr_auto_z00v05This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on GAMA matched aperture magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Eqkcorr_auto_z01v05This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on GAMA matched aperture magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Eqkcorr_auto_z02v05This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on GAMA matched aperture magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Eqkcorr_model_z00v05This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on SDSS DR7 model magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Eqkcorr_model_z01v05This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on SDSS DR7 model magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.Eqkcorr_model_z02v05This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on SDSS DR7 model magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02kcorr_z00v01This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G02 survey region, basedon CFHTLS AUTO magnitudes, where available, and SDSS modelmagnitudes otherwise.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02kcorr_z01v01This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G02 survey region, basedon CFHTLS AUTO magnitudes, where available, and SDSS modelmagnitudes otherwise.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G02kcorr_z02v01This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G02 survey region, basedon CFHTLS AUTO magnitudes, where available, and SDSS modelmagnitudes otherwise.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23kcorr_z00v01This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G23 survey region, basedon KiDS i-band and VIKING AUTO magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23kcorr_z01v01This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G23 survey region, basedon KiDS i-band and VIKING AUTO magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.G23kcorr_z02v01This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G23 survey region, basedon KiDS i-band and VIKING AUTO magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_pdr4v2.gkvInputCatv02ProFound segments have been visually regrouped to fix instances of fragmentation. Source detection is conducted on an r+Z stack of the image. After visual fixing of segment fragmentation, profoundMultiBand is implemented to extract photometry in the FUV-W2 bands. All fluxes and flux errors have been corrected for the foreground Galactic extinction (as given by the EBV value). See Bellstedt et al. (2020, MNRAS, 496, 3235 - https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3235B/abstract) for detailFrameNameName of frame that the object comes frommeta.idVARCHARprincipalFrameIDID of the frame that the object comes frommeta.idVARCHARprincipaluberIDUnique identifier of the objectmeta.idVARCHARprincipalsegIDSegment ID as given by ProFound of the object (unique within the frame, but not within the larger catalogue).meta.idVARCHARprincipalx_maxx position of the maximum fluxpixposVARCHARprincipaly_maxy position of the maximum fluxpixposVARCHARprincipalcensepOffset between the object and the frame centrepixVARCHARprincipalRAcenRight Ascension of flux-weighted centre (ICRS J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of flux-weighted centre (ICRS J2000)degpos.eq.decVARCHARprincipalRAmaxRight Ascension of maximum flux (ICRS J2000)degpos.eq.raVARCHARprincipalDecmaxDeclination of maximum flux (ICRS J2000)degpos.eq.decVARCHARprincipalRAGAIARight Ascension of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.raVARCHARprincipalDecGAIADeclination of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.decVARCHARprincipalsky_meanMean flux of the sky over all segment pixelsJyVARCHARprincipalskyRMS_meanMean value of the sky RMS over all segment pixelsJyVARCHARprincipallog10seeingSeeing, calculated as the median R50 value for objects with R50<2, Zmag>16 and Zmag<17log(arcsec)VARCHARprincipalEBVGalactic extinction, based on Planck E(B-V) values.magVARCHARprincipalmagMagnitude in the r+Z detection bandmagphot.magVARCHARprincipalR50Approximate elliptical semi-major axis containing 50% of the fluxarcsecphys.size.radiusVARCHARprincipalR90Approximate elliptical semi-major axis containing 90% of the fluxarcsecphys.size.radiusVARCHARprincipalR100Approximate elliptical semi-major axis containing 100% of the fluxarcsecphys.size.radiusVARCHARprincipalN100Total number of pixels in this segmentphys.areaVARCHARprincipalaxratAxial ratioVARCHARprincipalangOrientation of the semi-major axisdegpos.posAngVARCHARprincipalgroupIDID of the group containing the segment (unique within the frame, but not within the larger catalogue)meta.idVARCHARprincipalNgroupNumber of segments contained within the groupmeta.numberVARCHARprincipaleyeclassVisual classification of objectmeta.code.classVARCHARprincipalmag_app_ZtAperture magnitude in Z-band (based on the 1.4 arcsec fibre aperture)magphot.mag;em.opt.Z;VARCHARprincipalflux_FUVtTotal flux (FUV band) - using global sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_FUVlLocal flux (FUV band) - using local sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_err_FUVtFlux err (FUV band)Jyphot.flux.density;em.UV.100-200nm;stat.err;VARCHARprincipalflux_NUVtTotal flux (NUV band) - using global sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_NUVlLocal flux (NUV band) - using local sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_err_NUVtFlux err (NUV band)Jyphot.flux.density;em.UV.200-300nm;stat.err;VARCHARprincipalflux_utTotal flux (u band) - using global sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_ulLocal flux (u band) - using local sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_err_utFlux err (u band)Jyphot.flux.density;em.opt.U;stat.err;VARCHARprincipalflux_gtTotal flux (g band) - using global sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_glLocal flux (g band) - using local sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_err_gtFlux err (g band)Jyphot.flux.density;em.opt.G;stat.err;VARCHARprincipalflux_rtTotal flux (r band) - using global sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_rlLocal flux (r band) - using local sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_err_rtFlux err (r band)Jyphot.flux.density;em.opt.R;stat.err;VARCHARprincipalflux_itTotal flux (i band) - using global sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_ilLocal flux (i band) - using local sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_err_itFlux err (i band)Jyphot.flux.density;em.opt.I;stat.err;VARCHARprincipalflux_ZtTotal flux (Z band) - using global sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_ZlLocal flux (Z band) - using local sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_err_ZtFlux err (Z band)Jyphot.flux.density;em.opt.Z;stat.err;VARCHARprincipalflux_YtTotal flux (Y band) - using global sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_YlLocal flux (Y band) - using local sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_err_YtFlux err (Y band)Jyphot.flux.density;em.IR.Y;stat.err;VARCHARprincipalflux_JtTotal flux (J band) - using global sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_JlLocal flux (J band) - using local sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_err_JtFlux err (J band)Jyphot.flux.density;em.IR.J;stat.err;VARCHARprincipalflux_HtTotal flux (H band) - using global sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_HlLocal flux (H band) - using local sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_err_HtFlux err (H band)Jyphot.flux.density;em.IR.H;stat.err;VARCHARprincipalflux_KtTotal flux (Ks band) - using global sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_KlLocal flux (Ks band) - using local sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_err_KtFlux err (Ks band)Jyphot.flux.density;em.IR.K;stat.err;VARCHARprincipalflux_W1tTotal flux (W1 band) - using global sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_W1lLocal flux (W1 band) - using local sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_err_W1tFlux err (W1 band)Jyphot.flux.density;em.IR.3-4um;stat.err;VARCHARprincipalflux_W2tTotal flux (W2 band) - using global sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_W2lLocal flux (W2 band) - using local sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_err_W2tFlux err (W2 band)Jyphot.flux.density;em.IR.4-8um;stat.err;VARCHARprincipalduplicateFlag indicating if object is duplicated due to tile overlapmeta.code.classVARCHARprincipalmaskFlag indicating if object is within GAMA regionmeta.code.classVARCHARprincipalstarmaskFlag indicating if object is within a star maskmeta.code.classVARCHARprincipalstarscolStellar colour flagmeta.code.classVARCHARprincipalstarssizeStellar size flagmeta.code.classVARCHARprincipalclassAutomatic classification of objectmeta.code.classVARCHARprincipaluberclassFinal classification of objectmeta.code.classVARCHARprincipalnoOPTFlag indicating optical data is not presentmeta.code.classVARCHARprincipalnoIRFlag indicating IR data is not presentmeta.code.classVARCHARprincipalCATAIDID of objectmeta.id.cross;meta.mainVARCHARprincipalgama_pdr4v2.gkvScienceCatv02ProFound segments have been visually regrouped to fix instances of fragmentation. Source detection is conducted on an r+Z stack of the image. After visual fixing of segment fragmentation, profoundMultiBand is implemented to extract photometry in the FUV-W2 bands. All fluxes and flux errors have been corrected for the foreground Galactic extinction (as given by the EBV value). See Bellstedt et al. (2020, MNRAS, 496, 3235 - https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3235B/abstract) for detailFrameNameName of frame that the object comes frommeta.idVARCHARprincipalFrameIDID of the frame that the object comes frommeta.idVARCHARprincipaluberIDUnique identifier of the objectmeta.idVARCHARprincipalsegIDSegment ID as given by ProFound of the object (unique within the frame, but not within the larger catalogue).meta.idVARCHARprincipalx_maxx position of the maximum fluxpixposVARCHARprincipaly_maxy position of the maximum fluxpixposVARCHARprincipalcensepOffset between the object and the frame centrepixVARCHARprincipalRAcenRight Ascension of flux-weighted centre (ICRS J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of flux-weighted centre (ICRS J2000)degpos.eq.decVARCHARprincipalRAmaxRight Ascension of maximum flux (ICRS J2000)degpos.eq.raVARCHARprincipalDecmaxDeclination of maximum flux (ICRS J2000)degpos.eq.decVARCHARprincipalRAGAIARight Ascension of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.raVARCHARprincipalDecGAIADeclination of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.decVARCHARprincipalsky_meanMean flux of the sky over all segment pixelsJyVARCHARprincipalskyRMS_meanMean value of the sky RMS over all segment pixelsJyVARCHARprincipallog10seeingSeeing, calculated as the median R50 value for objects with R50<2, Zmag>16 and Zmag<17log(arcsec)VARCHARprincipalEBVGalactic extinction, based on Planck E(B-V) values.magVARCHARprincipalmagMagnitude in the r+Z detection bandmagphot.magVARCHARprincipalR50Approximate elliptical semi-major axis containing 50% of the fluxarcsecphys.size.radiusVARCHARprincipalR90Approximate elliptical semi-major axis containing 90% of the fluxarcsecphys.size.radiusVARCHARprincipalR100Approximate elliptical semi-major axis containing 100% of the fluxarcsecphys.size.radiusVARCHARprincipalN100Total number of pixels in this segmentphys.areaVARCHARprincipalaxratAxial ratioVARCHARprincipalangOrientation of the semi-major axisdegpos.posAngVARCHARprincipalgroupIDID of the group containing the segment (unique within the frame, but not within the larger catalogue)meta.idVARCHARprincipalNgroupNumber of segments contained within the groupmeta.numberVARCHARprincipalmag_app_ZtAperture magnitude in Z-band (based on the 1.4 arcsec fibre aperture)magphot.mag;em.opt.Z;VARCHARprincipalflux_FUVtTotal flux (FUV band) - using global sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_FUVlLocal flux (FUV band) - using local sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_err_FUVtFlux err (FUV band)Jyphot.flux.density;em.UV.100-200nm;stat.err;VARCHARprincipalflux_NUVtTotal flux (NUV band) - using global sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_NUVlLocal flux (NUV band) - using local sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_err_NUVtFlux err (NUV band)Jyphot.flux.density;em.UV.200-300nm;stat.err;VARCHARprincipalflux_utTotal flux (u band) - using global sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_ulLocal flux (u band) - using local sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_err_utFlux err (u band)Jyphot.flux.density;em.opt.U;stat.err;VARCHARprincipalflux_gtTotal flux (g band) - using global sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_glLocal flux (g band) - using local sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_err_gtFlux err (g band)Jyphot.flux.density;em.opt.G;stat.err;VARCHARprincipalflux_rtTotal flux (r band) - using global sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_rlLocal flux (r band) - using local sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_err_rtFlux err (r band)Jyphot.flux.density;em.opt.R;stat.err;VARCHARprincipalflux_itTotal flux (i band) - using global sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_ilLocal flux (i band) - using local sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_err_itFlux err (i band)Jyphot.flux.density;em.opt.I;stat.err;VARCHARprincipalflux_ZtTotal flux (Z band) - using global sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_ZlLocal flux (Z band) - using local sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_err_ZtFlux err (Z band)Jyphot.flux.density;em.opt.Z;stat.err;VARCHARprincipalflux_YtTotal flux (Y band) - using global sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_YlLocal flux (Y band) - using local sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_err_YtFlux err (Y band)Jyphot.flux.density;em.IR.Y;stat.err;VARCHARprincipalflux_JtTotal flux (J band) - using global sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_JlLocal flux (J band) - using local sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_err_JtFlux err (J band)Jyphot.flux.density;em.IR.J;stat.err;VARCHARprincipalflux_HtTotal flux (H band) - using global sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_HlLocal flux (H band) - using local sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_err_HtFlux err (H band)Jyphot.flux.density;em.IR.H;stat.err;VARCHARprincipalflux_KtTotal flux (Ks band) - using global sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_KlLocal flux (Ks band) - using local sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_err_KtFlux err (Ks band)Jyphot.flux.density;em.IR.K;stat.err;VARCHARprincipalflux_W1tTotal flux (W1 band) - using global sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_W1lLocal flux (W1 band) - using local sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_err_W1tFlux err (W1 band)Jyphot.flux.density;em.IR.3-4um;stat.err;VARCHARprincipalflux_W2tTotal flux (W2 band) - using global sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_W2lLocal flux (W2 band) - using local sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_err_W2tFlux err (W2 band)Jyphot.flux.density;em.IR.4-8um;stat.err;VARCHARprincipalduplicateFlag indicating if object is duplicated due to tile overlapmeta.code.classVARCHARprincipalmaskFlag indicating if object is within GAMA regionmeta.code.classVARCHARprincipalstarmaskFlag indicating if object is within a star maskmeta.code.classVARCHARprincipalstarscolStellar colour flagmeta.code.classVARCHARprincipalstarssizeStellar size flagmeta.code.classVARCHARprincipalclassAutomatic classification of objectmeta.code.classVARCHARprincipaleyeclassVisual classification of objectmeta.code.classVARCHARprincipaluberclassFinal classification of objectmeta.code.classVARCHARprincipalnoOPTFlag indicating optical data is not presentmeta.code.classVARCHARprincipalnoIRFlag indicating IR data is not presentmeta.code.classVARCHARprincipalCATAIDID of objectmeta.id.cross;meta.mainVARCHARprincipalNQRedshift quality flagmeta.code.qual;src.redshiftVARCHARprincipalZSpectroscopic redshiftsrc.redshiftVARCHARprincipalSCScience class flag. Values from 0-5 indicate progresively harsher cuts.meta.code.classVARCHARprincipalgama_pdr4v2.gkvCATAIDMatchv01Ancillary data product to accompany the gkvInputCat. For each CATAID in the TilingCat, this catalogue identifies the corresponding object in thenew ProFound photometry catalogue. This is intended to be particularly useful to identifythe segment ID of objects whose CATAIDs were not matched to a new segment, as can be possible ifa single ProFound segment contains more than one CATAID object. See Bellstedt et al. (2020, MNRAS, 496, 3235 - https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3235B/abstraCATAIDID of objectmeta.idVARCHARprincipalRARight Ascension of object from TilingCatdegpos.eq.raVARCHARprincipalDECDeclination of object from TilingCatdegpos.eq.decVARCHARprincipalsegIDSegment ID as given by ProFound of the segment encompassing the object coordinates. If duplicates exist, the segment containing the most flux is chosen.meta.idVARCHARprincipaluberIDCorresponding unique identifier of the segment. If duplicates exist, the segment containing the most flux is chosen.meta.idVARCHARprincipaluberID_allUnique identifiers of all segments containing the object. For objects in the duplicated borders of tiles, multiple matches will exist.meta.idVARCHARprincipalframeTile containing the segmentmeta.idVARCHARprincipalframeDistDistance between object and the tile centrepixVARCHARprincipalrZmagproFound magnitude of the objects as measured in the detection band (r+Z stack).magphot.magVARCHARprincipalgama_pdr4v2.gkvSFMPhotozv01uberIDID of objectmeta.idVARCHARprincipalzexpPhotometric redshift, marginalised over the full pdfsrc.redshiftVARCHARprincipalzerrPhotometric redshift error, calculated as half 16-84th range of the redshift pdfsrc.redshiftVARCHARprincipalzmaxPhotometric redshift, highest likelihood valuesrc.redshiftVARCHARprincipalgama_pdr4v2.gkvFarIRv03This catalogue is an extension to the GAMAKidsViking catalogue, providing photometry in the W3-S500 bands, thatare in general unresolved. In this PSF-limited regime, the output of the GAMAKidsViking catalogue is used to determine the coordinates for objects expected to emit in the FIR, and at these locations the flux is modelled.FIR fluxes are derived using the ProFound function ProFoundFitMagPSF, which fits fluxes iteratively according to a ProFitmodel of individual objects based on the band PSuberIDUnique identifier of the objectmeta.idVARCHARprincipaluberclassFinal classification of objectmeta.code.classVARCHARprincipalmag_PSF_w3PSF-derived magnitude (W3 band) - missing values are indicated via -999magphot.mag;em.IR.8-15umVARCHARprincipalmag_PSF_err_w3PSF-derived magnitude error (W3 band) - missing values are indicated via -999magphot.mag;stat.err;em.IR.8-15umVARCHARprincipalflux_PSF_w3PSF-derived flux (W3 band) - missing values are indicated via -999Jyphot.flux.density;em.IR.8-15umVARCHARprincipalflux_PSF_err_w3PSF-derived flux error (W3 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.IR.8-15umVARCHARprincipalmag_PSF_w4PSF-derived magnitude (W4 band) - missing values are indicated via -999magphot.mag;em.IR.15-30umVARCHARprincipalmag_PSF_err_w4PSF-derived magnitude error (W4 band) - missing values are indicated via -999magphot.mag;stat.err;em.IR.15-30umVARCHARprincipalflux_PSF_w4PSF-derived flux (W4 band) - missing values are indicated via -999Jyphot.flux.density;em.IR.15-30umVARCHARprincipalflux_PSF_err_w4PSF-derived flux error (W4 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.IR.15-30umVARCHARprincipalmag_PSF_p100PSF-derived magnitude (P100 band) - missing values are indicated via -999magphot.mag;em.mm.1500-3000GHzVARCHARprincipalmag_PSF_err_p100PSF-derived magnitude error (P100 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.1500-3000GHzVARCHARprincipalflux_PSF_p100PSF-derived flux (P100 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.1500-3000GHzVARCHARprincipalflux_PSF_err_p100PSF-derived flux error (P100 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.mm.1500-3000GHzVARCHARprincipalmag_PSF_p160PSF-derived magnitude (P160 band) - missing values are indicated via -999magphot.mag;m.mm.1500-3000GHzVARCHARprincipalmag_PSF_err_p160PSF-derived magnitude error (P160 band) - missing values are indicated via -999magphot.mag;stat.err;m.mm.1500-3000GHzVARCHARprincipalflux_PSF_p160PSF-derived flux (P160 band) - missing values are indicated via -999Jyphot.flux.density;m.mm.1500-3000GHzVARCHARprincipalflux_PSF_err_p160PSF-derived flux error (P160 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;m.mm.1500-3000GHzVARCHARprincipalmag_PSF_s250PSF-derived magnitude (S250 band) - missing values are indicated via -999magphot.mag;em.mm.750-1500GHzVARCHARprincipalmag_PSF_err_s250PSF-derived magnitude error (S250 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.750-1500GHzVARCHARprincipalflux_PSF_s250PSF-derived flux (S250 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalflux_PSF_err_s250PSF-derived flux error (S250 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.mm.750-1500GHzVARCHARprincipalmag_PSF_s350PSF-derived magnitude (S350 band) - missing values are indicated via -999magphot.mag;em.mm.750-1500GHzVARCHARprincipalmag_PSF_err_s350PSF-derived magnitude error (S350 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.750-1500GHzVARCHARprincipalflux_PSF_s350PSF-derived flux (S350 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalflux_PSF_err_s350PSF-derived flux error (S350 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.mm.750-1500GHzVARCHARprincipalmag_PSF_s500PSF-derived magnitude (S500 band) - missing values are indicated via -999magphot.mag;em.mm.400-750GHzVARCHARprincipalmag_PSF_err_s500PSF-derived magnitude error (S500 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.400-750GHzVARCHARprincipalflux_PSF_s500PSF-derived flux (S500 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.400-750GHzVARCHARprincipalflux_PSF_err_s500em.mm.400-750GHz PSF-derived flux error (S500 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;VARCHARprincipalFrameNameName of frame that the object comes frommeta.idVARCHARprincipalFrameIDID of the frame that the object comes frommeta.idVARCHARprincipalx_maxx position of the maximum fluxpixposVARCHARprincipaly_maxy position of the maximum fluxpixposVARCHARprincipalRAcenRight Ascension of flux-weighted centre (ICRS J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of flux-weighted centre (ICRS J2000)degpos.eq.decVARCHARprincipalgama_pdr4v2.gkvProSpectAGNv01Sabine Bellstedt <sabine.bellstedt@uwa.edu.au>CATAIDID of objectmeta.idVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SED(recommended)Msolphys.massVARCHARprincipalStellarMass_50Median stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_1616th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_8484th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SED(recommended)Msol/yrphys.SFRVARCHARprincipalSFR_50Median SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_1616th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_8484th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SED (recommended) (logged)phys.abund.ZVARCHARprincipalZgas_50Median Zgas from MCMC chain (logged)phys.abund.ZVARCHARprincipalZgas_1616th percentile Zgas from MCMC chain (logged)phys.abund.ZVARCHARprincipalZgas_8484th percentile Zgas from MCMC chain (logged)phys.abund.ZVARCHARprincipalDustMass_bestfitDust mass as determined by the best-fitting SED (recommended)Msolphys.massVARCHARprincipalDustMass_50Median dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_1616th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_8484th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustLum_bestfitDust luminosity as determined by the best-fitting SED (recommended)Lsolphys.lumVARCHARprincipalDustLum_50Median dust luminosity from MCMC chainLsolphys.lumVARCHARprincipalDustLum_1616th percentile dust luminosity from MCMC chainLsolphys.lumVARCHARprincipalDustLum_8484th percentile dust luminosity from MCMC chainLsolphys.lumVARCHARprincipalAGNlum_bestfitAGN bolometric luminosity as determined by the best-fitting SED (recommended) (logged)log(ergs/s)phys.lumVARCHARprincipalAGNlum_50Median AGN bolometric luminosity from MCMC chain (logged)log(ergs/s)phys.lumVARCHARprincipalAGNlum_1616th percentile AGN bolometric luminosity from MCMC chain (logged)log(ergs/s)phys.lumVARCHARprincipalAGNlum_8484th percentile AGN bolometric luminosity from MCMC chain (logged)log(ergs/s)phys.lumVARCHARprincipalfAGNFraction of flux contributed by the AGN model between 5-20micronsVARCHARprincipalLPlog-posterior value of for best-fit valuesVARCHARprincipaluberIDKiDS ID of objectmeta.idVARCHARprincipalgama_pdr4v2.gkvProSpectNEDv01uberIDKiDS ID of objectmeta.idVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalStellarMass_50Median stellar mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalStellarMass_1616th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_8484th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SEDMsol/yrphys.SFRVARCHARprincipalSFR_50Median SFR from MCMC chain (recommended)Msol/yrphys.SFRVARCHARprincipalSFR_1616th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_8484th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SEDphys.abund.ZVARCHARprincipalZgas_50Median Zgas from MCMC chain (recommended)phys.abund.ZVARCHARprincipalZgas_1616th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalZgas_8484th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalDustMass_bestfitDust mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalDustMass_50Median dust mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalDustMass_1616th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_8484th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustLum_50Median dust luminosity from MCMC chain (recommended)Msolphys.lumVARCHARprincipalDustLum_1616th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipalDustLum_8484th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipalNED_prefnameName of NED objectVARCHARprincipalNED_raRight Ascension of NED objectdegpos.eq.raVARCHARprincipalNED_decDeclination of NED objectdegpos.eq.decVARCHARprincipalNED_pretypeClass of objects from NEDVARCHARprincipalNED_zRedshift of NED objectsrc.redshiftVARCHARprincipalNED_zuncRedshift uncertainty of NED objectstat.errorVARCHARprincipalNED_zflagRedshift flagmeta.code.classVARCHARprincipalNED_zrefcodeReference to publication for NED redshiftVARCHARprincipalNED_matchDistSepaation radius between KiDS object and NED object.arcsecstat.valueVARCHARprincipalgama_pdr4v2.gkvProSpectv02CATAIDID of objectmeta.idVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalStellarMass_50Median stellar mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalStellarMass_1616th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_8484th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SEDMsol/yrphys.SFRVARCHARprincipalSFR_50Median SFR from MCMC chain (recommended)Msol/yrphys.SFRVARCHARprincipalSFR_1616th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_8484th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SEDphys.abund.ZVARCHARprincipalZgas_50Median Zgas from MCMC chain (recommended)phys.abund.ZVARCHARprincipalZgas_1616th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalZgas_8484th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalDustMass_bestfitDust mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalDustMass_50Median dust mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalDustMass_1616th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_8484th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustLum_50Median dust luminosity from MCMC chain (recommended)Msolphys.lumVARCHARprincipalDustLum_1616th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipalDustLum_8484th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipaluberIDKiDS ID of objectmeta.idVARCHARprincipalgama_pdr4v2.gkvSFMPhotoZProSpectv02CATAIDID of objectmeta.idVARCHARprincipaluberIDID of objectmeta.idVARCHARprincipalzexpPhotometric redshift, marginalised over the full pdfsrc.redshiftVARCHARprincipalzerrPhotometric redshift error, calculated as half 16-84th range of the redshift pdfsrc.redshiftVARCHARprincipalzmaxPhotometric redshift, highest likelihood valuesrc.redshiftVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SEDMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SEDphys.abund.ZVARCHARprincipalgama_pdr4v2.gkvMorphologyv02uberIDClassifier from GAMAKidsVikingv01meta.idVARCHARprincipalFrameNameName of Frame containing ProFound outputsmeta.idVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRAcendouble RA of centre of flux (J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of centre of flux (J2000)degpos.eq.decVARCHARprincipalmag_rtVST r band magnitude derived from flux_rtmagphot.mag;em.opt.RVARCHARprincipalR50Radius enclosing half the light in the detection band (rZ dilated)arcsecphys.size.radiusVARCHARprincipalZZ from SpecObjv27 or photo-Z from LSBGPhotoZ if NQ <3src.redshiftVARCHARprincipalNQNormalised redshift quality if NQ > 2 or photo-z if NQ=0meta.code.qual;src.redshiftVARCHARprincipalHUBBLE_TYPEFinal Hubble Type from VisualMorphologyv03 if known else Xmeta.code.classVARCHARprincipalINITIAL_CLASSInitial automated estimatemeta.code.classVARCHARprincipalSTART_CLASSFirst pass classification using custodian methodmeta.code.classVARCHARprincipalSABINE_CLASSSabine's visual Hubble type classificationsmeta.code.classVARCHARprincipalSIMON_CLASSSimon's visual Hubble type classificationsmeta.code.classVARCHARprincipalLUKE_CLASSLuke's visual Hubble type classificationsmeta.code.classVARCHARprincipalFINAL_CLASSFinal Classification (with tie = SIMON_CLASS)meta.code.classVARCHARprincipalMORPH_STAMPPointer to the postage stamp imagemeta.fileVARCHARprincipalgama_pdr4v2.EAZYPhotozv02_GAMAv02_SpecObjv24uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_pdr4v2.EAZYPhotozv02_GAMAv02_G12uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_pdr4v2.EAZYPhotozv02_GAMAv02_G09uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_pdr4v2.EAZYPhotozv02_GAMAv02_G23uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_pdr4v2.EAZYPhotozv02_GAMAv02_G15uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_pdr4v2.SourceCataloguev01This table is the source catalogue of the survey. It contains 338,772 objects and it was produced by the Data Central team.uberIDUnique GAMA III ID of objectmeta.id;meta.mainVARCHARindexedprincipalRAcenRight Ascension of flux-weighted centre (ICRS)degpos.eq.raVARCHARindexedprincipalDeccenDeclination of flux-weighted centre (ICRS)degpos.eq.decVARCHARindexedprincipalgama_dr4<p>GAMA is a project to exploit the latest generation of ground-based and space-borne survey facilities to study cosmology and galaxy formation and evolution. </p> <p>At the heart of this project lies the GAMA spectroscopic survey of ~300,000 galaxies down to r&nbsp;&lt;&nbsp;19.8&nbsp;mag over ~286&nbsp;deg<sup>2</sup>, carried out using the <a href="http://www.aao.gov.au/AAO/2df/aaomega/aaomega.html">AAOmega</a> multi-object spectrograph on the <a href="http://www.aao.gov.au/">Anglo-Australian Telescope (AAT)</a> by the GAMA team</a>. This project was awarded 210 nights over 7 years (2008–2014) and the observations are now completed. This survey builds on, and is augmented by, previous spectroscopic surveys such as the <a href="http://www.sdss.org/">Sloan Digital Sky Survey (SDSS)</a>, the <a href="http://www.mso.anu.edu.au/2dFGRS/">2dF Galaxy Redshift Survey(2dFGRS)</a> and the <a href="http://www.eso.org/~jliske/mgc/">Millennium Galaxy Catalogue (MGC)</a>.</p>gama_dr4.ApMatchedCatv06This table contains r-band defined aperture matched photometry andother Source Extractor outputs for all objects in the GAMA IIequatorial survey regions.CATAIDUnique GAMA IDmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinate from TilingCatdegpos.eq.raVARCHARprincipalDECJ2000 coordinate from TilingCatdegpos.eq.decVARCHARprincipalXx coordinate of aperture centre in r band cutoutpixelposVARCHARprincipalYy coordinate of aperture centre in r band cutoutpixelposVARCHARprincipalALPHA_J2000J2000 RA from SExtractor (r band)degpos.eq.ra;em.opt.RVARCHARprincipalDELTA_J2000J2000 Dec from SExtractor (r band)degpos.eq.dec;em.opt.RVARCHARprincipalA_IMAGEProfile RMS along major axis (r band)pixelphys.angSize;em.opt.RVARCHARprincipalB_IMAGEProfile RMS along minor axis (r band)pixelphys.angSize;em.opt.RVARCHARprincipalERRA_IMAGEMajor axis profile RMS error (r band)pixelstat.error;phys.angSize;em.opt.RVARCHARprincipalERRB_IMAGEMinor axis profile RMS error (r band)pixelstat.error;phys.angSize;em.opt.RVARCHARprincipalKRON_RADIUSKron radius (r band)pixelphys.size.radius;em.opt.RVARCHARprincipalPETRO_RADIUSPetrosian radius (r band)pixelphys.size.radius;em.opt.RVARCHARprincipalTHETA_IMAGEPosition angle on image (counterclockwise, r band)degpos.posAng;em.opt.RVARCHARprincipalTHETA_J2000Position angle on sky (east of north, r band)degpos.posAng;em.opt.RVARCHARprincipalERRTHETA_J2000J2000 position angle error (r band)degstat.error;pos.posAng;em.opt.RVARCHARprincipalTHRESHOLDDetection threshold above background (r band)countsinstr.sensitivity;phot.count;em.opt.RVARCHARprincipalMU_THRESHOLDDetection threshold above background (r band)mag/arcsec^2instr.sensitivity;phot.mag.sb;em.opt.RVARCHARprincipalISOAREAF_IMAGEIsophotal area (filtered) (r band)pixelphys.angArea;em.opt.RVARCHARprincipalFLUX_AUTO_uKron flux (u band)countsphot.flux;em.opt.UVARCHARprincipalFLUXERR_AUTO_uKron flux error (u band)countsstat.error;phot.flux;em.opt.UVARCHARprincipalMAG_AUTO_uKron magnitude (u band)magphot.mag;em.opt.UVARCHARprincipalMAGERR_AUTO_uKron magnitude error (u band)magstat.error;phot.mag;em.opt.UVARCHARprincipalFLUX_PETRO_uPetrosian flux (u band)countsphot.flux;em.opt.UVARCHARprincipalFLUXERR_PETRO_uPetrosian flux error (u band)countsstat.error;phot.flux;em.opt.UVARCHARprincipalMAG_PETRO_uPetrosian magnitude (u band)magphot.mag;em.opt.UVARCHARprincipalMAGERR_PETRO_uPetrosian magnitude error (u band)magstat.error;phot.mag;em.opt.UVARCHARprincipalBACKGROUND_uBackground at centroid (u band)countsinstr.background;phot.count;em.opt.UVARCHARprincipalFLUX_MAX_uPeak flux (u band)countsphot.flux;stat.max;em.opt.UVARCHARprincipalISOAREA_IMAGE_uIsophotal area (u band)pixelphys.angArea;em.opt.UVARCHARprincipalMU_MAX_uPeak surface brightness (u band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.UVARCHARprincipalFWHM_IMAGE_uFWHM assuming a Gaussian core (u band)pixelspect.line.width;obs.image;em.opt.UVARCHARprincipalFLAGS_uSource Extractor flags (u band)meta.code.qual;em.opt.UVARCHARprincipalFLUX_AUTO_gKron flux (g band)countsphot.flux;em.opt.GVARCHARprincipalFLUXERR_AUTO_gKron flux error (g band)countsstat.error;phot.flux;em.opt.GVARCHARprincipalMAG_AUTO_gKron magnitude (g band)magphot.mag;em.opt.GVARCHARprincipalMAGERR_AUTO_gKron magnitude error (g band)magstat.error;phot.mag;em.opt.GVARCHARprincipalFLUX_PETRO_gPetrosian flux (g band)countsphot.flux;em.opt.GVARCHARprincipalFLUXERR_PETRO_gPetrosian flux error (g band)countsstat.error;phot.flux;em.opt.GVARCHARprincipalMAG_PETRO_gPetrosian magnitude (g band)magphot.mag;em.opt.GVARCHARprincipalMAGERR_PETRO_gPetrosian magnitude error (g band)magstat.error;phot.mag;em.opt.GVARCHARprincipalBACKGROUND_gBackground at centroid (g band)countsinstr.background;phot.count;em.opt.GVARCHARprincipalFLUX_MAX_gPeak flux (g band)countsphot.flux;stat.max;em.opt.GVARCHARprincipalISOAREA_IMAGE_gIsophotal area (g band)pixelphys.angArea;em.opt.GVARCHARprincipalMU_MAX_gPeak surface brightness (g band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.GVARCHARprincipalFWHM_IMAGE_gFWHM assuming a Gaussian core (g band)pixelspect.line.width;obs.image;em.opt.GVARCHARprincipalFLAGS_gSource Extractor flags (g band)meta.code.qual;em.opt.GVARCHARprincipalFLUX_AUTO_rKron flux (r band)countsphot.flux;em.opt.RVARCHARprincipalFLUXERR_AUTO_rKron flux error (r band)countsstat.error;phot.flux;em.opt.RVARCHARprincipalMAG_AUTO_rKron magnitude (r band)magphot.mag;em.opt.RVARCHARprincipalMAGERR_AUTO_rKron magnitude error (r band)magstat.error;phot.mag;em.opt.RVARCHARprincipalFLUX_PETRO_rPetrosian flux (r band)countsphot.flux;em.opt.RVARCHARprincipalFLUXERR_PETRO_rPetrosian flux error (r band)countsstat.error;phot.flux;em.opt.RVARCHARprincipalMAG_PETRO_rPetrosian magnitude (r band)magphot.mag;em.opt.RVARCHARprincipalMAGERR_PETRO_rPetrosian magnitude error (r band)magstat.error;phot.mag;em.opt.RVARCHARprincipalBACKGROUND_rBackground at centroid (r band)countsinstr.background;phot.count;em.opt.RVARCHARprincipalFLUX_MAX_rPeak flux (r band)countsphot.flux;stat.max;em.opt.RVARCHARprincipalISOAREA_IMAGE_rIsophotal area (r band)pixelphys.angArea;em.opt.RVARCHARprincipalMU_MAX_rPeak surface brightness (r band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.RVARCHARprincipalFWHM_IMAGE_rFWHM assuming a Gaussian core (r band)pixelspect.line.width;obs.image;em.opt.RVARCHARprincipalFLAGS_rSource Extractor flags (r band)meta.code.qual;em.opt.RVARCHARprincipalFLUX_AUTO_iKron flux (i band)countsphot.flux;em.opt.IVARCHARprincipalFLUXERR_AUTO_iKron flux error (i band)countsstat.error;phot.flux;em.opt.IVARCHARprincipalMAG_AUTO_iKron magntiude (i band)magphot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_iKron magnitude error (i band)magstat.error;phot.mag;em.opt.IVARCHARprincipalFLUX_PETRO_iPetrosian flux (i band)countsphot.flux;em.opt.IVARCHARprincipalFLUXERR_PETRO_iPetrosian flux error (i band)countsstat.error;phot.flux;em.opt.IVARCHARprincipalMAG_PETRO_iPetrosian magnitude (i band)magphot.mag;em.opt.IVARCHARprincipalMAGERR_PETRO_iPetrosian magnitude error (i band)magstat.error;phot.mag;em.opt.IVARCHARprincipalBACKGROUND_iBackground at centroid (i band)countsinstr.background;phot.count;em.opt.IVARCHARprincipalFLUX_MAX_iPeak flux (i band)countsphot.flux;stat.max;em.opt.IVARCHARprincipalISOAREA_IMAGE_iIsophotal area (i band)pixelphys.angArea;em.opt.IVARCHARprincipalMU_MAX_iPeak surface brightness (i band)mag/arcsec^2phot.mag.sb;stat.max;em.opt.IVARCHARprincipalFWHM_IMAGE_iFWHM assuming a Gaussian core (i band)pixelspect.line.width;obs.image;em.opt.IVARCHARprincipalFLAGS_iSource Extractor flags (i band)meta.code.qual;em.opt.IVARCHARprincipalFLUX_AUTO_zKron flux (SDSS z band)countsphot.flux;em.opt.ZVARCHARprincipalFLUXERR_AUTO_zKron flux error (SDSS z band)countsstat.error;phot.flux;em.opt.ZVARCHARprincipalMAG_AUTO_zKron magnitude (SDSS z band)magphot.mag.em.opt.ZVARCHARprincipalMAGERR_AUTO_zKron magnitude error (SDSS z band)magstat.error;phot.mag;em.opt.ZVARCHARprincipalFLUX_PETRO_zPetrosian flux (SDSS z band)countsphot.flux;em.opt.ZVARCHARprincipalFLUXERR_PETRO_zPetrosian flux error (SDSS z band)countsstat.error;phot.flux;em.opt.ZVARCHARprincipalMAG_PETRO_zPetrosian magnitude (SDSS z band)magphot.mag;em.opt.ZVARCHARprincipalMAGERR_PETRO_zPetrosian magnitude error (SDSS z band)magstat.error;phot.mag;em.opt.ZVARCHARprincipalBACKGROUND_zBackground at centroid (SDSS z band)countsinstr.background;phot.count;em.opt.ZVARCHARprincipalFLUX_MAX_zPeak flux (SDSS z band)countsphot.flux;stat.max;em.opt.ZVARCHARprincipalISOAREA_IMAGE_zIsophotal area (SDSS z band)pixelphys.angArea;em.opt.ZVARCHARprincipalMU_MAX_zPeak surface brightness (SDSS z band)mag/arcsec^2phot.mag.sb;statm.ax;em.opt.ZVARCHARprincipalFWHM_IMAGE_zFWHM assuming a Gaussian core (SDSS z band)pixelspect.line.width;obs.image;em.opt.ZVARCHARprincipalFLAGS_zSource Extractor flags (SDSS z band)meta.code.qual;em.opt.ZVARCHARprincipalFLUX_AUTO_XKron flux (VIKING Z band)countsphot.flux;em.IR.ZVARCHARprincipalFLUXERR_AUTO_XKron flux error (VIKING Z band)countsstat.error;phot.flux;em.IR.ZVARCHARprincipalMAG_AUTO_XKron magnitude (VIKING Z band)magphot.mag;em.IR.ZVARCHARprincipalMAGERR_AUTO_XKron magnitude error (VIKING Z band)magstat.error;phot.mag;em.IR.ZVARCHARprincipalFLUX_PETRO_XPetrosian flux (VIKING Z band)countsphot.flux;em.IR.ZVARCHARprincipalFLUXERR_PETRO_XPetrosian flux error (VIKING Z band)countsstat.error;phot.flux;em.IR.ZVARCHARprincipalMAG_PETRO_XPetrosian magnitude (VIKING Z band)magphot.mag;em.IR.ZVARCHARprincipalMAGERR_PETRO_XPetrosian magnitude error (VIKING Z band)magstat.error;phot.mag;em.IR.ZVARCHARprincipalBACKGROUND_XBackground at centroid (VIKING Z band)countsinstr.background;phot.count;em.IR.ZVARCHARprincipalFLUX_MAX_XPeak flux (VIKING Z band)countsphot.flux;stat.max;em.IR.ZVARCHARprincipalISOAREA_IMAGE_XIsophotal area (VIKING Z band)pixelphys.angArea;em.IR.ZVARCHARprincipalMU_MAX_XPeak surface brightness (VIKING Z band)mag/arcsec^2phot.mag.sb;statm.ax;em.IR.ZVARCHARprincipalFWHM_IMAGE_XFWHM assuming a Gaussian core (VIKING Z band)pixelspect.line.width;obs.image;em.IR.ZVARCHARprincipalFLAGS_XSource Extractor flags (VIKING Z band)meta.code.qual;em.IR.ZVARCHARprincipalFLUX_AUTO_YKron flux (Y band)countsphot.flux;em.IR.YVARCHARprincipalFLUXERR_AUTO_YKron flux error (Y band)countsstat.error;phot.flux;em.IR.YVARCHARprincipalMAG_AUTO_YKron magnitude (Y band)magphot.mag;em.IR.YVARCHARprincipalMAGERR_AUTO_YKron magnitude error (Y band)magstat.error;phot.mag;em.IR.YVARCHARprincipalFLUX_PETRO_YPetrosian flux (Y band)countsphot.flux;em.IR.YVARCHARprincipalFLUXERR_PETRO_YPetrosian flux error (Y band)countsstat.error;phot.flux;em.IR.YVARCHARprincipalMAG_PETRO_YPetrosian magnitude (Y band)magphot.mag;em.IR.YVARCHARprincipalMAGERR_PETRO_YPetrosian magnitude error (Y band)magstat.error;phot.mag;em.IR.YVARCHARprincipalBACKGROUND_YBackground at centroid (Y band)countsinstr.background;phot.count;em.IR.YVARCHARprincipalFLUX_MAX_YPeak flux (Y band)countsphot.flux;stat.max;em.IR.YVARCHARprincipalISOAREA_IMAGE_YIsophotal area (Y band)pixelphys.angArea;em.IR.YVARCHARprincipalMU_MAX_YPeak surface brightness (Y band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.YVARCHARprincipalFWHM_IMAGE_YFWHM assuming a Gaussian core (Y band)pixelspect.line.width;obs.image;em.IR.YVARCHARprincipalFLAGS_YSource Extractor flags (Y band)meta.code.qual;em.IR.YVARCHARprincipalFLUX_AUTO_JKron flux (J band)countsphot.flux;em.IR.JVARCHARprincipalFLUXERR_AUTO_JKron flux error (J band)countsstat.error;phot.flux;em.IR.JVARCHARprincipalMAG_AUTO_JKron magnitude (J band)magphot.mag;em.IR.JVARCHARprincipalMAGERR_AUTO_JKron magnitude error (J band)magstat.error;phot.mag;em.IR.JVARCHARprincipalFLUX_PETRO_JPetrosian flux (J band)countsphot.flux;em.IR.JVARCHARprincipalFLUXERR_PETRO_JPetrosian flux error (J band)countsstat.error;phot.flux;em.IR.JVARCHARprincipalMAG_PETRO_JPetrosian magnitude (J band)magphot.mag;em.IR.JVARCHARprincipalMAGERR_PETRO_JPetrosian magnitude error (J band)magstat.error;phot.mag;em.IR.JVARCHARprincipalBACKGROUND_JBackground at centroid (J band)countsinstr.background;phot.count;em.IR.JVARCHARprincipalFLUX_MAX_JPeak flux (J band)countsphot.flux;stat.max;em.IR.JVARCHARprincipalISOAREA_IMAGE_JIsophotal area (J band)pixelphys.angArea;em.IR.JVARCHARprincipalMU_MAX_JPeak surface brightness (J band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.JVARCHARprincipalFWHM_IMAGE_JFWHM assuming a Gaussian core (J band)pixelspect.line.width;obs.image;em.IR.JVARCHARprincipalFLAGS_JSource Extractor flags (J band)meta.code.qual;em.IR.JVARCHARprincipalFLUX_AUTO_HKron flux (H band)countsphot.flux;em.IR.HVARCHARprincipalFLUXERR_AUTO_HKron flux error (H band)countsstat.error;phot.flux;em.IR.HVARCHARprincipalMAG_AUTO_HKron magnitude (H band)magphot.mag;em.IR.HVARCHARprincipalMAGERR_AUTO_HKron magnitude error (H band)magstat.error;phot.mag;em.IR.HVARCHARprincipalFLUX_PETRO_HPetrosian flux (H band)countsphot.flux;em.IR.HVARCHARprincipalFLUXERR_PETRO_HPetrosian flux error (H band)countsstat.error;phot.flux;em.IR.HVARCHARprincipalMAG_PETRO_HPetrosian magnitude (H band)magphot.mag;em.IR.HVARCHARprincipalMAGERR_PETRO_HPetrosian magnitude error (H band)magstat.error;phot.mag;em.IR.HVARCHARprincipalBACKGROUND_HBackground at centroid (H band)countsinstr.background;phot.count;em.IR.HVARCHARprincipalFLUX_MAX_HPeak flux (H band)countsphot.flux;stat.max;em.IR.HVARCHARprincipalISOAREA_IMAGE_HIsophotal area (H band)pixelphys.angArea;em.IR.HVARCHARprincipalMU_MAX_HPeak surface brightness (H band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.HVARCHARprincipalFWHM_IMAGE_HFWHM assuming a Gaussian core (H band)pixelspect.line.width;obs.image;em.IR.HVARCHARprincipalFLAGS_HSource Extractor flags (H band)meta.code.qual;em.IR.HVARCHARprincipalFLUX_AUTO_KKron flux (K band)countsphot.flux;em.IR.KVARCHARprincipalFLUXERR_AUTO_KKron flux error (K band)countsstat.error;phot.flux;em.IR.KVARCHARprincipalMAG_AUTO_KKron magnitude (K band)magphot.mag;em.IR.KVARCHARprincipalMAGERR_AUTO_KKron magnitude error (K band)magstat.error;phot.mag;em.IR.KVARCHARprincipalFLUX_PETRO_KPetrosian flux (K band)countsphot.flux;em.IR.KVARCHARprincipalFLUXERR_PETRO_KPetrosian flux error (K band)countsstat.error;phot.flux;em.IR.KVARCHARprincipalMAG_PETRO_KPetrosian magnitude (K band)magphot.mag;em.IR.KVARCHARprincipalMAGERR_PETRO_KPetrosian magnitude error (K band)magstat.error;phot.mag;em.IR.KVARCHARprincipalBACKGROUND_KBackground at centroid (K band)countsinstr.background;phot.count;em.IR.KVARCHARprincipalFLUX_MAX_KPeak flux (K band)countsphot.flux;stat.max;em.IR.KVARCHARprincipalISOAREA_IMAGE_KIsophotal area (K band)pixelphys.angArea;em.IR.KVARCHARprincipalMU_MAX_KPeak surface brightness (K band)mag/arcsec^2phot.mag.sb;stat.max;em.IR.KVARCHARprincipalFWHM_IMAGE_KFWHM assuming a Gaussian core (K band)pixelspect.line.width;obs.image;em.IR.KVARCHARprincipalFLAGS_KSource Extractor flags (K band)mag.code.qual;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.EnvironmentMeasuresv06This catalogue provides three different environment measures for allGAMA II galaxies with 0.002 < z < 0.18: a surface density, thenumber of galaxies within a cylinder, and the adaptive Gaussianenvironment parameter.CATAIDUnique GAMA IDmeta.idVARCHARprincipalRAJ2000degpos.eq.raVARCHARprincipalDECJ2000degpos.eq.decVARCHARprincipalZ_TONRYHeliocentric redshift corrected for the effects of peculiar velocitysrc.redshiftVARCHARprincipalnQRedshift quality flagmeta.code.qual;src.redshiftVARCHARprincipalMExtinction and k-corrected absolute r-band (G02-G15) or i-band (G23) magnitude, see notesmagphys.magAbsVARCHARprincipalDistanceToEdgeDistance to nearest angular survey edge in co-moving unitsMpcpos.distanceVARCHARprincipalCompletenessValue used to correct environment measures for local survey incompleteness, see notesarith.factorVARCHARprincipalDistanceTo5nnDistance to 5th nearest neighbour in co-moving unitsMpcpos.distanceVARCHARprincipalSurfaceDensitySurface density based on the distance to the 5th nearest neighbourMpc^-2src.densityVARCHARprincipalSurfaceDensityErrSurface density uncertaintyMpc^-2stat.error;src.densityVARCHARprincipalSurfaceDensityFlagFlag indicating problems with surface density measurement, see notesmeta.code.error;src.densityVARCHARprincipalCountInCylNumber of (other) galaxies within cylinder of radius 1 co-moving Mpcmeta.numberVARCHARprincipalCountInCylErrPoisson error on number of galaxies in cylinderstat.error;meta.numberVARCHARprincipalCountInCylFlagFlag indicating problems with CountInCyl, see notesmeta.code.error;meta.numberVARCHARprincipalAGEDenParAdaptive Gaussian environment parameterMpc^-1src.densityVARCHARprincipalAGEErrPoisson error on the number of galaxies used to calculate AGEDenParstat.error;meta.numberVARCHARprincipalAGEScaleAdaptive scaling factor used for the adaptive Gaussian ellipsoidarith.factorVARCHARprincipalAGEDenParFlagFlag indicating problems with AGEDenPar, see notesmeta.code.error;src.densityVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.TilingExtrav02Science targets in the GAMA II equatorial survey regions not foundin InputCatAv06. These are mainly FIRST-SDSS targets, but also sometargets just North of -1 deg in G09 where a different reduction wasused between GAMA I and GAMA II.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFLAGSSee SDSS photoobj tablemeta.code.qual;photVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalFIBERMAG_RSDSS DR7 r band fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalPETROMAG_RSDSS DR7 r band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalMODELMAG_RSDSS DR7 r band model magnitudemagphot.mag;em.opt.RVARCHARprincipalEXTINCTION_RGalactic extinction in r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalPSFMAG_ISDSS DR7 iband PSF magnitude, not entered for somemagphot.mag;em.opt.IVARCHARprincipalMODELMAG_ISDSS magnitudemagphot.mag;em.opt.IVARCHARprincipalEXTINCTION_IGalactic extinction in i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalSECTARGETSecondary target flag from SDSSmeta.code.classVARCHARprincipalPSFMAG_GSDSS DR7 g band PSF magnitude, not entered for somemagphot.mag;em.optVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.TilingCatv46Science targets in the GAMA II equatorial survey regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR7 r band fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 r band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalU_MODELExtinction-corrected SDSS DR7 u band model magnitudemagphot.mag;em.opt.UVARCHARprincipalG_MODELExtinction-corrected SDSS DR7 g band model magnitudemagphot.mag;em.opt.BVARCHARprincipalR_MODELExtinction-corrected SDSS DR7 r band model magnitudemagphot.mag;em.opt.RVARCHARprincipalI_MODELExtinction-corrected SDSS DR7 i band model magnitudemagphot.mag;em.opt.IVARCHARprincipalZ_MODELExtinction-corrected SDSS DR7 z band model magnitudemagphot.mag;em.opt.IVARCHARprincipalSURVEY_CODESurvey code for redshift source, see notesmeta.code;meta.datasetVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalNQ2_FLAGTests of NQ=2 redshifts, see notesmeta.code.qual;src.redshiftVARCHARprincipalSPECIDID of spectrum from SpecAll tablemeta.id.cross;spectVARCHARprincipalVEL_ERRRedshift uncertainty, c delta ln(1+z), see noteskm/ssrc.redshift;stat.errorVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra within 1 arcsecmeta.number;spectVARCHARprincipalR_SBSDSS Petro half-light surface brightnessmag/arcsec^2phot.mag.sb;em.opt.RVARCHARprincipalSG_SEPr_psf - r_model star-galaxy separation parametermagsrc.class.starGalaxyVARCHARprincipalSG_SEP_JKJ - K - f_locus star-galaxy separation parametermagsrc.class.starGalaxyVARCHARprincipalK_AUTOExtinction-corrected r-defined auto AB magmagphot.mag;em.IR.KVARCHARprincipalRADIO_FLUXFlux from FIRST-SDSS matchingmJyphot.flux.density;em.radioVARCHARprincipalHATLAS_FLAG1 for match to H-ATLAS SDSS possible IDmeta.codeVARCHARprincipalAREA_FLAG1-deg strip, 2 for GAMA I regionsmeta.codeVARCHARprincipalTARGET_FLAGSBitwise target criteria, see notesmeta.codeVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalPRIORITY_CLASSPriorities for targeting, see notesmeta.code.classVARCHARprincipalNEIGHBOUR_CLASSNumber of survey_class>=3 targets within 40 arcsecmeta.code.classVARCHARprincipalTC_V11_IDCATAID of object in TilingCatv11, see notesmeta.code.crossVARCHARprincipalMASK_IC_10Mask value 0.0 to 1.0 around V<10 starsmeta.codeVARCHARprincipalMASK_IC_12Mask value 0.0 to 1.0 around V<12 starsmeta.codeVARCHARprincipalVIS_CLASSVisual classification, see notesmata.code.qualVARCHARprincipalVIS_CLASS_USERInitials of classifiers, xxx for nonemeta.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.SpStandardsv09Standard stars from SDSS for the GAMA II equatorial survey regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR7 r band fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalPSFMAG_GSDSS DR7 g band PSF magnitudemagphot.mag;em.opt.BVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalPSFMAG_ISDSS DR7 i band PSF magnitudemagphot.mag;em.opt.IVARCHARprincipalSECTARGET2^1 for REDDEN_STD, 2^5 for SPECTROPHOTO_STDmeta.code.classVARCHARprincipalSTATUSSDSS status flag related to primary secondarymeta.code.statusVARCHARprincipalRUNSDSS run numberobs.paramVARCHARprincipalAREA_FLAG2 for GAMA I regions, 1 otherwisemeta.codeVARCHARprincipalPRIORITY_CLASSSee notesmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.InputCatAv07This is the GAMA II master input catalogue for the GAMA IIequatorial survey regions. It provides SDSS DR7 data for an enlargedarea of 14x6.5 deg^2 covering the GAMA II equatorial regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFLAGSSee SDSS photoobj tablemeta.code.qual;photVARCHARprincipalPRIMTARGETSee SDSS photoobj tablemeta.code.classVARCHARprincipalTYPESDSS photo type (3=galaxy, 6=star, 8=sky)src.classVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalFIBERMAG_RSDSS DR7 r band 3-arcsec fibre magnitudemagphot.mag;em.opt.RVARCHARprincipalFLAGS_RSee SDSS photoobj tablemeta.code.qual;phot;em.opt.RVARCHARprincipalEXTINCTION_RGalactic extinction in r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalPETRORAD_RPetrosian radius in r bandarcsecphys.angSize;em.opt.RVARCHARprincipalPETROR90_RRadius containing 90% of Petrosian fluxarcsecphys.angSize;em.opt.RVARCHARprincipalPETROR50_RRadius containing 50% of Petrosian fluxarcsecphys.angSize;em.opt.RVARCHARprincipalPETROMAG_GSDSS DR7 g band Petrosian magnitudemagphot.mag;em.optVARCHARprincipalPETROMAG_RSDSS DR7 r band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalPETROMAG_ISDSS DR7 i band Petrosian magnitudemagphot.mag;em.opt.IVARCHARprincipalMODELMAG_USDSS DR7 u band model magnitudemagphot.mag;em.opt.UVARCHARprincipalMODELMAG_GSDSS DR7 g band model magnitudemagphot.mag;em.optVARCHARprincipalMODELMAG_RSDSS DR7 r band model magnitudemagphot.mag;em.opt.RVARCHARprincipalMODELMAG_ISDSS DR7 i band model magnitudemagphot.mag;em.opt.IVARCHARprincipalMODELMAG_ZSDSS DR7 z band model magnitudemagphot.mag;em.optVARCHARprincipalSTATUSSee SDSS photoobj tablemeta.code.statusVARCHARprincipalRUNSDSS run numberobs.paramVARCHARprincipalMASK_IC_10Mask value 0.0 to 1.0 around V<10 stars, see notesmeta.codeVARCHARprincipalMASK_IC_12Mask value 0.0 to 1.0 around V<12 stars, see notesmeta.codeVARCHARprincipalMASK_SATURSaturation class from FLAGS and FLAGS_R, see notesmeta.codeVARCHARprincipalEXCEPTION_FLAGExceptions to mask criteria, targets to includemeta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GuideStarsv03Guide stars selected from SDSS DR7 for the GAMA II equatorial surveyregions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 positiondegpos.eq.raVARCHARprincipalDECJ2000 positiondegpos.eq.decVARCHARprincipalRAERRError in positiondegstat.error;pos.eq.raVARCHARprincipalDECERRError in positiondegstat.error;pos.eq.decVARCHARprincipalPSFMAG_GSDSS DR7 g band PSF magnitudemagphot.mag;em.optVARCHARprincipalPSFMAG_RSDSS DR7 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalPSFMAG_ISDSS DR7 i band PSF magnitudemagphot.mag;em.opt.IVARCHARprincipalPROPERMOTIONFrom USNO-B matchmas/yrpos.pmVARCHARprincipalAREA_FLAG2=GAMA I 4x12 areas, 1=extended GAMA II areasmeta.codeVARCHARprincipalVIS_CLASS0=unchecked, 1=okay, 2=not goodmeta.code.qualVARCHARprincipalVIS_CLASS_USERInitials of classifiermeta.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GamaIToGamaIIv01This table contains a match between all GAMA I and GAMA II objects,i.e. between all objects in InputCatAv05 and InputCatAv06. Itprovides flags to easily identify objects that are (only) in GAMA I,(only) in GAMA II, or in both. It also provides the CATAIDtranslation for those objects in both that have a different CATAIDin GAMA I and GAMA II.PairIDUnique GAMA I-II pair IDmeta.idVARCHARprincipalCATAID_IGAMA I ID (as in InputCatAv05)meta.idVARCHARprincipalOBJID_ISDSS DR6 objidmeta.idVARCHARprincipalRA_IJ2000 coordinate (DR6)degpos.eq.raVARCHARprincipalDEC_IJ2000 coordinate (DR6)degpos.eq.decVARCHARprincipalCATAID_IIGAMA II ID (as in InputCatAv06)meta.idVARCHARprincipalOBJID_IISDSS DR7 objidmeta.idVARCHARprincipalRA_IIJ2000 coordinate (DR7)degpos.eq.raVARCHARprincipalDEC_IIJ2000 coordinate (DR7)degpos.eq.decVARCHARprincipalInIFlag indicating that the object is in GAMA I (InputCatAv05)meta.codeVARCHARprincipalInIIFlag indicating that the object is in GAMA II (InputCatAv06)meta.codeVARCHARprincipalOnlyInIFlag indicating that the object is in GAMA I but not in GAMA IImeta.codeVARCHARprincipalOnlyInIIFlag indicating that the object is in GAMA II but not in GAMA Imeta.codeVARCHARprincipalInBothFlag indicating that the object is in both GAMA I and IImeta.codeVARCHARprincipalInBothDifferentIDFlag indicating that the object is in both GAMA I and II but with different CATAIDsmeta.codeVARCHARprincipalSeparationDistance between matched objects along a great circlearcsecpos.angDistanceVARCHARprincipalgama_dr4.GalaxyPartMatchesv12This table can be used to match a vis_class=3 object (deblended partof a galaxy) to a vis_class=0 or 1 object (chosen main part of agalaxy). Each galaxy should only have one main part but some haveseveral deblended parts.CATAID_VC3CATAID of vis_class=3 objectmeta.idVARCHARprincipalCATAID_MAINCATAID of main partmeta.idVARCHARprincipalgama_dr4.GalacticExtinctionv03This table provides the Galactic foreground extinction in all GALEX,SDSS (= KiDS), UKIDSS and VIKING bands for all objects in the GAMA IIequatorial survey regions, i.e. for every object in InputCatA,TilingExtra and SpStandards.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_B_MGCGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_uGalactic extinction in SDSS and KiDS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_gGalactic extinction in SDSS and KiDS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_rGalactic extinction in SDSS and KiDS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_iGalactic extinction in SDSS and KiDS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_zGalactic extinction in SDSS and KiDS z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_UKIDSSGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_UKIDSSGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_UKIDSSGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_UKIDSSGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_Z_VIKINGGalactic extinction in VIKING Z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_VIKINGGalactic extinction in VIKING Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_VIKINGGalactic extinction in VIKING J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_VIKINGGalactic extinction in VIKING H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_VIKINGGalactic extinction in VIKING K bandmagphys.absorption.gal;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.ExternalzAllv07This table lists a few redshifts in the GAMA II survey regions takenfrom the literature. The spectra from which these redshifts weremeasured are NOT available in the GAMA database.SPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.ExternalSpecAllv07This table lists all spectra that are available from previousspectroscopic surveys (such as the SDSS) in the GAMA II surveyregions, including duplicate observations. Every spectrum listed inthis table is available in the GAMA database.SPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in originating survey?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.VoidGalsv02Table of all galaxies in voids, i.e. of all galaxies not grouped infilaments or tendrils.CATAIDUnique ID of galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Tendrilsv02Table of galaxy tendrils.TendrilIDUnique iD of tendrilmeta.idVARCHARprincipalNgalNumber of galaxies in tendrilmeta.numberVARCHARprincipalLengthTotal length of all links in tendrilMpc/hphys.sizeVARCHARprincipalgama_dr4.TendrilLinksv02Table of links between galaxies in tendrils.LinkIDUnique ID of linkmeta.idVARCHARprincipalCATAID1CATAID of link startmeta.idVARCHARprincipalCATAID2CATAID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_dr4.TendrilGalsv02Table of all galaxies in tendrils.CATAIDUnique ID of galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinatesMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinatesMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinatesMpc/hpos.cartesian.zVARCHARprincipalTendrilIDID of tendril galaxy belongs tometa.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.MockVoidGalsv01Table of all mock galaxies in voids, i.e. of all mock galaxies notgrouped in filaments or tendrils.GalIDUnique ID of mock galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_dr4.MockTendrilsv01Table of mock galaxy tendrils.TendrilIDUnique ID of mock tendrilmeta.idVARCHARprincipalNgalNumber of galaxies in tendrilmeta.numberVARCHARprincipalLengthTotal length of all links in tendrilMpc/hphys.sizeVARCHARprincipalgama_dr4.MockTendrilLinksv01Table of links between mock galaxies in tendrils.LinkIDUnique ID of linkmeta.idVARCHARprincipalGalID1GalID of link startmeta.idVARCHARprincipalGalID2GalID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_dr4.MockTendrilGalsv01Table of all mock galaxies in tendrils.GalIDUnique ID of mock galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinatesMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinatesMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinatesMpc/hpos.cartesian.zVARCHARprincipalTendrilIDID of tendril galaxy belongs tometa.idVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_dr4.MockFilamentsv01Table of all filaments composed of groups of mock galaxies.FilIDUnique ID of mock filamentmeta.idVARCHARprincipalNbranchNumber of branches in filamentmeta.numberVARCHARprincipalNgroupNumber of groups in filamentmeta.numberVARCHARprincipalLengthTotal length of all links in filamentMpc/hphys.sizeVARCHARprincipalBBlengthTotal length of all links in the backboneMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the filament near survey edgemeta.numberVARCHARprincipalgama_dr4.MockFilLinksv01Table of links between mock groups.LinkIDUnique ID of linkmeta.idVARCHARprincipalGroupID1GroupID of link startmeta.idVARCHARprincipalGroupID2GroupID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_dr4.MockFilGroupsv01Table of all mock groups in filaments.GroupIDUnique ID of mock groupmeta.idVARCHARprincipalRAGroup centre RA (IterCenRA)degpos.eq.raVARCHARprincipalDecGroup centre Dec (IterCenDEC)degpos.eq.decVARCHARprincipalZfofGroup median redshiftsrc.redshiftVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipalBranchIDID of the branch the group is inmeta.idVARCHARprincipalBranchOrderOrder of branchmeta.codeVARCHARprincipalFilIDFilament the group is inmeta.idVARCHARprincipalCutIndicates if the group is near survey edgemeta.numberVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_dr4.MockFilGalsv01Table of all mock galaxies near filaments.GalIDUnique ID of mock galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipaldOrthogonal distance to nearest filamentMpc/hpos.distanceVARCHARprincipalGroupIDID of group galaxy belongs to (0 if ungrouped)meta.idVARCHARprincipalBranchIDID of branch galaxy is closest tometa.idVARCHARprincipalFilIDID of filamentmeta.idVARCHARprincipalVolumeGAMA mock volume numbermeta.idVARCHARprincipalgama_dr4.MockFilBranchesv01Table of all branches in mock filaments.BranchIDUnique ID of mock branchmeta.idVARCHARprincipalFilIDID of filament that the branch is inmeta.idVARCHARprincipalBranchOrderBranch ordermeta.codeVARCHARprincipalNgroupNumber of groups in the branchmeta.numberVARCHARprincipalLengthLength of all links in the branchMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the branch near survey edgemeta.numberVARCHARprincipalgama_dr4.Filamentsv02Table of all filaments composed of groups of galaxies.FilIDUnique ID of filamentmeta.idVARCHARprincipalNbranchNumber of branches in filamentmeta.numberVARCHARprincipalNgroupNumber of groups in filamentmeta.numberVARCHARprincipalLengthTotal length of all links in filamentMpc/hphys.sizeVARCHARprincipalBBlengthTotal length of all links in the backboneMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the filament near survey edgemeta.numberVARCHARprincipalgama_dr4.FilLinksv02Table of links between groups.LinkIDUnique ID of linkmeta.idVARCHARprincipalGroupID1GroupID of link startmeta.idVARCHARprincipalGroupID2GroupID of link endmeta.idVARCHARprincipalLengthLength of linkMpc/hpos.distanceVARCHARprincipalgama_dr4.FilGroupsv02Table of all groups in filaments.GroupIDUnique ID of groupmeta.idVARCHARprincipalRAGroup centre RA (IterCenRA)degpos.eq.raVARCHARprincipalDecGroup centre Dec (IterCenDEC)degpos.eq.decVARCHARprincipalZfofGroup median redshiftsrc.redshiftVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipalBranchIDID of the branch the group is inmeta.idVARCHARprincipalBranchOrderOrder of branchmeta.codeVARCHARprincipalFilIDFilament the group is inmeta.idVARCHARprincipalCutIndicates if the group is near survey edgemeta.numberVARCHARprincipalgama_dr4.FilGalsv02Table of all galaxies near filaments.CATAIDUnique ID of galaxymeta.idVARCHARprincipalX3D comoving cartesian coordinateMpc/hpos.cartesian.xVARCHARprincipalY3D comoving cartesian coordinateMpc/hpos.cartesian.yVARCHARprincipalZ3D comoving cartesian coordinateMpc/hpos.cartesian.zVARCHARprincipaldOrthogonal distance to nearest filamentMpc/hpos.distanceVARCHARprincipalGroupIDID of group galaxy belongs to (0 if ungrouped)meta.idVARCHARprincipalBranchIDID of branch galaxy is closest tometa.idVARCHARprincipalFilIDID of filamentmeta.idVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.FilBranchesv02Table of all branches in filaments.BranchIDUnique ID of branchmeta.idVARCHARprincipalFilIDID of filament that the branch is inmeta.idVARCHARprincipalBranchOrderBranch ordermeta.codeVARCHARprincipalNgroupNumber of groups in the branchmeta.numberVARCHARprincipalLengthLength of all links in the branchMpc/hphys.sizeVARCHARprincipalCutNumber of groups in the branch near survey edgemeta.numberVARCHARprincipalgama_dr4.G02TilingExtrav03This is a table of extra galaxy targets in the G02 survey region.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalCOBJIDG02CFHTLSInputCat IDmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalXXL_FLAG1 if X-ray AGN target selected by Antonis Georgakakismeta.codeVARCHARprincipalR_MAGExtinction-corrected r band SDSS Petrosian or CFHTLenS AUTO magnitude, 22.5 for unknownmagphot.mag;em.opt.RVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02TilingCatv07Science targets in the G02 survey region.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objid, -1 for no matchmeta.idVARCHARprincipalCOBJIDG02CFHTLSInputCat ID, xxx for no matchmeta.idVARCHARprincipalRAJ2000 coordinate, from G02CFHTLSInputCat if matchdegpos.eq.raVARCHARprincipalDECJ2000 coordinate, from G02CFHTLSInputCat if matchdegpos.eq.decVARCHARprincipalDIST_SDSSAngular distance between RA and DEC in this table and SDSS match, 9.99 for no matcharcsecpos.angDistanceVARCHARprincipalPRIORITY_CLASSPriorities for last targeting run, 9 high, 0 not a targetmeta.code.classVARCHARprincipalSURVEY_CLASS6=selected with SDSS and CFHTLenS; 5=selected with SDSS only; 4=selected with CFHTLenS only; 2=fillermeta.code.classVARCHARprincipalAREA_FLAG1 for DEC < -6, 2 for DEC > -6 = high-priority regionmeta.codeVARCHARprincipalFLAGS_SELECTSum of flags, 1 if mask=0, 2 if class_star<0.7 from CFHTLenS, 4 if passed SDSS star-galaxy separationmeta.code.memberVARCHARprincipalR_PETROExtinction-corrected r band SDSS Petrosian magnitude, 0 for no matchmagphot.mag;em.opt.RVARCHARprincipalR_AUTOExtinction-corrected r band CFHTLenS AUTO magnitude, 0 for no matchmagphot.mag;em.opt.RVARCHARprincipalR_MAGExtinction-corrected r bnd SDSS Petrosian or CFHTLenS AUTO magnitudemagphot.mag;em.opt.RVARCHARprincipalFIBERMAG_Rr band SDSS fibermag or CFHTLenS mag_aper12magphot.mag;em.opt.RVARCHARprincipalSURVEY_CODESurvey code for redshift source, see SpecCat notesmeta.code;meta.datasetVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalSPECIDID of spectrum from SpecCat tablemeta.id.cross;spectVARCHARprincipalVEL_ERRRedshift uncertainty, c delta ln(1+z)km/ssrc.redshift;stat.errorVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra within 1 arcsecmeta.numberVARCHARprincipalVIS_CLASSVisual classification, see notesmeta.code.qualVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02SpStandardsv01Standard stars from SDSS for the G02 survey regions.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR8 r band magnitude in 3 arcsec diameter fibermagphot.mag;em.opt.RVARCHARprincipalPSFMAG_RSDSS DR8 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipalPRIORITY_CLASSSpectroscopic prioritymeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02SDSSInputCatv01SDSS DR8 input catalogue and photometry for the G02 survey region.OBJIDUnique SDSS identifiermeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalflagsPhoto object attribute flagsmeta.code.qualVARCHARprincipalflags_rr band photo object attribute flagsmeta.code.qualVARCHARprincipaltypeMorphological type classificationmeta.code.classVARCHARprincipalrowcRow centre positionpixelpos.cartesian.yVARCHARprincipalcolcColumn centre positionpixelpos.cartesian.xVARCHARprincipalfiberMag_rr band magnitude in 3 arcsec diameter fiber radiusmagphot.magVARCHARprincipalpsfMag_uu band PSF magnitudemagphot.magVARCHARprincipalpsfMag_gg band PSF magnitudemagphot.magVARCHARprincipalpsfMag_rr band PSF magnitudemagphot.magVARCHARprincipalpsfMag_ii band PSF magnitudemagphot.magVARCHARprincipalpsfMag_zz band PSF magnitudemagphot.magVARCHARprincipalpsfMagErr_uu band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_gg band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_rr band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_ii band PSF magnitude errormagphot.magVARCHARprincipalpsfMagErr_zz band PSF magnitude errormagphot.magVARCHARprincipalpetroMag_uu band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_gg band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_rr band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_ii band Petrosian magnitudemagphot.magVARCHARprincipalpetroMag_zz band Petrosian magnitudemagphot.magVARCHARprincipalpetroMagErr_uu band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_gg band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_rr band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_ii band Petrosian magnitude errormagphot.magVARCHARprincipalpetroMagErr_zz band Petrosian magnitude errormagphot.magVARCHARprincipalmodelMag_uu band model magnitudemagphot.magVARCHARprincipalmodelMag_gg band model magnitude fitmagphot.magVARCHARprincipalmodelMag_rr band model magnitude fitmagphot.magVARCHARprincipalmodelMag_ii band model magnitude fitmagphot.magVARCHARprincipalmodelMag_zz band model magnitude fitmagphot.magVARCHARprincipalmodelMagErr_uu band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_gg band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_rr band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_ii band model magnitude fit errormagphot.magVARCHARprincipalmodelMagErr_zz band model magnitude fit errormagphot.magVARCHARprincipalextinction_uu band extinctionmagphys.absorption.gal;em.opt.UVARCHARprincipalextinction_gg band extinctionmagphys.absorption.gal;em.opt.BVARCHARprincipalextinction_rr band extinctionmagphys.absorption.gal;em.opt.VVARCHARprincipalextinction_ii band extinctionmagphys.absorption.gal;em.opt.RVARCHARprincipalextinction_zz band extinctionmagphys.absorption.gal;em.opt.IVARCHARprincipalgama_dr4.G02GuideStarsv01Guide stars for the G02 survey region.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalFIBERMAG_RSDSS DR8 r band magnitude in 3 arcsec diameter fibermagphot.mag;em.opt.RVARCHARprincipalPSFMAG_RSDSS DR8 r band PSF magnitudemagphot.mag;em.opt.RVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LambdarPACS160v01This catalogue contains the complete LAMBDAR output for the Herschel PACS 160 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.G02GalaxyPartMatchesv02This table can be used to match a vis_class=3 object (deblended partof a galaxy) to a vis_class=1 object (chosen main part of agalaxy). Each galaxy should only have one main part but some haveseveral deblended parts.CATAID_VC3CATAID of vis_class=3 objectmeta.idVARCHARprincipalCATAID_MAINCATAID of main partmeta.idVARCHARprincipalgama_dr4.G02GalacticExtinctionv01This table provides the Galactic foreground extinction in all GALEX,SDSS (= KiDS), UKIDSS and VIKING bands for every object inG02TilingCatv06, G02TilingExtrav03 and G02SpStandardsv01.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_B_MGCGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_uGalactic extinction in SDSS and KiDS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_gGalactic extinction in SDSS and KiDS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_rGalactic extinction in SDSS and KiDS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_iGalactic extinction in SDSS and KiDS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_zGalactic extinction in SDSS and KiDS z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_UKIDSSGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_UKIDSSGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_UKIDSSGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_UKIDSSGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_Z_VIKINGGalactic extinction in VIKING Z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_VIKINGGalactic extinction in VIKING Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_VIKINGGalactic extinction in VIKING J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_VIKINGGalactic extinction in VIKING H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_VIKINGGalactic extinction in VIKING K bandmagphys.absorption.gal;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02CFHTLSInputCatv04CFHTLS W1 input catalogue and photometry for the G02 survey region.COBJIDUnique ID from field number and sequence numbermeta.idVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.raVARCHARprincipalCLASS_STARStar-galaxy classifier outputsrc.classVARCHARprincipalKRON_RADIUSKron radius, unsure of unitsphys.angSizeVARCHARprincipalAProfile RMS along major axispixelphys.angSize.smajAxisVARCHARprincipalBProfile RMS along minor axispixelphys.angSize.sminAxisVARCHARprincipalELLIPTICITY1-B/Asrc.ellipticityVARCHARprincipalMAG_APER06_R6-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_APER12_R12-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_APER18_R18-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_APER24_R24-pixel diameter aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_UKron-like elliptical aperture magnitudemagphot.mag;em.opt.UVARCHARprincipalMAG_AUTO_GKron-like elliptical aperture magnitudemagphot.mag;em.opt.BVARCHARprincipalMAG_AUTO_RKron-like elliptical aperture magnitudemagphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_IKron-like elliptical aperture magnitudemagphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_ZKron-like elliptical aperture magnitudemagphot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_UAperture magnitude errormagphot.mag;em.opt.UVARCHARprincipalMAGERR_AUTO_GAperture magnitude errormagphot.mag;em.opt.BVARCHARprincipalMAGERR_AUTO_RAperture magnitude errormagphot.mag;em.opt.RVARCHARprincipalMAGERR_AUTO_IAperture magnitude errormagphot.mag;em.opt.IVARCHARprincipalMAGERR_AUTO_ZAperture magnitude errormagphot.mag;em.opt.IVARCHARprincipalEXTINCTION_Uu-band Galactic extinctionmagphys.absorption.gal;em.opt.UVARCHARprincipalEXTINCTION_Gg-band Galactic extinctionmagphys.absorption.gal;em.opt.BVARCHARprincipalEXTINCTION_Rr-band Galactic extinctionmagphys.absorption.gal;em.opt.RVARCHARprincipalEXTINCTION_Ii-band Galactic extinctionmagphys.absorption.gal;em.opt.IVARCHARprincipalEXTINCTION_Zz-band Galactic extinctionmagphys.absorption.gal;em.opt.IVARCHARprincipalMASKMask information from CFHTLenSmeta.code.qualVARCHARprincipalgama_dr4.G23TilingExtrav01Table of galaxy targets in G23 that are not (or no longer) mainsurvey targets.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalMAGMagnitude from the config filemagphot.magVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23TilingCatv11Science targets in the G23 survey region.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalI_AUTOi band Kron magnitude, extinction correctedmagphot.mag;em.opt.IVARCHARprincipalZ_AUTOZ band Kron magnitude, extinction correctedmagphot.mag;em.optVARCHARprincipalY_AUTOY band Kron magnitude, extinction correctedmagphot.mag;em.IR.NIRVARCHARprincipalJ_AUTOJ band Kron magnitude, extinction correctedmagphot.mag;em.IR.JVARCHARprincipalH_AUTOH band Kron magnitude, extinction correctedmagphot.mag;em.IR.HVARCHARprincipalK_AUTOK band Kron magnitude, extinction correctedmagphot.mag;em.IR.KVARCHARprincipalAPMAG_ZZ band 2 arcsec aperture magnitudemagphot.mag;em.optVARCHARprincipalNUV_AUTONUV magnitude, extinction correctedmagphot.mag;em.UV.200-300nmVARCHARprincipalSURVEY_CODESurvey code for redshift source, see SpecCat DMUmeta.code;meta.datasetVARCHARprincipalZSpectroscopic redshift, -1 for none attemptedsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalSPECIDID of spectrum from SpecAll tablemeta.id.cross;spectVARCHARprincipalVEL_ERRRedshift uncertainty, c delta ln(1+z)km/ssrc.redshift;stat.errorVARCHARprincipalNUM_GAMA_SPECNumber of GAMA spectra within 1 arcsecmeta.number;spectVARCHARprincipalTYPEType of object: 1=galaxy, 2=star, 3=unknown, 4=artifactmeta.numberVARCHARprincipalVIS_CLASSVisual classification, see notesmata.code.qualVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalPRIORITY_CLASSPriorities for targeting, see notesmeta.code.classVARCHARprincipalNEIGHBOUR_CLASSNumber of SURVEY_CLASS >= 3 targets within 40 arcsecmeta.code.classVARCHARprincipalAREA_FLAGSet to 1 for 2014 target region, 0 otherwisemeta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23SpStandardsv01Standard stars from KiDS and VIKING data for the G23 survey region.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalMAG_AUTO_IKiDS auto i band magnitudemagphot.mag;em.opt.IVARCHARprincipalRMSDIFFDeviation of colours from fiducial point in RMS unitsmagphot.magVARCHARprincipalPRIORITY_CLASS2 or 3 depending on RMSDIFFmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23InputCatv06This is the GAMA II master input catalogue for the G23 survey regionbased on KiDS and VIKING data.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalNPIXMASKNumber of masked pixels in i-band detected objectmeta.code.qualVARCHARprincipalMAG_AUTO_Ii band Kron magnitude, not extinction correctedmagphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_ZZ band Kron magnitude, not extinction correctedmagphot.mag;em.optVARCHARprincipalMAG_AUTO_YY band Kron magnitude, not extinction correctedmagphot.mag;em.IR.NIRVARCHARprincipalMAG_AUTO_JJ band Kron magnitude, not extinction correctedmagphot.mag;em.IR.JVARCHARprincipalMAG_AUTO_HH band Kron magnitude, not extinction correctedmagphot.mag;em.opt.HVARCHARprincipalMAG_AUTO_KK band Kron magnitude, not extinction correctedmagphot.mag;em.IR.KVARCHARprincipalAPMAG_ZZ band 2 arcsec aperture magnitude, not extinction correctedmagphot.mag;em.optVARCHARprincipalMU_E_Ii band effective surface brightness, not extinction correctedmag/arcsec^2phot.mag.sb;em.opt.IVARCHARprincipalFLUX_RADIUS_Ii band half-light radiusarcsecphys.angSize;em.opt.IVARCHARprincipalMAG_NUVNUV magnitude from LAMBDAR, not extinction correctedmagphot.mag;em.UV.200-300nmVARCHARprincipalEXTINCTION_IGalactic extinction in i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalEXTINCTION_YGalactic extinction in Y bandmagphys.absorption.gal;em.optVARCHARprincipalEXTINCTION_ZGalactic extinction in Z bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalEXTINCTION_JGalactic extinction in J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalEXTINCTION_HGalactic extinction in H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalEXTINCTION_KGalactic extinction in K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalEXTINCTION_NUVGalactic extinction in NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalCLASS_STAR_Ii band stellaricitysrc.class;em.opt.IVARCHARprincipalCLASS_STAR_ZZ band stellaricitysrc.class;em.optVARCHARprincipalCLASS_STAR_YY band stellaricitysrc.class;em.IR.NIRVARCHARprincipalCLASS_STAR_JJ band stellaricitysrc.class;em.IR.JVARCHARprincipalCLASS_STAR_HH band stellaricitysrc.class;em.IR.HVARCHARprincipalCLASS_STAR_KK band stellaricitysrc.class;em.IR.KVARCHARprincipalMASK_IC_14Bright star masking flag (stars i < 14)src.classVARCHARprincipalMASK_IC_13Bright star masking flag (stars i < 13)src.classVARCHARprincipalMASK_IC_12Bright star masking flag (stars i < 12)src.classVARCHARprincipalMASK_IC_THBright star masking flag (Hipparcos/Tycho stars)src.classVARCHARprincipalSGSEP_JKOffset from J-K stellar locusmagVARCHARprincipalTYPEType of object: 1=galaxy, 2=star, 3=unknown, 4=artifactsrc.classVARCHARprincipalVIS_CLASSVisual classification, see notessrc.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23GuideStarsv01Guide stars for the G23 survey region.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalRA_SEPRA offset between GAMA object and matched ATLAS object (GAMA-ATLAS)arcsecpos.angDistanceVARCHARprincipalDEC_SEPDEC offset between GAMA object and matched ATLAS object (GAMA-ATLAS)arcsecpos.angDistanceVARCHARprincipalMAG_PETRO_Rr band Petrosian magnitude from ATLAS, not corrected for extinctionmagphot.mag;em.opt.RVARCHARprincipalMAG_AUTO_Ii band Kron magnitude, not extinction correctedmagphot.mag;em.opt.IVARCHARprincipalMAG_AUTO_ZZ band Kron magnitude, not extinction correctedmagphot.mag;em.optVARCHARprincipalMAG_AUTO_YY band Kron magnitude, not extinction correctedmagphot.mag;em.IR.NIRVARCHARprincipalMAG_AUTO_JJ band Kron magnitude, not extinction correctedmagphot.mag;em.IR.JVARCHARprincipalMAG_AUTO_HH band Kron magnitude, not extinction correctedmagphot.mag;em.IR.HVARCHARprincipalMAG_AUTO_KK band Kron magnitude, not extinction correctedmagphot.mag;em.IR.KVARCHARprincipalCLASS_STAR_Ii band stellaricitysrc.classVARCHARprincipalTYPEType of object: 1=galaxy, 2=star, 3=unknown, 4=artifactsrc.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23GalacticExtinctionv01This table provides the Galactic foreground extinction in all GALEX,SDSS (= KiDS), UKIDSS and VIKING bands for every object inG23InputCatAv01.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARA of position for which the extinction was calculated (J2000)degpos.eq.raVARCHARprincipalDECDEC of position for which the extinction was calculated (J2000)degpos.eq.decVARCHARprincipalEBVE(B-V)magphys.absorption.galVARCHARprincipalA_FUVGalactic extinction in GALEX FUV bandmagphys.absorption.gal;em.UV.100-200nmVARCHARprincipalA_NUVGalactic extinction in GALEX NUV bandmagphys.absorption.gal;em.UV.200-300nmVARCHARprincipalA_B_MGCGalactic extinction in MGC B bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_uGalactic extinction in SDSS and KiDS u bandmagphys.absorption.gal;em.opt.UVARCHARprincipalA_gGalactic extinction in SDSS and KiDS g bandmagphys.absorption.gal;em.opt.BVARCHARprincipalA_rGalactic extinction in SDSS and KiDS r bandmagphys.absorption.gal;em.opt.RVARCHARprincipalA_iGalactic extinction in SDSS and KiDS i bandmagphys.absorption.gal;em.opt.IVARCHARprincipalA_zGalactic extinction in SDSS and KiDS z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_UKIDSSGalactic extinction in UKIDSS Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_UKIDSSGalactic extinction in UKIDSS J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_UKIDSSGalactic extinction in UKIDSS H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_UKIDSSGalactic extinction in UKIDSS K bandmagphys.absorption.gal;em.IR.KVARCHARprincipalA_Z_VIKINGGalactic extinction in VIKING Z bandmagphys.absorption.gal;em.optVARCHARprincipalA_Y_VIKINGGalactic extinction in VIKING Y bandmagphys.absorption.gal;em.IR.NIRVARCHARprincipalA_J_VIKINGGalactic extinction in VIKING J bandmagphys.absorption.gal;em.IR.JVARCHARprincipalA_H_VIKINGGalactic extinction in VIKING H bandmagphys.absorption.gal;em.IR.HVARCHARprincipalA_K_VIKINGGalactic extinction in VIKING K bandmagphys.absorption.gal;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GalexMainv02This is the main catalogue of the GalexPhotometry DMU. It reproducesthe most important information from the other catalogues in this DMUand provides a best estimate of the NUV and FUV fluxes of all GAMAobjects in the GAMA II equatorial survey regions that were detectedby GALEX.The following columns contain the output of the advanced matching procedureThe following columns contain the result of our CoG photometryThe following columns refer to the GAMA object's nearest neighbour GALEX objectCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalRARight Ascension of GAMA object (J2000)degpos.eq.raVARCHARprincipalDECDeclination of GAMA object (J2000)degpos.eq.decVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalBEST_FLUX_NUVBest estimate of the GAMA object's NUV fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalBEST_FLUXERR_NUVBest estimate NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalBEST_MAG_NUVBest estimate of the GAMA object's NUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalBEST_MAGERR_NUVBest estimate NUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalBEST_FLUX_FUVBest estimate of the GAMA object's FUV fluxmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalBEST_FLUXERR_FUVBest estimate FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalBEST_MAG_FUVBest estimate of the GAMA object's FUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalBEST_MAGERR_FUVBest estimate FUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalBEST_METHODMethod used for the best flux estimates (AdvancedMatch or CoG)meta.codeVARCHARprincipalNMATCHUVNumber of GALEX objects involved in advanced matching proceduremeta.numberVARCHARprincipalNMATCHOPTNumber of GAMA objects involved in advanced matching proceduremeta.numberVARCHARprincipalNUVFLAGCombination of the NUV artifact flags of all GALEX objects involved in advanced matching proceduremeta.code;em.UV.200-300nmVARCHARprincipalFUVFLAGCombination of the FUV artifact flags of all GALEX objects involved in advanced matching proceduremeta.code;em.UV.100-200nmVARCHARprincipalTOT_FLUX_NUVTotal NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.200-300nmVARCHARprincipalTOT_FLUXERR_NUVError on the total NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalTOT_MAG_NUVTotal NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.200-300nmVARCHARprincipalTOT_MAGERR_NUVError on total NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalTOT_FLUX_FUVTotal FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.100-200nmVARCHARprincipalTOT_FLUXERR_FUVError on total FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalTOT_MAG_FUVTotal FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.100-200nmVARCHARprincipalTOT_MAGERR_FUVError on total FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalSPLIT_FLUX_NUVRedistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalSPLIT_FLUXERR_NUVError on redistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalSPLIT_MAG_NUVRedistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nmVARCHARprincipalSPLIT_MAGERR_NUVError on redistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalSPLIT_FLUX_FUVRedistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalSPLIT_FLUXERR_FUVError on redistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalSPLIT_MAG_FUVRedistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nmVARCHARprincipalSPLIT_MAGERR_FUVError on redistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_FLUX_NUVCoG NUV flux at the position of the GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalCOG_FLUXERR_NUVCoG NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalCOG_MAG_NUVCoG NUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalCOG_MAGERR_NUVCoG NUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalCOG_FLUX_FUVCoG FUV flux at the position of the GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalCOG_FLUXERR_FUVCoG FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_MAG_FUVCoG FUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalCOG_MAGERR_FUVCoG FUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalCOG_RE_CRIT_NUVCoG NUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCOG_HP_RAD_NUVCoG NUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCOG_RE_CRIT_FUVCoG FUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCOG_HP_RAD_FUVCoG FUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCOG_CONFSOURCE_NUVCoG NUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCOG_CONFSOURCE_FUVCoG FUV flag indicating whether masking occurredmeta.codeVARCHARprincipalNN_GGOIDGlobal Object ID of nearest neighbour GALEX objectmeta.idVARCHARprincipalNN_RA_GALEXRight Ascension of nearest neighbour GALEX object (J2000)degpos.eq.raVARCHARprincipalNN_DEC_GALEXDeclination of nearest neighbour GALEX object (J2000)degpos.eq.decVARCHARprincipalNN_DISTDistance between GAMA object and nearest neighbour GALEX objectarcsecpos.angDistanceVARCHARprincipalNN_NMATCH4Number of GALEX objects found within 4 arcsec of GAMA objectmeta.numberVARCHARprincipalNN_MANY2ONENumber of GAMA objects the nearest neighbour GALEX object is matched tometa.numberVARCHARprincipalNN_FLUX_NUVNUV flux of nearest neighbour GALEX objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalNN_FLUXERR_NUVNUV flux error of nearest neighbour GALEX objectmicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalNN_MAG_NUVNUV AB Kron magnitude of nearest neighbour GALEX objectmagphot.mag;em.UV.200-300nmVARCHARprincipalNN_MAGERR_NUVNUV AB Kron magnitude error of nearest neighbour GALEX objectmagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalNN_FLUX_FUVFUV flux of nearest neighbour GALEX object using NUV aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalNN_FLUXERR_FUVFUV flux error of nearest neighbour GALEX object using NUV aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalNN_MAG_FUVFUV AB Kron magnitude of nearest neighbour GALEX object using NUV aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalNN_MAGERR_FUVFUV AB Kron magnitude error of nearest neighbour GALEX object using NUV aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalNN_ARTIFACT_NUVNUV artifact flag of nearest neighbour GALEX object (see GalexPhot notes)meta.code;em.UV.200-300nmVARCHARprincipalNN_ARTIFACT_FUVFUV artifact flag of nearest neighbour GALEX object (see GalexPhot notes)meta.code;em.UV.100-200nmVARCHARprincipalNN_SFLAGS_NUVNUV Sextraxtor extraction flags of nearest neighbour GALEX objectmeta.code;em.UV.200-300nmVARCHARprincipalNN_SFLAGS_FUVFUV Sextraxtor extraction flags of nearest neighbour GALEX objectmeta.code;em.UV.100-200nmVARCHARprincipalNN_FLUX50_RADIUS_NUVNUV 50 percent fraction-of-light radius of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_FLUX50_RADIUS_FUVFUV 50 percent fraction-of-light radius of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalNN_SEMIMAJOR_NUVNUV semimajor axis of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_SEMIMINOR_NUVNUV semiminor axis of nearest neighbour GALEX objectarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalNN_SEMIMAJORERR_NUVNUV semimajor axis error of nearest neighbour GALEX objectarcsecphys.size.radius;stat.errorVARCHARprincipalNN_SEMIMINORERR_NUVNUV semiminor axis error of nearest neighbour GALEX objectarcsecphys.size.radius;stat.errorVARCHARprincipalNN_POSANG_NUVNUV position angle (east of north) of nearest neighbour GALEX objectdegpos.posAngVARCHARprincipalNN_POSANGERR_NUVNUV position angle error of nearest neighbour GALEX objectdegpos.posAng;stat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GalexSimpleMatchv02This catalogue contains the result of a simple nearest neighbourmatch between InputCatAv06 and GalexPhot. GAMA objects without aGALEX nearest neighbour within a distance of 4 arcsec are consideredunmatched and are not included in this catalogue.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objid of GAMA objectmeta.idVARCHARprincipalGGOIDGlobal Object ID of nearest neighbour GALEX objectmeta.idVARCHARprincipalFUVMATCHFlag indicating whether matched GALEX source has FUV flux with S/N >=2.5 (-1=no FUV data)meta.code;em.UV.100-200nmVARCHARprincipalNN_DISTDistance between GAMA object and nearest neighbour GALEX objectarcsecpos.angDistanceVARCHARprincipalNMATCH4Number of GALEX objects found within 4 arcsec of GAMA objectmeta.numberVARCHARprincipalMANY2ONENumber of GAMA objects the GALEX object is matched tometa.numberVARCHARprincipalGNEIGHBOR_DISTString list of distances to all GALEX sources within 20 arcsecVARCHARprincipalGNEIGHBOR_NAMEString list of names of all GALEX sources within 20 arcsecVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GalexPhotv02This catalogue provides GALEX NUV and FUV photometry for primarysources with S/N_NUV >= 2.5 in the GAMA II equatorial surveyregions. This photometry was derived using the GALEXSExtractor-based pipeline.GGOIDGALEX Global Object IDmeta.idVARCHARprincipalNUMBER_MCATRunning object number from GALEX MCAT filemeta.idVARCHARprincipalNAMEObject IAU format namemeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalGLONGalactic longitudedegpos.galactic.lonVARCHARprincipalGLATGalactic latitudedegpos.galactic.latVARCHARprincipalPOSERRPosition errorarcsecstat.errorVARCHARprincipalTILENUMGALEX tile numbermeta.numberVARCHARprincipalTILEGALEX tile namemeta.idVARCHARprincipalFOV_RADIUSDistance of object from centre of FoVdegpos.angDistanceVARCHARprincipalHP_PIXELHEALPix pixel on sky coverage maps on GALEX-GAMA web site (nside = 16384; nested)VARCHARprincipalEXPTIME_NUVNUV exposure time of tilesobs.exposure;em.UV.200-300nmVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEXPTIME_FUVFUV exposure time of tilesobs.exposure;em.UV.100-200nmVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalFLUX_NUVNUV calibrated fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXERR_NUVNUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_NUVNUV calibrated AB Kron magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalMAGERR_NUVNUV calibrated AB Kron magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalS2N_NUVNUV signal-to-noise from flux valuestat.snr;em.UV.200-300nmVARCHARprincipalARTIFACT_NUVNUV artifact flag (see notes)meta.code;em.UV.200-300nmVARCHARprincipalBKGRND_FLUX_NUVNUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.200-300nm;src.netVARCHARprincipalBKGRND_MAG_NUVNUV sky background surface brightnessmag/arcsec^2phot.mag;em.UV.200-300nm;src.netVARCHARprincipalFLUX_FUVFUV calibrated flux using NUV aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXERR_FUVFUV flux error using NUV aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAG_FUVFUV calibrated AB Kron magnitude using NUV aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAGERR_FUVFUV calibrated AB Kron magnitude error using NUV aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalS2N_FUVFUV signal-to-noise from flux value (NB: can become negative for negative flux)stat.snr;em.UV.100-200nmVARCHARprincipalARTIFACT_FUVFUV artifact flag (see notes)meta.code;em.UV.100-200nmVARCHARprincipalBKGRND_FLUX_FUVFUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.100-200nm;src.netVARCHARprincipalBKGRND_MAG_FUVFUV sky background surface brightnessmag/arcsec^2phot.mag;em.UV.100-200nm;src.netVARCHARprincipalFLUX_D3p0_NUVNUV flux in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D4p5_NUVNUV flux in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D7p5_NUVNUV flux in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D12p0_NUVNUV flux in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D18p0_NUVNUV flux in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D25p5_NUVNUV flux in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUX_D34p5_NUVNUV flux in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXERR_D3p0_NUVNUV flux error in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D4p5_NUVNUV flux error in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D7p5_NUVNUV flux error in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D12p0_NUVNUV flux error in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D18p0_NUVNUV flux error in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D25p5_NUVNUV flux error in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXERR_D34p5_NUVNUV flux error in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_D3p0_NUVNUV AB magnitude in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D4p5_NUVNUV AB magnitude in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D7p5_NUVNUV AB magnitude in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D12p0_NUVNUV AB magnitude in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D18p0_NUVNUV AB magnitude in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D25p5_NUVNUV AB magnitude in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAG_D34p5_NUVNUV AB magnitude in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.200-300nmVARCHARprincipalMAGERR_D3p0_NUVNUV AB magnitude error in 3.0 arcsec (2 pixel)diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D4p5_NUVNUV AB magnitude error in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D7p5_NUVNUV AB magnitude error in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D12p0_NUVNUV AB magnitude error in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D18p0_NUVNUV AB magnitude error in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D25p5_NUVNUV AB magnitude error in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalMAGERR_D34p5_NUVNUV AB magnitude error in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalFLUX20_RADIUS_NUVNUV 20 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX50_RADIUS_NUVNUV 50 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX80_RADIUS_NUVNUV 80 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX90_RADIUS_NUVNUV 90 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX95_RADIUS_NUVNUV 95 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX_MAX_NUVNUV peak flux above backgroundmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalX_IMAGEObject pixel position on intensity mapspixelVARCHARprincipalY_IMAGEObject pixel position on intensity mapspixelVARCHARprincipalXPEAK_IMAGEPixel position of the brightest NUV pixel on intensity mapspixelVARCHARprincipalYPEAK_IMAGEPixel position of the brightest NUV pixel on intensity mapspixelVARCHARprincipalSEMIMAJORSemimajor axisarcsecphys.size.radiusVARCHARprincipalSEMIMINORSemiminor axisarcsecphys.size.radiusVARCHARprincipalSEMIMAJORERRSemimajor axis errorarcsecphys.size.radius;stat.errorVARCHARprincipalSEMIMINORERRSemiminor axis errorarcsecphys.size.radius;stat.errorVARCHARprincipalPOSANGPosition angle (east of north)degpos.posAngVARCHARprincipalPOSANGERRPosition angle errordegpos.posAng;stat.errorVARCHARprincipalFWHM_NUVNUV FWHM assuming a gaussian corearcsecphys.size;em.UV.200-300nmVARCHARprincipalFLAGS_NUVNUV Sextraxtor extraction flagsmeta.code;em.UV.200-300nmVARCHARprincipalCLASS_STARNUV Sextractor star/galaxy classifier outputmeta.code;em.UV.200-300nmVARCHARprincipalFLUX_D3p0_FUVFUV flux in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D4p5_FUVFUV flux in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D7p5_FUVFUV flux in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D12p0_FUVFUV flux in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D18p0_FUVFUV flux in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D25p5_FUVFUV flux in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUX_D34p5_FUVFUV flux in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXERR_D3p0_FUVFUV flux error in 3.0 arcsec (2 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D4p5_FUVFUV flux error in 4.5 arcsec (3 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D7p5_FUVFUV flux error in 7.5 arcsec (5 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D12p0_FUVFUV flux error in 12.0 arcsec (8 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D18p0_FUVFUV flux error in 18.0 arcsec (12 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D25p5_FUVFUV flux error in 25.5 arcsec (17 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXERR_D34p5_FUVFUV flux error in 34.5 arcsec (23 pixel) diameter aperturemicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAG_D3p0_FUVFUV AB magnitude in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D4p5_FUVFUV AB magnitude in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D7p5_FUVFUV AB magnitude in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D12p0_FUVFUV AB magnitude in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D18p0_FUVFUV AB magnitude in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D25p5_FUVFUV AB magnitude in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAG_D34p5_FUVFUV AB magnitude in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.100-200nmVARCHARprincipalMAGERR_D3p0_FUVFUV AB magnitude error in 3.0 arcsec (2 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D4p5_FUVFUV AB magnitude error in 4.5 arcsec (3 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D7p5_FUVFUV AB magnitude error in 7.5 arcsec (5 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D12p0_FUVFUV AB magnitude error in 12.0 arcsec (8 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D18p0_FUVFUV AB magnitude error in 18.0 arcsec (12 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D25p5_FUVFUV AB magnitude error in 25.5 arcsec (17 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalMAGERR_D34p5_FUVFUV AB magnitude error in 34.5 arcsec (23 pixel) diameter aperturemagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalFLUX20_RADIUS_FUVFUV 20 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX50_RADIUS_FUVFUV 50 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX80_RADIUS_FUVFUV 80 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX90_RADIUS_FUVFUV 90 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX95_RADIUS_FUVFUV 95 percent fraction-of-light radiusarcsecVARCHARprincipalFLUX_MAX_FUVFUV peak flux above backgroundmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFWHM_FUVFUV FWHM assuming a gaussian corearcsecphys.size;em.UV.100-200nmVARCHARprincipalFLAGS_FUVFUV Sextraxtor extraction flagsmeta.code;em.UV.100-200nmVARCHARprincipalgama_dr4.GalexObsInfov02This catalogue provides basic GALEX observational information,i.e. exposure times, background levels and detection limits, for allobjects in InputCatAv06.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalEFF_EXPTIME_NUVNUV effective exposure time (relative response)sobs.exposure;em.UV.200-300nmVARCHARprincipalEFF_EXPTIME_FUVFUV effective exposure time (relative response)sobs.exposure;em.UV.100-200nmVARCHARprincipalBKGRND_FLUX_NUVNUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.200-300nm;src.netVARCHARprincipalBKGRND_FLUX_FUVFUV sky background surface brightnessmicroJy/arcsec^2phot.flux;em.UV.100-200nm;src.netVARCHARprincipalNUVFLUXLIMIT2p5S/N=2.5 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalFUVFLUXLIMIT2p5S/N=2.5 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalNUVMAGLIMIT2p5S/N=2.5 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalFUVMAGLIMIT2p5S/N=2.5 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalNUVFLUXLIMIT5S/N=5 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalFUVFLUXLIMIT5S/N=5 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalNUVMAGLIMIT5S/N=5 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalFUVMAGLIMIT5S/N=5 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipalNUVFLUXLIMIT10S/N=10 NUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.200-300nm;stat.minVARCHARprincipalFUVFLUXLIMIT10S/N=10 FUV flux detection limit for a circular source at this positionmicroJyphot.flux;em.UV.100-200nm;stat.minVARCHARprincipalNUVMAGLIMIT10S/N=10 NUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.200-300nm;stat.minVARCHARprincipalFUVMAGLIMIT10S/N=10 FUV flux detection limit for a circular source at this positionmagphot.mag;em.UV.100-200nm;stat.minVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GalexCoGPhotv02This catalogue provides GALEX NUV and FUV curve-of-growth photometryfor all objects in SersicCatv07 (covering only the GAMA I surveyregions).CATAID_IUnique GAMA I ID of GAMA object (see notes)meta.idVARCHARprincipalCATAIDUnique GAMA II ID of GAMA object (see notes)meta.idVARCHARprincipalCPS_NUVNUV counts per secondcounts/sphot.count;em.UV.200-300nmVARCHARprincipalCPSERR_NUVNUV counts per second errorcounts/sphot.count;em.UV.200-300nm;stat.errorVARCHARprincipalFLUX_NUVNUV fluxmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXERR_NUVNUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAG_NUVNUV magnitudemagphot.mag;em.UV.200-300nmVARCHARprincipalMAGERR_NUVNUV magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalRE_CRIT_NUVNUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalHP_RAD_NUVNUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.200-300nmVARCHARprincipalCONFSOURCE_NUVNUV flag indicating whether masking occurredmeta.codeVARCHARprincipalCPS_FUVFUV counts per secondcounts/sphot.count;em.UV.100-200nmVARCHARprincipalCPSERR_FUVFUV counts per second errorcounts/sphot.count;em.UV.100-200nm;stat.errorVARCHARprincipalFLUX_FUVFUV fluxmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXERR_FUVFUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAG_FUVFUV magnitudemagphot.mag;em.UV.100-200nmVARCHARprincipalMAGERR_FUVFUV magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalRE_CRIT_FUVFUV integration radius (multiple of 3 arcsec)arcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalHP_RAD_FUVFUV radius enclosing 50% of the total fluxarcsecphys.size.radius;em.UV.100-200nmVARCHARprincipalCONFSOURCE_FUVFUV flag indicating whether masking occurredmeta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GalexAdvancedMatchv02This catalogue contains the result of an advanced match betweenInputCatAv06 and GalexPhot. The matching procedure takes intoaccount the possibility of multiple matches between GALEX and GAMAobjects and seeks to reconstruct the original UV flux of a givenGAMA object. GAMA objects without a GALEX match are not included inthis catalogue.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalOBJIDSDSS objidmeta.idVARCHARprincipalNMATCHUVNumber of GALEX objects involved in the matchingmeta.numberVARCHARprincipalNMATCHOPTNumber of GAMA objects involved in the matchingmeta.numberVARCHARprincipalUVIDXLISTID list of GALEX object used in the flux redistribution calculation using NAME from GalexPhot; string always ends with a commaVARCHARprincipalOPTIDXLISTID list of GAMA objects used in the flux redistribution calculation using SDSS OBJID; string always ends with a commaVARCHARprincipalNUVFLAGCombination of the NUV artifact flags of all GALEX objects involved in the matchingmeta.code;em.UV.200-300nmVARCHARprincipalFUVFLAGCombination of the FUV artifact flags of all GALEX objects involved in the matchingmeta.code;em.UV.100-200nmVARCHARprincipalFLUXTOT_NUVTotal NUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXTOTERR_NUVTotal NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAGTOT_NUVTotal NUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.200-300nmVARCHARprincipalMAGTOTERR_NUVTotal NUV AB magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXSPLIT_NUVRedistributed NUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.200-300nmVARCHARprincipalFLUXSPLITERR_NUVRedistributed NUV flux errormicroJyphot.flux;em.UV.200-300nm;stat.errorVARCHARprincipalMAGSPLIT_NUVRedistributed NUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.200-300nmVARCHARprincipalMAGSPLITERR_NUVRedistributed NUV AB magnitude errormagphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalFLUXTOT_FUVTotal FUV flux of all GALEX objects associated with GAMA object (unweighted sum of the flux)microJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXTOTERR_FUVTotal FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAGTOT_FUVTotal FUV AB magnitude of all GALEX objects associated with GAMA object (unweighted sum of the flux)magphot.mag;em.UV.100-200nmVARCHARprincipalMAGTOTERR_FUVTotal FUV AB magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalFLUXSPLIT_FUVRedistributed FUV flux of all GALEX objects associated with GAMA objectmicroJyphot.flux;em.UV.100-200nmVARCHARprincipalFLUXSPLITERR_FUVRedistributed FUV flux errormicroJyphot.flux;em.UV.100-200nm;stat.errorVARCHARprincipalMAGSPLIT_FUVRedistributed FUV AB magnitude of all GALEX objects associated with GAMA objectmagphot.mag;em.UV.100-200nmVARCHARprincipalMAGSPLITERR_FUVRedistributed FUV AB magnitude errormagphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GroupsClassifiedv01This table classifies the geometric environment of groups as eithera void, sheet, filament or knot.GroupIDUnique group IDmeta.idVARCHARprincipalRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalDECDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalZRedshift of the iterative central galaxysrc.redshiftVARCHARprincipalGeoS4Geometric environment of group computed with 4 Mpc/h smoothingmeta.code.classVARCHARprincipalGeoS10Geometric environment of group computed with 10 Mpc/h smoothingmeta.code.classVARCHARprincipalgama_dr4.GeometricGridv01This table lists the geometric environment classification of eachcell of a cartesian mesh on the GAMA II equatorial survey regions.CellIDUnique cell IDmeta.idVARCHARprincipalRARA of the centre of the mesh celldegpos.eq.raVARCHARprincipalDECDEC of the centre of the mesh celldegpos.eq.decVARCHARprincipalZRedshift of the centre of the mesh cellsrc.redshiftVARCHARprincipalGeoS4Geometric environment classification of cell computed with 4 Mpc/h smoothingmeta.code.classVARCHARprincipalGeoS10Geometric environment classification of cell computed with 10 Mpc/h smoothingmeta.code.classVARCHARprincipalgama_dr4.GalaxiesClassifiedv01This table classifies the geometric environment of galaxies aseither a void, sheet, filament or knot.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARA of galaxy (J2000)degpos.eq.raVARCHARprincipalDECDEC of galaxy (J2000)degpos.eq.decVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQRedshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalGeoS4Geometric environment of galaxy computed with 4 Mpc/h smoothingmeta.code.classVARCHARprincipalGeoS10Geometric environment of galaxy computed with 10 Mpc/h smoothingmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G3CLinkv10Catalogue that gives linking between all GAMA galaxies that share acommon group in G3CFoFGroup.LinkIDUnique linking IDmeta.id;meta.mainVARCHARindexedprincipalGal1CATAIDCATAID of galaxy 1 in G3CGalmeta.idVARCHARprincipalGal2CATAIDCATAID of galaxy 2 in G3CGalmeta.idVARCHARprincipalSepProjCoProjected separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hpos.distanceVARCHARprincipalLimProjCoMaximum allowed projected separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimProjCo>=SepProjCo)kpc/hpos.distanceVARCHARprincipalSepRadCoRadial separation of galaxy 1 and galaxy 2 in comoving coordinateskpc/hpos.distanceVARCHARprincipalLimRadCoMaximum allowed radial separation for galaxy 1 and galaxy 2 to be linked by the FoF algorithm in comoving coordinates (LimRadCo>=SepRadCo)kpc/hpos.distanceVARCHARprincipalgama_dr4.G3CGalv10Catalogue of all GAMA galaxies used in the G3C GroupFinding DMU.CATAIDGAMA CATAIDmeta.id;meta.mainVARCHARindexedprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDecDeclination (J2000)degpos.eq.decVARCHARprincipalZRedshift in CMB framesrc.redshiftVARCHARprincipalRpetroPetrosian apparent r-band magnitude (AB, extinction corrected) [GAMA selection magnitude]magphot.magVARCHARprincipalDM_100_25_75Distance modulus using H0=100km/s/Mpc, Omega_m=0.25 and Omega_L=0.75magphot.mag.distModVARCHARprincipalSURVEY_CODESource for redshift: 1=SDSS, 2=2dFGRS, 3=MGC, 4=2SLAQ-LRG, 5=GAMA, 6=6dFGS, 7=UZC, 8=2QZ, 9=2SLAQ-QSO, 10=NED, 11=GAMA-LT, 12=WiggleZVARCHARprincipalSigErrVelocity uncertainty (on redshift): assumed to be 30km/s for SDSS, 50km/s for GAMA and 80km/s for 2dFGRSkm/sphys.velocVARCHARprincipalGroupIDGroupID for this galaxy in G3CFoFGroup, 0 is un-groupedmeta.idVARCHARprincipalRankIterCenRelative rank of the galaxy to the RA and Dec of the group 'IterCen' coordinates, where 1 indicates closest and 2 second closest etcVARCHARprincipalSepIterCenProjected angular separation of the galaxy to the RA and Dec of the group 'IterCen' coordinatesarcsecphys.angSizeVARCHARprincipalCoSepIterCenProjected comoving distance separation of the galaxy to the RA and Dec of the group 'IterCen' coordinatesMpc/hphys.size.radiusVARCHARprincipalAngSepIterCenProjected angular size distance (comoving/(1+z)) separation of the galaxy to the RA and Dec of the group 'IterCen' coordinatesMpc/hphys.size.radiusVARCHARprincipalRankBCGRelative rank of the galaxy to the RA and Dec of the group 'BCG' coordinates, where 1 indicates closest and 2 second closest etcVARCHARprincipalSepBCGProjected angular separation of the galaxy to the RA and Dec of the group 'BCG' coordinatesarcsecphys.angSizeVARCHARprincipalCoSepBCGProjected comoving distance separation of the galaxy to the RA and Dec of the group 'BCG' coordinatesMpc/hphys.size.radiusVARCHARprincipalAngSepBCGProjected angular size distance (comoving/(1+z)) separation of the galaxy to the RA and Dec of the group 'BCG' coordinatesMpc/hphys.size.radiusVARCHARprincipalRankCenRelative rank of the galaxy to the RA and Dec of the group 'Cen' coordinates, where 1 indicates closest and 2 second closest etcVARCHARprincipalSepCenProjected angular separation of the galaxy to the RA and Dec of the group 'Cen' coordinatesarcsecphys.angSizeVARCHARprincipalCoSepCenProjected comoving distance separation of the galaxy to the RA and Dec of the group 'Cen' coordinatesMpc/hphys.size.radiusVARCHARprincipalAngSepCenProjected angular size distance (comoving/(1+z)) separation of the galaxy to the RA and Dec of the group 'Cen' coordinatesMpc/hphys.size.radiusVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G3CGalPairv10Catalogue of all galaxy pairs with a projected physical separationof 100 kpc/h and a velocity separation of 1000 km/s.PairIDUnique pair IDmeta.id;meta.mainVARCHARindexedprincipalCATAID1CATAID of galaxy 1 in G3CGalmeta.idVARCHARprincipalCATAID2CATAID of galaxy 2 in G3CGalmeta.idVARCHARprincipalSepProjAngPhysical projected separation between galaxy 1 and galaxy 2kpc/hpos.distanceVARCHARprincipalSepVelVelocity separation of galaxy 1 and galaxy 2km/sphys.velocVARCHARprincipalRAbarRA of the r-band (petro) flux weighted centre-of-light of the pairdegpos.eq.raVARCHARprincipalDecbarDec of the r-band (petro) flux weighted centre-of-light of the pairdegpos.eq.decVARCHARprincipalZbarRedshift of the r-band (petro) flux weighted centre-of-light of the pairsrc.redshiftVARCHARprincipalMagSumTotal r-band (petro) apparent magnitude of the pairmagphot.magVARCHARprincipalgama_dr4.G3CFoFGroupv10This is a catalogue of the galaxy group properties in the GAMA IIequatorial and G02 survey regions.GroupIDUnique group ID, as listed in the associated G3CGal linksmeta.id;meta.mainVARCHARindexedprincipalNfofGroup multiplicityVARCHARprincipalIterCenCATAIDReference ID of the iterative central galaxy (preferred position of the group centre)meta.idVARCHARprincipalIterCenRARA of the iterative central galaxy (J2000)degpos.eq.raVARCHARprincipalIterCenDecDec of the iterative central galaxy (J2000)degpos.eq.decVARCHARprincipalIterCenZRedshift of the iterative central galaxysrc.redshiftVARCHARprincipalZfofMedian redshift of the groupsrc.redshiftVARCHARprincipalRad50Group radius defined by the 50th percentile group member, based on the projected distance away from IterCenIDMpc/hphys.size.radiusVARCHARprincipalRad1SigGroup radius defined by the 68th percentile group member, based on the projected distance away from IterCenIDMpc/hphys.size.radiusVARCHARprincipalRad100Group radius defined by the most distant group member, based on the projected distance away from IterCenIDMpc/hphys.size.radiusVARCHARprincipalRelDenRelative galaxy space density (w.r.t. prediction based on the random catalogues) within a cylinder of radius 1.5Mpc/h and offset 18Mpc/h (i.e. diameter 3.0Mpc/h and total length 36Mpc/h) centred on IterCenIDVARCHARprincipalZcompAverage redshift completeness of the group: for each group member the redshift completeness within a projected 1.5Mpc/h radius (at the position of the galaxy) is estimated and then averaged over all group members to provide ZCompVARCHARprincipalGroupEdgeFraction of the group within the survey volume, as estimated from IterCen and Rad100VARCHARprincipalVelDispGroup velocity dispersion, corrected for the total group velocity dispersion error (VelErr); set to zero if VelErr>VelDispRawkm/sphys.velocVARCHARprincipalVelDispRawRaw group velocity dispersionkm/sphys.velocVARCHARprincipalVelErrTotal group velocity errorkm/sphys.velocVARCHARprincipalTotRmagr-band absolute magnitude of the group, obtained by adding up the r-band luminosities of its membersmag-5log(h)phys.magAbsVARCHARprincipalTotFluxProxyProxy for group total r-band luminosity down to M_r - 5 log_10 h = -14 in solar luminosities. It is based on the total observed r-band flux and the fraction of light (as estimated from the global galaxy LF) observable at the group redshift; value listed corresponds to B=1 in Eq. 22 of Robotham et al. (2011)VARCHARprincipalMassProxyProxy for dynamical group mass estimated via M \propto Rad50 * VelDisp^2; value listed corresponds to A=1 in Eq. 18 of Robotham et al. (2011), i.e. calibrated mass is given by A*M, with A the scaling factor described in section 4.3 of Robotham et al. (2011)VARCHARprincipalBCGCATAIDGAMA ID of BCGmeta.idVARCHARprincipalBCGRARA of BCG (J2000)degpos.eq.raVARCHARprincipalBCGDecDec of BCG (J2000)degpos.eq.decVARCHARprincipalRgapApparent r-band magnitude gap between BCG and second brightest group membermagphot.magVARCHARprincipalCenRARA of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.raVARCHARprincipalCenDecDec of group for a r-band luminosity weighted CoM of the system (J2000)degpos.eq.decVARCHARprincipalRadKurtUnbiased kurtosis of the radial distribution of galaxies based on the projected distance to IterCenVARCHARprincipalAxAngAngle of the group major axis on the sky (N -> E = 0 -> 90) using the Carter & Metcalfe (1980) algorithm (0<=AxAng<=180, requires 3 or more members, so -999 otherwise)degpos.posAngVARCHARprincipalAxRatAxial ratio of the minor and major axes of the group using the Carter & Metcalfe (1980) algorithm (0<=AxRat<=1, requires 3 or more members, so -999 otherwise)phys.size.axisRatioVARCHARprincipalSymKSKS test of the uniformity of groups once corrected for the axial-ratio; an elliptical group has an average p-value of 0.5 (requires 3 or more members, so -999 otherwise)VARCHARprincipalVelSkewUnbiased skew of the galaxy velocities (requires 3 or more members, so -999 otherwise)VARCHARprincipalVelKurtUnbiased kurtosis of the galaxy velocities (requires 4 or more members, so -999 otherwise)VARCHARprincipalModalityModality of the system: (1+VelSkew^2)/(3+VelKurt^2); this will be 1/3 for a normal distribution and 0.555 for a uniform oneVARCHARprincipalLinkTotTotal number of FoF links in the systemVARCHARprincipalLinkStrenProjLink strength in projection, 1 minus the average projected FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenProj<=1), i.e. larger values mean a stronger linkVARCHARprincipalLinkStrenRadLink strength radially, 1 minus the average radial FoF link relative to the separation allowed by the FoF algorithm (0<=LinkStrenZ<=1), i.e. larger values mean a stronger linkVARCHARprincipalLinkStrenCombLink strength combined, the average of LinkStrenProj*LinkStrenZ for all the links in the group (0<=LinkStrenComb<=1), i.e. larger values mean a stronger linkVARCHARprincipalMassAMass proxy times the global A factor required to get a median unbaised halo mass estimate (A=10.0, see Robotham et al. 2011 section 4.3 for details)Msun/hphys.massVARCHARprincipalMassAfuncMass proxy times the functional A factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.3 for details)Msun/hphys.massVARCHARprincipalLumBTotFluxProxy times the global B factor required to get a median unbaised r-band luminosity estimate (B=1.04, see Robotham et al. 2011 section 4.4 for details)Lsun/h^2phys.luminosityVARCHARprincipalLumBfuncTotFluxProxy times the functional B factor which is a function of Nfof and IterCenZ (see Robotham et al. 2011 section 4.4 for details)Lsun/h^2phys.luminosityVARCHARprincipald3vol3D convex hull volume in comoving units (only for Nfof>=4, -999 otherwise)(Mpc/h)^3VARCHARprincipald3areaSurface area of the 3D convex hull in comoving units (only for Nfof>=4, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipald2radecProjected area of the hull in the ra dec plane in comoving units (only for Nfof>=3, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipald2razProjected area of the hull in the ra redshift plane in comoving units (only for Nfof>=3, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipald2deczProjected area of the hull in the dec rdshift plane in comoving Mpc units (only for Nfof>=3, -999 otherwise)(Mpc/h)^2phys.areaVARCHARprincipaldistortcircReflects how non-circular the group projection appears to be, see notes, (only for Nfof>=3, -999 otherwise)VARCHARprincipaldistortellipReflects how non-elliptical the group appears to be, see notes, (only for Nfof>=4, -999 otherwise)VARCHARprincipaldistortsphReflects how non-spherical the system appears to be, see notes, (only for Nfof>=4, -999 otherwise)VARCHARprincipalURL_IMGURL of the group's imagemeta.ref.url;meta.fileVARCHARprincipalgama_dr4.HATLASCatv03This catalogue provides Herschel SPIRE and PACS photometry ofHerschel sources matched to GAMA objects in the GAMA II equatorialsurvey regions.CATAIDGAMA catalogue indexVARCHARprincipalHATLAS_IAU_IDHATLAS IAU identifier from the 250 micron positionVARCHARprincipalSOURCE_IDGAMA catalogue identifier. The * indicates which field a source lies inVARCHARprincipalRA_J2000RA (J2000), determined from the 250 micron data (degrees)VARCHARprincipalDEC_J2000Declination (J2000), determined from the 250 micron data (degrees)VARCHARprincipalF250_PPoint source 250 micron flux (Jy)VARCHARprincipalF350_PPoint source 350 micron flux (Jy)VARCHARprincipalF500_PPoint source 500 micron flux (Jy)VARCHARprincipalE250_PPoint source 250 micron 1 sigma error (Jy)VARCHARprincipalE350_PPoint source 350 micron 1 sigma error (Jy)VARCHARprincipalE500_PPoint source 500 micron 1 sigma error (Jy)VARCHARprincipalF250_BESTBest 250 micron flux, either point source or aperture value (Jy) (see README for more information)VARCHARprincipalF350_BESTBest 350 micron flux, either point source or aperture value (Jy) (see README for more information)VARCHARprincipalF500_BESTBest 500 micron flux, either point source or aperture value (Jy) (see README for more information)VARCHARprincipalE250_BESTBest 250 micron 1 sigma flux error (Jy)VARCHARprincipalE350_BESTBest 350 micron 1 sigma flux error (Jy)VARCHARprincipalE500_BESTBest 500 micron 1 sigma flux error (Jy)VARCHARprincipalAP_F250Aperture radius used for aperture flux in F250_BEST if source is extended (arcsec). A value of -99 indicates F250_BEST = F250_PVARCHARprincipalAP_F350Aperture radius used for aperture flux in F350_BEST if source is extended (arcsec). A value of -99 indicates F350_BEST = F350_PVARCHARprincipalAP_F500Aperture radius used for aperture flux in F500_BEST if source is extended (arcsec). A value of -99 indicates F500_BEST = F500_PVARCHARprincipalFLAGIf FLAG = 1 the aperture flux value was measured by hand. See extended_apertures.dat for details of ellipticity if a non-circular aperture was usedVARCHARprincipalF100_BESTBest 100 micron flux, either point or aperture value (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalF160_BESTBest 160 micron flux, either point or aperture value (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalE100_BESTBest 100 micron 1 sigma error (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalE160_BESTBest 160 micron 1 sigma error (Jy) -999. indicates flux is not reliable due to filteringVARCHARprincipalAP_F100Aperture radius used for PACS flux in F100_BEST (arcsec)VARCHARprincipalAP_F160Aperture radius used for PACS flux in F160_BEST (arcsec)VARCHARprincipalSDSS_OBJIDSDSS DR7 OBJIDVARCHARprincipalSDSS_RASDSS DR7 Right Ascension (J2000, double precision)VARCHARprincipalSDSS_DECSDSS DR7 Declination (J2000, double precision)VARCHARprincipalSDSS_RMODELMAGSDSS DR7 r band model magVARCHARprincipalSDSS_RMODELMAG_ERRSDSS DR7 r band model mag errorVARCHARprincipalSDSS_ISOASDSS DR7 isophotal major axis, used for extended source SPIRE/PACS aperture fluxesVARCHARprincipalSDSS_SEPSeparation between 250um and SDSS DR7 positionsVARCHARprincipalLRLikelihood ratioVARCHARprincipalRELIABILITYReliability (R>=0.8 is to be treated as reliable)VARCHARprincipalID_FLAGFlag indicating if reliability has been changed or if other warnings are required (m=merger,r=resolved source,s=affected by star or SSGEP changed)VARCHARprincipalSGSEPStar/Gal separation (0 = Gal, 1=unresolved)VARCHARprincipalPHOTOZPhotometric redshifts from ANNz by Dave Bonfield (Smith et al., 2011, arXiv:1007.5260)VARCHARprincipalPHOTOZERRError on photometric redshift from ANNz (Smith et al., 2011, arXiv:1007.5260)VARCHARprincipalPHOTOZBANDS_STRINGString containing the bands used to derive the photozVARCHARprincipalPHOTOZBANDS_INTInteger showing which bands are present for deriving photozVARCHARprincipalPHOTOZBANDS_COUNTNumber of bands used in deriving photozVARCHARprincipalZ_SPECThe spectroscopic redshiftVARCHARprincipalZ_QUALThe z_spec quality flag (only use z_qual >= 3, as these have at least 90% reliability)VARCHARprincipalZFLAGFlag indicating the source of the redshift (1=SDSS, 5=GAMA)VARCHARprincipalGAMA_IAU_IDGAMA IAU IDVARCHARprincipalGAMA_RAGAMA RA (J2000)VARCHARprincipalGAMA_DECGAMA Dec (J2000)VARCHARprincipalR_PETROPetrosian r band mag from GAMAVARCHARprincipalEXTINCTION_RSDSS r band extinctionVARCHARprincipalU_KRONextinction-corrected gama kron u magVARCHARprincipalG_KRONextinction-corrected gama kron g magVARCHARprincipalR_KRONextinction-corrected gama kron r magVARCHARprincipalI_KRONextinction-corrected gama kron i magVARCHARprincipalZ_KRONextinction-corrected gama kron z magVARCHARprincipalY_KRONextinction-corrected gama kron y magVARCHARprincipalJ_KRONextinction-corrected gama kron j magVARCHARprincipalH_KRONextinction-corrected gama kron h magVARCHARprincipalK_KRONextinction-corrected gama kron k magVARCHARprincipalU_KRON_ERRgama kron u mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalG_KRON_ERRgama kron g mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalR_KRON_ERRgama kron r mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalI_KRON_ERRgama kron i mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalZ_KRON_ERRgama kron z mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalY_KRON_ERRgama kron y mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalJ_KRON_ERRgama kron j mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalH_KRON_ERRgama kron h mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalK_KRON_ERRgama kron k mag err (corrected for factor of 4 in Hill et al., 2010)VARCHARprincipalUKIDSS_LAS_IDSource ID for UKIDSS LAS detections in YJHKVARCHARprincipalBEST_MAG_NUV_EXCORExtinction-corrected Best estimate NUV magnitudeVARCHARprincipalBEST_MAGERR_NUVBest estimate NUV magnitude errorVARCHARprincipalBEST_MAG_FUV_EXCORExtinction-corrected Best estimate FUV magnitudeVARCHARprincipalBEST_MAGERR_FUVBest estimate FUV magnitude errorVARCHARprincipalEBVE(B-V)VARCHARprincipalNUVMAGLIMIT5_EXCORGALEX NUV 5-sigma detection limit for a circular source with default radius 3.4", or radius GAL_RE_R if greaterVARCHARprincipalFUVMAGLIMIT5_EXCORGALEX FUV 5-sigma detection limit for a circular source with default radius 3.4", or radius GAL_RE_R if greaterVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LTRedshiftsv01Liverpool Telescope FrodoSpec redshifts of a small number of veryfibre-bright targets. There should normally be no need to use thistable.SPECIDID made from LTF and date and timemeta.id;meta.mainVARCHARindexedprincipalCATAIDCATAIDmeta.id.cross;srcVARCHARprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalTEMPLATESDSS template number see notesmeta.codeVARCHARprincipalCC_SIGMACross-correlation sigma see notesVARCHARprincipalQUALITYRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LambdarWISEW4v01This catalogue contains the complete LAMBDAR output for the WISE W4 band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarWISEW3v01This catalogue contains the complete LAMBDAR output for the WISE W3 band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarWISEW2v01This catalogue contains the complete LAMBDAR output for the WISE W2 band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarWISEW1v01This catalogue contains the complete LAMBDAR output for the WISE W1 band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarVIKINGZv01This catalogue contains the complete LAMBDAR output for the VIKING Z band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarVIKINGYv01This catalogue contains the complete LAMBDAR output for the VIKING Y band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarVIKINGKv01This catalogue contains the complete LAMBDAR output for the VIKING K band.DFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarVIKINGJv01This catalogue contains the complete LAMBDAR output for the VIKING J band.DFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarVIKINGHv01This catalogue contains the complete LAMBDAR output for the VIKING H band.X_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSPIRE500v01This catalogue contains the complete LAMBDAR output for the Herschel SPIRE 500 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSPIRE350v01This catalogue contains the complete LAMBDAR output for the Herschel SPIRE 350 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSPIRE250v01This catalogue contains the complete LAMBDAR output for the Herschel SPIRE 250 µm band.DFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalLAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSDSSzv01This catalogue contains the complete LAMBDAR output for the SDSS z band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSDSSuv01This catalogue contains the complete LAMBDAR output for the SDSS u band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSDSSrv01This catalogue contains the complete LAMBDAR output for the SDSS r band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSDSSiv01This catalogue contains the complete LAMBDAR output for the SDSS i band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarSDSSgv01This catalogue contains the complete LAMBDAR output for the SDSS g band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarPACS100v01This catalogue contains the complete LAMBDAR output for the Herschel PACS 100 µm band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarInputCatUVOptNIRv01This table contains the input catalogue of apertures used formeasuring the fluxes and uncertainties in the GALEX FUV - VIKING Kbands using the LAMBDAR program in the three GAMA II equatorialsurvey regions.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARight ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalROTN2EAperture orientation angledegpos.posAngVARCHARprincipalRADMAJAperture semimajor axis lengtharcsecphys.angSize.smajAxisVARCHARprincipalRADMINAperture semiminor axis lengtharcsecphys.angSize.sminAxisVARCHARprincipalAP_ORIGINOrigin of the object aperturemeta.noteVARCHARprincipalCONTAMContaminant flag; T=contaminantmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LambdarInputCatMIRv01This table contains the input catalogue of apertures used formeasuring the fluxes and uncertainties in the WISE W1 - WISE W2bands using the LAMBDAR program in the three GAMA II equatorialsurvey regions.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARight ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalROTN2EAperture orientation angledegpos.posAngVARCHARprincipalRADMAJAperture semimajor axis lengtharcsecphys.angSize.smajAxisVARCHARprincipalRADMINAperture semiminor axis lengtharcsecphys.angSize.sminAxisVARCHARprincipalAP_ORIGINOrigin of the object aperturemeta.noteVARCHARprincipalCONTAMContaminant flag; T=contaminantmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LambdarInputCatFIRv01This table contains the input catalogue of apertures used formeasuring the fluxes and uncertainties in the WISE W3 - SPIRE 500 µmbands using the LAMBDAR program in the three GAMA II equatorialsurvey regions.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalRARight ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalROTN2EAperture orientation angledegpos.posAngVARCHARprincipalRADMAJAperture semimajor axis lengtharcsecphys.angSize.smajAxisVARCHARprincipalRADMINAperture semiminor axis lengtharcsecphys.angSize.sminAxisVARCHARprincipalAP_ORIGINOrigin of the object aperturemeta.noteVARCHARprincipalCONTAMContaminant flag; T=contaminantmeta.code.classVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LambdarGALEXNUVv01This catalogue contains the complete LAMBDAR output for the GALEX NUV band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarGALEXFUVv01This catalogue contains the complete LAMBDAR output for the GALEX FUV band.LAMIDUnique ID of LAMBDAR sourcemeta.id;meta.mainVARCHARindexedprincipalRARight Ascension, same as inputdegpos.eq.raVARCHARprincipalDECDeclination, same as inputdegpos.eq.decVARCHARprincipalrotN2EAperture orientation angle, same as inputdegpos.posAngVARCHARprincipalradmajasecAperture semimajor axis length, same as inputarcsecphys.angSize.smajAxisVARCHARprincipalradminasecAperture semiminor axis length, same as inputarcsecphys.angSize.sminAxisVARCHARprincipalX_IMAGEAperture location in image coordinatespixelpos.cartesian.xVARCHARprincipalY_IMAGEAperture location in image coordinatespixelpos.cartesian.yVARCHARprincipalNX_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.xVARCHARprincipalNY_PIX2EDGENumber of pixels to the nearest image edgepixelpos.cartesian.yVARCHARprincipalStampDiameterDiameter of the aperture stamppixelobs.image;phys.size.diameterVARCHARprincipalSumPSFIntegral of the PSFpixel^2instr.beamVARCHARprincipalSumSAIntegral of catalogue aperture (i.e. the prior)pixel^2VARCHARprincipalSumSFAIntegral of post-convolution aperturepixel^2VARCHARprincipalSumDFAIntegral of deblended convolved aperturepixel^2VARCHARprincipalSumSFAxPSFIntegral of convolved aperture times PSFphot.countVARCHARprincipalSumSFAxDataIntegral of convolved aperture times data imagecountsphot.countVARCHARprincipalSumDFAxDataIntegral of deblended convolved aperture times data imagecountsphot.countVARCHARprincipalSumSFAsqxErrorsqIntegral of convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSumDFAsqxErrorsqIntegral of deblended convolved aperture squared times error image squaredcounts^2phot.count;stat.errorVARCHARprincipalSkyLocalMeasured median sky levelJy/pixinstr.skyLevel;stat.medianVARCHARprincipalSkyLocal_MeanMeasured mean sky levelJy/pixinstr.skyLevel;stat.meanVARCHARprincipalSkyFluxMedian sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.medianVARCHARprincipalSkyFlux_MeanMean sky flux contained in deblended convolved apertureJyphot.flux.density;instr.skyLevel;stat.meanVARCHARprincipalSkyErrorError on median sky flux contained in deblended convolved apertureJyphot.flux.density;stat.median;stat.errorVARCHARprincipalSkyError_MeanError on mean sky flux contained in deblended convolved apertureJyphot.flux.density;stat.errorVARCHARprincipalSkyRMSRMS of sky pixels calculated during median sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMS_MeanRMS of sky pixels calculated during mean sky level calculationJy/pixstat.stdevVARCHARprincipalSkyRMSpvalPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalSkyRMSpval_MeanPearson's normality p-value on sky pixelsstat.paramVARCHARprincipalNearSkyBinsNumber of sky bins equal to sky estimateVARCHARprincipalNearSkyBins_MeanNumber of sky bins equal to sky estimateVARCHARprincipalSFAFluxFinal blended fluxJyphot.flux.density;VARCHARprincipalSFAErrError on final blended fluxJyphot.flux.density;stat.errorVARCHARprincipalDFAFluxFinal deblended fluxJyphot.flux.densityVARCHARprincipalDFAErrError on final deblended fluxJyphot.flux.density;stat.errorVARCHARprincipalDeblendErrDeblend uncertaintyJyphot.flux.density;stat.errorVARCHARprincipalDFAFlux_Iter1Deblended flux after 1 iterationJyphot.flux.density;VARCHARprincipalDFAErr_Iter1Error on deblended flux after 1 iterationJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter1Sum of deblended convolved model after 1 iterationpixel^2VARCHARprincipalDFAFlux_Iter2Deblended flux after 2 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter2Error on deblended flux after 2 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter2Sum of deblended convolved model after 2 iterationspixel^2VARCHARprincipalDFAFlux_Iter3Deblended flux after 3 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter3Error on deblended flux after 3 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter3Sum of deblended convolved model after 3 iterationspixel^2VARCHARprincipalDFAFlux_Iter4Deblended flux after 4 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter4Error on deblended flux after 4 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter4Sum of deblended convolved model after 4 iterationspixel^2VARCHARprincipalDFAFlux_Iter5Deblended flux after 5 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter5Error on deblended flux after 5 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter5Sum of deblended convolved model after 5 iterationspixel^2VARCHARprincipalDFAFlux_Iter6Deblended flux after 6 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter6Error on deblended flux after 6 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter6Sum of deblended convolved model after 6 iterationspixel^2VARCHARprincipalDFAFlux_Iter7Deblended flux after 7 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter7Error on deblended flux after 7 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter7Sum of deblended convolved model after 7 iterationspixel^2VARCHARprincipalDFAFlux_Iter8Deblended flux after 8 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter8Error on deblended flux after 8 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter8Sum of deblended convolved model after 8 iterationspixel^2VARCHARprincipalDFAFlux_Iter9Deblended flux after 9 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter9Error on deblended flux after 9 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter9Sum of deblended convolved model after 9 iterationspixel^2VARCHARprincipalDFAFlux_Iter10Deblended flux after 10 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter10Error on deblended flux after 10 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter10Sum of deblended convolved model after 10 iterationspixel^2VARCHARprincipalDFAFlux_Iter11Deblended flux after 11 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter11Error on deblended flux after 11 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter11Sum of deblended convolved model after 11 iterationspixel^2VARCHARprincipalDFAFlux_Iter12Deblended flux after 12 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter12Error on deblended flux after 12 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter12Sum of deblended convolved model after 12 iterationspixel^2VARCHARprincipalDFAFlux_Iter13Deblended flux after 13 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter13Error on deblended flux after 13 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter13Sum of deblended convolved model after 13 iterationspixel^2VARCHARprincipalDFAFlux_Iter14Deblended flux after 14 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter14Error on deblended flux after 14 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter14Sum of deblended convolved model after 14 iterationspixel^2VARCHARprincipalDFAFlux_Iter15Deblended flux after 15 iterationsJyphot.flux.density;VARCHARprincipalDFAErr_Iter15Error on deblended flux after 15 iterationsJyphot.flux.density;stat.errorVARCHARprincipalSumDFA_Iter15Sum of deblended convolved model after 15 iterationspixel^2VARCHARprincipalABMagDFAAB magnitude of final deblended fluxmagphot.mag;VARCHARprincipalABMagErrDFAError on AB magnitude of final deblended fluxmagphot.mag;stat.errorVARCHARprincipalBlanksMeanMeanMean value of mean pixel values in n blank aperturesJyphot.flux.density;stat.meanVARCHARprincipalBlanksMeanSDStdev of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksMeanMADMAD RMS of mean pixel values in n blank aperturesJyphot.flux.density;stat.stdevVARCHARprincipalBlanksApMeanMean value of integral of n individually masked blank aperturespixel^2stat.meanVARCHARprincipalBlanksApSDStdev of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalBlanksApMADMAD RMS of integral of n individually masked blank aperturespixel^2stat.stdevVARCHARprincipalNumberMeasuredBlanksNumber of blank apertures measured per objectVARCHARprincipalMinApCorrMultiplicative minimum aperture correctionarith.factorVARCHARprincipalMaxApCorrMultiplicative maximum aperture correctionarith.factorVARCHARprincipalDetecThres_5sig5 sigma upper limit for this apertureJyphot.flux.densityVARCHARprincipalDetecThres_5sig_Mag5 sigma upper limit for this aperturemagphot.magVARCHARprincipalQuarteredPhot1Flux in quadrant 1 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2Flux in quadrant 2 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3Flux in quadrant 3 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4Flux in quadrant 4 of apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot1_DeblendedFlux in quadrant 1 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot2_DeblendedFlux in quadrant 2 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot3_DeblendedFlux in quadrant 3 of deblended apertureJyphot.flux.densityVARCHARprincipalQuarteredPhot4_DeblendedFlux in quadrant 4 of deblended apertureJyphot.flux.densityVARCHARprincipalPixelFluxPixel flux at object positionJyphot.flux.densityVARCHARprincipalPhotometryWarningBasic photometry warning flagsVARCHARprincipalPhotometryFlagBitwise flag encoding the photometry warningsVARCHARprincipalgama_dr4.LambdarCatv01This is the main catalogue of the LambdarPhotometry DMU. It containsthe final 21-band fluxes and uncertainties, measured using theLAMBDAR program, in the three GAMA II equatorial survey regions. Thefluxes for each object are aperture-matched and deblended, and thevariations of the PSF and pixel scale across the various bands arecorrectly accounted for.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRARight Ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalFUV_fluxExtinction corrected GALEX FUV fluxJyphot.flux.density;em.UV.100-200nmVARCHARprincipalFUV_fluxerrError in extinction corrected GALEX FUV fluxJyphot.flux.density;em.UV.100-200nm;stat.errorVARCHARprincipalNUV_fluxExinction corrected GALEX NUV fluxJyphot.flux.density;em.UV.200-300nmVARCHARprincipalNUV_fluxerrError in extinction corrected GALEX NUV fluxJyphot.flux.density;em.UV.200-300nm;stat.errorVARCHARprincipalu_fluxExtinction corrected SDSS u band fluxJyphot.flux.density;em.opt.UVARCHARprincipalu_fluxerrError in extinction corrected SDSS u band fluxJyphot.flux.density;em.opt.U;stat.errorVARCHARprincipalg_fluxExtinction corrected SDSS g band fluxJyphot.flux.density;em.opt.GVARCHARprincipalg_fluxerrError in extinction corrected SDSS g band fluxJyphot.flux.density;em.opt.G;stat.errorVARCHARprincipalr_fluxExtinction corrected SDSS r band fluxJyphot.flux.density;em.opt.RVARCHARprincipalr_fluxerrError in extinction corrected SDSS r band fluxJyphot.flux.density;em.opt.R;stat.errorVARCHARprincipali_fluxExtinction corrected SDSS i band fluxJyphot.flux.density;em.opt.IVARCHARprincipali_fluxerrError in extinction corrected SDSS i band fluxJyphot.flux.density;em.opt.I;stat.errorVARCHARprincipalz_fluxExtinction corrected SDSS z band fluxJyphot.flux.density;em.opt.ZVARCHARprincipalz_fluxerrError in extinction corrected SDSS z band fluxJyphot.flux.density;em.opt.Z;stat.errorVARCHARprincipalX_fluxExtinction correctd VISTA Z band fluxJyphot.flux.density;em.opt.ZVARCHARprincipalX_fluxerrError in extinction corrected VISTA Z band fluxJyphot.flux.density;em.opt.Z;stat.errorVARCHARprincipalY_fluxExtinction corrected VISTA Y band fluxJyphot.flux.density;em.IR.YVARCHARprincipalY_fluxerrError in extinction corrected VISTA Y band fluxJyphot.flux.density;em.IR.Y;stat.errorVARCHARprincipalJ_fluxExtinction corrected VISTA J band fluxJyphot.flux.density;em.IR.JVARCHARprincipalJ_fluxerrError in extinction corrected VISTA J band fluxJyphot.flux.density;em.IR.J;stat.errorVARCHARprincipalH_fluxExtinction corrected VISTA H band fluxJyphot.flux.density;em.IR.HVARCHARprincipalH_fluxerrError in extinction corrected VISTA H band fluxJyphot.flux.density;em.IR.H;stat.errorVARCHARprincipalK_fluxExtinction corrected VISTA K band fluxJyphot.flux.density;em.IR.KVARCHARprincipalK_fluxerrError in extinction corrected VISTA K band fluxJyphot.flux.density;em.IR.K;stat.errorVARCHARprincipalW1_fluxWISE W1 band fluxJyphot.flux.density;em.IR.3-4umVARCHARprincipalW1_fluxerrError in WISE W1 band fluxJyphot.flux.density;em.IR.3-4um;stat.errorVARCHARprincipalW2_fluxWISE W2 band fluxJyphot.flux.density;em.IR.4-8umVARCHARprincipalW2_fluxerrError in WISE W2 band fluxJyphot.flux.density;em.IR.4-8um;stat.errorVARCHARprincipalW3_fluxWISE W3 band fluxJyphot.flux.density;em.IR.8-15umVARCHARprincipalW3_fluxerrError in WISE W3 band fluxJyphot.flux.density;em.IR.8-15um;stat.errorVARCHARprincipalW4_fluxWISE W4 band fluxJyphot.flux.density;em.IR.15-30umVARCHARprincipalW4_fluxerrError in WISE W4 band fluxJyphot.flux.density;em.IR.15-30um;stat.errorVARCHARprincipalP100_fluxHerschel PACS 100 micron fluxJyphot.flux.density;em.mm.1500-3000GHzVARCHARprincipalP100_fluxerrError in Herschel PACS 100 micron fluxJyphot.flux.density;em.mm.1500-3000GHz;stat.errorVARCHARprincipalP160_fluxHerschel PACS 160 micron fluxJyphot.flux.density;em.mm.1500-3000GHzVARCHARprincipalP160_fluxerrError in Herschel PACS 160 micron fluxJyphot.flux.density;em.mm.1500-3000GHz;stat.errorVARCHARprincipalS250_fluxHerschel SPIRE 250 micron fluxJyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalS250_fluxerrError in Herschel SPIRE 250 micron fluxJyphot.flux.density;em.mm.750-1500GHz;stat.errorVARCHARprincipalS350_fluxHerschel SPIRE 350 micron fluxJyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalS350_fluxerrError in Herschel SPIRE 350 micron fluxJyphot.flux.density;em.mm.750-1500GHz;stat.errorVARCHARprincipalS500_fluxHerschel SPIRE 500 micron fluxJyphot.flux.density;em.mm.400-750GHzVARCHARprincipalS500_fluxerrError in Herschel SPIRE 500 micron fluxJyphot.flux.density;em.mm.400-750GHz;stat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.DistancesFramesv14This table provides redshifts in various reference frames,flow-corrected redshifts, and distance moduli for all GAMA IIobjects with redshifts.CATAIDUnique GAMA ID of objectmeta.id;meta.mainVARCHARindexedprincipalRAJ2000 coordinatedegpos.eq.raVARCHARprincipalDECJ2000 coordinatedegpos.eq.decVARCHARprincipalNQQuality of redshiftmeta.code.qual;src.redshiftVARCHARprincipalZ_HELIOHeliocentric redshiftsrc.redshiftVARCHARprincipalZ_LGLocal Group frame redshiftsrc.redshiftVARCHARprincipalZ_CMBCMB frame redshiftsrc.redshiftVARCHARprincipalZ_TONRYFlow-corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalZ_TONRY_HIGHRecomputed after adjusting z_helio by +180 km/ssrc.redshiftVARCHARprincipalZ_TONRY_LOWRecomputed after adjusting z_helio by -180 km/ssrc.redshiftVARCHARprincipalDM_70_30_70Distance modulus for 737 cosmologymagphot.mag.distModVARCHARprincipalDM_100_30_70Distance modulus for H0=100, om_m=0.30, om_L=0.70magphot.mag.distModVARCHARprincipalDM_70_25_75Distance modulus for H0=70, om_m=0.25, om_L=0.75magphot.mag.distModVARCHARprincipalDM_100_25_75Distance modulus for H0=100, om_m=0.25, om_L=0.75magphot.mag.distModVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.MagPhysv06This table provides physical stellar population and ISM parametersfor galaxies in the GAMA II equatorial survey regions, derived byrunning the SED-fitting code MAGPHYS on LambdarCatv01.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalZSpectroscopic redshiftsrc.redshiftVARCHARprincipalf_mu_SFH_best_fitBest fit fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile2_52.5th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile1616th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile50Median fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile8484th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_SFH_percentile97_597.5th percentile of fraction of tau_V^BC contributed by dust in the HII regionphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_best_fitBest fit fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile2_52.5th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile1616th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile50Median fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile8484th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalf_mu_IR_percentile97_597.5th percentile of fraction of L_sun accounted by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_best_fitBest fit fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile2_52.5th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile1616th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile50Median fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile8484th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmu_parameter_percentile97_597.5th percentile of fraction of tau_V contributed by dust in the ambient ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_best_fitBest fit total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile2_52.5th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile1616th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile50Median total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile8484th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_percentile97_597.5th percentile of total V-band optical depth of the dust seen by young stars in their birth cloudsphys.absorption.opticalDepth;em.opt.VVARCHARprincipalsSFR_0_1Gyr_best_fitBest fit specific star formation rateyr^-1phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile2_52.5th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile1616th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile50Median of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile8484th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalsSFR_0_1Gyr_percentile97_597.5th percentile of specific star formation ratedex(yr^-1)phys.SFRVARCHARprincipalmass_stellar_best_fitBest fit total mass of stars ever formed; integral of the star formation rateMsunphys.massVARCHARprincipalmass_stellar_percentile2_52.5th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile1616th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile50Median total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile8484th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalmass_stellar_percentile97_597.5th percentile of total mass of stars ever formed; integral of the star formation ratedex(Msun)phys.massVARCHARprincipalL_dust_best_fitBest fit total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)Lsunphys.luminosityVARCHARprincipalL_dust_percentile2_52.5th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile1616th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile50Median total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile8484th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalL_dust_percentile97_597.5th percentile of total stellar luminosity absorbed and re-radiated by dust (birth clouds + ambient ISM)dex(Lsun)phys.luminosityVARCHARprincipalT_C_ISM_best_fitBest fit equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile2_52.5th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile1616th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile50Median equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile8484th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_C_ISM_percentile97_597.5th percentile of equilibrium temperature of cold dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_best_fitBest fit equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile2_52.5th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile1616th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile50Median equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile8484th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalT_W_BC_percentile97_597.5th percentile of equilibrium temperature of warm dust in the ambient ISMKphys.temperatureVARCHARprincipalxi_C_tot_best_fitBest fit fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile2_52.5th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile1616th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile50Median fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile8484th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_C_tot_percentile97_597.5th percentile of fractional contribution by cold dust to the dust luminosity of the ambient ISMphys.luminosityVARCHARprincipalxi_PAH_tot_best_fitBest fit fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile2_52.5th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile1616th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile50Median fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile8484th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_PAH_tot_percentile97_597.5th percentile of fractional contribution by PAHs to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_best_fitBest fit fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile2_52.5th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile1616th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile50Median fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile8484th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_MIR_tot_percentile97_597.5th percentile of fractional contribution by the hot MIR continuum to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_best_fitBest fit fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile2_52.5th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile1616th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile50Median fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile8484th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipalxi_W_tot_percentile97_597.5th percentile of fractional contribution by warm dust to the dust luminosity of the stellar birth cloudsphys.luminosityVARCHARprincipaltau_V_ISM_best_fitBest fit total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile2_52.5th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile1616th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile50Median total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile8484th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipaltau_V_ISM_percentile97_597.5th percentile of total V-band optical depth of the dust seen through the ISMphys.absorption.opticalDepth;em.opt.VVARCHARprincipalmass_dust_best_fitBest fit total mass of dustMsunphys.massVARCHARprincipalmass_dust_percentile2_52.5th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile1616th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile50Median total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile8484th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalmass_dust_percentile97_597.5th percentile of total mass of dustdex(Msun)phys.massVARCHARprincipalSFR_0_1Gyr_best_fitBest fit star formation rateMsun/yrphys.SFRVARCHARprincipalSFR_0_1Gyr_percentile2_52.5th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile1616th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile50Median star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile8484th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalSFR_0_1Gyr_percentile97_597.5th percentile of star formation ratedex(Msun/yr)phys.SFRVARCHARprincipalmetalicity_Z_Zo_percentile2_52.5th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile1616th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile50Median metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile8484th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipalmetalicity_Z_Zo_percentile97_597.5th percentile of metallicity in solar unitsphys.abund.ZVARCHARprincipaltform_percentile2_52.5th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile1616th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile50Median age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile8484th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipaltform_percentile97_597.5th percentile of age of the oldest stars in the galaxydex(yr)time.ageVARCHARprincipalgamma_percentile2_52.5th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile1616th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile50Median star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile8484th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipalgamma_percentile97_597.5th percentile of star formation timescaleGyr^-1phys.SFR;time.scaleVARCHARprincipaltlastb_percentile2_52.5th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile1616th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile50Median time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile8484th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipaltlastb_percentile97_597.5th percentile of time since the last burst of star formation endeddex(yr)time.ageVARCHARprincipalagem_percentile2_52.5th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile1616th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile50Median mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile8484th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalagem_percentile97_597.5th percentile of mass-weighted agedex(yr)time.ageVARCHARprincipalager_percentile2_52.5th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile1616th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile50Median r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile8484th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalager_percentile97_597.5th percentile of r-band light-weighted agedex(yr)time.ageVARCHARprincipalsfr16_percentile2_52.5th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile1616th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile50Median star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile8484th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr16_percentile97_597.5th percentile of star-formation rate averaged over the last 10^6 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile2_52.5th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile1616th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile50Median star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile8484th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr17_percentile97_597.5th percentile of star-formation rate averaged over the last 10^7 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile2_52.5th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile1616th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile50Median star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile8484th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr18_percentile97_597.5th percentile of star-formation rate averaged over the last 10^8 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile2_52.5th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile1616th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile50Median star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile8484th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr19_percentile97_597.5th percentile of star-formation rate averaged over the last 10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile2_52.5th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile1616th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile50Median star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile8484th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalsfr29_percentile97_597.5th percentile of star-formation rate averaged over the last 2x10^9 yrdex(Msun/yr)phys.SFRVARCHARprincipalfb16_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile50Median fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb16_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^6 yrphys.massVARCHARprincipalfb17_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile50Median fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb17_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^7 yrphys.massVARCHARprincipalfb18_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile50Median fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb18_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^8 yrphys.massVARCHARprincipalfb19_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile1616th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile50Median fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile8484th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb19_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 10^9 yrphys.massVARCHARprincipalfb29_percentile2_52.5th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile1616th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile50Median fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile8484th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalfb29_percentile97_597.5th percentile of fraction of stellar mass formed in bursts over last 2x10^9 yrphys.massVARCHARprincipalURL_SEDURL of MAGPHYS output file containing the best-fit spectrummeta.ref.url;meta.fileVARCHARprincipalURL_FITURL of MAGPHYS output file containing individual parameter PDFsmeta.ref.url;meta.fileVARCHARprincipalURL_PNGURL of plot of the best-fit spectrum and input photometrymeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.MegaMorphCatv01This table provides the results of fitting both a single Sersiccomponent model as well as a two-component bulge-disk model to the2D surface brightness distributions of galaxies in the GAMA I G09survey region using the MegaMorph multi-band fitting method. In thismethod the ugriz (from SDSS) and YJHK (from UKIDSS-LAS) surfacebrightness distributions of a galaxy are fit simultaneously whileimposing some constraints on how some of the model parameters areallowed to vary with wavelength.CATAIDGAMA object IDmeta.idVARCHARprincipalRAJ2000 coordinate of the GAMA objectdegpos.eq.raVARCHARprincipalDECJ2000 coordinate of the GAMA objectdegpos.eq.decVARCHARprincipalALPHA_J2000J2000 coordinate of the MegaMorph fitdegpos.eq.raVARCHARprincipalDELTA_J2000J2000 coordinate of the MegaMorph fitdegpos.eq.decVARCHARprincipalTHETA_IMAGEPosition angle on the image, counterclockwise, 0 is the NAXIS1 image axisdegpos.posAngVARCHARprincipalELLIPTICITYAxial ratio of galaxy, b/asrc.ellipticityVARCHARprincipalBACKGROUNDLocal backgroundcountsphot.fluxVARCHARprincipalFLUX_BESTFlux estimatecountsphot.flux;em.optVARCHARprincipalFLUXERR_BESTFlux errorcountsphot.flux;stat.errorVARCHARprincipalMAG_BESTMagnitude estimatemagphot.magVARCHARprincipalMAGERR_BESTMagnitude estimate errormagphot.mag;stat.errorVARCHARprincipalFLUX_RADIUSHalflight radiusarcsecphys.angSizeVARCHARprincipalISOAREA_IMAGEObject area; number of pixels above analysis thresholdpixelphys.areaVARCHARprincipalFWHM_IMAGEImage FWHMpixelphys.size.diameter;instr.det.psfVARCHARprincipalFLAGSSExtractor flagsmeta.codeVARCHARprincipalCLASS_STARStar/galaxy classifiersrc.class.starGalaxyVARCHARprincipalRE_GALFIT_CHEB_0Chebyshev coefficients of effective radiusstat.fit.param;meta.modelledVARCHARprincipalRE_GALFIT_CHEB_1Chebyshev coefficients of effective radiusstat.fit.param;meta.modelledVARCHARprincipalRE_GALFIT_CHEB_2Chebyshev coefficients of effective radiusstat.fit.param;meta.modelledVARCHARprincipalREERR_GALFIT_CHEB_0Error on Chebyshev coefficients of effective radiusstat.fit.param;stat.error;meta.modelledVARCHARprincipalREERR_GALFIT_CHEB_1Error on Chebyshev coefficients of effective radiusstat.fit.param;stat.error;meta.modelledVARCHARprincipalREERR_GALFIT_CHEB_2Error on Chebyshev coefficients of effective radiusstat.fit.param;stat.error;meta.modelledVARCHARprincipalN_GALFIT_CHEB_0Chebyshev coefficients of Sersic indexstat.fit.param;meta.modelledVARCHARprincipalN_GALFIT_CHEB_1Chebyshev coefficients of Sersic indexstat.fit.param;meta.modelledVARCHARprincipalN_GALFIT_CHEB_2Chebyshev coefficients of Sersic indexstat.fit.param;meta.modelledVARCHARprincipalNERR_GALFIT_CHEB_0Error on Chebyshev coefficients of Sersic indexstat.fit.param;stat.error;meta.modelledVARCHARprincipalNERR_GALFIT_CHEB_1Error on Chebyshev coefficients of Sersic indexstat.fit.param;stat.error;meta.modelledVARCHARprincipalNERR_GALFIT_CHEB_2Error on Chebyshev coefficients of Sersic indexstat.fit.param;stat.error;meta.modelledVARCHARprincipalMAG_GALFIT_BAND_uApparent magnitudemagphot.mag;meta.modelled;em.opt.UVARCHARprincipalMAG_GALFIT_BAND_gApparent magnitudemagphot.mag;meta.modelled;em.opt.GVARCHARprincipalMAG_GALFIT_BAND_rApparent magnitudemagphot.mag;meta.modelled;em.opt.RVARCHARprincipalMAG_GALFIT_BAND_iApparent magnitudemagphot.mag;meta.modelled;em.opt.IVARCHARprincipalMAG_GALFIT_BAND_zApparent magnitudemagphot.mag;meta.modelled;em.opt.ZVARCHARprincipalMAG_GALFIT_BAND_YApparent magnitudemagphot.mag;meta.modelled;em.IR.YVARCHARprincipalMAG_GALFIT_BAND_JApparent magnitudemagphot.mag;meta.modelled;em.IR.JVARCHARprincipalMAG_GALFIT_BAND_HApparent magnitudemagphot.mag;meta.modelled;em.IR.HVARCHARprincipalMAG_GALFIT_BAND_KApparent magnitudemagphot.mag;meta.modelled;em.IR.KVARCHARprincipalMAGERR_GALFIT_BAND_uError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.UVARCHARprincipalMAGERR_GALFIT_BAND_gError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.GVARCHARprincipalMAGERR_GALFIT_BAND_rError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.RVARCHARprincipalMAGERR_GALFIT_BAND_iError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.IVARCHARprincipalMAGERR_GALFIT_BAND_zError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.opt.ZVARCHARprincipalMAGERR_GALFIT_BAND_YError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalMAGERR_GALFIT_BAND_JError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalMAGERR_GALFIT_BAND_HError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalMAGERR_GALFIT_BAND_KError on apparent magnitudemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalRE_GALFIT_BAND_uEffective radiusarcsecphys.angSize;meta.modelled;em.opt.UVARCHARprincipalRE_GALFIT_BAND_gEffective radiusarcsecphys.angSize;meta.modelled;em.opt.GVARCHARprincipalRE_GALFIT_BAND_rEffective radiusarcsecphys.angSize;meta.modelled;em.opt.RVARCHARprincipalRE_GALFIT_BAND_iEffective radiusarcsecphys.angSize;meta.modelled;em.opt.IVARCHARprincipalRE_GALFIT_BAND_zEffective radiusarcsecphys.angSize;meta.modelled;em.opt.ZVARCHARprincipalRE_GALFIT_BAND_YEffective radiusarcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalRE_GALFIT_BAND_JEffective radiusarcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalRE_GALFIT_BAND_HEffective radiusarcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalRE_GALFIT_BAND_KEffective radiusarcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalREERR_GALFIT_BAND_uError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.UVARCHARprincipalREERR_GALFIT_BAND_gError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.GVARCHARprincipalREERR_GALFIT_BAND_rError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.RVARCHARprincipalREERR_GALFIT_BAND_iError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.IVARCHARprincipalREERR_GALFIT_BAND_zError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.opt.ZVARCHARprincipalREERR_GALFIT_BAND_YError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalREERR_GALFIT_BAND_JError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalREERR_GALFIT_BAND_HError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalREERR_GALFIT_BAND_KError on effective radiusarcsecphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalN_GALFIT_BAND_uSersic indexphys.angSize;meta.modelled;em.opt.UVARCHARprincipalN_GALFIT_BAND_gSersic indexphys.angSize;meta.modelled;em.opt.GVARCHARprincipalN_GALFIT_BAND_rSersic indexphys.angSize;meta.modelled;em.opt.RVARCHARprincipalN_GALFIT_BAND_iSersic indexphys.angSize;meta.modelled;em.opt.IVARCHARprincipalN_GALFIT_BAND_zSersic indexphys.angSize;meta.modelled;em.opt.ZVARCHARprincipalN_GALFIT_BAND_YSersic indexphys.angSize;meta.modelled;em.IR.YVARCHARprincipalN_GALFIT_BAND_JSersic indexphys.angSize;meta.modelled;em.IR.JVARCHARprincipalN_GALFIT_BAND_HSersic indexphys.angSize;meta.modelled;em.IR.HVARCHARprincipalN_GALFIT_BAND_KSersic indexphys.angSize;meta.modelled;em.IR.KVARCHARprincipalNERR_GALFIT_BAND_uError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.UVARCHARprincipalNERR_GALFIT_BAND_gError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.GVARCHARprincipalNERR_GALFIT_BAND_rError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.RVARCHARprincipalNERR_GALFIT_BAND_iError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.IVARCHARprincipalNERR_GALFIT_BAND_zError on Sersic indexphys.angSize;stat.error;meta.modelled;em.opt.ZVARCHARprincipalNERR_GALFIT_BAND_YError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalNERR_GALFIT_BAND_JError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalNERR_GALFIT_BAND_HError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalNERR_GALFIT_BAND_KError on Sersic indexphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalQ_GALFIT_BANDAxial ratiosrc.ellipticity;meta.modelledVARCHARprincipalQERR_GALFIT_BANDError on axial ratiosrc.ellipticity;stat.error;meta.modelledVARCHARprincipalPA_GALFIT_BANDPosition angle on sky, counterclockwise, 0 is Northdegpos.posAng;meta.modelledVARCHARprincipalPAERR_GALFIT_BANDError on position angle on skydegpos.posAng;stat.error;meta.modelledVARCHARprincipalSKY_GALFIT_BAND_uSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.UVARCHARprincipalSKY_GALFIT_BAND_gSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.GVARCHARprincipalSKY_GALFIT_BAND_rSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.RVARCHARprincipalSKY_GALFIT_BAND_iSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.IVARCHARprincipalSKY_GALFIT_BAND_zSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.opt.ZVARCHARprincipalSKY_GALFIT_BAND_YSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.YVARCHARprincipalSKY_GALFIT_BAND_JSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.JVARCHARprincipalSKY_GALFIT_BAND_HSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.HVARCHARprincipalSKY_GALFIT_BAND_KSky level (determined by GALAPAGOS and held fixed)countsphot.flux;em.IR.KVARCHARprincipalMAG_GALFIT_BAND_D_uApparent magnitude of discmagphot.mag;meta.modelled;em.opt.UVARCHARprincipalMAG_GALFIT_BAND_D_gApparent magnitude of discmagphot.mag;meta.modelled;em.opt.GVARCHARprincipalMAG_GALFIT_BAND_D_rApparent magnitude of discmagphot.mag;meta.modelled;em.opt.RVARCHARprincipalMAG_GALFIT_BAND_D_iApparent magnitude of discmagphot.mag;meta.modelled;em.opt.IVARCHARprincipalMAG_GALFIT_BAND_D_zApparent magnitude of discmagphot.mag;meta.modelled;em.opt.ZVARCHARprincipalMAG_GALFIT_BAND_D_YApparent magnitude of discmagphot.mag;meta.modelled;em.IR.YVARCHARprincipalMAG_GALFIT_BAND_D_JApparent magnitude of discmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalMAG_GALFIT_BAND_D_HApparent magnitude of discmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalMAG_GALFIT_BAND_D_KApparent magnitude of discmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalMAGERR_GALFIT_BAND_D_uError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.UVARCHARprincipalMAGERR_GALFIT_BAND_D_gError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.GVARCHARprincipalMAGERR_GALFIT_BAND_D_rError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.RVARCHARprincipalMAGERR_GALFIT_BAND_D_iError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.IVARCHARprincipalMAGERR_GALFIT_BAND_D_zError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.opt.ZVARCHARprincipalMAGERR_GALFIT_BAND_D_YError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalMAGERR_GALFIT_BAND_D_JError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalMAGERR_GALFIT_BAND_D_HError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalMAGERR_GALFIT_BAND_D_KError on apparent magnitude of discmagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalMAG_GALFIT_BAND_B_uApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.UVARCHARprincipalMAG_GALFIT_BAND_B_gApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.GVARCHARprincipalMAG_GALFIT_BAND_B_rApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.RVARCHARprincipalMAG_GALFIT_BAND_B_iApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.IVARCHARprincipalMAG_GALFIT_BAND_B_zApparent magnitude of bulgemagphot.mag;meta.modelled;em.opt.ZVARCHARprincipalMAG_GALFIT_BAND_B_YApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.YVARCHARprincipalMAG_GALFIT_BAND_B_JApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.JVARCHARprincipalMAG_GALFIT_BAND_B_HApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.HVARCHARprincipalMAG_GALFIT_BAND_B_KApparent magnitude of bulgemagphot.mag;meta.modelled;em.IR.KVARCHARprincipalMAGERR_GALFIT_BAND_B_uError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.UVARCHARprincipalMAGERR_GALFIT_BAND_B_gError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.GVARCHARprincipalMAGERR_GALFIT_BAND_B_rError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.RVARCHARprincipalMAGERR_GALFIT_BAND_B_iError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.IVARCHARprincipalMAGERR_GALFIT_BAND_B_zError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.opt.ZVARCHARprincipalMAGERR_GALFIT_BAND_B_YError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalMAGERR_GALFIT_BAND_B_JError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalMAGERR_GALFIT_BAND_B_HError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalMAGERR_GALFIT_BAND_B_KError on apparent magnitude of bulgemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalRE_GALFIT_BAND_DEffective radius of discarcsecphys.angSize;meta.modelledVARCHARprincipalREERR_GALFIT_BAND_DError on effective radius of discarcsecphys.angSize;stat.error;meta.modelledVARCHARprincipalRE_GALFIT_BAND_BEffective radius of bulgearcsecphys.angSize;meta.modelledVARCHARprincipalREERR_GALFIT_BAND_BError on effective radius of bulgearcsecphys.angSize;stat.error;meta.modelledVARCHARprincipalN_GALFIT_BAND_DSersic index of discphys.angSize;meta.modelledVARCHARprincipalN_GALFIT_BAND_BSersic index of bulgephys.angSize;meta.modelledVARCHARprincipalNERR_GALFIT_BAND_BError on Sersic index of bulgephys.angSize;stat.error;meta.modelledVARCHARprincipalQ_GALFIT_BAND_DAxial ratio of discsrc.ellipticity;meta.modelledVARCHARprincipalQERR_GALFIT_BAND_DError on axial ratio of discsrc.ellipticity;stat.error;meta.modelledVARCHARprincipalQ_GALFIT_BAND_BAxial ratio of bulgesrc.ellipticity;meta.modelledVARCHARprincipalQERR_GALFIT_BAND_BError on axial ratio of bulgesrc.ellipticity;stat.error;meta.modelledVARCHARprincipalPA_GALFIT_BAND_DPosition angle of disc on sky, counterclockwise, 0 is Northdegpos.posAng;meta.modelledVARCHARprincipalPAERR_GALFIT_BAND_DError on position angle of disc on skydegpos.posAng;stat.error;meta.modelledVARCHARprincipalPA_GALFIT_BAND_BPosition angle of bulge on sky, counterclockwise, 0 is Northdegpos.posAng;meta.modelledVARCHARprincipalPAERR_GALFIT_BAND_BError on position angle of bulge on skydegpos.posAng;stat.error;meta.modelledVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.21BandPhotomv03This table combines available flux measurements from theGalexPhotometry, ApMatchedPhotom and WISEPhotometry DMUs withbespoke flux measurements in the Herschel PACS and SPIRE bands byKate Rowlands and Nathan Bourne for all objects in the GAMA IIequatorial survey regions. The data are presented in the formrequired by MAGPHYS.W4_fluxerrError in WISE band 4 fluxJyphot.mag;em.IR.15-30um;stat.errorVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalZHeliocentric redshift of objectsrc.redshiftVARCHARprincipalFUV_fluxExtinction corrected GALEX FUV fluxJyphot.mag;em.UV.100-200nmVARCHARprincipalFUV_fluxerrError in extinction corrected GALEX FUV fluxJyphot.mag;em.UV.100-200nm;stat.errorVARCHARprincipalNUV_fluxExinction corrected GALEX NUV fluxJyphot.mag;em.UV.200-300nmVARCHARprincipalNUV_fluxerrError in extinction corrected GALEX NUV fluxJyphot.mag;em.UV.200-300nm;stat.errorVARCHARprincipalu_fluxExtinction corrected SDSS u band fluxJyphot.mag;em.opt.UVARCHARprincipalu_fluxerrError in extinction corrected SDSS u band fluxJyphot.mag;em.opt.U;stat.errorVARCHARprincipalg_fluxExtinction corrected SDSS g band fluxJyphot.mag;em.opt.GVARCHARprincipalg_fluxerrError in extinction corrected SDSS g band fluxJyphot.mag;em.opt.G;stat.errorVARCHARprincipalr_fluxExtinction corrected SDSS r band fluxJyphot.mag;em.opt.RVARCHARprincipalr_fluxerrError in extinction corrected SDSS r band fluxJyphot.mag;em.opt.R;stat.errorVARCHARprincipali_fluxExtinction corrected SDSS i band fluxJyphot.mag;em.opt.IVARCHARprincipali_fluxerrError in extinction corrected SDSS i band fluxJyphot.mag;em.opt.I;stat.errorVARCHARprincipalz_fluxExtinction corrected SDSS z band fluxJyphot.mag;em.opt.ZVARCHARprincipalz_fluxerrError in extinction corrected SDSS z band fluxJyphot.mag;em.opt.Z;stat.errorVARCHARprincipalX_fluxExtinction correctd VISTA Z band fluxJyphot.mag;em.opt.ZVARCHARprincipalX_fluxerrError in extinction corrected VISTA Z band fluxJyphot.mag;em.opt.Z;stat.errorVARCHARprincipalY_fluxExtinction corrected VISTA Y band fluxJyphot.mag;em.IR.YVARCHARprincipalY_fluxerrError in extinction corrected VISTA Y band fluxJyphot.mag;em.IR.Y;stat.errorVARCHARprincipalJ_fluxExtinction corrected VISTA J band fluxJyphot.mag;em.IR.JVARCHARprincipalJ_fluxerrError in extinction corrected VISTA J band fluxJyphot.mag;em.IR.J;stat.errorVARCHARprincipalH_fluxExtinction corrected VISTA H band fluxJyphot.mag;em.IR.HVARCHARprincipalH_fluxerrError in extinction corrected VISTA H band fluxJyphot.mag;em.IR.H;stat.errorVARCHARprincipalK_fluxExtinction corrected VISTA Ks band fluxJyphot.mag;em.IR.KVARCHARprincipalK_fluxerrError in extinction corrected VISTA Ks band fluxJyphot.mag;em.IR.K;stat.errorVARCHARprincipalW1_fluxWISE band 1 fluxJyphot.mag;em.IR.3-4umVARCHARprincipalW1_fluxerrError in WISE band 1 fluxJyphot.mag;em.IR.3-4um;stat.errorVARCHARprincipalW2_fluxWISE band 2 fluxJyphot.mag;em.IR.4-8umVARCHARprincipalW2_fluxerrError in WISE band 2 fluxJyphot.mag;em.IR.4-8um;stat.errorVARCHARprincipalW3_fluxWISE band 3 fluxJyphot.mag;em.IR.8-15umVARCHARprincipalW3_fluxerrError in WISE band 3 fluxJyphot.mag;em.IR.8-15um;stat.errorVARCHARprincipalW4_fluxWISE band 4 fluxJyphot.mag;em.IR.15-30umVARCHARprincipal100_fluxHerschel PACS 100 micron fluxJyphot.mag;em.mm.1500-3000GHzVARCHARprincipal100_fluxerrError in Herschel PACS 100 micron fluxJyphot.mag;em.mm.1500-3000GHz;stat.errorVARCHARprincipal160_fluxHerschel PACS 160 micron fluxJyphot.mag;em.mm.1500-3000GHzVARCHARprincipal160_fluxerrError in Herschel PACS 160 micron fluxJyphot.mag;em.mm.1500-3000GHz;stat.errorVARCHARprincipal250_fluxHerschel SPIRE 250 micron fluxJyphot.mag;em.mm.750-1500GHzVARCHARprincipal250_fluxerrError in Herschel SPIRE 250 micron fluxJyphot.mag;em.mm.750-1500GHz;stat.errorVARCHARprincipal350_fluxHerschel SPIRE 350 micron fluxJyphot.mag;em.mm.750-1500GHzVARCHARprincipal350_fluxerrError in Herschel SPIRE 350 micron fluxJyphot.mag;em.mm.750-1500GHz;stat.errorVARCHARprincipal450_fluxHerschel SPIRE 450 micron fluxJyphot.mag;em.mm.400-750GHzVARCHARprincipal450_fluxerrError in Herschel SPIRE 450 micron fluxJyphot.mag;em.mm.400-750GHz;stat.errorVARCHARprincipalURL_PNGURL of SED summary plotmeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.RadialDensityv01This table provides the radial density variation of galaxies in theGAMA II equatorial survey regions.ZBinIDID of the redshift binmeta.id;meta.mainVARCHARindexedprincipalZRedshift of bin centresrc.redshiftVARCHARprincipaldelta_G09Multiplicative overdensity in G09src.densityVARCHARprincipaldelta_G12Multiplicative overdensity in G12src.densityVARCHARprincipaldelta_G15Multiplicative overdensity in G15src.densityVARCHARprincipaldelta_AVMultiplicative overdensity averaged over all equatorial regionssrc.densityVARCHARprincipalgama_dr4.Randomsv02This table provides a set of randomly distributed points with thesame selection function as the galaxies in the GAMA II equatorialsurvey regions. Each point is a clone of a real GAMA galaxy,identified by its CATAID, which can be used to assign properties tothe random points. The redshifts of randoms are restricted to aGaussian window around the redshift of the real galaxy being cloned.RANDIDUnique random IDmeta.id;meta.mainVARCHARindexedprincipalCATAIDGAMA galaxy IDmeta.idVARCHARprincipalRARight Ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalZRedshiftsrc.redshiftVARCHARprincipalR_PETRO_ABSAbsolute r-band Petrosian magnitudemagphys.magAbs;em.opt.RVARCHARprincipalR_PETROApparent r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalRAND_NUMA random number in the range (0,1] to select subsetsstat.valueVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.RandomsUnwindowedv02This table provides a set of randomly distributed points with thesame selection function as the galaxies in the GAMA II equatorialsurvey regions. Each point is a clone of a real GAMA galaxy,identified by its CATAID, which can be used to assign properties tothe random points. The redshifts of randoms are NOT restricted to aGaussian window around the redshift of the real galaxy being cloned.RANDIDUnique random IDmeta.id;meta.mainVARCHARindexedprincipalCATAIDGAMA galaxy IDmeta.idVARCHARprincipalRARight Ascensiondegpos.eq.raVARCHARprincipalDECDeclinationdegpos.eq.decVARCHARprincipalZRedshiftsrc.redshiftVARCHARprincipalR_PETRO_ABSAbsolute r-band Petrosian magnitudemagphys.magAbs;em.opt.RVARCHARprincipalR_PETROApparent r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalRAND_NUMA random number in the range (0,1] to select subsetsstat.valueVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.SersicCatVIKINGv09This table provides the results of a single-Sersic-component fit tothe 2D surface brightness distribution of every object in theGAMA II equatorial survey regions in the VIKING ZYJHK bands.CATAIDGAMA Object IDmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalCENFLUX_ZCentral pixel flux value prior to background estimationcountsphot.count;em.IR.ZVARCHARprincipalBACKFLUX_ZSEx subtracted background at object positioncountsphot.count;em.IR.ZVARCHARprincipalPSFNUM_ZPSFEx number of stars usedmeta.number;em.IR.ZVARCHARprincipalPSFCHI2_ZPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.ZVARCHARprincipalPSFFWHM_ZPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.ZVARCHARprincipalNSEC_ZSEx number of secondary components detectedmeta.number;em.IR.ZVARCHARprincipalGALXCEN_ZGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.ZVARCHARprincipalGALYCEN_ZGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.ZVARCHARprincipalGALMAG_ZGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.ZVARCHARprincipalGALRE_ZGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.ZVARCHARprincipalGALINDEX_ZGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.ZVARCHARprincipalGALELLIP_ZGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.ZVARCHARprincipalGALPA_ZGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.ZVARCHARprincipalGALXCENERR_ZGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALYCENERR_ZGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALMAGERR_ZGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALREERR_ZGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALINDEXERR_ZGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALELLIPERR_ZGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALPAERR_ZGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.ZVARCHARprincipalGALRA_ZGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.ZVARCHARprincipalGALDEC_ZGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.ZVARCHARprincipalGALMAG10RE_ZGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.ZVARCHARprincipalGALMU0_ZGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.ZVARCHARprincipalGALMUE_ZGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.ZVARCHARprincipalGALMUEAVG_ZGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.ZVARCHARprincipalGALR90_ZGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.ZVARCHARprincipalGALCHI2FULL_ZGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.ZVARCHARprincipalGALNDOF_ZGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.ZVARCHARprincipalGALCHI2_ZGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.ZVARCHARprincipalGALPLAN_ZSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.ZVARCHARprincipalPRICHI2FULL_ZPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalPRINFP_ZPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalPRINDOF_ZPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalPRICHI2_ZPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.ZVARCHARprincipalCENFLUX_YCentral pixel flux value prior to background estimationcountsphot.count;em.IR.YVARCHARprincipalBACKFLUX_YSEx subtracted background at object positioncountsphot.count;em.IR.YVARCHARprincipalPSFNUM_YPSFEx number of stars usedmeta.number;em.IR.YVARCHARprincipalPSFCHI2_YPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.YVARCHARprincipalPSFFWHM_YPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.YVARCHARprincipalNSEC_YSEx number of secondary components detectedmeta.number;em.IR.YVARCHARprincipalGALXCEN_YGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.YVARCHARprincipalGALYCEN_YGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.YVARCHARprincipalGALMAG_YGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALRE_YGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALINDEX_YGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.YVARCHARprincipalGALELLIP_YGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.YVARCHARprincipalGALPA_YGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.YVARCHARprincipalGALXCENERR_YGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALYCENERR_YGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALMAGERR_YGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALREERR_YGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALINDEXERR_YGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALELLIPERR_YGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALPAERR_YGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALRA_YGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.YVARCHARprincipalGALDEC_YGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.YVARCHARprincipalGALMAG10RE_YGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALMU0_YGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUE_YGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUEAVG_YGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALR90_YGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALCHI2FULL_YGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALNDOF_YGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALCHI2_YGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALPLAN_YSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2FULL_YPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINFP_YPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINDOF_YPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2_YPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalCENFLUX_JCentral pixel flux value prior to background estimationcountsphot.count;em.IR.JVARCHARprincipalBACKFLUX_JSEx subtracted background at object positioncountsphot.count;em.IR.JVARCHARprincipalPSFNUM_JPSFEx number of stars usedmeta.number;em.IR.JVARCHARprincipalPSFCHI2_JPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.JVARCHARprincipalPSFFWHM_JPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.JVARCHARprincipalNSEC_JSEx number of secondary components detectedmeta.number;em.IR.JVARCHARprincipalGALXCEN_JGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.JVARCHARprincipalGALYCEN_JGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.JVARCHARprincipalGALMAG_JGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALRE_JGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALINDEX_JGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.JVARCHARprincipalGALELLIP_JGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.JVARCHARprincipalGALPA_JGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.JVARCHARprincipalGALXCENERR_JGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALYCENERR_JGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALMAGERR_JGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALREERR_JGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALINDEXERR_JGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALELLIPERR_JGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALPAERR_JGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALRA_JGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.JVARCHARprincipalGALDEC_JGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.JVARCHARprincipalGALMAG10RE_JGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALMU0_JGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUE_JGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUEAVG_JGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALR90_JGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALCHI2FULL_JGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALNDOF_JGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALCHI2_JGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALPLAN_JSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2FULL_JPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINFP_JPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINDOF_JPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2_JPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalCENFLUX_HCentral pixel flux value prior to background estimationcountsphot.count;em.IR.HVARCHARprincipalBACKFLUX_HSEx subtracted background at object positioncountsphot.count;em.IR.HVARCHARprincipalPSFNUM_HPSFEx number of stars usedmeta.number;em.IR.HVARCHARprincipalPSFCHI2_HPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.HVARCHARprincipalPSFFWHM_HPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.HVARCHARprincipalNSEC_HSEx number of secondary components detectedmeta.number;em.IR.HVARCHARprincipalGALXCEN_HGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.HVARCHARprincipalGALYCEN_HGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.HVARCHARprincipalGALMAG_HGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALRE_HGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALINDEX_HGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.HVARCHARprincipalGALELLIP_HGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.HVARCHARprincipalGALPA_HGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.HVARCHARprincipalGALXCENERR_HGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALYCENERR_HGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALMAGERR_HGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALREERR_HGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALINDEXERR_HGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALELLIPERR_HGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALPAERR_HGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALRA_HGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.HVARCHARprincipalGALDEC_HGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.HVARCHARprincipalGALMAG10RE_HGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALMU0_HGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUE_HGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUEAVG_HGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALR90_HGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALCHI2FULL_HGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALNDOF_HGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALCHI2_HGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALPLAN_HSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2FULL_HPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINFP_HPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINDOF_HPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2_HPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalCENFLUX_KCentral pixel flux value prior to background estimationcountsphot.count;em.IR.KVARCHARprincipalBACKFLUX_KSEx subtracted background at object positioncountsphot.count;em.IR.KVARCHARprincipalPSFNUM_KPSFEx number of stars usedmeta.number;em.IR.KVARCHARprincipalPSFCHI2_KPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.KVARCHARprincipalPSFFWHM_KPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.KVARCHARprincipalNSEC_KSEx number of secondary components detectedmeta.number;em.IR.KVARCHARprincipalGALXCEN_KGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.KVARCHARprincipalGALYCEN_KGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.KVARCHARprincipalGALMAG_KGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALRE_KGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALINDEX_KGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.KVARCHARprincipalGALELLIP_KGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.KVARCHARprincipalGALPA_KGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.KVARCHARprincipalGALXCENERR_KGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALYCENERR_KGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALMAGERR_KGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALREERR_KGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALINDEXERR_KGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALELLIPERR_KGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALPAERR_KGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALRA_KGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.KVARCHARprincipalGALDEC_KGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.KVARCHARprincipalGALMAG10RE_KGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALMU0_KGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUE_KGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUEAVG_KGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALR90_KGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALCHI2FULL_KGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALNDOF_KGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALCHI2_KGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALPLAN_KSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2FULL_KPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINFP_KPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINDOF_KPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2_KPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.SersicCatUKIDSSv09This table provides the results of a single-Sersic-component fit tothe 2D surface brightness distribution of every object in theGAMA II equatorial survey regions in the UKIDSS-LAS YJHK bands.PSFCHI2_YPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.YVARCHARprincipalCATAIDGAMA Object IDmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalCENFLUX_YCentral pixel flux value prior to background estimationcountsphot.count;em.IR.YVARCHARprincipalBACKFLUX_YSEx subtracted background at object positioncountsphot.count;em.IR.YVARCHARprincipalPSFNUM_YPSFEx number of stars usedmeta.number;em.IR.YVARCHARprincipalPSFFWHM_YPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.YVARCHARprincipalNSEC_YSEx number of secondary components detectedmeta.number;em.IR.YVARCHARprincipalGALXCEN_YGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.YVARCHARprincipalGALYCEN_YGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.YVARCHARprincipalGALMAG_YGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALRE_YGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALINDEX_YGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.YVARCHARprincipalGALELLIP_YGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.YVARCHARprincipalGALPA_YGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.YVARCHARprincipalGALXCENERR_YGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALYCENERR_YGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALMAGERR_YGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALREERR_YGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALINDEXERR_YGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALELLIPERR_YGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALPAERR_YGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.YVARCHARprincipalGALRA_YGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.YVARCHARprincipalGALDEC_YGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.YVARCHARprincipalGALMAG10RE_YGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.YVARCHARprincipalGALMU0_YGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUE_YGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALMUEAVG_YGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.YVARCHARprincipalGALR90_YGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.YVARCHARprincipalGALCHI2FULL_YGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALNDOF_YGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALCHI2_YGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.YVARCHARprincipalGALPLAN_YSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2FULL_YPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINFP_YPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRINDOF_YPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalPRICHI2_YPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.YVARCHARprincipalCENFLUX_JCentral pixel flux value prior to background estimationcountsphot.count;em.IR.JVARCHARprincipalBACKFLUX_JSEx subtracted background at object positioncountsphot.count;em.IR.JVARCHARprincipalPSFNUM_JPSFEx number of stars usedmeta.number;em.IR.JVARCHARprincipalPSFCHI2_JPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.JVARCHARprincipalPSFFWHM_JPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.JVARCHARprincipalNSEC_JSEx number of secondary components detectedmeta.number;em.IR.JVARCHARprincipalGALXCEN_JGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.JVARCHARprincipalGALYCEN_JGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.JVARCHARprincipalGALMAG_JGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALRE_JGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALINDEX_JGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.JVARCHARprincipalGALELLIP_JGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.JVARCHARprincipalGALPA_JGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.JVARCHARprincipalGALXCENERR_JGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALYCENERR_JGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALMAGERR_JGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALREERR_JGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALINDEXERR_JGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALELLIPERR_JGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALPAERR_JGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.JVARCHARprincipalGALRA_JGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.JVARCHARprincipalGALDEC_JGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.JVARCHARprincipalGALMAG10RE_JGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.JVARCHARprincipalGALMU0_JGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUE_JGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALMUEAVG_JGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.JVARCHARprincipalGALR90_JGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.JVARCHARprincipalGALCHI2FULL_JGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALNDOF_JGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALCHI2_JGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.JVARCHARprincipalGALPLAN_JSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2FULL_JPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINFP_JPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRINDOF_JPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalPRICHI2_JPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.JVARCHARprincipalCENFLUX_HCentral pixel flux value prior to background estimationcountsphot.count;em.IR.HVARCHARprincipalBACKFLUX_HSEx subtracted background at object positioncountsphot.count;em.IR.HVARCHARprincipalPSFNUM_HPSFEx number of stars usedmeta.number;em.IR.HVARCHARprincipalPSFCHI2_HPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.HVARCHARprincipalPSFFWHM_HPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.HVARCHARprincipalNSEC_HSEx number of secondary components detectedmeta.number;em.IR.HVARCHARprincipalGALXCEN_HGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.HVARCHARprincipalGALYCEN_HGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.HVARCHARprincipalGALMAG_HGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALRE_HGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALINDEX_HGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.HVARCHARprincipalGALELLIP_HGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.HVARCHARprincipalGALPA_HGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.HVARCHARprincipalGALXCENERR_HGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALYCENERR_HGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALMAGERR_HGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALREERR_HGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALINDEXERR_HGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALELLIPERR_HGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALPAERR_HGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.HVARCHARprincipalGALRA_HGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.HVARCHARprincipalGALDEC_HGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.HVARCHARprincipalGALMAG10RE_HGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.HVARCHARprincipalGALMU0_HGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUE_HGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALMUEAVG_HGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.HVARCHARprincipalGALR90_HGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.HVARCHARprincipalGALCHI2FULL_HGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALNDOF_HGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALCHI2_HGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.HVARCHARprincipalGALPLAN_HSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2FULL_HPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINFP_HPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRINDOF_HPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalPRICHI2_HPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.HVARCHARprincipalCENFLUX_KCentral pixel flux value prior to background estimationcountsphot.count;em.IR.KVARCHARprincipalBACKFLUX_KSEx subtracted background at object positioncountsphot.count;em.IR.KVARCHARprincipalPSFNUM_KPSFEx number of stars usedmeta.number;em.IR.KVARCHARprincipalPSFCHI2_KPSFEx PSF reduced Chi^2stat.fit.goodness;em.IR.KVARCHARprincipalPSFFWHM_KPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.IR.KVARCHARprincipalNSEC_KSEx number of secondary components detectedmeta.number;em.IR.KVARCHARprincipalGALXCEN_KGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.IR.KVARCHARprincipalGALYCEN_KGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.IR.KVARCHARprincipalGALMAG_KGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALRE_KGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALINDEX_KGALFIT Sersic indexstat.fit.param;meta.modelled;em.IR.KVARCHARprincipalGALELLIP_KGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.IR.KVARCHARprincipalGALPA_KGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.IR.KVARCHARprincipalGALXCENERR_KGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALYCENERR_KGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALMAGERR_KGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALREERR_KGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALINDEXERR_KGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALELLIPERR_KGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALPAERR_KGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.IR.KVARCHARprincipalGALRA_KGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.IR.KVARCHARprincipalGALDEC_KGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.IR.KVARCHARprincipalGALMAG10RE_KGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.IR.KVARCHARprincipalGALMU0_KGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUE_KGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALMUEAVG_KGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.IR.KVARCHARprincipalGALR90_KGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.IR.KVARCHARprincipalGALCHI2FULL_KGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALNDOF_KGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALCHI2_KGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.IR.KVARCHARprincipalGALPLAN_KSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2FULL_KPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINFP_KPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRINDOF_KPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.IR.KVARCHARprincipalPRICHI2_KPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.IR.KVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.SersicCatSDSSv09This table provides the results of a single-Sersic-component fit tothe 2D surface brightness distribution of every object in theGAMA II equatorial survey regions in the SDSS ugriz bands.CATAIDGAMA Object IDmeta.idVARCHARprincipalRARight Ascension (J2000)degpos.eq.raVARCHARprincipalDECDeclination (J2000)degpos.eq.decVARCHARprincipalR_PETROExtinction-corrected SDSS DR7 Petrosian magmagphot.mag;em.opt.RVARCHARprincipalSURVEY_OLDCLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalSURVEY_CLASSUseful for selecting samples, see notesmeta.code.classVARCHARprincipalCENFLUX_uCentral pixel flux value prior to background estimationcountsphot.count;em.opt.uVARCHARprincipalBACKFLUX_uSEx subtracted background at object positioncountsphot.count;em.opt.uVARCHARprincipalPSFNUM_uPSFEx number of stars usedmeta.number;em.opt.uVARCHARprincipalPSFCHI2_uPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.uVARCHARprincipalPSFFWHM_uPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.uVARCHARprincipalNSEC_uSEx number of secondary components detectedmeta.number;em.opt.uVARCHARprincipalGALXCEN_uGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.uVARCHARprincipalGALYCEN_uGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.uVARCHARprincipalGALMAG_uGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.uVARCHARprincipalGALRE_uGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.uVARCHARprincipalGALINDEX_uGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.uVARCHARprincipalGALELLIP_uGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.uVARCHARprincipalGALPA_uGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.uVARCHARprincipalGALXCENERR_uGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALYCENERR_uGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALMAGERR_uGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALREERR_uGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALINDEXERR_uGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALELLIPERR_uGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALPAERR_uGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.uVARCHARprincipalGALRA_uGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.uVARCHARprincipalGALDEC_uGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.uVARCHARprincipalGALMAG10RE_uGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.uVARCHARprincipalGALMU0_uGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.uVARCHARprincipalGALMUE_uGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.uVARCHARprincipalGALMUEAVG_uGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.uVARCHARprincipalGALR90_uGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.uVARCHARprincipalGALCHI2FULL_uGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.uVARCHARprincipalGALNDOF_uGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.uVARCHARprincipalGALCHI2_uGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.uVARCHARprincipalGALPLAN_uSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.uVARCHARprincipalPRICHI2FULL_uPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalPRINFP_uPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalPRINDOF_uPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalPRICHI2_uPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.uVARCHARprincipalCENFLUX_gCentral pixel flux value prior to background estimationcountsphot.count;em.opt.gVARCHARprincipalBACKFLUX_gSEx subtracted background at object positioncountsphot.count;em.opt.gVARCHARprincipalPSFNUM_gPSFEx number of stars usedmeta.number;em.opt.gVARCHARprincipalPSFCHI2_gPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.gVARCHARprincipalPSFFWHM_gPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.gVARCHARprincipalNSEC_gSEx number of secondary components detectedmeta.number;em.opt.gVARCHARprincipalGALXCEN_gGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.gVARCHARprincipalGALYCEN_gGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.gVARCHARprincipalGALMAG_gGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.gVARCHARprincipalGALRE_gGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.gVARCHARprincipalGALINDEX_gGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.gVARCHARprincipalGALELLIP_gGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.gVARCHARprincipalGALPA_gGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.gVARCHARprincipalGALXCENERR_gGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALYCENERR_gGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALMAGERR_gGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALREERR_gGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALINDEXERR_gGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALELLIPERR_gGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALPAERR_gGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.gVARCHARprincipalGALRA_gGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.gVARCHARprincipalGALDEC_gGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.gVARCHARprincipalGALMAG10RE_gGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.gVARCHARprincipalGALMU0_gGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.gVARCHARprincipalGALMUE_gGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.gVARCHARprincipalGALMUEAVG_gGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.gVARCHARprincipalGALR90_gGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.gVARCHARprincipalGALCHI2FULL_gGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.gVARCHARprincipalGALNDOF_gGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.gVARCHARprincipalGALCHI2_gGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.gVARCHARprincipalGALPLAN_gSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.gVARCHARprincipalPRICHI2FULL_gPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalPRINFP_gPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalPRINDOF_gPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalPRICHI2_gPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.gVARCHARprincipalCENFLUX_rCentral pixel flux value prior to background estimationcountsphot.count;em.opt.rVARCHARprincipalBACKFLUX_rSEx subtracted background at object positioncountsphot.count;em.opt.rVARCHARprincipalPSFNUM_rPSFEx number of stars usedmeta.number;em.opt.rVARCHARprincipalPSFCHI2_rPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.rVARCHARprincipalPSFFWHM_rPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.rVARCHARprincipalNSEC_rSEx number of secondary components detectedmeta.number;em.opt.rVARCHARprincipalGALXCEN_rGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.rVARCHARprincipalGALYCEN_rGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.rVARCHARprincipalGALMAG_rGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.rVARCHARprincipalGALRE_rGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.rVARCHARprincipalGALINDEX_rGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.rVARCHARprincipalGALELLIP_rGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.rVARCHARprincipalGALPA_rGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.rVARCHARprincipalGALXCENERR_rGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALYCENERR_rGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALMAGERR_rGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALREERR_rGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALINDEXERR_rGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALELLIPERR_rGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALPAERR_rGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.rVARCHARprincipalGALRA_rGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.rVARCHARprincipalGALDEC_rGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.rVARCHARprincipalGALMAG10RE_rGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.rVARCHARprincipalGALMU0_rGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.rVARCHARprincipalGALMUE_rGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.rVARCHARprincipalGALMUEAVG_rGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.rVARCHARprincipalGALR90_rGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.rVARCHARprincipalGALCHI2FULL_rGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.rVARCHARprincipalGALNDOF_rGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.rVARCHARprincipalGALCHI2_rGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.rVARCHARprincipalGALPLAN_rSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.rVARCHARprincipalPRICHI2FULL_rPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalPRINFP_rPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalPRINDOF_rPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalPRICHI2_rPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.rVARCHARprincipalCENFLUX_iCentral pixel flux value prior to background estimationcountsphot.count;em.opt.iVARCHARprincipalBACKFLUX_iSEx subtracted background at object positioncountsphot.count;em.opt.iVARCHARprincipalPSFNUM_iPSFEx number of stars usedmeta.number;em.opt.iVARCHARprincipalPSFCHI2_iPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.iVARCHARprincipalPSFFWHM_iPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.iVARCHARprincipalNSEC_iSEx number of secondary components detectedmeta.number;em.opt.iVARCHARprincipalGALXCEN_iGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.iVARCHARprincipalGALYCEN_iGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.iVARCHARprincipalGALMAG_iGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.iVARCHARprincipalGALRE_iGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.iVARCHARprincipalGALINDEX_iGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.iVARCHARprincipalGALELLIP_iGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.iVARCHARprincipalGALPA_iGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.iVARCHARprincipalGALXCENERR_iGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALYCENERR_iGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALMAGERR_iGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALREERR_iGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALINDEXERR_iGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALELLIPERR_iGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALPAERR_iGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.iVARCHARprincipalGALRA_iGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.iVARCHARprincipalGALDEC_iGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.iVARCHARprincipalGALMAG10RE_iGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.iVARCHARprincipalGALMU0_iGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.iVARCHARprincipalGALMUE_iGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.iVARCHARprincipalGALMUEAVG_iGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.iVARCHARprincipalGALR90_iGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.iVARCHARprincipalGALCHI2FULL_iGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.iVARCHARprincipalGALNDOF_iGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.iVARCHARprincipalGALCHI2_iGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.iVARCHARprincipalGALPLAN_iSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.iVARCHARprincipalPRICHI2FULL_iPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalPRINFP_iPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalPRINDOF_iPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalPRICHI2_iPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.iVARCHARprincipalCENFLUX_zCentral pixel flux value prior to background estimationcountsphot.count;em.opt.zVARCHARprincipalBACKFLUX_zSEx subtracted background at object positioncountsphot.count;em.opt.zVARCHARprincipalPSFNUM_zPSFEx number of stars usedmeta.number;em.opt.zVARCHARprincipalPSFCHI2_zPSFEx PSF reduced Chi^2stat.fit.goodness;em.opt.zVARCHARprincipalPSFFWHM_zPSFEx PSF FWHMarcsecinstr.det.psf;meta.modelled;em.opt.zVARCHARprincipalNSEC_zSEx number of secondary components detectedmeta.number;em.opt.zVARCHARprincipalGALXCEN_zGALFIT pixel pos. of model in cutout (x)pixelpos.cartesian.x;meta.modelled;em.opt.zVARCHARprincipalGALYCEN_zGALFIT pixel pos. of model in cutout (y)pixelpos.cartesian.y;meta.modelled;em.opt.zVARCHARprincipalGALMAG_zGALFIT magnitude of Sersic modelmagphot.mag;meta.modelled;em.opt.zVARCHARprincipalGALRE_zGALFIT effective (half-light) radius (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.zVARCHARprincipalGALINDEX_zGALFIT Sersic indexstat.fit.param;meta.modelled;em.opt.zVARCHARprincipalGALELLIP_zGALFIT ellipticity (1-(b/a))src.ellipticity;meta.modelled;em.opt.zVARCHARprincipalGALPA_zGALFIT position angle (x+, CCW) (see notes)degpos.posAng;meta.modelled;em.opt.zVARCHARprincipalGALXCENERR_zGALFIT error on x positionpixelpos.cartesian.x;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALYCENERR_zGALFIT error on y positionpixelpos.cartesian.y;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALMAGERR_zGALFIT error on magnitudemagphot.mag;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALREERR_zGALFIT error on rearcsecphys.angSize;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALINDEXERR_zGALFIT error on Sersic indexstat.fit.param;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALELLIPERR_zGALFIT error on ellipticitysrc.ellipticity;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALPAERR_zGALFIT error on position angledegpos.posAng;stat.error;meta.modelled;em.opt.zVARCHARprincipalGALRA_zGALFIT Right Ascension as determined by GALFITdegpos.eq.ra;meta.modelled;em.opt.zVARCHARprincipalGALDEC_zGALFIT Declination as determined by GALFITdegpos.eq.dec;meta.modelled;em.opt.zVARCHARprincipalGALMAG10RE_zGALFIT magnitude of model, truncated at 10*remagphot.mag;meta.modelled;em.opt.zVARCHARprincipalGALMU0_zGALFIT central surface brightnessmag/arcsec^2phot.mag.sb;meta.modelled;em.opt.zVARCHARprincipalGALMUE_zGALFIT effective surface brightness at remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.zVARCHARprincipalGALMUEAVG_zGALFIT effective surface brightness within remag/arcsec^2phot.mag.sb;meta.modelled;em.opt.zVARCHARprincipalGALR90_zGALFIT rad containing 90% of total light (semi-major axis)arcsecphys.angSize;meta.modelled;em.opt.zVARCHARprincipalGALCHI2FULL_zGALFIT Chi^2 goodness-of-fit parameter (pri + sec)stat.fit.goodness;em.opt.zVARCHARprincipalGALNDOF_zGALFIT model number of degrees of freedom (pri + sec)stat.fit.goodness;em.opt.zVARCHARprincipalGALCHI2_zGALFIT reduced Chi^2 of output model (pri + sec)stat.fit.goodness;em.opt.zVARCHARprincipalGALPLAN_zSIGMA chosen GALFIT modelling plan (see notes)stat.fit.goodness;em.opt.zVARCHARprincipalPRICHI2FULL_zPRIMARY Chi^2 goodness-of-fit paramter (primary only)stat.fit.goodness;em.opt.zVARCHARprincipalPRINFP_zPRIMARY model number of free parameters (primary only)stat.fit.goodness;em.opt.zVARCHARprincipalPRINDOF_zPRIMARY model number of degrees of freedom (primary only)stat.fit.goodness;em.opt.zVARCHARprincipalPRICHI2_zPRIMARY reduced Chi^2 of output model (primary only)stat.fit.goodness;em.opt.zVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.SpecObjv27This table lists each observed target and the spectrum thatprovides its best redshift (from GAMA or otherwise).CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalIC_FLAGCatalogue source(s) of GAMA objectmeta.code.memberVARCHARprincipalN_SPECNumber of spectra available for this objectmeta.number;spectVARCHARprincipalN_GAMA_SPECNumber of GAMA spectra available for this objectmeta.number;spectVARCHARprincipalDISTDistance between GAMA object and best matched spectrumarcsecpos.angDistanceVARCHARprincipalSPECIDID of best matched spectrummeta.id.cross;spectVARCHARprincipalSURVEYSurvey best matched spectrum originated frommeta.datasetVARCHARprincipalSURVEY_CODENumerical code for originating surveymeta.code;meta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.SpecAllv27This table lists all spectra that are available in the GAMA surveyregions, including GAMA spectra and those from previousspectroscopic surveys (such as the SDSS). Duplicate observations ofthe same object are retained in this table (but a flag is providedto mark the spectrum that provided the best available redshift of agiven object). Every spectrum listed in this table is available inthe GAMA DR4 database.SPECIDUnique ID of spectrummeta.id;meta.mainVARCHARindexedprincipalSURVEYSurvey this spectrum originated frommeta.datasetVARCHARprincipalSURVEY_CODENumerical code for originating surveymeta.code;meta.datasetVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTSpectrum with best redshift for this object in originating survey?meta.codeVARCHARprincipalIS_BESTSpectrum with best redshift for this object?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.LTSpecAllv03This table lists a small number of spectra of fibre-bright targetscollected by the GAMA team at the Liverpool Telescope (LT).WMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalSPECIDID of GAMA LT spectrummeta.id;meta.mainVARCHARindexedprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTGAMA LT spectrum with best redshift for this object?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.DoublezCandidatesv01This table provides a list of GAMA AAT spectra that probably includethe light from two galaxies and thus show two redshifts.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.idVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalCC_SIGMACross-correlation peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATETemplate ID; 0-22 for stars, 40-47 for galaxiesmeta.idVARCHARprincipalZ2Heliocentric redshift of second peaksrc.redshiftVARCHARprincipalCC_SIGMA2Cross-correlation 2nd peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATE2Template ID for second peakmeta.idVARCHARprincipalCC_SIGMA2TO342nd peak value divided by RMS of 3rd and 4th peak valuesstat.valueVARCHARprincipalCC_SIGMA2TO34_OLDOld value of CC_SIGMA2TO34, using templates 23-28 for galaxiesstat.valueVARCHARprincipalIS_DBESTSpectrum of object with highest CC_SIGMA2TO34 value?meta.codeVARCHARprincipalSPECTYPESpectral classification: PG=templates 40-42, ELG=43-47, lowest redshift firstmeta.codeVARCHARprincipalVISUALTYPEPreliminary visual classfication by Benne Holwerdameta.codeVARCHARprincipalCOMMENTComments by Benne Holwerda on visual classificationmeta.noteVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.AATSpecAutozCombv27This table provides a fully automated redshift estimate forcombinations of two or three GAMA AAT spectra of the same target.COMBIDID for spectral coaddmeta.id;meta.mainVARCHARindexedprincipalSPECID1ID of GAMA AAT spectrummeta.idVARCHARprincipalSPECID2ID of GAMA AAT spectrummeta.idVARCHARprincipalSPECID3ID of GAMA AAT spectrum, set to xxx if only two spectra are combinedmeta.idVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.idVARCHARprincipalRMS_MAD_RATIORMS divided by mean absolute deviation for the HP spectrumstat.valueVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalCC_SIGMACross-correlation peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATETemplate ID; 0-22 for stars, 40-47 for galaxiesmeta.idVARCHARprincipalZ2Heliocentric redshift of second peaksrc.redshiftVARCHARprincipalCC_SIGMA2Cross-correlation 2nd peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATE2Template ID for second peakmeta.idVARCHARprincipalCC_SIGMA3Cross-correlation 3rd peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA4Cross-correlation 4th peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA1TO234Peak value divided by RMS of 2nd-4th peak valuesstat.valueVARCHARprincipalCC_FOMFigure of merit for primary redshift confidencestat.valueVARCHARprincipalPROBEstimated probability of redshift successstat.valueVARCHARprincipalVEL_ERRUncertainty in redshift, given as a velocity, delta c ln(1+z)km/sstat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.AATSpecAutozAllv27This table provides a fully automated redshift estimate for eachGAMA AAT spectrum. These redshifts are completely independent fromthe ones derived by runz, and are considered more reliable.RARA of spectrum (J2000)degpos.eq.raVARCHARprincipalSPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.idVARCHARprincipalCOUNT_BADPIXELNumber of bad pixels masked in spectrummeta.numberVARCHARprincipalCOUNT_HIGHVALNumber of high values in the high-passed spectrummeta.numberVARCHARprincipalCOUNT_LOWVALNumber of low values in the high-passed spectrummeta.numberVARCHARprincipalRMS_MAD_RATIORMS divided by mean absolute deviation for the HP spectrumstat.valueVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalCC_SIGMACross-correlation peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATETemplate ID; 0-22 for stars, 40-47 for galaxiesmeta.idVARCHARprincipalZ2Heliocentric redshift of second peaksrc.redshiftVARCHARprincipalCC_SIGMA2Cross-correlation 2nd peak value divided by RMS CC valuestat.valueVARCHARprincipalTEMPLATE2Template ID for second peakmeta.idVARCHARprincipalCC_SIGMA3Cross-correlation 3rd peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA4Cross-correlation 4th peak value divided by RMS CC valuestat.valueVARCHARprincipalCC_SIGMA1TO234Peak value divided by RMS of 2nd-4th peak valuesstat.valueVARCHARprincipalCC_FOMFigure of merit for primary redshift confidencestat.valueVARCHARprincipalPROBEstimated probability of redshift successstat.valueVARCHARprincipalVEL_ERRUncertainty in redshift, given as a velocity, delta c ln(1+z)km/sstat.errorVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.AATSpecAllzAllv27Many GAMA AAT spectra were redshifted more than once using the coderunz. This table contains one line per spectrum summarising all ofthe redshifting results for this spectrum, as well as listing theresults of the analysis to determine the best redshift based on thereliabilities of the redshifters.OP5_QQmeta.code.qual;src.redshiftVARCHARprincipalOP5_ZRedshiftsrc.redshiftVARCHARprincipalSPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalN_OPNumber of opinions for this spectrummeta.numberVARCHARprincipalN_OPQGNumber of opinions with Q >= 2meta.numberVARCHARprincipalN_OPQBNumber of opinions with Q < 2meta.numberVARCHARprincipalN_ZNumber of different redshiftsmeta.numberVARCHARprincipalBEST_PROBProbability that the most probable possibility is correctstat.probability;src.redshiftVARCHARprincipalBEST_ZRedshift of the most probable possibilitysrc.redshiftVARCHARprincipalBEST_Z_NQNormalised Q of the most probable possibilitymeta.code.qual;src.redshiftVARCHARprincipalBEST_Z_NNumber of opinions supporting the most probable possibilitymeta.numberVARCHARprincipalBEST_Z_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q1Number of supporting Q=1 opinionsmeta.numberVARCHARprincipalBEST_Z_N_Q0Number of supporting Q=0 opinionsmeta.numberVARCHARprincipalZ1_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ1_ZPossible redshiftsrc.redshiftVARCHARprincipalZ1_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ1_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ1_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ1_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ1_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ2_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ2_ZPossible redshiftsrc.redshiftVARCHARprincipalZ2_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ2_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ2_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ2_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ2_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ3_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ3_ZPossible redshiftsrc.redshiftVARCHARprincipalZ3_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ3_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ3_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ3_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ3_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ4_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ4_ZPossible redshiftsrc.redshiftVARCHARprincipalZ4_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ4_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ4_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ4_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ4_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalZ5_PROBProbability that ZX_Z is correctstat.probabilityVARCHARprincipalZ5_ZPossible redshiftsrc.redshiftVARCHARprincipalZ5_NQNormalised Q of ZX_Zmeta.code.qual;src.redshiftVARCHARprincipalZ5_NNumber of opinions supporting ZX_Zmeta.numberVARCHARprincipalZ5_N_Q4Number of supporting Q=4 opinionsmeta.numberVARCHARprincipalZ5_N_Q3Number of supporting Q=3 opinionsmeta.numberVARCHARprincipalZ5_N_Q2Number of supporting Q=2 opinionsmeta.numberVARCHARprincipalBEST_IDXIndex of best possibility in the above listVARCHARprincipalQ1_PROBProbability that no redshift can be found (i.e. that Q=1 is correct)stat.probabilityVARCHARprincipalQ1_N_Q1Number of supporting Q=1 opinionsmeta.numberVARCHARprincipalQ1_N_Q0Number of supporting Q=0 opinionsmeta.numberVARCHARprincipalCOMP_PROBProbability that none of the offered possibilities are correctstat.probabilityVARCHARprincipalCOMMENTS_FLAGFlag encoding all user comments on this spectrummeta.codeVARCHARprincipalOP1_RUNZRESIDID of original runz result in AATRunzResultsmeta.idVARCHARprincipalOP1_RSOriginal redshiftermeta.idVARCHARprincipalOP1_QOriginal Qmeta.code.qual;src.redshiftVARCHARprincipalOP1_ZOriginal redshiftsrc.redshiftVARCHARprincipalOP1_CFFlag encoding original user comment on this spectrummeta.codeVARCHARprincipalOP1_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP2_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP2_RSRedshiftermeta.idVARCHARprincipalOP2_QQmeta.code.qual;src.redshiftVARCHARprincipalOP2_ZRedshiftsrc.redshiftVARCHARprincipalOP2_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP2_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP3_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP3_RSRedshiftermeta.idVARCHARprincipalOP3_QQmeta.code.qual;src.redshiftVARCHARprincipalOP3_ZRedshiftsrc.redshiftVARCHARprincipalOP3_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP3_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP4_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP4_RSRedshiftermeta.idVARCHARprincipalOP4_QQmeta.code.qual;src.redshiftVARCHARprincipalOP4_ZRedshiftsrc.redshiftVARCHARprincipalOP4_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP4_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP5_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP5_RSRedshiftermeta.idVARCHARprincipalOP5_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP5_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP6_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP6_RSRedshiftermeta.idVARCHARprincipalOP6_QQmeta.code.qual;src.redshiftVARCHARprincipalOP6_ZRedshiftsrc.redshiftVARCHARprincipalOP6_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP6_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipalOP7_RUNZRESIDID of additional runz result in AATRunzResultsmeta.idVARCHARprincipalOP7_RSRedshiftermeta.idVARCHARprincipalOP7_QQmeta.code.qual;src.redshiftVARCHARprincipalOP7_ZRedshiftsrc.redshiftVARCHARprincipalOP7_CFFlag encoding user comment on this spectrummeta.codeVARCHARprincipalOP7_ZIDXIndex of possibility in ZX list that is supported by this redshiftVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.AATSpecAllv27This is a table of all GAMA AAT spectra. Many targets were observedmore than once by GAMA, and these duplications are retained here.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalWMINMinimum wavelength of spectrumAem.wl;stat.minVARCHARprincipalWMAXMaximum wavelength of spectrumAem.wl;stat.maxVARCHARprincipalZHeliocentric redshiftsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalZ_RUNZHeliocentric redshift as determined by runz (incl re-redshifting)src.redshiftVARCHARprincipalNQ_RUNZNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROB_RUNZProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalCOMBIDCombined spectrum this spectrum contributes tometa.idVARCHARprincipalCOMBNOFirst, second or third spectrum in the combination?meta.idVARCHARprincipalZ_COMBHeliocentric redshift of the combined spectrumsrc.redshiftVARCHARprincipalNQ_COMBNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalPROB_COMBProbability that redshift is correctstat.probability;src.redshiftVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalS_NS/N of spectrumstat.snrVARCHARprincipalWARNING_FLAGWarnings raised for this spectrummeta.code.qualVARCHARprincipalCOMMENTS_FLAGFlag encoding all user comments on this spectrummeta.codeVARCHARprincipalPLATEPlate numbermeta.id;instrVARCHARprincipalX_POSNFibre x position on platepos.cartesian.x;instrVARCHARprincipalY_POSNFibre y position on platepos.cartesian.y;instrVARCHARprincipalFILENAMEFull path and filename of the spectrummeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the spectrummeta.ref.url;meta.file;meta.fitsVARCHARprincipalURL_IMGURL of the spectrum's imagemeta.ref.url;meta.fileVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalIS_SBESTGAMA AAT spectrum with best redshift for this object?meta.codeVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.AATRunzResultsv27All spectra collected for GAMA at the AAT were redshifted using thecode runz. This table contains the complete redshifting results.Note that many spectra were redshifted more than once and thiscatalogue contains all duplications.DATE_ZDate of runz runtime.processingVARCHARprincipalRUNZRESIDID of runz outputmeta.id;meta.mainVARCHARindexedprincipalSPECIDID of GAMA AAT spectrummeta.id;spectVARCHARprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalUSERRedshiftermeta.idVARCHARprincipalCATAIDID of matched GAMA objectmeta.id.cross;srcVARCHARprincipalGAMA_NAMEName of matched GAMA objectmeta.id.cross;srcVARCHARprincipalIC_FLAGCatalogue source(s) of matched GAMA objectmeta.code.memberVARCHARprincipalDISTDistance between spectrum and matched GAMA objectarcsecpos.angDistanceVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalOBJECTObject nameVARCHARprincipalRAHRA hours of spectrum (J2000)hVARCHARprincipalRAMRA minutesmVARCHARprincipalRASRA secondssVARCHARprincipalDECDDEC degree of spectrum (J2000)degVARCHARprincipalDECMDEC minutesmVARCHARprincipalDECSDEC secondssVARCHARprincipalRMAGExtinction corrected SDSS r-band Petrosian magnitudemagphot.mag;em.opt.RVARCHARprincipalNEBNumber of matching emission lines at best emission line redshiftmeta.numberVARCHARprincipalNEGTotal number of detected potential emission linesmeta.numberVARCHARprincipalZEMEmission line redshiftsrc.redshiftVARCHARprincipalZEM_ERREmission line redshift errorstat.error;src.redshiftVARCHARprincipalQEMEmission line redshift qualitymeta.code.qual;src.redshiftVARCHARprincipalTEMPCross-correlation templateVARCHARprincipalXCORCross-correlation peak heightVARCHARprincipalZXCross-correlation redshiftsrc.redshiftVARCHARprincipalZX_ERRCross-correlation redshift errorstat.error;src.redshiftVARCHARprincipalQXCross-correlation redshift qualitymeta.code.qual;src.redshiftVARCHARprincipalZ_FINFinal selected redshiftsrc.redshiftVARCHARprincipalZ_FIN_ERRError of final selected redshiftstat.error;src.redshiftVARCHARprincipalQAAutomatic quality of final selected redshiftmeta.code.qual;src.redshiftVARCHARprincipalQOPUser assigned quality of final selected redshiftmeta.code.qual;src.redshiftVARCHARprincipalFFlag indicating whether Z_FIN is different from automatic redshifts: 0 = equal to best auto redshift; 1 = not equal to best auto redshift; 2 = not equal to either auto redshiftsmeta.codeVARCHARprincipalFLDUnusedVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalCCDCCD numbermeta.id;instrVARCHARprincipalPLATEPlate numbermeta.id;instrVARCHARprincipalX_POSNFibre x position on plateVARCHARprincipalY_POSNFibre y position on plateVARCHARprincipalS_NS/N of spectrumstat.snrVARCHARprincipalSPMAGUnusedmagVARCHARprincipalVSPApproximate V-band fibre mag with zeropoint 32magVARCHARprincipalRSPApproximate R-band fibre mag with zeropoint 32.3magVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalCOMMENT_FLAGFlag encoding the user commentmeta.codeVARCHARprincipalCOMMENTFree format user comment on this spectrummeta.noteVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.AATFieldsv27This is a table of all AAT 2dF/AAOmega fields observed for GAMA.FIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalRARA of field centre (J2000)degpos.eq.ra;obs.fieldVARCHARprincipalDECDEC of field centre (J2000)degpos.eq.dec;obs.fieldVARCHARprincipalDATE_OBSUT date of observationtime.epoch;obs.exposureVARCHARprincipalUTMJDMean MJD of start of exposurestime.epoch;obs.exposureVARCHARprincipalUTSTARTUT of start of first exposuretime.start;obs.exposureVARCHARprincipalUTENDUT of end of last exposuretime.end;obs.exposureVARCHARprincipalZDSTARTZenith distance at start of first exposuredegpos.az.zd;time.startVARCHARprincipalZDENDZenith distance at end of last exposuredegpos.az.zd;time.rndVARCHARprincipalHASTARTHour angle at start of first exposuredegpos.eq.ha;time.startVARCHARprincipalHAENDHour angle at end of last exposuredegpos.eq.ha;time.endVARCHARprincipalN_EXPNumber of exposuresmeta.number;obs.exposureVARCHARprincipalN_NIGHTSNumber of nights over which exposures were spreadmeta.numberVARCHARprincipalT_EXPTotal exposure timestime.duration;obs.exposureVARCHARprincipalMEAN_SNMean S/N of spectrastat.snr;spectVARCHARprincipalPLATE2dF plate numbermeta.id;instrVARCHARprincipalCONFIG_FILEName of configuration filemeta.id;meta.file;instr.setupVARCHARprincipalTDFDRVERVersion of 2dfdr data reduction softwaremeta.version;meta.softwareVARCHARprincipalUSEROriginal redshifter of this fieldmeta.idVARCHARprincipalDATE_ZDate of original redshifting runtime.processingVARCHARprincipalCRCORVERRunz version used for original redshifting runmeta.version;meta.softwareVARCHARprincipalHEL_VCHeliocentric velocity correctionkm/sphys.velocity;pos.heliocentricVARCHARprincipalN_SPECNumber of spectra observedmeta.number;spectVARCHARprincipalN_GALNumber of galaxy targets observedmeta.number;srcVARCHARprincipalN_STARNumber of calibration stars observedmeta.number;src.calibVARCHARprincipalN_GOODNumber of spectra with a good quality redshift, i.e. nQ >= 3meta.number;spectVARCHARprincipalN_GAL_GOODNumber of galaxy target spectra with a good quality redshift, i.e. nQ >= 3meta.number;srcVARCHARprincipalCOMPLRedshift success ratearith.ratio;meta.number;spectVARCHARprincipalGAL_COMPLRedshift success rate among galaxy targetsarith.ratio;meta.number;srcVARCHARprincipalFILENAMEFull path and filename of the field's FITS filemeta.id;meta.file;meta.fitsVARCHARprincipalURLURL of the field's FITS filemeta.ref.url;meta.file;meta.fitsVARCHARprincipalgama_dr4.AATFibreAllv27This table contains all fibre information for all GAMA AATobservations in AATFields from the fibre fits extension ofthe final reduced 2d data files.SPECIDID of GAMA AAT spectrummeta.id;meta.mainVARCHARindexedprincipalFIELDIDID of GAMA AAT fieldmeta.id;obs.fieldVARCHARprincipalFIBREFibre numbermeta.id;instrVARCHARprincipalNAMEName of target in config filemeta.id;srcVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDEC of spectrum (J2000)degpos.eq.decVARCHARprincipalXFibre x position on platepos.cartesian.xVARCHARprincipalYFibre y position on platepos.cartesian.yVARCHARprincipalXERRError on Xstat.error;pos.cartesian.xVARCHARprincipalYERRError on Ystat.error;pos.cartesian.yVARCHARprincipalTHETAAngle of fibre on field platepos.posAngVARCHARprincipalTYPEFibre type: F=guide, N=broken, P=program, S=sky, U=unusedmeta.code.classVARCHARprincipalPIVOT2dF fibre pivot numbermeta.id;instrVARCHARprincipalMAGNITUDEMagnitude of target from config filephot.magVARCHARprincipalPIDProgram IDmeta.idVARCHARprincipalRETRACTOR2dF retractor numbermeta.id;instrVARCHARprincipalWLENUnknownmeta.crypticVARCHARprincipalCOMMENTComment from the config filemeta.noteVARCHARprincipalgama_dr4.GaussFitSimplev05This table provides emission line measurements from simple Gaussianfits for all spectra of those objects that have a best redshift withnQ > 1 and 0.002 < z < 1.35.SPECIDUnique spectrum IDVARCHARprincipalCATAIDUnique GAMA object IDVARCHARprincipalRAJ2000degVARCHARprincipalDECJ2000degVARCHARprincipalZRedshift with heliocentric correction removedVARCHARprincipalNQRedshift qualityVARCHARprincipalSURVEYSurvey spectrum originated fromVARCHARprincipalSURVEY_CODENumerical code for originating surveyVARCHARprincipalIS_BESTSpectrum with best redshift for this object?VARCHARprincipalIS_SBESTSpectrum with best redshift for originating survey?VARCHARprincipalSNS/N ratio per pixel in the 6383 - 6536 A window in the galaxy frameVARCHARprincipalMEAN_CONTSigma clipped mean continuum level used for S in S/NVARCHARprincipalSIGMA_CONTScatter around continuum used for N in S/NVARCHARprincipalFSCALEFor SDSS spectra, the flux is scaled by this value to approximate the scaling used for AAOmega spectraVARCHARprincipalD4000N4000 A break strength (see notes for description)VARCHARprincipalD4000N_ERRUncertainty on the 4000 A break strengthVARCHARprincipalOII_CONTOII continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_CONT_ERROII continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_GRADOII continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_GRAD_ERROII continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalOII_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalOII_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalOII_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalOII_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalOII_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalOII_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalOII_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_OIIROIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIR_ERROIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIROIIR line position from Gaussian fit measured relative to OII_CENAVARCHARprincipalPOS_OIIR_ERROIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIROIIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIIR_ERRUncertainty on the OIIR line sigma from the Gaussian fitAVARCHARprincipalOIIR_FLUXOIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIR_FLUX_ERROIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIR_EWOIIR line equivalent widthAVARCHARprincipalOIIR_EW_ERROIIR equivalent width uncertaintyAVARCHARprincipalAMP_OIIBOIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIB_ERROIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIBOIIB line position from Gaussian fit measured relative to OII_CENAVARCHARprincipalPOS_OIIB_ERROIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIBOIIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIIB_ERRUncertainty on the OIIB line sigma from the Gaussian fitAVARCHARprincipalOIIB_FLUXOIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIB_FLUX_ERROIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIB_EWOIIB line equivalent widthAVARCHARprincipalOIIB_EW_ERROIIB equivalent width uncertaintyAVARCHARprincipalOIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIBVARCHARprincipalOIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIRVARCHARprincipalHB_CONTHB/OIIIB/OIIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_CONT_ERRHB/OIIIB/OIIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRADHB/OIIIB/OIIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRAD_ERRHB continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalHB_REDCHI_ABSReduced chisquared for the continuum plus absorption line fitVARCHARprincipalHB_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalHB_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHB_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHB_MODSEL_ABS_LINEModel selection score for the continuum-plus-absorption-line fit compared to the straight-line continuum fitVARCHARprincipalHB_MODSEL_EM_ABSModel selection score for the continuum-plus-emission-line fit compared to the continuum-plus-absorption-line fitVARCHARprincipalHB_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHB_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHB_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHB_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HBHB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_ERRHB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HBHB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_ERRHB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HBHB line sigma from Gaussian fitAVARCHARprincipalSIG_HB_ERRUncertainty on the HB line sigma from the Gaussian fitAVARCHARprincipalHB_FLUXHB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_FLUX_ERRHB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_EWHB line equivalent widthAVARCHARprincipalHB_EW_ERRHB equivalent width uncertaintyAVARCHARprincipalHB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalAMP_OIIIBOIIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIB_ERROIIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIBOIIIB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIB_ERROIIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIBOIIIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIB_ERRUncertainty on the OIIIB line sigma from the Gaussian fitAVARCHARprincipalOIIIB_FLUXOIIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_FLUX_ERROIIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_EWOIIIB line equivalent widthAVARCHARprincipalOIIIB_EW_ERROIIIB equivalent width uncertaintyAVARCHARprincipalAMP_OIIIROIIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIR_ERROIIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIROIIIR line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIR_ERROIIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIROIIIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIR_ERRUncertainty on the OIIIR line sigma from the Gaussian fitAVARCHARprincipalOIIIR_FLUXOIIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_FLUX_ERROIIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_EWOIIIR line equivalent widthAVARCHARprincipalOIIIR_EW_ERROIIIR equivalent width uncertaintyAVARCHARprincipalOIIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIBVARCHARprincipalOIIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIRVARCHARprincipalHA_CONTNIIB/HA/NIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_CONT_ERRNIIB/HA/NIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRADNIIB/HA/NIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRAD_ERRHA continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalHA_REDCHI_ABSReduced chisquared for the continuum plus absorption line fitVARCHARprincipalHA_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalHA_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHA_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHA_MODSEL_ABS_LINEModel selection score for the continuum-plus-absorption-line fit compared to the straight-line continuum fitVARCHARprincipalHA_MODSEL_EM_ABSModel selection score for the continuum-plus-emission-line fit compared to the continuum-plus-absorption-line fitVARCHARprincipalHA_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHA_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHA_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHA_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HAHA line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_ERRHA uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HAHA line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_ERRHA uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HAHA line sigma from Gaussian fitAVARCHARprincipalSIG_HA_ERRUncertainty on the HA line sigma from the Gaussian fitAVARCHARprincipalHA_FLUXHA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_FLUX_ERRHA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_EWHA line equivalent widthAVARCHARprincipalHA_EW_ERRHA equivalent width uncertaintyAVARCHARprincipalHA_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalAMP_NIIBNIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIB_ERRNIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIBNIIB line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIB_ERRNIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIBNIIB line sigma from Gaussian fitAVARCHARprincipalSIG_NIIB_ERRUncertainty on the NIIB line sigma from the Gaussian fitAVARCHARprincipalNIIB_FLUXNIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_FLUX_ERRNIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_EWNIIB line equivalent widthAVARCHARprincipalNIIB_EW_ERRNIIB equivalent width uncertaintyAVARCHARprincipalAMP_NIIRNIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIR_ERRNIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIRNIIR line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIR_ERRNIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIRNIIR line sigma from Gaussian fitAVARCHARprincipalSIG_NIIR_ERRUncertainty on the NIIR line sigma from the Gaussian fitAVARCHARprincipalNIIR_FLUXNIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_FLUX_ERRNIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_EWNIIR line equivalent widthAVARCHARprincipalNIIR_EW_ERRNIIR equivalent width uncertaintyAVARCHARprincipalNIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIBVARCHARprincipalNIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIRVARCHARprincipalSII_CONTSII continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_CONT_ERRSII continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_GRADSII continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_GRAD_ERRSII continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSII_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalSII_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalSIG_OIB_ERRUncertainty on the OIB line sigma from the Gaussian fitAVARCHARprincipalSII_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalSII_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalSII_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalSII_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalSII_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalSII_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_SIIBSIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_SIIB_ERRSIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_SIIBSIIB line position from Gaussian fit measured relative to SII_CENAVARCHARprincipalPOS_SIIB_ERRSIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_SIIBSIIB line sigma from Gaussian fitAVARCHARprincipalSIG_SIIB_ERRUncertainty on the SIIB line sigma from the Gaussian fitAVARCHARprincipalSIIB_FLUXSIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_FLUX_ERRSIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_EWSIIB line equivalent widthAVARCHARprincipalSIIB_EW_ERRSIIB equivalent width uncertaintyAVARCHARprincipalAMP_SIIRSIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_SIIR_ERRSIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_SIIRSIIR line position from Gaussian fit measured relative to SII_CENAVARCHARprincipalPOS_SIIR_ERRSIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_SIIRSIIR line sigma from Gaussian fitAVARCHARprincipalSIG_SIIR_ERRUncertainty on the SIIR line sigma from the Gaussian fitAVARCHARprincipalSIIR_FLUXSIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_FLUX_ERRSIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_EWSIIR line equivalent widthAVARCHARprincipalSIIR_EW_ERRSIIR equivalent width uncertaintyAVARCHARprincipalSIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to SIIBVARCHARprincipalSIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to SIIRVARCHARprincipalOI_CONTOI continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_CONT_ERROI continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_GRADOI continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_GRAD_ERROI continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI_REDCHI_LINEReduced chisquared for the straight line continuum fitVARCHARprincipalOI_REDCHI_EMReduced chisquared for the continuum plus emission line fitVARCHARprincipalOI_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalOI_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalOI_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalOI_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalOI_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalOI_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_OIBOIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIB_ERROIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIBOIB line position from Gaussian fit measured relative to OI_CENAVARCHARprincipalPOS_OIB_ERROIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIBOIB line sigma from Gaussian fitAVARCHARprincipalOIB_FLUXOIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIB_FLUX_ERROIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIB_EWOIB line equivalent widthAVARCHARprincipalOIB_EW_ERROIB equivalent width uncertaintyAVARCHARprincipalAMP_OIROIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIR_ERROIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIROIR line position from Gaussian fit measured relative to OI_CENAVARCHARprincipalPOS_OIR_ERROIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIROIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIR_ERRUncertainty on the OIR line sigma from the Gaussian fitAVARCHARprincipalOIR_FLUXOIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIR_FLUX_ERROIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIR_EWOIR line equivalent widthAVARCHARprincipalOIR_EW_ERROIR equivalent width uncertaintyAVARCHARprincipalOIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIBVARCHARprincipalOIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIRVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.GaussFitComplexv05This table provides emission line measurements from more complicatedGaussian fits to the OIII/Hbeta and NII/Halpha regions for allspectra of those objects that have a best redshift with nQ > 1and 0.002 < z < 1.35.SPECIDUnique spectrum IDVARCHARprincipalCATAIDUnique GAMA object IDVARCHARprincipalHB_CONTHB/OIIIB/OIIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_CONT_ERRHB/OIIIB/OIIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRADHB/OIIIB/OIIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_GRAD_ERRHB continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_REDCHI_EMBReduced chisquared for the continuum+narrow+broad emission line fitVARCHARprincipalHB_REDCHI_EMABSReduced chisquared for the continuum+narrow+absorption emission line fitVARCHARprincipalHB_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalHB_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHB_MODSEL_EMB_EMModel selection score for the continuum and Narrow+Broad emission-line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHB_MODSEL_NABS_NModel selection score for the continuum and Narrow emission plus absorption line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHB_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHB_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHB_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHB_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HBHB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_ERRHB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HBHB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_ERRHB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HBHB line sigma from Gaussian fitAVARCHARprincipalSIG_HB_ERRUncertainty on the HB line sigma from the Gaussian fitAVARCHARprincipalHB_FLUXHB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_FLUX_ERRHB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_EWHB line equivalent widthAVARCHARprincipalHB_EW_ERRHB equivalent width uncertaintyAVARCHARprincipalAMP_HB_ABSHB_ABS line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_ABS_ERRHB_ABS uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HB_ABSHB_ABS line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_ABS_ERRHB_ABS uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HB_ABSHB_ABS line sigma from Gaussian fitAVARCHARprincipalSIG_HB_ABS_ERRUncertainty on the HB_ABS line sigma from the Gaussian fitAVARCHARprincipalHB_ABS_FLUXHB_ABS line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_ABS_FLUX_ERRHB_ABS flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_ABS_EWHB_ABS line equivalent widthAVARCHARprincipalHB_ABS_EW_ERRHB_ABS equivalent width uncertaintyAVARCHARprincipalHB_ABS_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalAMP_HB_BHB_B line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HB_B_ERRHB_B uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HB_BHB_B line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_HB_B_ERRHB_B uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HB_BHB_B line sigma from Gaussian fitAVARCHARprincipalSIG_HB_B_ERRUncertainty on the HB_B line sigma from the Gaussian fitAVARCHARprincipalHB_B_FLUXHB_B line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_B_FLUX_ERRHB_B flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_B_EWHB_B line equivalent widthAVARCHARprincipalHB_B_EW_ERRHB_B equivalent width uncertaintyAVARCHARprincipalHB_B_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HBVARCHARprincipalAMP_OIIIBOIIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIB_ERROIIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIBOIIIB line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIB_ERROIIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIBOIIIB line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIB_ERRUncertainty on the OIIIB line sigma from the Gaussian fitAVARCHARprincipalOIIIB_FLUXOIIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_FLUX_ERROIIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_EWOIIIB line equivalent widthAVARCHARprincipalOIIIB_EW_ERROIIIB equivalent width uncertaintyAVARCHARprincipalAMP_OIIIROIIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_OIIIR_ERROIIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_OIIIROIIIR line position from Gaussian fit measured relative to HB_CENAVARCHARprincipalPOS_OIIIR_ERROIIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_OIIIROIIIR line sigma from Gaussian fitAVARCHARprincipalSIG_OIIIR_ERRUncertainty on the OIIIR line sigma from the Gaussian fitAVARCHARprincipalOIIIR_FLUXOIIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_FLUX_ERROIIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_EWOIIIR line equivalent widthAVARCHARprincipalOIIIR_EW_ERROIIIR equivalent width uncertaintyAVARCHARprincipalOIIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIRVARCHARprincipalOIIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to OIIIBVARCHARprincipalHA_CONTNIIB/HA/NIIR group continuum intercept (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_CONT_ERRNIIB/HA/NIIR group continuum intercept uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRADNIIB/HA/NIIR group continuum gradient (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_GRAD_ERRHA continuum gradient uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_REDCHI_EMBReduced chisquared for the continuum+narrow+broad emission line fitVARCHARprincipalHA_REDCHI_EMABSReduced chisquared for the continuum+narrow+absorption emission line fitVARCHARprincipalHA_FITFAILIf for code failed prior to fitting this line, then FITFAIL=1, if fitted then FITFAIL=0VARCHARprincipalHA_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalHA_MODSEL_EM_LINEModel selection score for the continuum-plus-emission-line fit compared to the straight-line continuum fitVARCHARprincipalHA_MODSEL_EMB_EMModel selection score for the continuum and Narrow+Broad emission-line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHA_MODSEL_NABS_NModel selection score for the continuum and Narrow emission plus absorption line fit compared to the continuum-plus-narrow line fitVARCHARprincipalHA_BFAnalytic approximation to the Baye's factor for the best modelVARCHARprincipalHA_DELBICChange in the Bayesian Information Criterion which compares the two modelsVARCHARprincipalHA_DELAICSimilar to BIC, not used in the model selectionVARCHARprincipalHA_CENFor the fits, the wavelength positions were measured with respect to this valueAVARCHARprincipalAMP_HAHA line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_ERRHA uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HAHA line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_ERRHA uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HAHA line sigma from Gaussian fitAVARCHARprincipalSIG_HA_ERRUncertainty on the HA line sigma from the Gaussian fitAVARCHARprincipalHA_FLUXHA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_FLUX_ERRHA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_EWHA line equivalent widthAVARCHARprincipalHA_EW_ERRHA equivalent width uncertaintyAVARCHARprincipalAMP_HA_ABSHA_ABS line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_ABS_ERRHA_ABS uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HA_ABSHA_ABS line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_ABS_ERRHA_ABS uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HA_ABSHA_ABS line sigma from Gaussian fitAVARCHARprincipalSIG_HA_ABS_ERRUncertainty on the HA_ABS line sigma from the Gaussian fitAVARCHARprincipalHA_ABS_FLUXHA_ABS line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_ABS_FLUX_ERRHA_ABS flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_ABS_EWHA_ABS line equivalent widthAVARCHARprincipalHA_ABS_EW_ERRHA_ABS equivalent width uncertaintyAVARCHARprincipalHA_ABS_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalAMP_HA_BHA_B line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_HA_B_ERRHA_B uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_HA_BHA_B line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_HA_B_ERRHA_B uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_HA_BHA_B line sigma from Gaussian fitAVARCHARprincipalSIG_HA_B_ERRUncertainty on the HA_B line sigma from the Gaussian fitAVARCHARprincipalHA_B_FLUXHA_B line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_B_FLUX_ERRHA_B flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_B_EWHA_B line equivalent widthAVARCHARprincipalHA_B_EW_ERRHA_B equivalent width uncertaintyAVARCHARprincipalHA_B_NPEGNumber of parameters pegged at their boundaries for gaussian fit to HAVARCHARprincipalAMP_NIIBNIIB line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIB_ERRNIIB uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIBNIIB line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIB_ERRNIIB uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIBNIIB line sigma from Gaussian fitAVARCHARprincipalSIG_NIIB_ERRUncertainty on the NIIB line sigma from the Gaussian fitAVARCHARprincipalNIIB_FLUXNIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_FLUX_ERRNIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_EWNIIB line equivalent widthAVARCHARprincipalNIIB_EW_ERRNIIB equivalent width uncertaintyAVARCHARprincipalAMP_NIIRNIIR line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalAMP_NIIR_ERRNIIR uncertainty on line amplitude from Gaussian fit (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalPOS_NIIRNIIR line position from Gaussian fit measured relative to HA_CENAVARCHARprincipalPOS_NIIR_ERRNIIR uncertainty on line position from Gaussian fitAVARCHARprincipalSIG_NIIRNIIR line sigma from Gaussian fitAVARCHARprincipalSIG_NIIR_ERRUncertainty on the NIIR line sigma from the Gaussian fitAVARCHARprincipalNIIR_FLUXNIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_FLUX_ERRNIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_EWNIIR line equivalent widthAVARCHARprincipalNIIR_EW_ERRNIIR equivalent width uncertaintyAVARCHARprincipalNIIB_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIBVARCHARprincipalNIIR_NPEGNumber of parameters pegged at their boundaries for gaussian fit to NIIRVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.DirectSummationv05This table provides direct summation line measurements for allspectra of those objects that have a best redshift with nQ > 1and 0.002 < z < 1.35.BH_MH_EW_ERRBH_MH equivalent width uncertaintymagVARCHARprincipalSPECIDUnique spectrum IDVARCHARprincipalCATAIDUnique GAMA object IDVARCHARprincipalRAJ2000degVARCHARprincipalDECJ2000degVARCHARprincipalZRedshift with heliocentric correction removedVARCHARprincipalNQRedshift qualityVARCHARprincipalSURVEYSurvey spectrum originated fromVARCHARprincipalSURVEY_CODENumerical code for originating surveyVARCHARprincipalIS_BESTSpectrum with best redshift for this object?VARCHARprincipalIS_SBESTSpectrum with best redshift for originating survey?VARCHARprincipalSNS/N ratio per pixel in the 6383 - 6536 A window in the galaxy frameVARCHARprincipalD4000N4000 A break strength (see notes for description)VARCHARprincipalD4000N_ERRUncertainty on the 4000 A break strengthVARCHARprincipalBH_NAD_CONTBH_NAD continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_NAD_EW_ERRBH_NAD equivalent width uncertaintymagVARCHARprincipalBH_NAD_EWBH_NAD line equivalent widthmagVARCHARprincipalBH_NAD_FLUX_ERRBH_NAD flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_NAD_FLUXBH_NAD line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_FC_CONTBH_FC continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_FC_EW_ERRBH_FC equivalent width uncertaintymagVARCHARprincipalBH_FC_EWBH_FC line equivalent widthmagVARCHARprincipalBH_FC_FLUX_ERRBH_FC flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_FC_FLUXBH_FC line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MH_CONTBH_MH continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_MH_EWBH_MH line equivalent widthmagVARCHARprincipalBH_MH_FLUX_ERRBH_MH flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MH_FLUXBH_MH line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MGG_CONTBH_MGG continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_MGG_EW_ERRBH_MGG equivalent width uncertaintymagVARCHARprincipalBH_MGG_EWBH_MGG line equivalent widthmagVARCHARprincipalBH_MGG_FLUX_ERRBH_MGG flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_MGG_FLUXBH_MGG line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HB_CONTBH_HB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_HB_EW_ERRBH_HB equivalent width uncertaintymagVARCHARprincipalBH_HB_EWBH_HB line equivalent widthmagVARCHARprincipalBH_HB_FLUX_ERRBH_HB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HB_FLUXBH_HB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_G_CONTBH_G continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_G_EW_ERRBH_G equivalent width uncertaintymagVARCHARprincipalBH_G_EWBH_G line equivalent widthmagVARCHARprincipalBH_G_FLUX_ERRBH_G flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_G_FLUXBH_G line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CAI_CONTBH_CAI continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_CAI_EW_ERRBH_CAI equivalent width uncertaintymagVARCHARprincipalBH_CAI_EWBH_CAI line equivalent widthmagVARCHARprincipalBH_CAI_FLUX_ERRBH_CAI flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CAI_FLUXBH_CAI line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HK_CONTBH_HK continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_HK_EW_ERRBH_HK equivalent width uncertaintymagVARCHARprincipalBH_HK_EWBH_HK line equivalent widthmagVARCHARprincipalBH_HK_FLUX_ERRBH_HK flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_HK_FLUXBH_HK line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CNB_CONTBH_CNB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalBH_CNB_EW_ERRBH_CNB equivalent width uncertaintymagVARCHARprincipalBH_CNB_EWBH_CNB line equivalent widthmagVARCHARprincipalBH_CNB_FLUX_ERRBH_CNB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalBH_CNB_FLUXBH_CNB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_CONTSIIR continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSIIR_EW_ERRSIIR equivalent width uncertaintyAVARCHARprincipalSIIR_EWSIIR line equivalent widthAVARCHARprincipalSIIR_FLUX_ERRSIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIR_FLUXSIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_CONTSIIB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSIIB_EW_ERRSIIB equivalent width uncertaintyAVARCHARprincipalSIIB_EWSIIB line equivalent widthAVARCHARprincipalSIIB_FLUX_ERRSIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIIB_FLUXSIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_CONTNIIR continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNIIR_EW_ERRNIIR equivalent width uncertaintyAVARCHARprincipalNIIR_EWNIIR line equivalent widthAVARCHARprincipalNIIR_FLUX_ERRNIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIR_FLUXNIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_CONTNIIB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNIIB_EW_ERRNIIB equivalent width uncertaintyAVARCHARprincipalNIIB_EWNIIB line equivalent widthAVARCHARprincipalNIIB_FLUX_ERRNIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNIIB_FLUXNIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_CONTHA continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHA_EW_ERRHA equivalent width uncertaintyAVARCHARprincipalHA_EWHA line equivalent widthAVARCHARprincipalHA_FLUX_ERRHA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHA_FLUXHA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6364_CONTOI6364 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI6364_EW_ERROI6364 equivalent width uncertaintyAVARCHARprincipalOI6364_EWOI6364 line equivalent widthAVARCHARprincipalOI6364_FLUX_ERROI6364 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6364_FLUXOI6364 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIII6312_CONTSIII6312 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalSIII6312_EW_ERRSIII6312 equivalent width uncertaintyAVARCHARprincipalSIII6312_EWSIII6312 line equivalent widthAVARCHARprincipalSIII6312_FLUX_ERRSIII6312 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalSIII6312_FLUXSIII6312 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6300_CONTOI6300 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOI6300_EW_ERROI6300 equivalent width uncertaintyAVARCHARprincipalOI6300_EWOI6300 line equivalent widthAVARCHARprincipalOI6300_FLUX_ERROI6300 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOI6300_FLUXOI6300 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO2_CONTTIO2 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalTIO2_EW_ERRTIO2 equivalent width uncertaintymagVARCHARprincipalTIO2_EWTIO2 line equivalent widthmagVARCHARprincipalTIO2_FLUX_ERRTIO2 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO2_FLUXTIO2 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO1_CONTTIO1 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalTIO1_EW_ERRTIO1 equivalent width uncertaintymagVARCHARprincipalTIO1_EWTIO1 line equivalent widthmagVARCHARprincipalTIO1_FLUX_ERRTIO1 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalTIO1_FLUXTIO1 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNA5895_CONTNA5895 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNA5895_EW_ERRNA5895 equivalent width uncertaintyAVARCHARprincipalNA5895_EWNA5895 line equivalent widthAVARCHARprincipalNA5895_FLUX_ERRNA5895 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNA5895_FLUXNA5895 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNII5755_CONTNII5755 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalNII5755_EW_ERRNII5755 equivalent width uncertaintyAVARCHARprincipalNII5755_EWNII5755 line equivalent widthAVARCHARprincipalNII5755_FLUX_ERRNII5755 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalNII5755_FLUXNII5755 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5782_CONTFE5782 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5782_EW_ERRFE5782 equivalent width uncertaintyAVARCHARprincipalFE5782_EWFE5782 line equivalent widthAVARCHARprincipalFE5782_FLUX_ERRFE5782 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5782_FLUXFE5782 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5709_CONTFE5709 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5709_EW_ERRFE5709 equivalent width uncertaintyAVARCHARprincipalFE5709_EWFE5709 line equivalent widthAVARCHARprincipalFE5709_FLUX_ERRFE5709 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5709_FLUXFE5709 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5406_CONTFE5406 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5406_EW_ERRFE5406 equivalent width uncertaintyAVARCHARprincipalFE5406_EWFE5406 line equivalent widthAVARCHARprincipalFE5406_FLUX_ERRFE5406 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5406_FLUXFE5406 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5335_CONTFE5335 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5335_EW_ERRFE5335 equivalent width uncertaintyAVARCHARprincipalFE5335_EWFE5335 line equivalent widthAVARCHARprincipalFE5335_FLUX_ERRFE5335 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5335_FLUXFE5335 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5270_CONTFE5270 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5270_EW_ERRFE5270 equivalent width uncertaintyAVARCHARprincipalFE5270_EWFE5270 line equivalent widthAVARCHARprincipalFE5270_FLUX_ERRFE5270 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5270_FLUXFE5270 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMGB5177_CONTMGB5177 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalMGB5177_EW_ERRMGB5177 equivalent width uncertaintyAVARCHARprincipalMGB5177_EWMGB5177 line equivalent widthAVARCHARprincipalMGB5177_FLUX_ERRMGB5177 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMGB5177_FLUXMGB5177 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG2_CONTMG2 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalMG2_EW_ERRMG2 equivalent width uncertaintymagVARCHARprincipalMG2_EWMG2 line equivalent widthmagVARCHARprincipalMG2_FLUX_ERRMG2 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG2_FLUXMG2 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG1_CONTMG1 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalMG1_EW_ERRMG1 equivalent width uncertaintymagVARCHARprincipalMG1_EWMG1 line equivalent widthmagVARCHARprincipalMG1_FLUX_ERRMG1 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalMG1_FLUXMG1 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5015_CONTFE5015 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE5015_EW_ERRFE5015 equivalent width uncertaintyAVARCHARprincipalFE5015_EWFE5015 line equivalent widthAVARCHARprincipalFE5015_FLUX_ERRFE5015 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE5015_FLUXFE5015 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_CONTOIIIR continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOIIIR_EW_ERROIIIR equivalent width uncertaintyAVARCHARprincipalOIIIR_EWOIIIR line equivalent widthAVARCHARprincipalOIIIR_FLUX_ERROIIIR flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIR_FLUXOIIIR line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_CONTOIIIB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOIIIB_EW_ERROIIIB equivalent width uncertaintyAVARCHARprincipalOIIIB_EWOIIIB line equivalent widthAVARCHARprincipalOIIIB_FLUX_ERROIIIB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIIIB_FLUXOIIIB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_P_CONTHB_P continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_P_EW_ERRHB_P equivalent width uncertaintyAVARCHARprincipalHB_P_EWHB_P line equivalent widthAVARCHARprincipalHB_P_FLUX_ERRHB_P flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_P_FLUXHB_P line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_CONTHB continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHB_EW_ERRHB equivalent width uncertaintyAVARCHARprincipalHB_EWHB line equivalent widthAVARCHARprincipalHB_FLUX_ERRHB flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHB_FLUXHB line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4668_CONTFE4668 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE4668_EW_ERRFE4668 equivalent width uncertaintyAVARCHARprincipalFE4668_EWFE4668 line equivalent widthAVARCHARprincipalFE4668_FLUX_ERRFE4668 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4668_FLUXFE4668 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4531_CONTFE4531 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE4531_EW_ERRFE4531 equivalent width uncertaintyAVARCHARprincipalFE4531_EWFE4531 line equivalent widthAVARCHARprincipalFE4531_FLUX_ERRFE4531 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4531_FLUXFE4531 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4455_CONTCA4455 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCA4455_EW_ERRCA4455 equivalent width uncertaintyAVARCHARprincipalCA4455_EWCA4455 line equivalent widthAVARCHARprincipalCA4455_FLUX_ERRCA4455 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4455_FLUXCA4455 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4383_CONTFE4383 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalFE4383_EW_ERRFE4383 equivalent width uncertaintyAVARCHARprincipalFE4383_EWFE4383 line equivalent widthAVARCHARprincipalFE4383_FLUX_ERRFE4383 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalFE4383_FLUXFE4383 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIII4363_CONTOIII4363 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOIII4363_EW_ERROIII4363 equivalent width uncertaintyAVARCHARprincipalOIII4363_EWOIII4363 line equivalent widthAVARCHARprincipalOIII4363_FLUX_ERROIII4363 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOIII4363_FLUXOIII4363 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA275_CONTHGVA275 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGVA275_EW_ERRHGVA275 equivalent width uncertaintymagVARCHARprincipalHGVA275_EWHGVA275 line equivalent widthmagVARCHARprincipalHGVA275_FLUX_ERRHGVA275 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA275_FLUXHGVA275 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA200_CONTHGVA200 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGVA200_EW_ERRHGVA200 equivalent width uncertaintymagVARCHARprincipalHGVA200_EWHGVA200 line equivalent widthmagVARCHARprincipalHGVA200_FLUX_ERRHGVA200 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA200_FLUXHGVA200 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA125_CONTHGVA125 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGVA125_EW_ERRHGVA125 equivalent width uncertaintymagVARCHARprincipalHGVA125_EWHGVA125 line equivalent widthmagVARCHARprincipalHGVA125_FLUX_ERRHGVA125 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGVA125_FLUXHGVA125 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGF_CONTHGF continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGF_EW_ERRHGF equivalent width uncertaintyAVARCHARprincipalHGF_EWHGF line equivalent widthAVARCHARprincipalHGF_FLUX_ERRHGF flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGF_FLUXHGF line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGA_CONTHGA continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHGA_EW_ERRHGA equivalent width uncertaintyAVARCHARprincipalHGA_EWHGA line equivalent widthAVARCHARprincipalHGA_FLUX_ERRHGA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHGA_FLUXHGA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalG4300_CONTG4300 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalG4300_EW_ERRG4300 equivalent width uncertaintyAVARCHARprincipalG4300_EWG4300 line equivalent widthAVARCHARprincipalG4300_FLUX_ERRG4300 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalG4300_FLUXG4300 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4227_CONTCA4227 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCA4227_EW_ERRCA4227 equivalent width uncertaintyAVARCHARprincipalCA4227_EWCA4227 line equivalent widthAVARCHARprincipalCA4227_FLUX_ERRCA4227 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCA4227_FLUXCA4227 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN2_CONTCN2 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCN2_EW_ERRCN2 equivalent width uncertaintymagVARCHARprincipalCN2_EWCN2 line equivalent widthmagVARCHARprincipalCN2_FLUX_ERRCN2 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN2_FLUXCN2 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN1_CONTCN1 continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalCN1_EW_ERRCN1 equivalent width uncertaintymagVARCHARprincipalCN1_EWCN1 line equivalent widthmagVARCHARprincipalCN1_FLUX_ERRCN1 flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalCN1_FLUXCN1 line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDF_CONTHDF continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHDF_EW_ERRHDF equivalent width uncertaintyAVARCHARprincipalHDF_EWHDF line equivalent widthAVARCHARprincipalHDF_FLUX_ERRHDF flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDF_FLUXHDF line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDA_CONTHDA continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalHDA_EW_ERRHDA equivalent width uncertaintyAVARCHARprincipalHDA_EWHDA line equivalent widthAVARCHARprincipalHDA_FLUX_ERRHDA flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalHDA_FLUXHDA line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOII_CONTOII continuum (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2/AVARCHARprincipalOII_EW_ERROII equivalent width uncertaintyAVARCHARprincipalOII_EWOII line equivalent widthAVARCHARprincipalOII_FLUX_ERROII flux uncertainty (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipalOII_FLUXOII line flux (NB: units only valid for SDSS and AAOmega spectra)10^(-17)erg/s/cm^2VARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.StellarMassesv24_LambdarCatv01catidCATAID from LambdarCatv01VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_dr4.StellarMassesv24_GAMAKidsVikingv02uberIDuberID from GAMAKidsVikingv02VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_dr4.StellarMassesv24_GAMAKidsVikingv01catidCATAID from GAMAKidsVikingv01VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_dr4.StellarMassesv24_G02SDSSInputCatv01catidCATAID from G02TilingCatv07.fitsVARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_zz-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_zstatistical uncertainty in absmag_zVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_z_starsintrinsic stellar z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_z_starsstatistical uncertainty in absmag_z_starsVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_zobservers frame z-band flux from SPS fitVARCHARprincipaldelfitflux_zstatistical uncertainty in fitflux_zVARCHARprincipalgama_dr4.StellarMassesv24_G02CFHTLSInputCatv04catidCATAID from G02TilingCatv07.fitsVARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_zz-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_zstatistical uncertainty in absmag_zVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_z_starsintrinsic stellar z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_z_starsstatistical uncertainty in absmag_z_starsVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_zobservers frame z-band flux from SPS fitVARCHARprincipaldelfitflux_zstatistical uncertainty in fitflux_zVARCHARprincipalgama_dr4.StellarMassesv24_21BandPhotomv03catidCATAID from 21BandPhotomv03VARCHARprincipalredshiftheliocentric redshift from DistancesFramesv14VARCHARprincipalcomovingdistcomoving distance, derived using Z_TONRY from DistancesFramesv14VARCHARprincipalnefffilteffective number of filters/bands used in SPS fitVARCHARprincipalsnrationet signal-to-noise across all filters/bands used for SPS fitVARCHARprincipalpppPosterior Predictive P-value goodness-of-fit statisticVARCHARprincipalnefftempeffective number of filters/bands contributing to SPS fitVARCHARprincipallogmstarstellar mass estimate in logarithmic solar unitsVARCHARprincipaldellogmstarstatistical uncertainty in logmstar stellar mass estimateVARCHARprincipalmstarstellar mass estimate in linear solar unitsVARCHARprincipaldelmstarstatistical uncertainty in mstar linear stellar mass estimateVARCHARprincipallogagetime since start of star formation in log yearsVARCHARprincipaldellogagestatistical uncertainty in logageVARCHARprincipallogtaustar formation history e-folding time in log yearsVARCHARprincipaldellogtaustatistical uncertainty in logtauVARCHARprincipallogmetstellar metallicity Z = log [O/H] (Z_sol = 0.02)VARCHARprincipaldellogmetstatistical uncertainty in logmetVARCHARprincipaldustEBVsingle screen dust extinction E(B-V)VARCHARprincipaldeldustEBVstatistical uncertainty in dustEBVVARCHARprincipallogmremnantsmass in subluminous stellar remanants in logarithmic solar unitsVARCHARprincipaldellogmremnantsstatistical uncertainty in logmremnantsVARCHARprincipallogmintsfhmass inferred from integration over the full SFHVARCHARprincipaldellogmintsfhstatistical uncertainty in logmintsfhVARCHARprincipallogLWagelight-weighted mean stellar age in log yearsVARCHARprincipaldellogLWagestatistical uncertainty in logLWageVARCHARprincipaluminusrrestframe (u-r) colourVARCHARprincipaldeluminusrstatistical uncertainty in uminusrVARCHARprincipaluminusr_starsintrinsic stellar (u-r) colour (corrected for internal dust)VARCHARprincipaldeluminusr_starsstatistical uncertainty in uminusr_starsVARCHARprincipalgminusirestframe (g-i) colourVARCHARprincipaldelgminusistatistical uncertainty in gminusiVARCHARprincipalgminusi_starsintrinsic stellar (g-i) colour (corrected for internal dust)VARCHARprincipaldelgminusi_starsstatistical uncertainty in gminusi_starsVARCHARprincipallogmoverl_ii-band mass-to-light ratio in AB-centric unitsVARCHARprincipaldellogmoverl_istatistical uncertainty in logmoverl_iVARCHARprincipalC_logM_gicorrelation coefficient for logmstar and gminusiVARCHARprincipalC_logM_gistarscorrelation coefficient for logmstar and gminusi_starsVARCHARprincipalC_logM_urcorrelation coefficient for logmstar and uminusrVARCHARprincipalC_logM_urstarscorrelation coefficient for logmstar and uminusr_starsVARCHARprincipalC_logM_logLWagecorrelation coefficient for logmstar and logLWageVARCHARprincipalC_logM_EBVcorrelation coefficient for logmstar and dustEBVVARCHARprincipalabsmag_FUVFUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUVstatistical uncertainty in absmag_FUVVARCHARprincipalabsmag_NUVNUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUVstatistical uncertainty in absmag_NUVVARCHARprincipalabsmag_uu-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_ustatistical uncertainty in absmag_uVARCHARprincipalabsmag_gg-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_gstatistical uncertainty in absmag_gVARCHARprincipalabsmag_rr-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_rstatistical uncertainty in absmag_rVARCHARprincipalabsmag_ii-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_istatistical uncertainty in absmag_iVARCHARprincipalabsmag_ZZ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Zstatistical uncertainty in absmag_ZVARCHARprincipalabsmag_YY-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Ystatistical uncertainty in absmag_YVARCHARprincipalabsmag_JJ-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Jstatistical uncertainty in absmag_JVARCHARprincipalabsmag_HH-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Hstatistical uncertainty in absmag_HVARCHARprincipalabsmag_KK-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Kstatistical uncertainty in absmag_KVARCHARprincipalabsmag_W1W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1statistical uncertainty in absmag_W1VARCHARprincipalabsmag_W2W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2statistical uncertainty in absmag_W2VARCHARprincipalabsmag_FUV_starsintrinsic stellar FUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_FUV_starsstatistical uncertainty in absmag_FUV_starsVARCHARprincipalabsmag_NUV_starsintrinsic stellar NUV-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_NUV_starsstatistical uncertainty in absmag_NUV_starsVARCHARprincipalabsmag_u_starsintrinsic stellar u-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_u_starsstatistical uncertainty in absmag_u_starsVARCHARprincipalabsmag_g_starsintrinsic stellar g-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_g_starsstatistical uncertainty in absmag_g_starsVARCHARprincipalabsmag_r_starsintrinsic stellar r-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_r_starsstatistical uncertainty in absmag_r_starsVARCHARprincipalabsmag_i_starsintrinsic stellar i-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_i_starsstatistical uncertainty in absmag_i_starsVARCHARprincipalabsmag_Z_starsintrinsic stellar Z-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Z_starsstatistical uncertainty in absmag_Z_starsVARCHARprincipalabsmag_Y_starsintrinsic stellar Y-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_Y_starsstatistical uncertainty in absmag_Y_starsVARCHARprincipalabsmag_J_starsintrinsic stellar J-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_J_starsstatistical uncertainty in absmag_J_starsVARCHARprincipalabsmag_H_starsintrinsic stellar H-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_H_starsstatistical uncertainty in absmag_H_starsVARCHARprincipalabsmag_K_starsintrinsic stellar K-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_K_starsstatistical uncertainty in absmag_K_starsVARCHARprincipalabsmag_W1_starsintrinsic stellar W1-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W1_starsstatistical uncertainty in absmag_W1_starsVARCHARprincipalabsmag_W2_starsintrinsic stellar W2-band absolute magnitude (restframe; AB)VARCHARprincipaldelabsmag_W2_starsstatistical uncertainty in absmag_W2_starsVARCHARprincipalfitflux_FUVobservers frame FUV-band flux from SPS fitVARCHARprincipaldelfitflux_FUVstatistical uncertainty in fitflux_FUVVARCHARprincipalfitflux_NUVobservers frame NUV-band flux from SPS fitVARCHARprincipaldelfitflux_NUVstatistical uncertainty in fitflux_NUVVARCHARprincipalfitflux_uobservers frame u-band flux from SPS fitVARCHARprincipaldelfitflux_ustatistical uncertainty in fitflux_uVARCHARprincipalfitflux_gobservers frame g-band flux from SPS fitVARCHARprincipaldelfitflux_gstatistical uncertainty in fitflux_gVARCHARprincipalfitflux_robservers frame r-band flux from SPS fitVARCHARprincipaldelfitflux_rstatistical uncertainty in fitflux_rVARCHARprincipalfitflux_iobservers frame i-band flux from SPS fitVARCHARprincipaldelfitflux_istatistical uncertainty in fitflux_iVARCHARprincipalfitflux_Zobservers frame Z-band flux from SPS fitVARCHARprincipaldelfitflux_Zstatistical uncertainty in fitflux_ZVARCHARprincipalfitflux_Yobservers frame Y-band flux from SPS fitVARCHARprincipaldelfitflux_Ystatistical uncertainty in fitflux_YVARCHARprincipalfitflux_Jobservers frame J-band flux from SPS fitVARCHARprincipaldelfitflux_Jstatistical uncertainty in fitflux_JVARCHARprincipalfitflux_Hobservers frame H-band flux from SPS fitVARCHARprincipaldelfitflux_Hstatistical uncertainty in fitflux_HVARCHARprincipalfitflux_Kobservers frame K-band flux from SPS fitVARCHARprincipaldelfitflux_Kstatistical uncertainty in fitflux_KVARCHARprincipalfitflux_W1observers frame W1-band flux from SPS fitVARCHARprincipaldelfitflux_W1statistical uncertainty in fitflux_W1VARCHARprincipalfitflux_W2observers frame W2-band flux from SPS fitVARCHARprincipaldelfitflux_W2statistical uncertainty in fitflux_W2VARCHARprincipalgama_dr4.VisualMorphologyv03This table provides a number of visual morphological classificationsperformed by various people for various samples of GAMA II galaxiesin the equatorial survey regions.CATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalELLIPTICALSimon`s and Stephen`s visual classificationmeta.code.classVARCHARprincipalELLIPTICAL_CODENumerical code for ELLIPTICAL, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPE_SPDSimon`s and Stephen`s visual Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_SPD_CODENumerical code for HUBBLE_TYPE_SPD, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPE_LSKLee`s and Uros` visual Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_LSK_CODENumerical code for HUBBLE_TYPE_LSK, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPE_ASGRAaron`s and Rebecca`s visual Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_ASGR_CODENumerical code for HUBBLE_TYPE_ASGR, see notesmeta.code.classVARCHARprincipalHUBBLE_TYPEFinal Hubble type classificationmeta.code.classVARCHARprincipalHUBBLE_TYPE_CODENumerical code for HUBBLE_TYPE, see notesmeta.code.classVARCHARprincipalASGR_DISTURBEDRenormalised votes that galaxy is disturbed, see notesmeta.code.classVARCHARprincipalASGR_NORMALRenormalised votes that galaxy is undisturbed, see notesmeta.code.classVARCHARprincipalASGR_UNSURERenormalised votes that classification in unclearmeta.code.classVARCHARprincipalASGR_CLASSIFIERSTotal number of classifiers (renormalised)meta.code.classVARCHARprincipalASGR_PROBDISTProbability galaxy is disturbed (ASGR_DISTURBED/ASGR_CLASSIFIERS)meta.code.classVARCHARprincipalP_ELFraction of Galaxy Zoo votes for Elliptical (biased)meta.code.classVARCHARprincipalP_CSFraction of Galaxy Zoo votes for NotElliptical (biased)meta.code.classVARCHARprincipalP_EL_DEBIASEDFraction of Galaxy Zoo votes for Elliptical (debiased)meta.code.classVARCHARprincipalP_CS_DEBIASEDFraction of Galaxy Zoo votes for NotElliptical (debiased)meta.code.classVARCHARprincipalURL_IMGURL of SDSS/UKIDSS-LAS/VIKING giH postage stampmeta.ref.url;meta.fileVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.WISECatv02This table provides mid-IR photometry from WISE for all objects inthe GAMA II equatorial survey regions detected by WISE.CATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalDESIG_ALLWISEDesignation of matched WISE source from AllWISE Cataloguemeta.id.crossVARCHARprincipalDESIG_ALLSKYDesignation of matched WISE source from All-Sky Cataloguemeta.id.crossVARCHARprincipalRARight ascension (J2000) of matched WISE sourcedegpos.eq.raVARCHARprincipalDECDeclination (J2000) of matched WISE sourcedegpos.eq.decVARCHARprincipalSEPARATIONDistance between GAMA object and matched WISE sourcearcsecpos.angDistanceVARCHARprincipalW1MNumber of individual W1 exposures on which profile-fit was possibleVARCHARprincipalW2MNumber of individual W2 exposures on which profile-fit was possibleVARCHARprincipalW3MNumber of individual W3 exposures on which profile-fit was possibleVARCHARprincipalW4MNumber of individual W4 exposures on which profile-fit was possibleVARCHARprincipalW1COVMean pixel coverage in W1VARCHARprincipalW2COVMean pixel coverage in W2VARCHARprincipalW3COVMean pixel coverage in W3VARCHARprincipalW4COVMean pixel coverage in W4VARCHARprincipalMAG_W1Recommended W1 magnitudemagphot.mag;em.IR.3-4umVARCHARprincipalMAGERR_W1Recommended W1 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W1Recommended W1 photometry flag: 1=profile-fit, 2=isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W1Radius of aperture measurement in W1arcsecphys.angSizeVARCHARprincipalMAGPRO_W1Profile-fit W1 magnitudemagphot.mag;em.IR.3-4umVARCHARprincipalMAGPROERR_W1Profile-fit W1 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W1Reduced chi^2 of profile-fit W1 measurementstat.fit.chi2VARCHARprincipalFLUX_W1Raw W1 source flux measured in profile-fit photometrymJyphot.flux;em.IR.3-4umVARCHARprincipalFLUXERR_W1Uncertainty in the raw W1 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W1Standard aperture magnitude for W1magphot.mag;em.IR.3-4umVARCHARprincipalMAGSTDAPERR_W1Standard aperture magnitude error for W1magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W1Standard aperture magnitude flag for W1meta.codeVARCHARprincipalRADIUS_ISO_W1Isophotal radius in W1arcsecphys.angSizeVARCHARprincipalMAGISO_W1Isophotal W1 magnitudemagphot.mag;em.IR.3-4umVARCHARprincipalMAGISOERR_W1Isophotal W1 magnitude errormagstat.error;phot.magVARCHARprincipalMAG_W2Recommended W2 magnitudemagphot.mag;em.IR.4-8umVARCHARprincipalMAGERR_W2Recommended W2 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W2Recommended W2 photometry flag: 1=profile-fit, 2=derived from isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W2Radius of aperture measurement in W2arcsecphys.angSizeVARCHARprincipalMAGPRO_W2Profile-fit W2 magnitudemagphot.mag;em.IR.4-8umVARCHARprincipalMAGPROERR_W2Profile-fit W2 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W2Reduced chi^2 of profile-fit W2 measurementstat.fit.chi2VARCHARprincipalFLUX_W2Raw W2 source flux measured in profile-fit photometrymJyphot.flux;em.IR.4-8umVARCHARprincipalFLUXERR_W2Uncertainty in the raw W2 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W2Standard aperture magnitude for W2magphot.mag;em.IR.4-8umVARCHARprincipalMAGSTDAPERR_W2Standard aperture magnitude error for W2magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W2Standard aperture magnitude flag for W2meta.codeVARCHARprincipalRADIUS_ISO_W2Isophotal radius in W2arcsecphys.angSizeVARCHARprincipalMAGISO_W2Isophotal W2 magnitudemagphot.mag;em.IR.4-8umVARCHARprincipalMAGISOERR_W2Isophotal W2 magnitude errormagstat.error;phot.magVARCHARprincipalMAGDER_W2Derived W2 magnitude (from MAGISO_W1 and W1-W2 colour)magphot.mag;em.IR.4-8umVARCHARprincipalMAGDERERR_W2Derived W2 magnitude errormagstat.error;phot.magVARCHARprincipalMAG_W3Recommended W3 magnitudemagphot.mag;em.IR.8-15umVARCHARprincipalMAGERR_W3Recommended W3 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W3Recommended W3 photometry flag: 1=profile-fit, 2=isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W3Radius of aperture measurement in W3arcsecphys.angSizeVARCHARprincipalMAGPRO_W3Profile-fit W3 magnitudemagphot.mag;em.IR.8-15umVARCHARprincipalMAGPROERR_W3Profile-fit W3 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W3Reduced chi^2 of profile-fit W3 measurementstat.fit.chi2VARCHARprincipalFLUX_W3Raw W3 source flux measured in profile-fit photometrymJyphot.flux;em.IR.8-15umVARCHARprincipalFLUXERR_W3Uncertainty in the raw W3 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W3Standard aperture magnitude for W3magphot.mag;em.IR.8-15umVARCHARprincipalMAGSTDAPERR_W3Standard aperture magnitude error for W3magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W3Standard aperture magnitude flag for W3meta.codeVARCHARprincipalRADIUS_ISO_W3Isophotal radius in W3arcsecphys.angSizeVARCHARprincipalMAGISO_W3Isophotal W3 magnitudemagphot.mag;em.IR.8-15umVARCHARprincipalMAGISOERR_W3Isophotal W3 magnitude errormagstat.error;phot.magVARCHARprincipalMAG_W4Recommended W4 magnitudemagphot.mag;em.IR.15-30umVARCHARprincipalMAGERR_W4Recommended W4 magnitude errormagstat.error;phot.magVARCHARprincipalPHOTFLAG_W4Recommended W4 photometry flag: 1=profile-fit, 2=derived from isophotal, 3=standard aperture, -1=upper limit or nullmeta.codeVARCHARprincipalRADIUS_W4Radius of aperture measurement in W4arcsecphys.angSizeVARCHARprincipalMAGPRO_W4Profile-fit W4 magnitudemagphot.mag;em.IR.15-30umVARCHARprincipalMAGPROERR_W4Profile-fit W4 magnitude errormagstat.error;phot.magVARCHARprincipalREDUCED_CHI_W4Reduced chi^2 of profile-fit W4 measurementstat.fit.chi2VARCHARprincipalFLUX_W4Raw W4 source flux measured in profile-fit photometrymJyphot.flux;em.IR.15-30umVARCHARprincipalFLUXERR_W4Uncertainty in the raw W4 source flux measurementmJystat.error;phot.fluxVARCHARprincipalMAGSTDAP_W4Standard aperture magnitude for W4magphot.mag;em.IR.15-30umVARCHARprincipalMAGSTDAPERR_W4Standard aperture magnitude error for W4magstat.error;phot.magVARCHARprincipalMAGSTDAPFLAG_W4Standard aperture magnitude flag for W4meta.codeVARCHARprincipalRADIUS_ISO_W4Isophotal radius in W4arcsecphys.angSizeVARCHARprincipalMAGISO_W4Isophotal W4 magnitudemagphot.mag;em.IR.15-30umVARCHARprincipalMAGISOERR_W4Isophotal W4 magnitude errormagstat.error;phot.magVARCHARprincipalMAGDER_W4Derived W4 magnitude (from MAGISO_W3 and W3-W4 colour)magphot.mag;em.IR.15-30umVARCHARprincipalMAGDERERR_W4Derived W4 magnitude errormagstat.error;phot.magVARCHARprincipalXSCPROXDistance between WISE source and nearest 2MASS XSC sourcearcsecpos.angDistanceVARCHARprincipalBA_ISOAxis ratio of the isophotal ellipse in W1phys.size.axisRatioVARCHARprincipalPA_ISOPosition angle (E of N) of the isophotal ellipse in W1degpos.posAngVARCHARprincipalRFUZZYMeasure of resolvedness of WISE source, see notesarcsecVARCHARprincipalNAActive deblend flagmeta.codeVARCHARprincipalNBNumber of deblended componentsmeta.numberVARCHARprincipalCC_FLAGSContamination and confusion flag, see notesmeta.codeVARCHARprincipalDeblendedFractionLAMBDAR deblended fraction, see notesarith.ratioVARCHARprincipalSApFlagStandard Aperture Deblend Flag, see notesmeta.codeVARCHARprincipalNnearSApNumber of intersecting Standard Apertures, see notesmeta.numberVARCHARprincipalGApFlagGAMA Aperture Deblend Flag, see notesmeta.codeVARCHARprincipalNnearGApNumber of intersecting GAMA objects, see notesmeta.numberVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.XXLPointSourceProbsv01For several different reasons (see notes), 33 x-ray sources werematched manually to GAMA objects. These were visually inspected andthe results recorded in this table. Some of the objects in thiscatalogue also appear in XXLPointSourceAssoc. This catalogue is oneof the outputs of the GAMA/XXL Matching Group. It was produced byAngela Bongiorno and was not modified in any way.XIDXXL identifiermeta.id;meta.mainVARCHARindexedprincipalXNAMEXXL namemeta.idVARCHARprincipalRARA of x-ray source (J200)degpos.eq.raVARCHARprincipalDECDec of x-ray source (J2000)degpos.eq.decVARCHARprincipalCOUNTS_SOFTCounts in the 0.5-2.0 keV bandVARCHARprincipalCOUNTS_HARDCounts in the 2-10 keV bandVARCHARprincipalDISTDistance between XXL source and GAMA objectarcsecpos.angDistanceVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalCOMMENTComment from visual inspectionVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.XXLPointSourceCatv01This catalogue provides XXL photometry of XMM detected point sourcesin the G02 survey region. Specifically, it contains the x-rayproperties of those XMM point source detections that have a matchamong GAMA spectra (i.e. those that appear in the tableXXLPointSourceAssoc). This catalogue is one of the outputs of theGAMA/XXL Matching Group. It was produced by Angela Bongiorno and wasnot modified in any way.XIDXXL identifiermeta.id;meta.mainVARCHARindexedprincipalXNAMEXXL namemeta.idVARCHARprincipalRARA of x-ray source (J2000)degpos.eq.raVARCHARprincipalDECDec of x-ray source (J2000)degpos.eq.decVARCHARprincipalCOUNTS_SOFTCounts in the 0.5-2.0 keV bandVARCHARprincipalCOUNTS_HARDCounts in the 2-10 keV bandVARCHARprincipalFLUX_SOFTAveraged flux in the 0.5-2.0 keV banderg/s/cm^2VARCHARprincipalFLUX_HARDAveraged flux in the 2-10 keV banderg/s/cm^2VARCHARprincipalgama_dr4.XXLPointSourceAssocv01This catalogue provides the result of matching XXL point sourceswith GAMA objects. It contains the properties of the associationbetween an XXL point source and a GAMA object in the G02 surveyregion. Both the x-ray sources and the GAMA objects in thiscatalogue may appear multiple times. This catalogue is one of theoutputs of the GAMA/XXL Matching Group. It was produced by AngelaBongiorno and was not modified in any way.MATCHIDUnique ID of association between XXL point source and GAMA objectmeta.id;meta.mainVARCHARindexedprincipalXIDXXL IDmeta.idVARCHARprincipalXNAMEName of XXL sourcemeta.idVARCHARprincipalDISTDistance between XXL source and GAMA objectarcsecpos.angDistanceVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalZ_FLAG_ASSOCQuality of the match: 3=secure, 2=unsecure, 0=unsure, -1=no association, see notesmeta.code.qualVARCHARprincipalSECURE_ASSOCFlag indicating matches with Z_FLAG_ASSOC=3VARCHARprincipalUNSECURE_ASSOCFlag indicating matches with Z_FLAG_ASSOC=2VARCHARprincipalUNSURE_ASSOCFlag indicating matches with Z_FLAG_ASSOC=0VARCHARprincipalNO_ASSOCFlag indicating matches with Z_FLAG_ASSOC=-1VARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.XXLClusterCatv01This catalogue provides the x-ray properties and cluster redshiftsof XXL clusters that were matched to GAMA objects (i.e. those thatappear in the table XXLClusterAssoc). This catalogue is one of theoutputs of the GAMA/XXL Matching Group. It was produced by TatyanaSadibekova and was not modified in any way.CLUSTERIDUnique ID of a combination of XXL source and cluster redshiftmeta.id;meta.mainVARCHARindexedprincipalXIDXXL ID of clustermeta.idVARCHARprincipalXNAMEXXL name of clustermeta.idVARCHARprincipalRARA of XXL clusterdegpos.eq.raVARCHARprincipalDECDec of XXL clusterdegpos.eq.decVARCHARprincipalFLUXSOFTPipeline flux in 0.5-2 keV band, see notes10^(-14)erg/s/cm^2VARCHARprincipalEXTSOFTPipeline extension, see notesarcsecVARCHARprincipalFLUX60Flux measured within r=60" aperture in 0.5-2 keV band, see notes10^(-14)erg/s/cm^2VARCHARprincipalTX60Temperature measured from x-ray spectrum within 60" aperture, see noteskeVVARCHARprincipalZ_CLSpectroscopic redshift used for the correlation within 2 MpcVARCHARprincipalR_2MPCMatching radius corresponding to 2 Mpcarcminpos.angDistanceVARCHARprincipalN_GALNumber of GAMA objects matched within 2 MpcVARCHARprincipalMULTMultiplicity of XXL source (number of projected optical clusters), see notesVARCHARprincipalgama_dr4.XXLClusterAssocv01This catalogue provides the result of matching GAMA objects to XXLclusters in the G02 survey region. Both the x-ray sources and theGAMA objects in this catalogue may appear multiple times. Thiscatalogue is one of the outputs of the GAMA/XXL Matching Group. Itwas produced by Tatyana Sadibekova and was not modified in any way.MATCHIDUnique ID of association between XXL cluster and GAMA objectmeta.id;meta.mainVARCHARindexedprincipalXIDXXL ID of matched clustermeta.idVARCHARprincipalXNAMEXXL name of matched clustermeta.idVARCHARprincipalSEPLinear separation between the XXL cluster and the GAMA objectMpcpos.distanceVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.idVARCHARprincipalGAMA_NAMEName of GAMA objectmeta.idVARCHARprincipalSPECIDUnique ID of GAMA spectrummeta.idVARCHARprincipalRARA of spectrum (J2000)degpos.eq.raVARCHARprincipalDECDec of spectrum (J2000)degpos.eq.decVARCHARprincipalN_SPECNumber of spectra available for a GAMA positionVARCHARprincipalZ_GAMARedshift from GAMAsrc.redshiftVARCHARprincipalNQNormalised redshift quality (use nQ > 2 for science)meta.code.qual;src.redshiftVARCHARprincipalSYSNOIndex for optical system (can be >1 if there is more than one counterpart)VARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23kcorr_z02v01This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G23 survey region, basedon KiDS i-band and VIKING AUTO magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23kcorr_z01v01This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G23 survey region, basedon KiDS i-band and VIKING AUTO magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G23kcorr_z00v01This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G23 survey region, basedon KiDS i-band and VIKING AUTO magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_I_1Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_2Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_3Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_4Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalPCOEFF_I_5Coefficient of polynomial fit to K(z) in SDSS i bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02kcorr_z02v01This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G02 survey region, basedon CFHTLS AUTO magnitudes, where available, and SDSS modelmagnitudes otherwise.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02kcorr_z01v01This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G02 survey region, basedon CFHTLS AUTO magnitudes, where available, and SDSS modelmagnitudes otherwise.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.G02kcorr_z00v01This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II G02 survey region, basedon CFHTLS AUTO magnitudes, where available, and SDSS modelmagnitudes otherwise.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Eqkcorr_model_z02v05This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on SDSS DR7 model magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Eqkcorr_model_z01v05This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on SDSS DR7 model magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Eqkcorr_model_z00v05This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on SDSS DR7 model magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Eqkcorr_auto_z02v05This table provides k-corrections at redshift 0.2 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on GAMA matched aperture magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Eqkcorr_auto_z01v05This table provides k-corrections at redshift 0.1 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on GAMA matched aperture magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.Eqkcorr_auto_z00v05This table provides k-corrections at redshift 0.0 in the GALEX FUVand NUV bands, the SDSS ugriz bands and the UKIDSS YJHK bands forall galaxies with redshifts in the GAMA II equatorial surveyregions, based on GAMA matched aperture magnitudes.CATAIDUnique GAMA IDmeta.id;meta.mainVARCHARindexedprincipalZ_TONRYFlow corrected redshift using Tonry et al. modelsrc.redshiftVARCHARprincipalNQRedshift qualitymeta.code.qual;src.redshiftVARCHARprincipalKCORR_FUVK-correction in GALEX FUV bandmagphot.mag;em.UV.100-200nmVARCHARprincipalKCORR_NUVK-correction in GALEX NUV bandmagphot.mag;em.UV.200-300nmVARCHARprincipalKCORR_UK-correction in SDSS u bandmagphot.mag;em.opt.UVARCHARprincipalKCORR_GK-correction in SDSS g bandmagphot.mag;em.opt.GVARCHARprincipalKCORR_RK-correction in SDSS r bandmagphot.mag;em.opt.RVARCHARprincipalKCORR_IK-correction in SDSS i bandmagphot.mag;em.opt.IVARCHARprincipalKCORR_ZK-correction in SDSS z bandmagphot.mag;em.opt.ZVARCHARprincipalKCORR_YK-correction in UKIDSS Y bandmagphot.mag;em.IR.NIRVARCHARprincipalKCORR_JK-correction in UKIDSS J bandmagphot.mag;em.IR.JVARCHARprincipalKCORR_HK-correction in UKIDSS H bandmagphot.mag;em.IR.HVARCHARprincipalKCORR_KK-correction in UKIDSS K bandmagphot.mag;em.IR.KVARCHARprincipalPCOEFF_R_1Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_2Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_3Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_4Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalPCOEFF_R_5Coefficient of polynomial fit to K(z) in SDSS r bandarith.factorVARCHARprincipalCOEFFS_1kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_2kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_3kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_4kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCOEFFS_5kcorrect eigenspectra coefficientarith.factorVARCHARprincipalCHI2Chi^2 of fit returned by kcorrectstat.fit.chi2VARCHARprincipalMASSStellar mass of currently surviving starsM_solarphys.massVARCHARprincipalINTSFHTotal integrated star-formation history (number of stars formed total)meta.numberVARCHARprincipalMETSAverage metallicity of currently surviving starsphys.abund.ZVARCHARprincipalB300Fraction of the total star formation that has occurred in the last 0.3 Gyrarith.ratioVARCHARprincipalB1000Fraction of the total star formation that has occurred in the last 1 Gyrarith.ratioVARCHARprincipaluberIDClassifier from GAMAKidsVikingv01. Column added by Data Central from gkvCATAIDMatchv01 (gkvInputCat) and by crossmatching CATAIDmeta.idVARCHARprincipalgama_dr4.gkvCATAIDMatchv01Ancillary data product to accompany the gkvInputCat. For each CATAID in the TilingCat, this catalogue identifies the corresponding object in thenew ProFound photometry catalogue. This is intended to be particularly useful to identifythe segment ID of objects whose CATAIDs were not matched to a new segment, as can be possible ifa single ProFound segment contains more than one CATAID object. See Bellstedt et al. (2020, MNRAS, 496, 3235 - https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3235B/abstraCATAIDID of objectmeta.idVARCHARprincipalRARight Ascension of object from TilingCatdegpos.eq.raVARCHARprincipalDECDeclination of object from TilingCatdegpos.eq.decVARCHARprincipalsegIDSegment ID as given by ProFound of the segment encompassing the object coordinates. If duplicates exist, the segment containing the most flux is chosen.meta.idVARCHARprincipaluberIDCorresponding unique identifier of the segment. If duplicates exist, the segment containing the most flux is chosen.meta.idVARCHARprincipaluberID_allUnique identifiers of all segments containing the object. For objects in the duplicated borders of tiles, multiple matches will exist.meta.idVARCHARprincipalframeTile containing the segmentmeta.idVARCHARprincipalframeDistDistance between object and the tile centrepixVARCHARprincipalrZmagproFound magnitude of the objects as measured in the detection band (r+Z stack).magphot.magVARCHARprincipalgama_dr4.gkvScienceCatv02ProFound segments have been visually regrouped to fix instances of fragmentation. Source detection is conducted on an r+Z stack of the image. After visual fixing of segment fragmentation, profoundMultiBand is implemented to extract photometry in the FUV-W2 bands. All fluxes and flux errors have been corrected for the foreground Galactic extinction (as given by the EBV value). See Bellstedt et al. (2020, MNRAS, 496, 3235 - https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3235B/abstract) for detailFrameNameName of frame that the object comes frommeta.idVARCHARprincipalFrameIDID of the frame that the object comes frommeta.idVARCHARprincipaluberIDUnique identifier of the objectmeta.idVARCHARprincipalsegIDSegment ID as given by ProFound of the object (unique within the frame, but not within the larger catalogue).meta.idVARCHARprincipalx_maxx position of the maximum fluxpixposVARCHARprincipaly_maxy position of the maximum fluxpixposVARCHARprincipalcensepOffset between the object and the frame centrepixVARCHARprincipalRAcenRight Ascension of flux-weighted centre (ICRS J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of flux-weighted centre (ICRS J2000)degpos.eq.decVARCHARprincipalRAmaxRight Ascension of maximum flux (ICRS J2000)degpos.eq.raVARCHARprincipalDecmaxDeclination of maximum flux (ICRS J2000)degpos.eq.decVARCHARprincipalRAGAIARight Ascension of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.raVARCHARprincipalDecGAIADeclination of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.decVARCHARprincipalsky_meanMean flux of the sky over all segment pixelsJyVARCHARprincipalskyRMS_meanMean value of the sky RMS over all segment pixelsJyVARCHARprincipallog10seeingSeeing, calculated as the median R50 value for objects with R50<2, Zmag>16 and Zmag<17log(arcsec)VARCHARprincipalEBVGalactic extinction, based on Planck E(B-V) values.magVARCHARprincipalmagMagnitude in the r+Z detection bandmagphot.magVARCHARprincipalR50Approximate elliptical semi-major axis containing 50% of the fluxarcsecphys.size.radiusVARCHARprincipalR90Approximate elliptical semi-major axis containing 90% of the fluxarcsecphys.size.radiusVARCHARprincipalR100Approximate elliptical semi-major axis containing 100% of the fluxarcsecphys.size.radiusVARCHARprincipalN100Total number of pixels in this segmentphys.areaVARCHARprincipalaxratAxial ratioVARCHARprincipalangOrientation of the semi-major axisdegpos.posAngVARCHARprincipalgroupIDID of the group containing the segment (unique within the frame, but not within the larger catalogue)meta.idVARCHARprincipalNgroupNumber of segments contained within the groupmeta.numberVARCHARprincipalmag_app_ZtAperture magnitude in Z-band (based on the 1.4 arcsec fibre aperture)magphot.mag;em.opt.Z;VARCHARprincipalflux_FUVtTotal flux (FUV band) - using global sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_FUVlLocal flux (FUV band) - using local sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_err_FUVtFlux err (FUV band)Jyphot.flux.density;em.UV.100-200nm;stat.err;VARCHARprincipalflux_NUVtTotal flux (NUV band) - using global sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_NUVlLocal flux (NUV band) - using local sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_err_NUVtFlux err (NUV band)Jyphot.flux.density;em.UV.200-300nm;stat.err;VARCHARprincipalflux_utTotal flux (u band) - using global sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_ulLocal flux (u band) - using local sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_err_utFlux err (u band)Jyphot.flux.density;em.opt.U;stat.err;VARCHARprincipalflux_gtTotal flux (g band) - using global sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_glLocal flux (g band) - using local sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_err_gtFlux err (g band)Jyphot.flux.density;em.opt.G;stat.err;VARCHARprincipalflux_rtTotal flux (r band) - using global sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_rlLocal flux (r band) - using local sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_err_rtFlux err (r band)Jyphot.flux.density;em.opt.R;stat.err;VARCHARprincipalflux_itTotal flux (i band) - using global sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_ilLocal flux (i band) - using local sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_err_itFlux err (i band)Jyphot.flux.density;em.opt.I;stat.err;VARCHARprincipalflux_ZtTotal flux (Z band) - using global sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_ZlLocal flux (Z band) - using local sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_err_ZtFlux err (Z band)Jyphot.flux.density;em.opt.Z;stat.err;VARCHARprincipalflux_YtTotal flux (Y band) - using global sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_YlLocal flux (Y band) - using local sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_err_YtFlux err (Y band)Jyphot.flux.density;em.IR.Y;stat.err;VARCHARprincipalflux_JtTotal flux (J band) - using global sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_JlLocal flux (J band) - using local sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_err_JtFlux err (J band)Jyphot.flux.density;em.IR.J;stat.err;VARCHARprincipalflux_HtTotal flux (H band) - using global sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_HlLocal flux (H band) - using local sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_err_HtFlux err (H band)Jyphot.flux.density;em.IR.H;stat.err;VARCHARprincipalflux_KtTotal flux (Ks band) - using global sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_KlLocal flux (Ks band) - using local sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_err_KtFlux err (Ks band)Jyphot.flux.density;em.IR.K;stat.err;VARCHARprincipalflux_W1tTotal flux (W1 band) - using global sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_W1lLocal flux (W1 band) - using local sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_err_W1tFlux err (W1 band)Jyphot.flux.density;em.IR.3-4um;stat.err;VARCHARprincipalflux_W2tTotal flux (W2 band) - using global sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_W2lLocal flux (W2 band) - using local sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_err_W2tFlux err (W2 band)Jyphot.flux.density;em.IR.4-8um;stat.err;VARCHARprincipalduplicateFlag indicating if object is duplicated due to tile overlapmeta.code.classVARCHARprincipalmaskFlag indicating if object is within GAMA regionmeta.code.classVARCHARprincipalstarmaskFlag indicating if object is within a star maskmeta.code.classVARCHARprincipalstarscolStellar colour flagmeta.code.classVARCHARprincipalstarssizeStellar size flagmeta.code.classVARCHARprincipalclassAutomatic classification of objectmeta.code.classVARCHARprincipaleyeclassVisual classification of objectmeta.code.classVARCHARprincipaluberclassFinal classification of objectmeta.code.classVARCHARprincipalnoOPTFlag indicating optical data is not presentmeta.code.classVARCHARprincipalnoIRFlag indicating IR data is not presentmeta.code.classVARCHARprincipalCATAIDID of objectmeta.id.cross;meta.mainVARCHARprincipalNQRedshift quality flagmeta.code.qual;src.redshiftVARCHARprincipalZSpectroscopic redshiftsrc.redshiftVARCHARprincipalSCScience class flag. Values from 0-5 indicate progresively harsher cuts.meta.code.classVARCHARprincipalgama_dr4.gkvInputCatv02ProFound segments have been visually regrouped to fix instances of fragmentation. Source detection is conducted on an r+Z stack of the image. After visual fixing of segment fragmentation, profoundMultiBand is implemented to extract photometry in the FUV-W2 bands. All fluxes and flux errors have been corrected for the foreground Galactic extinction (as given by the EBV value). See Bellstedt et al. (2020, MNRAS, 496, 3235 - https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.3235B/abstract) for detailFrameNameName of frame that the object comes frommeta.idVARCHARprincipalFrameIDID of the frame that the object comes frommeta.idVARCHARprincipaluberIDUnique identifier of the objectmeta.idVARCHARprincipalsegIDSegment ID as given by ProFound of the object (unique within the frame, but not within the larger catalogue).meta.idVARCHARprincipalx_maxx position of the maximum fluxpixposVARCHARprincipaly_maxy position of the maximum fluxpixposVARCHARprincipalcensepOffset between the object and the frame centrepixVARCHARprincipalRAcenRight Ascension of flux-weighted centre (ICRS J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of flux-weighted centre (ICRS J2000)degpos.eq.decVARCHARprincipalRAmaxRight Ascension of maximum flux (ICRS J2000)degpos.eq.raVARCHARprincipalDecmaxDeclination of maximum flux (ICRS J2000)degpos.eq.decVARCHARprincipalRAGAIARight Ascension of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.raVARCHARprincipalDecGAIADeclination of maximum flux, corrected for GAIA offset (ICRS J2000)degpos.eq.decVARCHARprincipalsky_meanMean flux of the sky over all segment pixelsJyVARCHARprincipalskyRMS_meanMean value of the sky RMS over all segment pixelsJyVARCHARprincipallog10seeingSeeing, calculated as the median R50 value for objects with R50<2, Zmag>16 and Zmag<17log(arcsec)VARCHARprincipalEBVGalactic extinction, based on Planck E(B-V) values.magVARCHARprincipalmagMagnitude in the r+Z detection bandmagphot.magVARCHARprincipalR50Approximate elliptical semi-major axis containing 50% of the fluxarcsecphys.size.radiusVARCHARprincipalR90Approximate elliptical semi-major axis containing 90% of the fluxarcsecphys.size.radiusVARCHARprincipalR100Approximate elliptical semi-major axis containing 100% of the fluxarcsecphys.size.radiusVARCHARprincipalN100Total number of pixels in this segmentphys.areaVARCHARprincipalaxratAxial ratioVARCHARprincipalangOrientation of the semi-major axisdegpos.posAngVARCHARprincipalgroupIDID of the group containing the segment (unique within the frame, but not within the larger catalogue)meta.idVARCHARprincipalNgroupNumber of segments contained within the groupmeta.numberVARCHARprincipalmag_app_ZtAperture magnitude in Z-band (based on the 1.4 arcsec fibre aperture)magphot.mag;em.opt.Z;VARCHARprincipalflux_FUVtTotal flux (FUV band) - using global sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_FUVlLocal flux (FUV band) - using local sky subtractionJyphot.flux.density;em.UV.100-200nm;VARCHARprincipalflux_err_FUVtFlux err (FUV band)Jyphot.flux.density;em.UV.100-200nm;stat.err;VARCHARprincipalflux_NUVtTotal flux (NUV band) - using global sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_NUVlLocal flux (NUV band) - using local sky subtractionJyphot.flux.density;em.UV.200-300nm;VARCHARprincipalflux_err_NUVtFlux err (NUV band)Jyphot.flux.density;em.UV.200-300nm;stat.err;VARCHARprincipalflux_utTotal flux (u band) - using global sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_ulLocal flux (u band) - using local sky subtractionJyphot.flux.density;em.opt.U;VARCHARprincipalflux_err_utFlux err (u band)Jyphot.flux.density;em.opt.U;stat.err;VARCHARprincipalflux_gtTotal flux (g band) - using global sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_glLocal flux (g band) - using local sky subtractionJyphot.flux.density;em.opt.G;VARCHARprincipalflux_err_gtFlux err (g band)Jyphot.flux.density;em.opt.G;stat.err;VARCHARprincipalflux_rtTotal flux (r band) - using global sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_rlLocal flux (r band) - using local sky subtractionJyphot.flux.density;em.opt.R;VARCHARprincipalflux_err_rtFlux err (r band)Jyphot.flux.density;em.opt.R;stat.err;VARCHARprincipalflux_itTotal flux (i band) - using global sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_ilLocal flux (i band) - using local sky subtractionJyphot.flux.density;em.opt.I;VARCHARprincipalflux_err_itFlux err (i band)Jyphot.flux.density;em.opt.I;stat.err;VARCHARprincipalflux_ZtTotal flux (Z band) - using global sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_ZlLocal flux (Z band) - using local sky subtractionJyphot.flux.density;em.opt.Z;VARCHARprincipalflux_err_ZtFlux err (Z band)Jyphot.flux.density;em.opt.Z;stat.err;VARCHARprincipalflux_YtTotal flux (Y band) - using global sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_YlLocal flux (Y band) - using local sky subtractionJyphot.flux.density;em.IR.Y;VARCHARprincipalflux_err_YtFlux err (Y band)Jyphot.flux.density;em.IR.Y;stat.err;VARCHARprincipalflux_JtTotal flux (J band) - using global sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_JlLocal flux (J band) - using local sky subtractionJyphot.flux.density;em.IR.J;VARCHARprincipalflux_err_JtFlux err (J band)Jyphot.flux.density;em.IR.J;stat.err;VARCHARprincipalflux_HtTotal flux (H band) - using global sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_HlLocal flux (H band) - using local sky subtractionJyphot.flux.density;em.IR.H;VARCHARprincipalflux_err_HtFlux err (H band)Jyphot.flux.density;em.IR.H;stat.err;VARCHARprincipalflux_KtTotal flux (Ks band) - using global sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_KlLocal flux (Ks band) - using local sky subtractionJyphot.flux.density;em.IR.K;VARCHARprincipalflux_err_KtFlux err (Ks band)Jyphot.flux.density;em.IR.K;stat.err;VARCHARprincipalflux_W1tTotal flux (W1 band) - using global sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_W1lLocal flux (W1 band) - using local sky subtractionJyphot.flux.density;em.IR.3-4um;VARCHARprincipalflux_err_W1tFlux err (W1 band)Jyphot.flux.density;em.IR.3-4um;stat.err;VARCHARprincipalflux_W2tTotal flux (W2 band) - using global sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_W2lLocal flux (W2 band) - using local sky subtractionJyphot.flux.density;em.IR.4-8um;VARCHARprincipalflux_err_W2tFlux err (W2 band)Jyphot.flux.density;em.IR.4-8um;stat.err;VARCHARprincipalduplicateFlag indicating if object is duplicated due to tile overlapmeta.code.classVARCHARprincipalmaskFlag indicating if object is within GAMA regionmeta.code.classVARCHARprincipalstarmaskFlag indicating if object is within a star maskmeta.code.classVARCHARprincipalstarscolStellar colour flagmeta.code.classVARCHARprincipalstarssizeStellar size flagmeta.code.classVARCHARprincipalclassAutomatic classification of objectmeta.code.classVARCHARprincipaleyeclassVisual classification of objectmeta.code.classVARCHARprincipaluberclassFinal classification of objectmeta.code.classVARCHARprincipalnoOPTFlag indicating optical data is not presentmeta.code.classVARCHARprincipalnoIRFlag indicating IR data is not presentmeta.code.classVARCHARprincipalCATAIDID of objectmeta.id.cross;meta.mainVARCHARprincipalgama_dr4.gkvSFMPhotozv01uberIDID of objectmeta.idVARCHARprincipalzexpPhotometric redshift, marginalised over the full pdfsrc.redshiftVARCHARprincipalzerrPhotometric redshift error, calculated as half 16-84th range of the redshift pdfsrc.redshiftVARCHARprincipalzmaxPhotometric redshift, highest likelihood valuesrc.redshiftVARCHARprincipalgama_dr4.gkvFarIRv03This catalogue is an extension to the GAMAKidsViking catalogue, providing photometry in the W3-S500 bands, thatare in general unresolved. In this PSF-limited regime, the output of the GAMAKidsViking catalogue is used to determine the coordinates for objects expected to emit in the FIR, and at these locations the flux is modelled.FIR fluxes are derived using the ProFound function ProFoundFitMagPSF, which fits fluxes iteratively according to a ProFitmodel of individual objects based on the band PSuberIDUnique identifier of the objectmeta.idVARCHARprincipaluberclassFinal classification of objectmeta.code.classVARCHARprincipalmag_PSF_w3PSF-derived magnitude (W3 band) - missing values are indicated via -999magphot.mag;em.IR.8-15umVARCHARprincipalmag_PSF_err_w3PSF-derived magnitude error (W3 band) - missing values are indicated via -999magphot.mag;stat.err;em.IR.8-15umVARCHARprincipalflux_PSF_w3PSF-derived flux (W3 band) - missing values are indicated via -999Jyphot.flux.density;em.IR.8-15umVARCHARprincipalflux_PSF_err_w3PSF-derived flux error (W3 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.IR.8-15umVARCHARprincipalmag_PSF_w4PSF-derived magnitude (W4 band) - missing values are indicated via -999magphot.mag;em.IR.15-30umVARCHARprincipalmag_PSF_err_w4PSF-derived magnitude error (W4 band) - missing values are indicated via -999magphot.mag;stat.err;em.IR.15-30umVARCHARprincipalflux_PSF_w4PSF-derived flux (W4 band) - missing values are indicated via -999Jyphot.flux.density;em.IR.15-30umVARCHARprincipalflux_PSF_err_w4PSF-derived flux error (W4 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.IR.15-30umVARCHARprincipalmag_PSF_p100PSF-derived magnitude (P100 band) - missing values are indicated via -999magphot.mag;em.mm.1500-3000GHzVARCHARprincipalmag_PSF_err_p100PSF-derived magnitude error (P100 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.1500-3000GHzVARCHARprincipalflux_PSF_p100PSF-derived flux (P100 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.1500-3000GHzVARCHARprincipalflux_PSF_err_p100PSF-derived flux error (P100 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.mm.1500-3000GHzVARCHARprincipalmag_PSF_p160PSF-derived magnitude (P160 band) - missing values are indicated via -999magphot.mag;m.mm.1500-3000GHzVARCHARprincipalmag_PSF_err_p160PSF-derived magnitude error (P160 band) - missing values are indicated via -999magphot.mag;stat.err;m.mm.1500-3000GHzVARCHARprincipalflux_PSF_p160PSF-derived flux (P160 band) - missing values are indicated via -999Jyphot.flux.density;m.mm.1500-3000GHzVARCHARprincipalflux_PSF_err_p160PSF-derived flux error (P160 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;m.mm.1500-3000GHzVARCHARprincipalmag_PSF_s250PSF-derived magnitude (S250 band) - missing values are indicated via -999magphot.mag;em.mm.750-1500GHzVARCHARprincipalmag_PSF_err_s250PSF-derived magnitude error (S250 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.750-1500GHzVARCHARprincipalflux_PSF_s250PSF-derived flux (S250 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalflux_PSF_err_s250PSF-derived flux error (S250 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.mm.750-1500GHzVARCHARprincipalmag_PSF_s350PSF-derived magnitude (S350 band) - missing values are indicated via -999magphot.mag;em.mm.750-1500GHzVARCHARprincipalmag_PSF_err_s350PSF-derived magnitude error (S350 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.750-1500GHzVARCHARprincipalflux_PSF_s350PSF-derived flux (S350 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.750-1500GHzVARCHARprincipalflux_PSF_err_s350PSF-derived flux error (S350 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;em.mm.750-1500GHzVARCHARprincipalmag_PSF_s500PSF-derived magnitude (S500 band) - missing values are indicated via -999magphot.mag;em.mm.400-750GHzVARCHARprincipalmag_PSF_err_s500PSF-derived magnitude error (S500 band) - missing values are indicated via -999magphot.mag;stat.err;em.mm.400-750GHzVARCHARprincipalflux_PSF_s500PSF-derived flux (S500 band) - missing values are indicated via -999Jyphot.flux.density;em.mm.400-750GHzVARCHARprincipalflux_PSF_err_s500em.mm.400-750GHz PSF-derived flux error (S500 band) - missing values are indicated via -999Jyphot.flux.density;stat.err;VARCHARprincipalFrameNameName of frame that the object comes frommeta.idVARCHARprincipalFrameIDID of the frame that the object comes frommeta.idVARCHARprincipalx_maxx position of the maximum fluxpixposVARCHARprincipaly_maxy position of the maximum fluxpixposVARCHARprincipalRAcenRight Ascension of flux-weighted centre (ICRS J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of flux-weighted centre (ICRS J2000)degpos.eq.decVARCHARprincipalgama_dr4.gkvSFMPhotoZProSpectv02CATAIDID of objectmeta.idVARCHARprincipaluberIDID of objectmeta.idVARCHARprincipalzexpPhotometric redshift, marginalised over the full pdfsrc.redshiftVARCHARprincipalzerrPhotometric redshift error, calculated as half 16-84th range of the redshift pdfsrc.redshiftVARCHARprincipalzmaxPhotometric redshift, highest likelihood valuesrc.redshiftVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SEDMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SEDphys.abund.ZVARCHARprincipalgama_dr4.gkvProSpectv02CATAIDID of objectmeta.idVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalStellarMass_50Median stellar mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalStellarMass_1616th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_8484th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SEDMsol/yrphys.SFRVARCHARprincipalSFR_50Median SFR from MCMC chain (recommended)Msol/yrphys.SFRVARCHARprincipalSFR_1616th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_8484th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SEDphys.abund.ZVARCHARprincipalZgas_50Median Zgas from MCMC chain (recommended)phys.abund.ZVARCHARprincipalZgas_1616th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalZgas_8484th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalDustMass_bestfitDust mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalDustMass_50Median dust mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalDustMass_1616th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_8484th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustLum_50Median dust luminosity from MCMC chain (recommended)Msolphys.lumVARCHARprincipalDustLum_1616th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipalDustLum_8484th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipaluberIDKiDS ID of objectmeta.idVARCHARprincipalgama_dr4.gkvProSpectNEDv01SFR_1616th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipaluberIDKiDS ID of objectmeta.idVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalStellarMass_50Median stellar mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalStellarMass_1616th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_8484th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SEDMsol/yrphys.SFRVARCHARprincipalSFR_50Median SFR from MCMC chain (recommended)Msol/yrphys.SFRVARCHARprincipalSFR_8484th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SEDphys.abund.ZVARCHARprincipalZgas_50Median Zgas from MCMC chain (recommended)phys.abund.ZVARCHARprincipalZgas_1616th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalZgas_8484th percentile Zgas from MCMC chainphys.abund.ZVARCHARprincipalDustMass_bestfitDust mass as determined by the best-fitting SEDMsolphys.massVARCHARprincipalDustMass_50Median dust mass from MCMC chain (recommended)Msolphys.massVARCHARprincipalDustMass_1616th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_8484th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustLum_50Median dust luminosity from MCMC chain (recommended)Msolphys.lumVARCHARprincipalDustLum_1616th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipalDustLum_8484th percentile dust luminosity from MCMC chainMsolphys.lumVARCHARprincipalNED_prefnameName of NED objectVARCHARprincipalNED_raRight Ascension of NED objectdegpos.eq.raVARCHARprincipalNED_decDeclination of NED objectdegpos.eq.decVARCHARprincipalNED_pretypeClass of objects from NEDVARCHARprincipalNED_zRedshift of NED objectsrc.redshiftVARCHARprincipalNED_zuncRedshift uncertainty of NED objectstat.errorVARCHARprincipalNED_zflagRedshift flagmeta.code.classVARCHARprincipalNED_zrefcodeReference to publication for NED redshiftVARCHARprincipalNED_matchDistSepaation radius between KiDS object and NED object.arcsecstat.valueVARCHARprincipalgama_dr4.gkvProSpectAGNv01Sabine Bellstedt <sabine.bellstedt@uwa.edu.au>CATAIDID of objectmeta.idVARCHARprincipalStellarMass_bestfitStellar mass as determined by the best-fitting SED(recommended)Msolphys.massVARCHARprincipalStellarMass_50Median stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_1616th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalStellarMass_8484th percentile stellar mass from MCMC chainMsolphys.massVARCHARprincipalSFR_bestfitSFR as determined by the best-fitting SED(recommended)Msol/yrphys.SFRVARCHARprincipalSFR_50Median SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_1616th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalSFR_8484th percentile SFR from MCMC chainMsol/yrphys.SFRVARCHARprincipalZgas_bestfitZgas as determined by the best-fitting SED (recommended) (logged)phys.abund.ZVARCHARprincipalZgas_50Median Zgas from MCMC chain (logged)phys.abund.ZVARCHARprincipalZgas_1616th percentile Zgas from MCMC chain (logged)phys.abund.ZVARCHARprincipalZgas_8484th percentile Zgas from MCMC chain (logged)phys.abund.ZVARCHARprincipalDustMass_bestfitDust mass as determined by the best-fitting SED (recommended)Msolphys.massVARCHARprincipalDustMass_50Median dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_1616th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustMass_8484th percentile dust mass from MCMC chainMsolphys.massVARCHARprincipalDustLum_bestfitDust luminosity as determined by the best-fitting SED (recommended)Lsolphys.lumVARCHARprincipalDustLum_50Median dust luminosity from MCMC chainLsolphys.lumVARCHARprincipalDustLum_1616th percentile dust luminosity from MCMC chainLsolphys.lumVARCHARprincipalDustLum_8484th percentile dust luminosity from MCMC chainLsolphys.lumVARCHARprincipalAGNlum_bestfitAGN bolometric luminosity as determined by the best-fitting SED (recommended) (logged)log(ergs/s)phys.lumVARCHARprincipalAGNlum_50Median AGN bolometric luminosity from MCMC chain (logged)log(ergs/s)phys.lumVARCHARprincipalAGNlum_1616th percentile AGN bolometric luminosity from MCMC chain (logged)log(ergs/s)phys.lumVARCHARprincipalAGNlum_8484th percentile AGN bolometric luminosity from MCMC chain (logged)log(ergs/s)phys.lumVARCHARprincipalfAGNFraction of flux contributed by the AGN model between 5-20micronsVARCHARprincipalLPlog-posterior value of for best-fit valuesVARCHARprincipaluberIDKiDS ID of objectmeta.idVARCHARprincipalgama_dr4.gkvMorphologyv02uberIDClassifier from GAMAKidsVikingv01meta.idVARCHARprincipalFrameNameName of Frame containing ProFound outputsmeta.idVARCHARprincipalCATAIDUnique ID of GAMA objectmeta.id;meta.mainVARCHARindexedprincipalRAcendouble RA of centre of flux (J2000)degpos.eq.raVARCHARprincipalDeccenDeclination of centre of flux (J2000)degpos.eq.decVARCHARprincipalmag_rtVST r band magnitude derived from flux_rtmagphot.mag;em.opt.RVARCHARprincipalR50Radius enclosing half the light in the detection band (rZ dilated)arcsecphys.size.radiusVARCHARprincipalZZ from SpecObjv27 or photo-Z from LSBGPhotoZ if NQ <3src.redshiftVARCHARprincipalNQNormalised redshift quality if NQ > 2 or photo-z if NQ=0meta.code.qual;src.redshiftVARCHARprincipalHUBBLE_TYPEFinal Hubble Type from VisualMorphologyv03 if known else Xmeta.code.classVARCHARprincipalINITIAL_CLASSInitial automated estimatemeta.code.classVARCHARprincipalSTART_CLASSFirst pass classification using custodian methodmeta.code.classVARCHARprincipalSABINE_CLASSSabine's visual Hubble type classificationsmeta.code.classVARCHARprincipalSIMON_CLASSSimon's visual Hubble type classificationsmeta.code.classVARCHARprincipalLUKE_CLASSLuke's visual Hubble type classificationsmeta.code.classVARCHARprincipalFINAL_CLASSFinal Classification (with tie = SIMON_CLASS)meta.code.classVARCHARprincipalMORPH_STAMPPointer to the postage stamp imagemeta.fileVARCHARprincipalgama_dr4.EAZYPhotozv02_GAMAv02_G15uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_dr4.EAZYPhotozv02_GAMAv02_G23uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_dr4.EAZYPhotozv02_GAMAv02_G09uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_dr4.EAZYPhotozv02_GAMAv02_G12uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_dr4.EAZYPhotozv02_GAMAv02_SpecObjv24uberIDunique photometry identifier in GAMAKiDSVikingv02meta.idVARCHARprincipalchi_1minimised chi2 value for z_1 fitstat.fit.chi2VARCHARprincipaltemp_1template number associated with z_1 fitmeta.idVARCHARprincipalz_m1Bayesian minimum variance redshift estimate for uniform redshift priorsrc.redshiftVARCHARprincipalz_psimple maximum likelihood redshift for luminosity dependent redshift priormeta.idVARCHARprincipalchi_pchi2 value for z_p fit (not prior weighted)stat.fit.chi2VARCHARprincipaltemp_ptemplate number associated with z_1 fitVARCHARprincipalz_1simple maximum likelihood redshift for uniform redshift priorsrc.redshiftVARCHARprincipalz_m2Bayesian minimum variance redshift estimate for luminosity dependent priorsrc.redshiftVARCHARprincipalq_zEAZY metric: see Eq. 7 of Brammer, van Dokkum, Coppi (2008); prefer Qz < 1src.redshiftVARCHARprincipall68lower bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu68upper bound of 68% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall95lower bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalu95upper bound of 95% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipall99lower bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipaloddsBenitez (2000) metric: fraction of probability within +/- 0.2 of z_m2VARCHARprincipalu99upper bound of 99% confidence interval from prior-weighted p(z)src.redshiftVARCHARprincipalfitflux_Kbest fit (Max. Like.) template K-band flux, assuming z_peakJyphot.flux.density;em.IR.KVARCHARprincipalfitflux_Jbest fit (Max. Like.) template J-band flux, assuming z_peakJyphot.flux.density;em.IR.JVARCHARprincipalCATAIDmatched object identifier taken from GAMAKiDSVikingv02meta.id.crossVARCHARprincipalprimaryrequire True to exclude duplicates and masked areasVARCHARprincipalscience_primaryTrue implies primary and uberclass = galaxy/ambiguousVARCHARprincipalstar_primaryTrue implies primary and uberclass = starVARCHARprincipalnfiltnumber of photometric points contributing to the fitVARCHARprincipalz_peakTHIS IS THE ESTIMATOR TO USE IF YOU DO NOT HAVE REASON TO PREFER ANOTHER.src.redshiftVARCHARprincipalfitflux_Hbest fit (Max. Like.) template H-band flux, assuming z_peakJyphot.flux.density;em.IR.HVARCHARprincipalpeak_probrelative probability that true redshift lies within the peak intervalstat.probability;src.redshiftVARCHARprincipalfitflux_ubest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.UVARCHARprincipalfitflux_gbest fit (Max. Like.) template u-band flux, assuming z_peakJyphot.flux.density;em.opt.GVARCHARprincipalfitflux_rbest fit (Max. Like.) template g-band flux, assuming z_peakJyphot.flux.density;em.opt.RVARCHARprincipalfitflux_ibest fit (Max. Like.) template r-band flux, assuming z_peakJyphot.flux.density;em.opt.IVARCHARprincipalfitflux_Zbest fit (Max. Like.) template Z-band flux, assuming z_peakJyphot.flux.density;em.IR.ZVARCHARprincipalfitflux_Ybest fit (Max. Like.) template Y-band flux, assuming z_peakJyphot.flux.density;em.IR.YVARCHARprincipalchi2fitchi2 value for z_peak fit (not prior weighted)stat.fit.chi2VARCHARprincipalz_mca random Monte Carlo draw from the posterior P(z)src.redshiftVARCHARprincipalgama_dr4.SourceCataloguev01This table is the source catalogue of the survey. It contains 338,772 objects and it was produced by the Data Central team.uberIDUnique GAMA III ID of objectmeta.id;meta.mainVARCHARindexedprincipalRAcenRight Ascension of flux-weighted centre (ICRS)degpos.eq.raVARCHARindexedprincipalDeccenDeclination of flux-weighted centre (ICRS)degpos.eq.decVARCHARindexedprincipalgleamx_dr2The GLEAM-x survey coveres the entire sky south of Dec+30, using the extended configuration of the MWA. The first data release (DR1) contains a smaller area of 1,447 sq deg associated with the survey description paper (Hurley-Walker et al. 2022).The second data release covers ~12,000 sq deg. centered around the South Galactic Pole region. Both releases contain 26 mosaics covering 72-231MHz and associated background and RMS maps.gleamx_dr2.filtered_prime_sedfit_paperGLEAM-X DR2 catalogueNameIAU Namemeta.id;srcVARCHARindexedprincipalbackground_wideBackground level in wide imageJy/beamstat.median;phot.flux.densityREALprincipallocal_rms_wideLocal noise leve in wide imageJy/beamstat.variance;phot.flux.densityREALprincipalra_strRight Ascension J2000pos.eq.ra;meta.mainVARCHARindexedprincipaldec_strDeclination J2000d:m:spos.eq.dec;meta.mainVARCHARindexedprincipalRAJ2000Right Ascension J2000degpos.eq.raREALindexedprincipalerr_RAJ2000Uncertainty in Right Ascensiondegstat.error;pos.eq.raREALprincipalDEJ2000Declination J2000degpos.eq.decREALindexedprincipalerr_DEJ2000Uncertainty in Declinationdegstat.error;pos.eq.decREALprincipalpeak_flux_widePeak flux in wide imageJy/beamphot.flux.density;em.radio.170-231MHzREALprincipalerr_peak_flux_wideUncertainty in fit for peak flux in wide imageJy/beamstat.error;phot.flux.density;em.radio.170-231MHzREALprincipalint_flux_wideIntegrated flux in wide imageJyphot.flux;em.radio.170-231MHzREALprincipalerr_int_flux_wideUncertainty in fit for integrated flux in wide imageJystat.error;phot.flux;em.radio.170-231MHzREALprincipala_wideFitted semi-major axis in wide imagearcsecphys.angSize.smajAxis;meta.modelledREALprincipalerr_a_wideUncertainty in fitted semi-major axis in wide imagearcsecstat.error;phys.angSize.smajAxisREALprincipalb_wideFitted semi-minor axis in wide imagearcsecphys.angSize.sminAxis;meta.modelledREALprincipalerr_b_wideUncertainty in fitted semi-minor axis in wide imagearcsecstat.error;phys.angSize.sminAxisREALprincipalpa_wideFitted position angle in wide imagedegpos.posAng;meta.modelledREALprincipalerr_pa_wideUncertainty in fitted position angle in wide imagedegstat.error;pos.posAngREALprincipalresidual_mean_wideMean value of data-model in wide imageJy/beamstat.fit.residualREALprincipalresidual_std_wideStandard deviation of data-model in wide imageJy/beamstat.fit.residualREALprincipalpsf_a_wideSemi-major axis of the point spread function in wide imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalerr_abs_flux_pctPercent error in absolute flux scale - all frequencies%stat.error;phot.flux;em.radioREALprincipalerr_fit_flux_pctPercent error on internal flux scale - all frequencies%stat.error;phot.flux;em.radioREALprincipalpsf_b_wideSemi-minor axis of the point spread function in wide imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_widePosition angle of the point spread function in wide imagedegpos.posAng;instr.det.psfREALprincipalbackground_076Background level in 072-080MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_076Local noise level in 072-080MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_076Peak flux in 072-080MHz imageJy/beamphot.flux.density;em.radio.072-080MHzREALprincipalerr_peak_flux_076Uncertainty in fit for peak flux in 072-080MHz imageJy/beamstat.error;phot.flux.density;em.radio.072-080MHzREALprincipalint_flux_076Integrated flux in 072-080MHz imageJyphot.flux;em.radio.072-080MHzREALprincipalerr_int_flux_076Uncertainty in fit for integrated flux in 072-080MHz imageJystat.error;phot.flux;em.radio.072-080MHzREALprincipala_076Fitted semi-major axis in 072-080MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_076Fitted semi-minor axis in 072-080MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_076Fitted position angle in 072-080MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_076Mean value of data-model in 072-080MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_076Standard deviation of data-model in 072-080MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_076Semi-major axis of the point spread function in 072-080MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_076Semi-minor axis of the point spread function in 072-080MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_076Position angle of the point spread function in 072-080MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_084Background level in 080-088MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_084Local noise level in 080-088MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_084Peak flux in 080-088MHz imageJy/beamphot.flux.density;em.radio.080-088MHzREALprincipalerr_peak_flux_084Uncertainty in fit for peak flux in 080-088MHz imageJy/beamstat.error;phot.flux.density;em.radio.080-088MHzREALprincipalint_flux_084Integrated flux in 080-088MHz imageJyphot.flux;em.radio.080-088MHzREALprincipalerr_int_flux_084Uncertainty in fit for integrated flux in 080-088MHz imageJystat.error;phot.flux;em.radio.080-088MHzREALprincipala_084Fitted semi-major axis in 080-088MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_084Fitted semi-minor axis in 080-088MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_084Fitted position angle in 080-088MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_084Mean value of data-model in 080-088MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_084Standard deviation of data-model in 080-088MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_084Semi-major axis of the point spread function in 080-088MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_084Semi-minor axis of the point spread function in 080-088MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_084Position angle of the point spread function in 080-088MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_092Background level in 088-095MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_092Local noise level in 088-095MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_092Peak flux in 088-095MHz imageJy/beamphot.flux.density;em.radio.088-095MHzREALprincipalerr_peak_flux_092Uncertainty in fit for peak flux in 088-095MHz imageJy/beamstat.error;phot.flux.density;em.radio.088-095MHzREALprincipalint_flux_092Integrated flux in 088-095MHz imageJyphot.flux;em.radio.088-095MHzREALprincipalerr_int_flux_092Uncertainty in fit for integrated flux in 088-095MHz imageJystat.error;phot.flux;em.radio.088-095MHzREALprincipala_092Fitted semi-major axis in 088-095MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_092Fitted semi-minor axis in 088-095MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_092Fitted position angle in 088-095MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_092Mean value of data-model in 088-095MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_092Standard deviation of data-model in 088-095MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_092Semi-major axis of the point spread function in 088-095MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_092Semi-minor axis of the point spread function in 088-095MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_092Position angle of the point spread function in 088-095MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_099Background level in 095-103MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_099Local noise level in 095-103MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_099Peak flux in 095-103MHz imageJy/beamphot.flux.density;em.radio.095-103MHzREALprincipalerr_peak_flux_099Uncertainty in fit for peak flux in 095-103MHz imageJy/beamstat.error;phot.flux.density;em.radio.095-103MHzREALprincipalint_flux_099Integrated flux in 095-103MHz imageJyphot.flux;em.radio.095-103MHzREALprincipalerr_int_flux_099Uncertainty in fit for integrated flux in 095-103MHz imageJystat.error;phot.flux;em.radio.095-103MHzREALprincipala_099Fitted semi-major axis in 095-103MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_099Fitted semi-minor axis in 095-103MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_099Fitted position angle in 095-103MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_099Mean value of data-model in 095-103MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_099Standard deviation of data-model in 095-103MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_099Semi-major axis of the point spread function in 095-103MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_099Semi-minor axis of the point spread function in 095-103MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_099Position angle of the point spread function in 095-103MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_107Background level in 103-111MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_107Local noise level in 103-111MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_107Peak flux in 103-111MHz imageJy/beamphot.flux.density;em.radio.103-111MHzREALprincipalerr_peak_flux_107Uncertainty in fit for peak flux in 103-111MHz imageJy/beamstat.error;phot.flux.density;em.radio.103-111MHzREALprincipalint_flux_107Integrated flux in 103-111MHz imageJyphot.flux;em.radio.103-111MHzREALprincipalerr_int_flux_107Uncertainty in fit for integrated flux in 103-111MHz imageJystat.error;phot.flux;em.radio.103-111MHzREALprincipala_107Fitted semi-major axis in 103-111MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_107Fitted semi-minor axis in 103-111MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_107Fitted position angle in 103-111MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_107Mean value of data-model in 103-111MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_107Standard deviation of data-model in 103-111MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_107Semi-major axis of the point spread function in 103-111MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_107Semi-minor axis of the point spread function in 103-111MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_107Position angle of the point spread function in 103-111MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_115Background level in 111-118MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_115Local noise level in 111-118MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_115Peak flux in 111-118MHz imageJy/beamphot.flux.density;em.radio.111-118MHzREALprincipalerr_peak_flux_115Uncertainty in fit for peak flux in 111-118MHz imageJy/beamstat.error;phot.flux.density;em.radio.111-118MHzREALprincipalint_flux_115Integrated flux in 111-118MHz imageJyphot.flux;em.radio.111-118MHzREALprincipalerr_int_flux_115Uncertainty in fit for integrated flux in 111-118MHz imageJystat.error;phot.flux;em.radio.111-118MHzREALprincipala_115Fitted semi-major axis in 111-118MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_115Fitted semi-minor axis in 111-118MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_115Fitted position angle in 111-118MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_115Mean value of data-model in 111-118MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_115Standard deviation of data-model in 111-118MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_115Semi-major axis of the point spread function in 111-118MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_115Semi-minor axis of the point spread function in 111-118MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_115Position angle of the point spread function in 111-118MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_122Background level in 118-126MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_122Local noise level in 118-126MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_122Peak flux in 118-126MHz imageJy/beamphot.flux.density;em.radio.118-126MHzREALprincipalerr_peak_flux_122Uncertainty in fit for peak flux in 118-126MHz imageJy/beamstat.error;phot.flux.density;em.radio.118-126MHzREALprincipalint_flux_122Integrated flux in 118-126MHz imageJyphot.flux;em.radio.118-126MHzREALprincipalerr_int_flux_122Uncertainty in fit for integrated flux in 118-126MHz imageJystat.error;phot.flux;em.radio.118-126MHzREALprincipala_122Fitted semi-major axis in 118-126MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_122Fitted semi-minor axis in 118-126MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_122Fitted position angle in 118-126MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_122Mean value of data-model in 118-126MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_122Standard deviation of data-model in 118-126MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_122Semi-major axis of the point spread function in 118-126MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_122Semi-minor axis of the point spread function in 118-126MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_122Position angle of the point spread function in 118-126MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_130Background level in 126-134MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_130Local noise level in 126-134MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_130Peak flux in 126-134MHz imageJy/beamphot.flux.density;em.radio.126-134MHzREALprincipalerr_peak_flux_130Uncertainty in fit for peak flux in 126-134MHz imageJy/beamstat.error;phot.flux.density;em.radio.126-134MHzREALprincipalint_flux_130Integrated flux in 126-134MHz imageJyphot.flux;em.radio.126-134MHzREALprincipalerr_int_flux_130Uncertainty in fit for integrated flux in 126-134MHz imageJystat.error;phot.flux;em.radio.126-134MHzREALprincipala_130Fitted semi-major axis in 126-134MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_130Fitted semi-minor axis in 126-134MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_130Fitted position angle in 126-134MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_130Mean value of data-model in 126-134MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_130Standard deviation of data-model in 126-134MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_130Semi-major axis of the point spread function in 126-134MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_130Semi-minor axis of the point spread function in 126-134MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_130Position angle of the point spread function in 126-134MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_143Background level in 139-147MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_143Local noise level in 139-147MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_143Peak flux in 139-147MHz imageJy/beamphot.flux.density;em.radio.139-147MHzREALprincipalerr_peak_flux_143Uncertainty in fit for peak flux in 139-147MHz imageJy/beamstat.error;phot.flux.density;em.radio.139-147MHzREALprincipalint_flux_143Integrated flux in 139-147MHz imageJyphot.flux;em.radio.139-147MHzREALprincipalerr_int_flux_143Uncertainty in fit for integrated flux in 139-147MHz imageJystat.error;phot.flux;em.radio.139-147MHzREALprincipala_143Fitted semi-major axis in 139-147MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_143Fitted semi-minor axis in 139-147MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_143Fitted position angle in 139-147MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_143Mean value of data-model in 139-147MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_143Standard deviation of data-model in 139-147MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_143Semi-major axis of the point spread function in 139-147MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_143Semi-minor axis of the point spread function in 139-147MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_143Position angle of the point spread function in 139-147MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_151Background level in 147-154MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_151Local noise level in 147-154MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_151Peak flux in 147-154MHz imageJy/beamphot.flux.density;em.radio.147-154MHzREALprincipalerr_peak_flux_151Uncertainty in fit for peak flux in 147-154MHz imageJy/beamstat.error;phot.flux.density;em.radio.147-154MHzREALprincipalint_flux_151Integrated flux in 147-154MHz imageJyphot.flux;em.radio.147-154MHzREALprincipalerr_int_flux_151Uncertainty in fit for integrated flux in 147-154MHz imageJystat.error;phot.flux;em.radio.147-154MHzREALprincipala_151Fitted semi-major axis in 147-154MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_151Fitted semi-minor axis in 147-154MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_151Fitted position angle in 147-154MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_151Mean value of data-model in 147-154MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_151Standard deviation of data-model in 147-154MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_151Semi-major axis of the point spread function in 147-154MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_151Semi-minor axis of the point spread function in 147-154MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_151Position angle of the point spread function in 147-154MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_158Background level in 154-162MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_158Local noise level in 154-162MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_158Peak flux in 154-162MHz imageJy/beamphot.flux.density;em.radio.154-162MHzREALprincipalerr_peak_flux_158Uncertainty in fit for peak flux in 154-162MHz imageJy/beamstat.error;phot.flux.density;em.radio.154-162MHzREALprincipalint_flux_158Integrated flux in 154-162MHz imageJyphot.flux;em.radio.154-162MHzREALprincipalerr_int_flux_158Uncertainty in fit for integrated flux in 154-162MHz imageJystat.error;phot.flux;em.radio.154-162MHzREALprincipala_158Fitted semi-major axis in 154-162MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_158Fitted semi-minor axis in 154-162MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_158Fitted position angle in 154-162MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_158Mean value of data-model in 154-162MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_158Standard deviation of data-model in 154-162MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_158Semi-major axis of the point spread function in 154-162MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_158Semi-minor axis of the point spread function in 154-162MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_158Position angle of the point spread function in 154-162MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_166Background level in 162-170MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_166Local noise level in 162-170MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_166Peak flux in 162-170MHz imageJy/beamphot.flux.density;em.radio.162-170MHzREALprincipalerr_peak_flux_166Uncertainty in fit for peak flux in 162-170MHz imageJy/beamstat.error;phot.flux.density;em.radio.162-170MHzREALprincipalint_flux_166Integrated flux in 162-170MHz imageJyphot.flux;em.radio.162-170MHzREALprincipalerr_int_flux_166Uncertainty in fit for integrated flux in 162-170MHz imageJystat.error;phot.flux;em.radio.162-170MHzREALprincipala_166Fitted semi-major axis in 162-170MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_166Fitted semi-minor axis in 162-170MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_166Fitted position angle in 162-170MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_166Mean value of data-model in 162-170MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_166Standard deviation of data-model in 162-170MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_166Semi-major axis of the point spread function in 162-170MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_166Semi-minor axis of the point spread function in 162-170MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_166Position angle of the point spread function in 162-170MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_174Background level in 170-177MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_174Local noise level in 170-177MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_174Peak flux in 170-177MHz imageJy/beamphot.flux.density;em.radio.170-177MHzREALprincipalerr_peak_flux_174Uncertainty in fit for peak flux in 170-177MHz imageJy/beamstat.error;phot.flux.density;em.radio.170-177MHzREALprincipalint_flux_174Integrated flux in 170-177MHz imageJyphot.flux;em.radio.170-177MHzREALprincipalerr_int_flux_174Uncertainty in fit for integrated flux in 170-177MHz imageJystat.error;phot.flux;em.radio.170-177MHzREALprincipala_174Fitted semi-major axis in 170-177MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_174Fitted semi-minor axis in 170-177MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_174Fitted position angle in 170-177MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_174Mean value of data-model in 170-177MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_174Standard deviation of data-model in 170-177MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_174Semi-major axis of the point spread function in 170-177MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_174Semi-minor axis of the point spread function in 170-177MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_174Position angle of the point spread function in 170-177MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_181Background level in 177-185MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_181Local noise level in 177-185MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_181Peak flux in 177-185MHz imageJy/beamphot.flux.density;em.radio.177-185MHzREALprincipalerr_peak_flux_181Uncertainty in fit for peak flux in 177-185MHz imageJy/beamstat.error;phot.flux.density;em.radio.177-185MHzREALprincipalint_flux_181Integrated flux in 177-185MHz imageJyphot.flux;em.radio.177-185MHzREALprincipalerr_int_flux_181Uncertainty in fit for integrated flux in 177-185MHz imageJystat.error;phot.flux;em.radio.177-185MHzREALprincipala_181Fitted semi-major axis in 177-185MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_181Fitted semi-minor axis in 177-185MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_181Fitted position angle in 177-185MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_181Mean value of data-model in 177-185MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_181Standard deviation of data-model in 177-185MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_181Semi-major axis of the point spread function in 177-185MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_181Semi-minor axis of the point spread function in 177-185MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_181Position angle of the point spread function in 177-185MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_189Background level in 185-193MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_189Local noise level in 185-193MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_189Peak flux in 185-193MHz imageJy/beamphot.flux.density;em.radio.185-193MHzREALprincipalerr_peak_flux_189Uncertainty in fit for peak flux in 185-193MHz imageJy/beamstat.error;phot.flux.density;em.radio.185-193MHzREALprincipalint_flux_189Integrated flux in 185-193MHz imageJyphot.flux;em.radio.185-193MHzREALprincipalerr_int_flux_189Uncertainty in fit for integrated flux in 185-193MHz imageJystat.error;phot.flux;em.radio.185-193MHzREALprincipala_189Fitted semi-major axis in 185-193MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_189Fitted semi-minor axis in 185-193MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_189Fitted position angle in 185-193MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_189Mean value of data-model in 185-193MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_189Standard deviation of data-model in 185-193MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_189Semi-major axis of the point spread function in 185-193MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_189Semi-minor axis of the point spread function in 185-193MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_189Position angle of the point spread function in 185-193MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_197Background level in 193-200MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_197Local noise level in 193-200MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_197Peak flux in 193-200MHz imageJy/beamphot.flux.density;em.radio.193-200MHzREALprincipalerr_peak_flux_197Uncertainty in fit for peak flux in 193-200MHz imageJy/beamstat.error;phot.flux.density;em.radio.193-200MHzREALprincipalint_flux_197Integrated flux in 193-200MHz imageJyphot.flux;em.radio.193-200MHzREALprincipalerr_int_flux_197Uncertainty in fit for integrated flux in 193-200MHz imageJystat.error;phot.flux;em.radio.193-200MHzREALprincipala_197Fitted semi-major axis in 193-200MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_197Fitted semi-minor axis in 193-200MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_197Fitted position angle in 193-200MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_197Mean value of data-model in 193-200MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_197Standard deviation of data-model in 193-200MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_197Semi-major axis of the point spread function in 193-200MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_197Semi-minor axis of the point spread function in 193-200MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_197Position angle of the point spread function in 193-200MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_204Background level in 200-208MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_204Local noise level in 200-208MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_204Peak flux in 200-208MHz imageJy/beamphot.flux.density;em.radio.200-208MHzREALprincipalerr_peak_flux_204Uncertainty in fit for peak flux in 200-208MHz imageJy/beamstat.error;phot.flux.density;em.radio.200-208MHzREALprincipalint_flux_204Integrated flux in 200-208MHz imageJyphot.flux;em.radio.200-208MHzREALprincipalerr_int_flux_204Uncertainty in fit for integrated flux in 200-208MHz imageJystat.error;phot.flux;em.radio.200-208MHzREALprincipala_204Fitted semi-major axis in 200-208MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_204Fitted semi-minor axis in 200-208MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_204Fitted position angle in 200-208MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_204Mean value of data-model in 200-208MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_204Standard deviation of data-model in 200-208MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_204Semi-major axis of the point spread function in 200-208MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_204Semi-minor axis of the point spread function in 200-208MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_204Position angle of the point spread function in 200-208MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_212Background level in 208-216MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_212Local noise level in 208-216MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_212Peak flux in 208-216MHz imageJy/beamphot.flux.density;em.radio.208-216MHzREALprincipalerr_peak_flux_212Uncertainty in fit for peak flux in 208-216MHz imageJy/beamstat.error;phot.flux.density;em.radio.208-216MHzREALprincipalint_flux_212Integrated flux in 208-216MHz imageJyphot.flux;em.radio.208-216MHzREALprincipalerr_int_flux_212Uncertainty in fit for integrated flux in 208-216MHz imageJystat.error;phot.flux;em.radio.208-216MHzREALprincipala_212Fitted semi-major axis in 208-216MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_212Fitted semi-minor axis in 208-216MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_212Fitted position angle in 208-216MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_212Mean value of data-model in 208-216MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_212Standard deviation of data-model in 208-216MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_212Semi-major axis of the point spread function in 208-216MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_212Semi-minor axis of the point spread function in 208-216MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_212Position angle of the point spread function in 208-216MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_220Background level in 216-223MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_220Local noise level in 216-223MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_220Peak flux in 216-223MHz imageJy/beamphot.flux.density;em.radio.216-223MHzREALprincipalerr_peak_flux_220Uncertainty in fit for peak flux in 216-223MHz imageJy/beamstat.error;phot.flux.density;em.radio.216-223MHzREALprincipalint_flux_220Integrated flux in 216-223MHz imageJyphot.flux;em.radio.216-223MHzREALprincipalerr_int_flux_220Uncertainty in fit for integrated flux in 216-223MHz imageJystat.error;phot.flux;em.radio.216-223MHzREALprincipala_220Fitted semi-major axis in 216-223MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_220Fitted semi-minor axis in 216-223MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_220Fitted position angle in 216-223MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_220Mean value of data-model in 216-223MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_220Standard deviation of data-model in 216-223MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_220Semi-major axis of the point spread function in 216-223MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_220Semi-minor axis of the point spread function in 216-223MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_220Position angle of the point spread function in 216-223MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_227Background level in 223-231MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_227Local noise level in 223-231MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_227Peak flux in 223-231MHz imageJy/beamphot.flux.density;em.radio.223-231MHzREALprincipalerr_peak_flux_227Uncertainty in fit for peak flux in 223-231MHz imageJy/beamstat.error;phot.flux.density;em.radio.223-231MHzREALprincipalint_flux_227Integrated flux in 223-231MHz imageJyphot.flux;em.radio.223-231MHzREALprincipalerr_int_flux_227Uncertainty in fit for integrated flux in 223-231MHz imageJystat.error;phot.flux;em.radio.223-231MHzREALprincipala_227Fitted semi-major axis in 223-231MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_227Fitted semi-minor axis in 223-231MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_227Fitted position angle in 223-231MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_227Mean value of data-model in 223-231MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_227Standard deviation of data-model in 223-231MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_227Semi-major axis of the point spread function in 223-231MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_227Semi-minor axis of the point spread function in 223-231MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_227Position angle of the point spread function in 223-231MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_087Background level in 072-103MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_087Local noise level in 072-103MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_087Peak flux in 072-103MHz imageJy/beamphot.flux.density;em.radio.072-103MHzREALprincipalerr_peak_flux_W_087Uncertainty in fit for peak flux in 072-103MHz imageJy/beamstat.error;phot.flux.density;em.radio.072-103MHzREALprincipalint_flux_W_087Integrated flux in 072-103MHz imageJyphot.flux;em.radio.072-103MHzREALprincipalerr_int_flux_W_087Uncertainty in fit for integrated flux in 072-103MHz imageJystat.error;phot.flux;em.radio.072-103MHzREALprincipala_W_087Fitted semi-major axis in 072-103MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_087Fitted semi-minor axis in 072-103MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_087Fitted position angle in 072-103MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_087Mean value of data-model in 072-103MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_087Standard deviation of data-model in 072-103MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_087Semi-major axis of the point spread function in 072-103MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_087Semi-minor axis of the point spread function in 072-103MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_087Position angle of the point spread function in 072-103MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_118Background level in 103-134MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_118Local noise level in 103-134MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_118Peak flux in 103-134MHz imageJy/beamphot.flux.density;em.radio.103-134MHzREALprincipalerr_peak_flux_W_118Uncertainty in fit for peak flux in 103-134MHz imageJy/beamstat.error;phot.flux.density;em.radio.103-134MHzREALprincipalint_flux_W_118Integrated flux in 103-134MHz imageJyphot.flux;em.radio.103-134MHzREALprincipalerr_int_flux_W_118Uncertainty in fit for integrated flux in 103-134MHz imageJystat.error;phot.flux;em.radio.103-134MHzREALprincipala_W_118Fitted semi-major axis in 103-134MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_118Fitted semi-minor axis in 103-134MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_118Fitted position angle in 103-134MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_118Mean value of data-model in 103-134MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_118Standard deviation of data-model in 103-134MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_118Semi-major axis of the point spread function in 103-134MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_118Semi-minor axis of the point spread function in 103-134MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_118Position angle of the point spread function in 103-134MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_154Background level in 139-170MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_154Local noise level in 139-170MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_154Peak flux in 139-170MHz imageJy/beamphot.flux.density;em.radio.139-170MHzREALprincipalerr_peak_flux_W_154Uncertainty in fit for peak flux in 139-170MHz imageJy/beamstat.error;phot.flux.density;em.radio.139-170MHzREALprincipalint_flux_W_154Integrated flux in 139-170MHz imageJyphot.flux;em.radio.139-170MHzREALprincipalerr_int_flux_W_154Uncertainty in fit for integrated flux in 139-170MHz imageJystat.error;phot.flux;em.radio.139-170MHzREALprincipala_W_154Fitted semi-major axis in 139-170MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_154Fitted semi-minor axis in 139-170MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_154Fitted position angle in 139-170MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_154Mean value of data-model in 139-170MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_154Standard deviation of data-model in 139-170MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_154Semi-major axis of the point spread function in 139-170MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_154Semi-minor axis of the point spread function in 139-170MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_154Position angle of the point spread function in 139-170MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_185Background level in 170-200MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_185Local noise level in 170-200MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_185Peak flux in 170-200MHz imageJy/beamphot.flux.density;em.radio.170-200MHzREALprincipalerr_peak_flux_W_185Uncertainty in fit for peak flux in 170-200MHz imageJy/beamstat.error;phot.flux.density;em.radio.170-200MHzREALprincipalint_flux_W_185Integrated flux in 170-200MHz imageJyphot.flux;em.radio.170-200MHzREALprincipalerr_int_flux_W_185Uncertainty in fit for integrated flux in 170-200MHz imageJystat.error;phot.flux;em.radio.170-200MHzREALprincipala_W_185Fitted semi-major axis in 170-200MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_185Fitted semi-minor axis in 170-200MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_185Fitted position angle in 170-200MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_185Mean value of data-model in 170-200MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_185Standard deviation of data-model in 170-200MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_185Semi-major axis of the point spread function in 170-200MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_185Semi-minor axis of the point spread function in 170-200MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_185Position angle of the point spread function in 170-200MHz imagedegpos.posAng;instr.det.psfREALprincipalbackground_W_215Background level in 200-231MHz imageJy/beamstat.median;src;phot.flux.densityREALprincipallocal_rms_W_215Local noise level in 200-231MHz imageJy/beamstat.variance;src;phot.flux.densityREALprincipalpeak_flux_W_215Peak flux in 200-231MHz imageJy/beamphot.flux.density;em.radio.200-231MHzREALprincipalerr_peak_flux_W_215Uncertainty in fit for peak flux in 200-231MHz imageJy/beamstat.error;phot.flux.density;em.radio.200-231MHzREALprincipalint_flux_W_215Integrated flux in 200-231MHz imageJyphot.flux;em.radio.200-231MHzREALprincipalerr_int_flux_W_215Uncertainty in fit for integrated flux in 200-231MHz imageJystat.error;phot.flux;em.radio.200-231MHzREALprincipala_W_215Fitted semi-major axis in 200-231MHz imagearcsecphys.angSize.smajAxis;src;meta.modelledREALprincipalb_W_215Fitted semi-minor axis in 200-231MHz imagearcsecphys.angSize.sminAxis;src;meta.modelledREALprincipalpa_W_215Fitted position angle in 200-231MHz imagedegpos.posAng;meta.modelledREALprincipalresidual_mean_W_215Mean value of data-model in 200-231MHz imageJy/beamstat.fit.residualREALprincipalresidual_std_W_215Standard deviation of data-model in 200-231MHz imageJy/beamstat.fit.residualREALprincipalpsf_a_W_215Semi-major axis of the point spread function in 200-231MHz imagearcsecphys.angSize.smajAxis;instr.det.psfREALprincipalpsf_b_W_215Semi-minor axis of the point spread function in 200-231MHz imagearcsecphys.angSize.sminAxis;instr.det.psfREALprincipalpsf_pa_W_215Position angle of the point spread function in 200-231MHz imagedegpos.posAng;instr.det.psfREALprincipalsp_int_flux_fit_200Power-law fitted flux density at 200 MHzJyphot.flux;em.radio.200MHzREALprincipalerr_sp_int_flux_fit_200Error on power-law fitted flux density at 200 MHzJystat.error;phot.flux;em.radio.200MHzREALprincipalsp_alphaFitted spectral index assuming power-law SEDspec.index;em.radioREALprincipalerr_sp_alphaError on fitted spectral index assuming power-law SEDstat.error;spec.index;em.radioREALprincipalsp_reduced_chi2Reduced chi-squared statistic for power-law SED fitstat.fit.goodnessREALprincipalcsp_int_flux_fit_200Curved SED fitted flux density at 200 MHzJyphot.flux;em.radio.200MHzREALprincipalerr_csp_int_flux_fit_200Error on curved SED fitted flux density at 200 MHzJystat.error;phot.flux;em.radio.200MHzREALprincipalcsp_alphaFitted spectral index assuming curved SEDspec.index;em.radioREALprincipalerr_csp_alphaError on fitted spectral index assuming curved SEDstat.error;spec.index;em.radioREALprincipalcsp_betaFitted curvature index assuming curved SEDstat.fitREALprincipalerr_csp_betaError on fitted curvature index assuming curved SEDstat.errorREALprincipalcsp_reduced_chi2Reduced chi-squared statistic for curved SED fitstat.fit.goodnessREALprincipaldevils_dr1<p>DEVILS is a spectroscopic campaign at the Anglo-Australian Telescope aimed at bridging the near and distant Universe by producing the highest completeness survey of galaxies and groups at intermediate redshifts (0.3&lt;z&lt;1.0). Our sample will consist of ~58k galaxies to Ymag&lt;21.2, over ~6deg² to &gt;95% completeness in three well studies deep extragalactic fields (COSMOS, ECDFS and XMM-LSS).</p>devils_dr1.D10VisualMorphologyVisual morphological classifications of galaxies in the DEVILS D10 region produced from the HST imaging in the COSMOS region. Objects are classified by multiple team members and a final master classification provided.UIDUID based on feild, RA, DEC taken from DEVILS profound photometry catalogue - UID<-as.numeric(paste("field number", round(RAmax*1000000), abs(round(DECmax*1000000)), sep=""))meta.idBIGINTprincipalDEVILS_IDDEVILS spectroscopic CATAIDmeta.idVARCHARprincipalDECcenDeclination position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.decDOUBLEprincipalRAcenRight assecention position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.raDOUBLEprincipalzBestBest redshift from source taken from DEVILS_D10MasterRedshiftCatsrc.redshiftDOUBLEprincipalProSpect_MstarProSpect stellar mass taken from Torne et al in preplog(solMass)phys.mass.starsDOUBLEprincipalProSpect_Mstar_LBProSpect stellar mass lower bound of final MCMC chain taken from Torne et al in preplog(solMass)phys.mass.stars;stat.minDOUBLEprincipalProSpect_Mstar_UBProSpect stellar mass upper bound of final MCMC chain taken from Torne et al in preplog(solMass)phys.mass.stars;stat.maxDOUBLEprincipalProSpect_SFRProSpect burst SFR taken from Torne et al in preplog(solMass/yr)phys.sfrDOUBLEprincipalProSpect_SFR_LBProSpect burst SFR lower bound of final MCMC chain taken from Torne et al in preplog(solMass/yr)phys.sfr;stat.minDOUBLEprincipalProSpect_SFR_UBProSpect burst SFR upper bound of final MCMC chain taken from Torne et al in preplog(solMass/yr)phys.sfr;stat.maxDOUBLEprincipalLaigle_logMstarLog10 Stellar mass measurement from the Laigale et al COSMOS2015 cataloguelog(solMass)phys.mass.starsDOUBLEprincipalG10_zBestBest redshfit from the Davies et al 2015 G10/COSMOS cataloguesrc.redshiftDOUBLEprincipalSERSIC_n_SINGLESersic index from ProFit single component sersic fit to HST F814W bandphys.size.sersicDOUBLEprincipalAUTO_CLASSAutomatic morphology class from Galaxy Zoo and ANN combinationmeta.idVARCHARprincipalFIRST_CLASSFirst rough classificationmeta.idVARCHARprincipalCHECKERSecond pass name of visual checkermeta.idVARCHARprincipalSPD_CLASSSimon Driver visual classificationmeta.idVARCHARprincipalSB_CLASSSabine Bellstedt visual classifcaitionmeta.idVARCHARprincipalLJMD_CLASSLuke Davies visual classificationmeta.idVARCHARprincipalFINAL_CLASSFinal visual classificationmeta.idVARCHARprincipalHSTregIs galaxy within the useable HST region? 1=yes, 0=nometa.idINTEGERprincipalsampSelIs galaxy within the DEVILS morphology sample selection (ProSpect_Mstar>10^9.5 & zBest<1.0 & RAcen>=149.5)? 1=yes, 0=nometa.idINTEGERprincipaldevils_dr1.D10ProFitStructureStructural properties of galaxies in the DEVILS D10 region produced from the HST imaging in the COSMOS region using the ProFit package. Cook et al in prepUIDUID based on feild, RA, DEC taken from DEVILS profound photometry catalogue - UID<-as.numeric(paste("field number", round(RAmax*1000000), abs(round(DECmax*1000000)), sep=""))meta.idBIGINTprincipalRAcenRight assecention position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.raDOUBLEprincipalDECcenDeclination position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.decDOUBLEprincipalRAmaxRight assecention position of the brightest pixel in the ProFound segment in the VISTA Y-band imagedegpos.eq.raDOUBLEprincipalDECmaxDeclination position of the brightest pixel in the ProFound segment in the VISTA Y-band imagedegpos.eq.decDOUBLEprincipalmaskMask flag to identify is segement falls in a masked region. 0=not masked, 1=maskedmeta.idINTEGERprincipalartefactFlagArtefact flag to identify if a segment is deemd to be an artefact (see description paper). 0=Not artefact, >0=artefactmeta.idINTEGERprincipalstarFlagStar/galaxy classifier. 0=galaxy, 1=starmeta.idVARCHARprincipalmag_YTotal magnitude measured in VISTA Y bandmagphot.mag;em.IR.YVARCHARprincipalvis_morphVisual morphology class from Visual Morphology Cataloguesrc.morph.typeVARCHARprincipalbest_modelThe preferred model based on the outputs of the model fit: twocomps, puredisk, spheroid, failed (see readme)meta.idVARCHARprincipalclassThe preferred model based on the visual inspections and adjusted accordingly based on the best-fitting model parameters: twocomps, puredisk, spheroid, failed (see readme)meta.idVARCHARprincipalmagBulgeFinal Class: Bulge Profile integrated HST F814W magnitudemagphot.mag;em.opt.IDOUBLEprincipalmagDiskFinal Class: Disk Profile integrated HST F814W magnitudemagphot.mag;em.opt.IDOUBLEprincipalreBulge_pixFinal Class: Bulge Observed effective radius (R50) in pixelspixelphys.size.radius;em.opt.IDOUBLEprincipalreDisk_pixFinal Class: Disk Observed effective radius (R50) in pixelspixelphys.size.radius;em.opt.IDOUBLEprincipalreTotal_pixFinal Class: Total (disk+bulge) Observed effective radius (R50) in pixelspixelphys.size.radius;em.opt.IDOUBLEprincipalreBulge_kpcFinal Class: Bulge physical effective radius (R50) in kpckpcphys.size.radius;em.opt.IDOUBLEprincipalreDisk_kpcFinal Class: Disk physical effective radius (R50) in kpckpcphys.size.radius;em.opt.IDOUBLEprincipalreTotal_kpcFinal Class: Total (disk+bulge) Observed effective radius (R50) in kpckpcphys.size.radius;em.opt.IDOUBLEprincipalnserBulgeFinal Class: Bulge Sersic Indexsrc.morph.type;em.opt.IDOUBLEprincipalnserDiskFinal Class: Disk Sersic Indexsrc.morph.type;em.opt.IDOUBLEprincipalaxratBulgeFinal Class: Bulge Axial Ratiophys.size.axisRatio;em.opt.IDOUBLEprincipalaxratDiskFinal Class: Disk Axial Ratiophys.size.axisRatio;em.opt.IDOUBLEprincipalB2T_corrFinal Class: Bulge Position angle (increasing clockwise 0 deg from North)degpos.posAng;em.opt.IDOUBLEprincipalangDiskFinal Class: Disk Position angle (increasing clockwise 0 deg from North)degpos.posAng;em.opt.IDOUBLEprincipalangBulgeFinal Class: Light-weighted Bulge-to-total ratiosrc.morph.typeDOUBLEprincipalxcen_singleSingle component fit: Central x pixel positionpixelpos.centroidDOUBLEprincipalycen_singleSingle component fit: Central y pixel positionpixelpos.centroidDOUBLEprincipalmag_singleSingle component fit: Profile integrated HST F814W magnitudemagphot.mag;em.opt.IDOUBLEprincipalre_single_kpcSingle component fit: Effective radius (R50) in kpckpcphys.size.radius;em.opt.IDOUBLEprincipalnser_singleSingle component fit: Sersic Indexsrc.morph.type;em.opt.IDOUBLEprincipalang_singleSingle component fit: Position angle (increasing clockwise 0 deg from North)degpos.posAng;em.opt.IDOUBLEprincipalaxrat_singleSingle component fit: Axial Ratiophys.size.axisRatio;em.opt.IDOUBLEprincipalxcen_err_singleSingle component fit: Central x pixel position Errorpixelstat.error;pos.centroidDOUBLEprincipalycen_err_singleSingle component fit: Central y pixel position Errorpixelstat.error;pos.centroidDOUBLEprincipalmag_err_singleSingle component fit: Profile integrated HST F814W magnitude Errormagstat.error;phot.mag;em.opt.IDOUBLEprincipalre_err_singleSingle component fit: Effective radius (R50) in kpc Errorkpcstat.error;phys.size.radius;em.opt.IDOUBLEprincipalnser_err_singleSingle component fit: Sersic Index Errorstat.error;src.morph.type;em.opt.IDOUBLEprincipalang_err_singleSingle component fit: Position angle (increasing clockwise 0 deg from North) Errordegstat.error;pos.posAng;em.opt.IDOUBLEprincipalaxrat_err_singleSingle component fit: Axial Ratio Errorstat.error;phys.size.axisRatio;em.opt.IDOUBLEprincipalLP_singleSingle component fit: LP for best fitstat.fit.goodnessDOUBLEprincipalDIC_singleSingle component fit: deviance information criterion for best fitstat.fit.goodnessDOUBLEprincipaltime_singleSingle component fit: time to run ProFuse fitsectime.durationDOUBLEprincipalxcen_serexpSersic Bulge + Exponential Disk fit: Central x pixel positionpixelpos.centroidDOUBLEprincipalycen_serexpSersic Bulge + Exponential Disk fit: Central y pixel positionpixelpos.centroidDOUBLEprincipalmag1_serexpSersic Bulge + Exponential Disk fit: Comp1 Profile integrated HST F814W magnitudemagphot.mag;em.opt.IDOUBLEprincipalmag2_serexpSersic Bulge + Exponential Disk fit: Comp2 Profile integrated HST F814W magnitudemagphot.mag;em.opt.IDOUBLEprincipalre1_serexp_kpcSersic Bulge + Exponential Disk fit: Comp1 Effective radius (R50) in kpckpcphys.size.radius;em.opt.IDOUBLEprincipalre2_serexp_kpcSersic Bulge + Exponential Disk fit: Comp2 effective radius (R50) in kpckpcphys.size.radius;em.opt.IDOUBLEprincipalnser1_serexpSersic Bulge + Exponential Disk fit: Comp1 Sersic Indexsrc.morph.type;em.opt.IDOUBLEprincipalang2_serexpSersic Bulge + Exponential Disk fit: Comp2 Position angle (increasing clockwise 0 deg from North)degpos.posAng;em.opt.IDOUBLEprincipalaxrat2_serexpSersic Bulge + Exponential Disk fit: Comp2 Axial Ratiophys.size.axisRatio;em.opt.IDOUBLEprincipalxcen_err_serexpSersic Bulge + Exponential Disk fit: Central x pixel position Errorpixelstat.error;pos.centroidDOUBLEprincipalycen_err_serexpSersic Bulge + Exponential Disk fit: Central y pixel position Errorpixelstat.error;pos.centroidDOUBLEprincipalmag1_err_serexpSersic Bulge + Exponential Disk fit: Comp1 Profile integrated HST F814W magnitude Errormagstat.error;phot.mag;em.opt.IDOUBLEprincipalmag2_err_serexpSersic Bulge + Exponential Disk fit: Comp2 Profile integrated HST F814W magnitude Errormagstat.error;phot.mag;em.opt.IDOUBLEprincipalre1_err_serexpSersic Comp1 + Exponential Disk fit: Comp1 Effective radius (R50) in kpc Errorkpcstat.error;phys.size.radius;em.opt.IDOUBLEprincipalre2_err_serexpSersic Bulge + Exponential Disk fit: Comp2 effective radius (R50) in kpc Errorkpcstat.error;phys.size.radius;em.opt.IDOUBLEprincipalnser1_err_serexpSersic Bulge + Exponential Disk fit: Comp1 Sersic Index Errorstat.error;src.morph.type;em.opt.IDOUBLEprincipalang2_err_serexpSersic Bulge + Exponential Disk fit: Comp2 Position angle (increasing clockwise 0 deg from North) Errordegstat.error;pos.posAng;em.opt.IDOUBLEprincipalaxrat2_err_serexpSersic Bulge + Exponential Disk fit: Comp2 Axial Ratio Errorstat.error;phys.size.axisRatio;em.opt.IDOUBLEprincipalLP_serexpSersic Bulge + Exponential Disk fit: LP for best fitstat.fit.goodnessDOUBLEprincipalDIC_serexpSersic Bulge + Exponential Disk fit: deviance information criterion for best fitstat.fit.goodnessDOUBLEprincipaltime_serexpSersic Bulge + Exponential Disk fit: time to run ProFuse fitsecsrc.morph.typeDOUBLEprincipalB2T_serexpSersic Bulge + Exponential Disk fit: Light-weighted Comp1-to-Comp1+2 ratiotime.durationDOUBLEprincipalnexpsNumber of HST exposures included in fitstat.valueDOUBLEprincipalnpixelsNumber of HST pixels used in the profile fittinginstr.pixelDOUBLEprincipaldevils_dr1.D10ProSpectAGNSED-derived properties (stellar mass, SFR, metallicity, etc) for galaxies in the DEVILS D10 region derived using the photometry in the D10ProFoundPhotometry catalogue and the ProSpect SED-fitting code. This catalogue fits the data with a possible AGN component. It therefore also contain properties detailing the AGN fit parameters. Thorne et al 2022UIDUnique Identifier for each galaxymeta.idBIGINTprincipalflux.irac_1best fit flux in irac_1Jyphot.flux.densityDOUBLEprincipalzRedshiftsrc.redshiftDOUBLEprincipalmSFRProSpect parameter that controls the maximum star formation rate in the skewed normal - loggedlog(solMass/yr)stat.paramDOUBLEprincipalmpeakProSpect parameter that controls where the peak of star formation occursGyrstat.paramDOUBLEprincipalmperiodProSpect parameter that controls the width of the star formation skewed Normal - loggedlog(Gyr)stat.paramDOUBLEprincipalmskewProSpect Parameter that controls the skew of the skewed Normalstat.paramDOUBLEprincipaltau_birthProSpect Parameter to describes the column density of dust in the birth clouds - loggedstat.paramDOUBLEprincipaltau_screenProSpect Parameter to describes the column density of dust in the ISM- loggedstat.paramDOUBLEprincipalalpha_SF_birthProSpect Parameter to describes the temperature of the dust in the birth cloudsstat.paramDOUBLEprincipalalpha_SF_screenProSpect Parameter to describes the temperature of the dust in the ISMstat.paramDOUBLEprincipalZfinalFinal Gas Phase Metallicity, modelled in ProSpect - loggedstat.param;phys.abund.ZDOUBLEprincipalAGNlumbolometric luminosity of AGN source - loggedlog(erg/s)phys.luminosity.bolDOUBLEprincipalAGNanangle of observation of AGN sourcedegphys.angDOUBLEprincipalAGNtaoptical depth tau of AGN source - loggedphys.absorption.opticalDepthDOUBLEprincipalLPlog posterior of best fit model in ProSpectstat.likelihoodDOUBLEprincipalStellarMassremaining stellar mass, generally this should be the value you usesolMassphys.massDOUBLEprincipalStellarMassFormedtotal stellar mass formed, not remainingsolMassphys.massDOUBLEprincipaldustmass.birthdust mass in birth cloudssolMassphys.massDOUBLEprincipaldustmass.screendust mass in ISMsolMassphys.massDOUBLEprincipaldustmass.totaldust mass totalsolMassphys.massDOUBLEprincipaldustlum.birthdust luminosity in birth cloudssolLumphys.luminosityDOUBLEprincipaldustlum.screendust luminosity in ISMsolLumphys.luminosityDOUBLEprincipaldustlum.totaldust luminosity totalsolLumphys.luminosityDOUBLEprincipalSFRburstSFR measured over 100Myr baselinesolMass/yrphys.SFRDOUBLEprincipalflux.galex_fuvbest fit flux in galex_fuvJyphot.flux.densityDOUBLEprincipalflux.galex_nuvbest fit flux in galex_nuvJyphot.flux.densityDOUBLEprincipalflux.cfht_ubest fit flux in cfht_uJyphot.flux.densityDOUBLEprincipalflux.hsc_gbest fit flux in hsc_gJyphot.flux.densityDOUBLEprincipalflux.hsc_rbest fit flux in hsc_rJyphot.flux.densityDOUBLEprincipalflux.hsc_ibest fit flux in hsc_iJyphot.flux.densityDOUBLEprincipalflux.hsc_zbest fit flux in hsc_zJyphot.flux.densityDOUBLEprincipalflux.vista_Ybest fit flux in vista_YJyphot.flux.densityDOUBLEprincipalflux.vista_Jbest fit flux in vista_JJyphot.flux.densityDOUBLEprincipalflux.vista_Hbest fit flux in vista_HJyphot.flux.densityDOUBLEprincipalflux.vista_Ksbest fit flux in vista_KsJyphot.flux.densityDOUBLEprincipalflux.irac_2best fit flux in irac_2Jyphot.flux.densityDOUBLEprincipalflux.irac_3best fit flux in irac_3Jyphot.flux.densityDOUBLEprincipalflux.irac_4best fit flux in irac_4Jyphot.flux.densityDOUBLEprincipalflux.mips_24best fit flux in mips_24Jyphot.flux.densityDOUBLEprincipalflux.mips_70best fit flux in mips_70Jyphot.flux.densityDOUBLEprincipalflux.pacs_100best fit flux in pacs_100Jyphot.flux.densityDOUBLEprincipalflux.pacs_160best fit flux in pacs_160Jyphot.flux.densityDOUBLEprincipalflux.spire_250best fit flux in spire_250Jyphot.flux.densityDOUBLEprincipalflux.spire_350best fit flux in spire_350Jyphot.flux.densityDOUBLEprincipalflux.spire_500best fit flux in spire_500Jyphot.flux.densityDOUBLEprincipalmSFR_LBLower bound of ProSpect parameter that controls the maximum star formation rate in the skewed normal - loggedlog(solMass/yr)stat.param;stat.minDOUBLEprincipalmpeak_LBLower bound of ProSpect parameter that controls where the peak of star formation occursGyrstat.param;stat.minDOUBLEprincipalmperiod_LBLower bound of ProSpect parameter that controls the width of the star formation skewed Normal - loggedlog(Gyr)stat.param;stat.minDOUBLEprincipalmskew_LBLower bound of ProSpect Parameter that controls the skew of the skewed Normalstat.param;stat.minDOUBLEprincipaltau_birth_LBLower bound of ProSpect Parameter to describes the column density of dust in the birth clouds - loggedstat.param;stat.minDOUBLEprincipaltau_screen_LBLower bound of ProSpect Parameter to describes the column density of dust in the ISM- loggedstat.param;stat.minDOUBLEprincipalalpha_SF_birth_LBLower bound of ProSpect Parameter to describes the temperature of the dust in the birth cloudsstat.param;stat.minDOUBLEprincipalalpha_SF_screen_LBLower bound of ProSpect Parameter to describes the temperature of the dust in the ISMstat.param;stat.minDOUBLEprincipalZfinal_LBLower bound of Final Gas Phase Metallicity, modelled in ProSpect - loggedstat.param;phys.abund.Z;stat.minDOUBLEprincipalAGNlum_LBLower bound of bolometric luminosity of AGN source - loggedlog(erg/s)phys.luminosity.bol;stat.minDOUBLEprincipalAGNan_LBLower bound of angle of observation of AGN sourcedegphys.ang;stat.minDOUBLEprincipalAGNta_LBLower bound of optical depth tau of AGN source - loggedphys.absorption.opticalDepth;stat.minDOUBLEprincipalLP_LBLower bound of log posterior of best fit model in ProSpectstat.likelihood;stat.minDOUBLEprincipalStellarMass_LBLower bound of remaining stellar mass, generally this should be the value you usesolMassphys.mass;stat.minDOUBLEprincipalStellarMassFormed_LBLower bound of total stellar mass formed, not remainingsolMassphys.mass;stat.minDOUBLEprincipaldustmass.birth_LBLower bound of dust mass in birth cloudssolMassphys.mass;stat.minDOUBLEprincipaldustmass.screen_LBLower bound of dust mass in ISMsolMassphys.mass;stat.minDOUBLEprincipaldustmass.total_LBLower bound of dust mass totalsolMassphys.mass;stat.minDOUBLEprincipaldustlum.birth_LBLower bound of dust luminosity in birth cloudssolLumphys.luminosity;stat.minDOUBLEprincipaldustlum.screen_LBLower bound of dust luminosity in ISMsolLumphys.luminosity;stat.minDOUBLEprincipaldustlum.total_LBLower bound of dust luminosity totalsolLumphys.luminosity;stat.minDOUBLEprincipalSFRburst_LBLower bound of SFR measured over 100Myr baselinesolMass/yrphys.SFR;stat.minDOUBLEprincipalflux.galex_fuv_LBLower bound of best fit flux in galex_fuvJyphot.flux.density;stat.minDOUBLEprincipalflux.galex_nuv_LBLower bound of best fit flux in galex_nuvJyphot.flux.density;stat.minDOUBLEprincipalflux.cfht_u_LBLower bound of best fit flux in cfht_uJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_g_LBLower bound of best fit flux in hsc_gJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_r_LBLower bound of best fit flux in hsc_rJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_i_LBLower bound of best fit flux in hsc_iJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_z_LBLower bound of best fit flux in hsc_zJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_Y_LBLower bound of best fit flux in vista_YJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_J_LBLower bound of best fit flux in vista_JJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_H_LBLower bound of best fit flux in vista_HJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_Ks_LBLower bound of best fit flux in vista_KsJyphot.flux.density;stat.minDOUBLEprincipalflux.irac_1_LBLower bound of best fit flux in irac_1Jyphot.flux.density;stat.minDOUBLEprincipalflux.irac_2_LBLower bound of best fit flux in irac_2Jyphot.flux.density;stat.minDOUBLEprincipalflux.irac_3_LBLower bound of best fit flux in irac_3Jyphot.flux.density;stat.minDOUBLEprincipalflux.irac_4_LBLower bound of best fit flux in irac_4Jyphot.flux.density;stat.minDOUBLEprincipalflux.mips_24_LBLower bound of best fit flux in mips_24Jyphot.flux.density;stat.minDOUBLEprincipalflux.mips_70_LBLower bound of best fit flux in mips_70Jyphot.flux.density;stat.minDOUBLEprincipalflux.pacs_100_LBLower bound of best fit flux in pacs_100Jyphot.flux.density;stat.minDOUBLEprincipalflux.pacs_160_LBLower bound of best fit flux in pacs_160Jyphot.flux.density;stat.minDOUBLEprincipalflux.spire_250_LBLower bound of best fit flux in spire_250Jyphot.flux.density;stat.minDOUBLEprincipalflux.spire_350_LBLower bound of best fit flux in spire_350Jyphot.flux.density;stat.minDOUBLEprincipalflux.spire_500_LBLower bound of best fit flux in spire_500Jyphot.flux.density;stat.minDOUBLEprincipalmSFR_UBUpper bound of ProSpect parameter that controls the maximum star formation rate in the skewed normal - loggedlog(solMass/yr)stat.param;stat.maxDOUBLEprincipalmpeak_UBUpper bound of ProSpect parameter that controls where the peak of star formation occursGyrstat.param;stat.maxDOUBLEprincipalmperiod_UBUpper bound of ProSpect parameter that controls the width of the star formation skewed Normal - loggedlog(Gyr)stat.param;stat.maxDOUBLEprincipalmskew_UBUpper bound of ProSpect Parameter that controls the skew of the skewed Normalstat.param;stat.maxDOUBLEprincipaltau_birth_UBUpper bound of ProSpect Parameter to describes the column density of dust in the birth clouds - loggedstat.param;stat.maxDOUBLEprincipaltau_screen_UBUpper bound of ProSpect Parameter to describes the column density of dust in the ISM- loggedstat.param;stat.maxDOUBLEprincipalalpha_SF_birth_UBUpper bound of ProSpect Parameter to describes the temperature of the dust in the birth cloudsstat.param;stat.maxDOUBLEprincipalalpha_SF_screen_UBUpper bound of ProSpect Parameter to describes the temperature of the dust in the ISMstat.param;stat.maxDOUBLEprincipalZfinal_UBUpper bound of Final Gas Phase Metallicity, modelled in ProSpect - loggedstat.param;phys.abund.Z;stat.maxDOUBLEprincipalAGNlum_UBUpper bound of bolometric luminosity of AGN source - loggedlog(erg/s)phys.luminosity.bol;stat.maxDOUBLEprincipalAGNan_UBUpper bound of angle of observation of AGN sourcedegphys.ang;stat.maxDOUBLEprincipalAGNta_UBUpper bound of optical depth tau of AGN source - loggedphys.absorption.opticalDepth;stat.minDOUBLEprincipalLP_UBUpper bound of log posterior of best fit model in ProSpectstat.likelihood;stat.maxDOUBLEprincipalStellarMass_UBUpper bound of remaining stellar mass, generally this should be the value you usesolMassphys.mass;stat.maxDOUBLEprincipalStellarMassFormed_UBUpper bound of total stellar mass formed, not remainingsolMassphys.mass;stat.maxDOUBLEprincipaldustmass.birth_UBUpper bound of dust mass in birth cloudssolMassphys.mass;stat.maxDOUBLEprincipaldustmass.screen_UBUpper bound of dust mass in ISMsolMassphys.mass;stat.maxDOUBLEprincipaldustmass.total_UBUpper bound of dust mass totalsolMassphys.mass;stat.maxDOUBLEprincipaldustlum.birth_UBUpper bound of dust luminosity in birth cloudssolLumphys.luminosity;stat.maxDOUBLEprincipaldustlum.screen_UBUpper bound of dust luminosity in ISMsolLumphys.luminosity;stat.maxDOUBLEprincipaldustlum.total_UBUpper bound of dust luminosity totalsolLumphys.luminosity;stat.maxDOUBLEprincipalSFRburst_UBUpper bound of SFR measured over 100Myr baselinesolMass/yrphys.SFR;stat.maxDOUBLEprincipalflux.galex_fuv_UBUpper bound of best fit flux in galex_fuvJyphot.flux.density;stat.maxDOUBLEprincipalflux.galex_nuv_UBUpper bound of best fit flux in galex_nuvJyphot.flux.density;stat.maxDOUBLEprincipalflux.cfht_u_UBUpper bound of best fit flux in cfht_uJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_g_UBUpper bound of best fit flux in hsc_gJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_r_UBUpper bound of best fit flux in hsc_rJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_i_UBUpper bound of best fit flux in hsc_iJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_z_UBUpper bound of best fit flux in hsc_zJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_Y_UBUpper bound of best fit flux in vista_YJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_J_UBUpper bound of best fit flux in vista_JJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_H_UBUpper bound of best fit flux in vista_HJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_Ks_UBUpper bound of best fit flux in vista_KsJyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_1_UBUpper bound of best fit flux in irac_1Jyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_2_UBUpper bound of best fit flux in irac_2Jyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_3_UBUpper bound of best fit flux in irac_3Jyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_4_UBUpper bound of best fit flux in irac_4Jyphot.flux.density;stat.maxDOUBLEprincipalflux.mips_24_UBUpper bound of best fit flux in mips_24Jyphot.flux.density;stat.maxDOUBLEprincipalflux.mips_70_UBUpper bound of best fit flux in mips_70Jyphot.flux.density;stat.maxDOUBLEprincipalflux.pacs_100_UBUpper bound of best fit flux in pacs_100Jyphot.flux.density;stat.maxDOUBLEprincipalflux.pacs_160_UBUpper bound of best fit flux in pacs_160Jyphot.flux.density;stat.maxDOUBLEprincipalflux.spire_250_UBUpper bound of best fit flux in spire_250Jyphot.flux.density;stat.maxDOUBLEprincipalflux.spire_350_UBUpper bound of best fit flux in spire_350Jyphot.flux.density;stat.maxDOUBLEprincipalflux.spire_500_UBUpper bound of best fit flux in spire_500Jyphot.flux.density;stat.maxDOUBLEprincipalAGNfracfraction of flux contributed by the AGN component between 5−20micronphys.luminosity.bol;stat.weightDOUBLEprincipalTypeAGN type 1 or 2meta.code.classINTEGERprincipalIterationIteration?meta.numberINTEGERprincipalflux_3GHzpredicted flux at 3GHz from ProSpect fitJyem.radio.3-6GHz;stat.valueDOUBLEprincipalHalfMassAgeThe age taken to form half the galaxy's mass based on the best for SFHGyrphys.ageDOUBLEprincipaldevils_dr1.D10ProSpectNoAGNSED-derived properties (stellar mass, SFR, metallicity, etc) for galaxies in the DEVILS D10 region derived using the photometry in the D10ProFoundPhotometry catalogue and the ProSpect SED-fitting code. This catalogue fits the data with no possible AGN component. Thorne et al 2021UIDUID - Unique Identifier for each galaxymeta.idBIGINTprincipalzz - Redshiftsrc.redshiftDOUBLEprincipalmSFRmSFR - ProSpect parameter that controls the maximum star formation rate in the skewed normal - loggedlog(solMass/yr)stat.paramDOUBLEprincipalmpeakmpeak - ProSpect parameter that controls where the peak of star formation occursGyrstat.paramDOUBLEprincipalmperiodmperiod - ProSpect parameter that controls the width of the star formation skewed Normal - loggedlog(Gyr)stat.paramDOUBLEprincipalmskewmskew - ProSpect Parameter that controls the skew of the skewed Normalstat.paramDOUBLEprincipaltau_birthtau_birth - ProSpect Parameter to describes the column density of dust in the birth clouds - loggedstat.paramDOUBLEprincipaltau_screentau_screen - ProSpect Parameter to describes the column density of dust in the ISM- loggedstat.paramDOUBLEprincipalalpha_SF_birthalpha_SF_birth - ProSpect Parameter to describes the temperature of the dust in the birth cloudsstat.paramDOUBLEprincipalalpha_SF_screenalpha_SF_screen - ProSpect Parameter to describes the temperature of the dust in the ISMstat.paramDOUBLEprincipalZfinalZfinal - Final Gas Phase Metallicity, modelled in ProSpect - loggedstat.param;phys.abund.ZDOUBLEprincipalLPLP - log posterior of best fit model in ProSpectstat.likelihoodDOUBLEprincipalStellarMassStellarMass - remaining stellar mass, generally this should be the value you usesolMassphys.massDOUBLEprincipalStellarMassFormedStellarMassFormed - total stellar mass formed, not remainingsolMassphys.massDOUBLEprincipaldustmass.birthdustmass.birth - dust mass in birth cloudssolMassphys.massDOUBLEprincipaldustmass.screendustmass.screen - dust mass in ISMsolMassphys.massDOUBLEprincipaldustmass.totaldustmass.total - dust mass totalsolMassphys.massDOUBLEprincipaldustlum.birthdustlum.birth - dust luminosity in birth cloudssolLumphys.luminosityDOUBLEprincipaldustlum.screendustlum.screen - dust luminosity in ISMsolLumphys.luminosityDOUBLEprincipaldustlum.totaldustlum.total - dust luminosity totalsolLumphys.luminosityDOUBLEprincipalSFRburstSFRburst - SFR measured over 100Myr baselinesolMass/yrphys.SFRDOUBLEprincipalflux.galex_fuvflux.galex_fuv - best fit flux in galex_fuvJyphot.flux.densityDOUBLEprincipalflux.galex_nuvflux.galex_nuv - best fit flux in galex_nuvJyphot.flux.densityDOUBLEprincipalflux.cfht_uflux.cfht_u - best fit flux in cfht_uJyphot.flux.densityDOUBLEprincipalflux.hsc_gflux.hsc_g - best fit flux in hsc_gJyphot.flux.densityDOUBLEprincipalflux.hsc_rflux.hsc_r - best fit flux in hsc_rJyphot.flux.densityDOUBLEprincipalflux.hsc_iflux.hsc_i - best fit flux in hsc_iJyphot.flux.densityDOUBLEprincipalflux.hsc_zflux.hsc_z - best fit flux in hsc_zJyphot.flux.densityDOUBLEprincipalflux.vista_Yflux.vista_Y - best fit flux in vista_YJyphot.flux.densityDOUBLEprincipalflux.vista_Jflux.vista_J - best fit flux in vista_JJyphot.flux.densityDOUBLEprincipalflux.vista_Hflux.vista_H - best fit flux in vista_HJyphot.flux.densityDOUBLEprincipalflux.vista_Ksflux.vista_Ks - best fit flux in vista_KsJyphot.flux.densityDOUBLEprincipalflux.irac_1flux.irac_1 - best fit flux in irac_1Jyphot.flux.densityDOUBLEprincipalflux.irac_2flux.irac_2 - best fit flux in irac_2Jyphot.flux.densityDOUBLEprincipalflux.irac_3flux.irac_3 - best fit flux in irac_3Jyphot.flux.densityDOUBLEprincipalflux.irac_4flux.irac_4 - best fit flux in irac_4Jyphot.flux.densityDOUBLEprincipalflux.mips_24flux.mips_24 - best fit flux in mips_24Jyphot.flux.densityDOUBLEprincipalflux.mips_70flux.mips_70 - best fit flux in mips_70Jyphot.flux.densityDOUBLEprincipalflux.pacs_100flux.pacs_100 - best fit flux in pacs_100Jyphot.flux.densityDOUBLEprincipalflux.pacs_160flux.pacs_160 - best fit flux in pacs_160Jyphot.flux.densityDOUBLEprincipalflux.spire_250flux.spire_250 - best fit flux in spire_250Jyphot.flux.densityDOUBLEprincipalflux.spire_350flux.spire_350 - best fit flux in spire_350Jyphot.flux.densityDOUBLEprincipalflux.spire_500flux.spire_500 - best fit flux in spire_500Jyphot.flux.densityDOUBLEprincipalmSFR_LBmSFR_LB - Lower bound of ProSpect parameter that controls the maximum star formation rate in the skewed normal - loggedlog(solMass/yr)stat.param;stat.minDOUBLEprincipalmpeak_LBmpeak_LB - Lower bound of ProSpect parameter that controls where the peak of star formation occursGyrstat.param;stat.minDOUBLEprincipalmperiod_LBmperiod_LB - Lower bound of ProSpect parameter that controls the width of the star formation skewed Normal - loggedlog(Gyr)stat.param;stat.minDOUBLEprincipalmskew_LBmskew_LB - Lower bound of ProSpect Parameter that controls the skew of the skewed Normalstat.param;stat.minDOUBLEprincipaltau_birth_LBtau_birth_LB - Lower bound of ProSpect Parameter to describes the column density of dust in the birth clouds - loggedstat.param;stat.minDOUBLEprincipaltau_screen_LBtau_screen_LB - Lower bound of ProSpect Parameter to describes the column density of dust in the ISM- loggedstat.param;stat.minDOUBLEprincipalalpha_SF_birth_LBalpha_SF_birth_LB - Lower bound of ProSpect Parameter to describes the temperature of the dust in the birth cloudsstat.param;stat.minDOUBLEprincipalalpha_SF_screen_LBalpha_SF_screen_LB - Lower bound of ProSpect Parameter to describes the temperature of the dust in the ISMstat.param;stat.minDOUBLEprincipalZfinal_LBZfinal_LB - Lower bound of Final Gas Phase Metallicity, modelled in ProSpect - loggedstat.param;phys.abund.Z;stat.minDOUBLEprincipalLP_LBLP_LB - Lower bound of log posterior of best fit model in ProSpectstat.likelihood;stat.minDOUBLEprincipalStellarMass_LBStellarMass_LB - Lower bound of remaining stellar mass, generally this should be the value you usesolMassphys.mass;stat.minDOUBLEprincipalStellarMassFormed_LBStellarMassFormed_LB - Lower bound of total stellar mass formed, not remainingsolMassphys.mass;stat.minDOUBLEprincipaldustmass.birth_LBdustmass.birth_LB - Lower bound of dust mass in birth cloudssolMassphys.mass;stat.minDOUBLEprincipaldustmass.screen_LBdustmass.screen_LB - Lower bound of dust mass in ISMsolMassphys.mass;stat.minDOUBLEprincipaldustmass.total_LBdustmass.total_LB - Lower bound of dust mass totalsolMassphys.mass;stat.minDOUBLEprincipaldustlum.birth_LBdustlum.birth_LB - Lower bound of dust luminosity in birth cloudssolLumphys.luminosity;stat.minDOUBLEprincipaldustlum.screen_LBdustlum.screen_LB - Lower bound of dust luminosity in ISMsolLumphys.luminosity;stat.minDOUBLEprincipaldustlum.total_LBdustlum.total_LB - Lower bound of dust luminosity totalsolLumphys.luminosity;stat.minDOUBLEprincipalSFRburst_LBSFRburst_LB - Lower bound of SFR measured over 100Myr baselinesolMass/yrphys.SFR;stat.minDOUBLEprincipalflux.galex_fuv_LBflux.galex_fuv_LB - Lower bound of best fit flux in galex_fuvJyphot.flux.density;stat.minDOUBLEprincipalflux.galex_nuv_LBflux.galex_nuv_LB - Lower bound of best fit flux in galex_nuvJyphot.flux.density;stat.minDOUBLEprincipalflux.cfht_u_LBflux.cfht_u_LB - Lower bound of best fit flux in cfht_uJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_g_LBflux.hsc_g_LB - Lower bound of best fit flux in hsc_gJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_r_LBflux.hsc_r_LB - Lower bound of best fit flux in hsc_rJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_i_LBflux.hsc_i_LB - Lower bound of best fit flux in hsc_iJyphot.flux.density;stat.minDOUBLEprincipalflux.hsc_z_LBflux.hsc_z_LB - Lower bound of best fit flux in hsc_zJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_Y_LBflux.vista_Y_LB - Lower bound of best fit flux in vista_YJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_J_LBflux.vista_J_LB - Lower bound of best fit flux in vista_JJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_H_LBflux.vista_H_LB - Lower bound of best fit flux in vista_HJyphot.flux.density;stat.minDOUBLEprincipalflux.vista_Ks_LBflux.vista_Ks_LB - Lower bound of best fit flux in vista_KsJyphot.flux.density;stat.minDOUBLEprincipalflux.irac_1_LBflux.irac_1_LB - Lower bound of best fit flux in irac_1Jyphot.flux.density;stat.minDOUBLEprincipalflux.irac_2_LBflux.irac_2_LB - Lower bound of best fit flux in irac_2Jyphot.flux.density;stat.minDOUBLEprincipalflux.irac_3_LBflux.irac_3_LB - Lower bound of best fit flux in irac_3Jyphot.flux.density;stat.minDOUBLEprincipalflux.irac_4_LBflux.irac_4_LB - Lower bound of best fit flux in irac_4Jyphot.flux.density;stat.minDOUBLEprincipalflux.mips_24_LBflux.mips_24_LB - Lower bound of best fit flux in mips_24Jyphot.flux.density;stat.minDOUBLEprincipalflux.mips_70_LBflux.mips_70_LB - Lower bound of best fit flux in mips_70Jyphot.flux.density;stat.minDOUBLEprincipalflux.pacs_100_LBflux.pacs_100_LB - Lower bound of best fit flux in pacs_100Jyphot.flux.density;stat.minDOUBLEprincipalflux.pacs_160_LBflux.pacs_160_LB - Lower bound of best fit flux in pacs_160Jyphot.flux.density;stat.minDOUBLEprincipalflux.spire_250_LBflux.spire_250_LB - Lower bound of best fit flux in spire_250Jyphot.flux.density;stat.minDOUBLEprincipalflux.spire_350_LBflux.spire_350_LB - Lower bound of best fit flux in spire_350Jyphot.flux.density;stat.minDOUBLEprincipalflux.spire_500_LBflux.spire_500_LB - Lower bound of best fit flux in spire_500Jyphot.flux.density;stat.minDOUBLEprincipalmSFR_UBmSFR_UB - Upper bound of ProSpect parameter that controls the maximum star formation rate in the skewed normal - loggedlog(solMass/yr)stat.param;stat.maxDOUBLEprincipalmpeak_UBmpeak_UB - Upper bound of ProSpect parameter that controls where the peak of star formation occursGyrstat.param;stat.maxDOUBLEprincipalmperiod_UBmperiod_UB - Upper bound of ProSpect parameter that controls the width of the star formation skewed Normal - loggedlog(Gyr)stat.param;stat.maxDOUBLEprincipalmskew_UBmskew_UB - Upper bound of ProSpect Parameter that controls the skew of the skewed Normalstat.param;stat.maxDOUBLEprincipaltau_birth_UBtau_birth_UB - Upper bound of ProSpect Parameter to describes the column density of dust in the birth clouds - loggedstat.param;stat.maxDOUBLEprincipaltau_screen_UBtau_screen_UB - Upper bound of ProSpect Parameter to describes the column density of dust in the ISM- loggedstat.param;stat.maxDOUBLEprincipalalpha_SF_birth_UBalpha_SF_birth_UB - Upper bound of ProSpect Parameter to describes the temperature of the dust in the birth cloudsstat.param;stat.maxDOUBLEprincipalalpha_SF_screen_UBalpha_SF_screen_UB - Upper bound of ProSpect Parameter to describes the temperature of the dust in the ISMstat.param;stat.maxDOUBLEprincipalZfinal_UBZfinal_UB - Upper bound of Final Gas Phase Metallicity, modelled in ProSpect - loggedstat.param;phys.abund.Z;stat.maxDOUBLEprincipalLP_UBLP_UB - Upper bound of log posterior of best fit model in ProSpectstat.likelihood;stat.maxDOUBLEprincipalStellarMass_UBStellarMass_UB - Upper bound of remaining stellar mass, generally this should be the value you usesolMassphys.mass;stat.maxDOUBLEprincipalStellarMassFormed_UBStellarMassFormed_UB - Upper bound of total stellar mass formed, not remainingsolMassphys.mass;stat.maxDOUBLEprincipaldustmass.birth_UBdustmass.birth_UB - Upper bound of dust mass in birth cloudssolMassphys.mass;stat.maxDOUBLEprincipaldustmass.screen_UBdustmass.screen_UB - Upper bound of dust mass in ISMsolMassphys.mass;stat.maxDOUBLEprincipaldustmass.total_UBdustmass.total_UB - Upper bound of dust mass totalsolMassphys.mass;stat.maxDOUBLEprincipaldustlum.birth_UBdustlum.birth_UB - Upper bound of dust luminosity in birth cloudssolLumphys.luminosity;stat.maxDOUBLEprincipaldustlum.screen_UBdustlum.screen_UB - Upper bound of dust luminosity in ISMsolLumphys.luminosity;stat.maxDOUBLEprincipaldustlum.total_UBdustlum.total_UB - Upper bound of dust luminosity totalsolLumphys.luminosity;stat.maxDOUBLEprincipalSFRburst_UBSFRburst_UB - Upper bound of SFR measured over 100Myr baselinesolMass/yrphys.SFR;stat.maxDOUBLEprincipalflux.galex_fuv_UBflux.galex_fuv_UB - Upper bound of best fit flux in galex_fuvJyphot.flux.density;stat.maxDOUBLEprincipalflux.galex_nuv_UBflux.galex_nuv_UB - Upper bound of best fit flux in galex_nuvJyphot.flux.density;stat.maxDOUBLEprincipalflux.cfht_u_UBflux.cfht_u_UB - Upper bound of best fit flux in cfht_uJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_g_UBflux.hsc_g_UB - Upper bound of best fit flux in hsc_gJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_r_UBflux.hsc_r_UB - Upper bound of best fit flux in hsc_rJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_i_UBflux.hsc_i_UB - Upper bound of best fit flux in hsc_iJyphot.flux.density;stat.maxDOUBLEprincipalflux.hsc_z_UBflux.hsc_z_UB - Upper bound of best fit flux in hsc_zJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_Y_UBflux.vista_Y_UB - Upper bound of best fit flux in vista_YJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_J_UBflux.vista_J_UB - Upper bound of best fit flux in vista_JJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_H_UBflux.vista_H_UB - Upper bound of best fit flux in vista_HJyphot.flux.density;stat.maxDOUBLEprincipalflux.vista_Ks_UBflux.vista_Ks_UB - Upper bound of best fit flux in vista_KsJyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_1_UBflux.irac_1_UB - Upper bound of best fit flux in irac_1Jyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_2_UBflux.irac_2_UB - Upper bound of best fit flux in irac_2Jyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_3_UBflux.irac_3_UB - Upper bound of best fit flux in irac_3Jyphot.flux.density;stat.maxDOUBLEprincipalflux.irac_4_UBflux.irac_4_UB - Upper bound of best fit flux in irac_4Jyphot.flux.density;stat.maxDOUBLEprincipalflux.mips_24_UBflux.mips_24_UB - Upper bound of best fit flux in mips_24Jyphot.flux.density;stat.maxDOUBLEprincipalflux.mips_70_UBflux.mips_70_UB - Upper bound of best fit flux in mips_70Jyphot.flux.density;stat.maxDOUBLEprincipalflux.pacs_100_UBflux.pacs_100_UB - Upper bound of best fit flux in pacs_100Jyphot.flux.density;stat.maxDOUBLEprincipalflux.pacs_160_UBflux.pacs_160_UB - Upper bound of best fit flux in pacs_160Jyphot.flux.density;stat.maxDOUBLEprincipalflux.spire_250_UBflux.spire_250_UB - Upper bound of best fit flux in spire_250Jyphot.flux.density;stat.maxDOUBLEprincipalflux.spire_350_UBflux.spire_350_UB - Upper bound of best fit flux in spire_350Jyphot.flux.density;stat.maxDOUBLEprincipalflux.spire_500_UBflux.spire_500_UB - Upper bound of best fit flux in spire_500Jyphot.flux.density;stat.maxDOUBLEprincipaldevils_dr1.D10ProFoundPhotometryPhotometric measurments for galaxies in the DEVILS D10 region derived using th e ProFound phototmetry code applied to deep imaging data. Measurments are provied in FUV,NUV,u,g,r,i,Z,Y,J,H,K, Spitzer-IRAC1-4, Spitzer-MIPS, and Herschel bands. Davies et al 2018UIDUID based on feild, RA, DEC - UID<-as.numeric(paste("field number", round(RAmax*1000000), abs(round(DECmax*1000000)), sep=""))meta.idBIGINTindexedprincipalNewSegIDsegment ID derived from segmentation maps - unique over full fieldmeta.idINTEGERprincipalfieldDEVILS Field identifier (D02/D03/D10)meta.idVARCHARprincipalRAcenRight assecention position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.raDOUBLEindexedprincipalDECcenDeclination position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.decDOUBLEindexedprincipalRAmaxRight assecention position of the brightest pixel in the ProFound segment in the VISTA Y-band imagedegpos.eq.raDOUBLEprincipalDECmaxDeclination position of the brightest pixel in the ProFound segment in the VISTA Y-band imagedegpos.eq.decDOUBLEprincipalmaskMask flag to identify is segement falls in a masked region. 0=not masked, 1=maskedmeta.idINTEGERprincipalartefactFlagArtefact flag to identify if a segment is deemd to be an artefact (see description paper). 0=Not artefact, >0=artefactmeta.idINTEGERprincipalstarFlagStar/galaxy classifier. 0=galaxy, 1=starmeta.idINTEGERprincipalR50_YThe segment radius contain 50% of the VISTA Y-band fluxarcsecphys.angSize;em.IR.YDOUBLEprincipalN100_YNumber of segment pixels in the VISTA Y-bandphys.areaINTEGERprincipalsubFrameProFound processing subFrame within the field that the segment is taken frommeta.idINTEGERprincipalsegIDFrameSegment ID within subFramemeta.idINTEGERprincipalxcenFramex position of the centre of the segment within the subFrame in the VISTA Y-band imagepixelinstr.pixelDOUBLEprincipalycenFramey position of the centre of the segment within the subFrame in the VISTA Y-band imagepixelinstr.pixelDOUBLEprincipalxmaxFramex position of the brightest pixel of the segment within the subFrame in the VISTA Y-band imagepixelinstr.pixelDOUBLEprincipalymaxFramey position of the brightest pixel of the segment within the subFrame in the VISTA Y-band imagepixelinstr.pixelDOUBLEprincipalEBVGalactic Extinction correction coefficient applied to photomtery - derived from Planck mapsphys.excitParamDOUBLEprincipalflux_FUVTotal flux measured in GALEX FUV bandJyphot.flux.density;em.UV.100-200nmDOUBLEprincipalflux_err_FUVError on total flux measured in GALEX FUV bandJystat.error;phot.flux.density;em.UV.100-200nmDOUBLEprincipalflux_NUVTotal flux measured in GALEX NUV bandJyphot.flux.density;em.UV.200-300nmDOUBLEprincipalflux_err_NUVError on total flux measured in GALEX NUV bandJystat.error;phot.flux.density;em.UV.200-300nmDOUBLEprincipalflux_uTotal flux measured in CFHT-MEGAcam u band (D02/D10) or VST-OmegaCam u band (D03)Jyphot.flux.density;em.opt.uDOUBLEprincipalflux_err_uError on total flux measured in CFHT-MEGAcam u band (D02/D10) or VST-OmegaCam u band (D03)Jystat.error;phot.flux.density;em.opt.uDOUBLEprincipalflux_gTotal flux measured in Subaru-HSC g band (D02/D10) or VST-OmegaCam g band (D03)Jyphot.flux.density;em.opt.gDOUBLEprincipalflux_err_gError on total flux measured in Subaru-HSC g band (D02/D10) or VST-OmegaCam g band (D03)Jystat.error;phot.flux.density;em.opt.gDOUBLEprincipalflux_rTotal flux measured in Subaru-HSC r band (D02/D10) or VST-OmegaCam r band (D03)Jyphot.flux.density;em.opt.rDOUBLEprincipalflux_err_rError on total flux measured in Subaru-HSC r band (D02/D10) or VST-OmegaCam r band (D03)Jystat.error;phot.flux.density;em.opt.rDOUBLEprincipalflux_iTotal flux measured in Subaru-HSC i band (D02/D10) or VST-OmegaCam i band (D03)Jyphot.flux.density;em.opt.iDOUBLEprincipalflux_err_iError on total flux measured in Subaru-HSC i band (D02/D10) or VST-OmegaCam i band (D03)Jystat.error;phot.flux.density;em.opt.iDOUBLEprincipalflux_zTotal flux measured in Subaru-HSC z band (D02/D10) or VISTA-VIRCAM r band (D03)Jyphot.flux.density;em.opt.zDOUBLEprincipalflux_err_zError on total flux measured in Subaru-HSC z band (D02/D10) or VISTA-VIRCAM r band (D03)Jystat.error;phot.flux.density;em.opt.zDOUBLEprincipalflux_HYTotal flux measured in Subaru-HSC Y bandJyphot.flux.density;em.IR.YDOUBLEprincipalflux_err_HYError on total flux measured in Subaru-HSC Y bandJystat.error;phot.flux.density;em.IR.YDOUBLEprincipalflux_YTotal flux measured in VISTA-VIRCAM Y bandJyphot.flux.density;em.IR.YDOUBLEprincipalflux_err_YError on total flux measured in VISTA-VIRCAM Y bandJystat.error;phot.flux.density;em.IR.YDOUBLEprincipalflux_JTotal flux measured in VISTA-VIRCAM J bandJyphot.flux.density;em.IR.JDOUBLEprincipalflux_err_JError on total flux measured in VISTA-VIRCAM J bandJystat.error;phot.flux.density;em.IR.JDOUBLEprincipalflux_HTotal flux measured in VISTA-VIRCAM H bandJyphot.flux.density;em.IR.HDOUBLEprincipalflux_err_HError on total flux measured in VISTA-VIRCAM H bandJystat.error;phot.flux.density;em.IR.HDOUBLEprincipalflux_KsTotal flux measured in VISTA-VIRCAM Ks bandJyphot.flux.density;em.IR.KsDOUBLEprincipalflux_err_KsError on total flux measured in VISTA-VIRCAM Ks bandJystat.error;phot.flux.density;em.IR.KsDOUBLEprincipalflux_S36Total flux measured in Spitzer-IRAC 3.6micron bandJyphot.flux.density;em.IR.3-4umDOUBLEprincipalflux_err_S36Error on total flux measured in Spitzer-IRAC 3.6micron bandJystat.error;phot.flux.density;em.IR.3-4umDOUBLEprincipalflux_S45Total flux measured in Spitzer-IRAC 4.5micron bandJyphot.flux.density;em.IR.4-8umDOUBLEprincipalflux_err_S45Error on total flux measured in Spitzer-IRAC 4.5micron bandJystat.error;phot.flux.density;em.IR.4-8umDOUBLEprincipalflux_S58Total flux measured in Spitzer-IRAC 5.8micron bandJyphot.flux.density;em.IR.4-8umDOUBLEprincipalflux_err_S58Error on total flux measured in Spitzer-IRAC 5.8micron bandJystat.error;phot.flux.density;em.IR.4-8umDOUBLEprincipalflux_S80Total flux measured in Spitzer-IRAC 8.0micron bandJyphot.flux.density;em.IR.4-8umDOUBLEprincipalflux_err_S80Error on total flux measured in Spitzer-IRAC 8.0micron bandJystat.error;phot.flux.density;em.IR.4-8umDOUBLEprincipalflux_M24Total flux measured in Spitzer-MIPS 24micron bandJyphot.flux.density;em.IR.15-30umDOUBLEprincipalflux_err_M24Error on total flux measured in Spitzer-MIPS 24micron bandJystat.error;phot.flux.density;em.IR.15-30umDOUBLEprincipalflux_M70Total flux measured in Spitzer-MIPS 70micron bandJyphot.flux.density;em.IR.60-100umDOUBLEprincipalflux_err_M70Error on total flux measured in Spitzer-MIPS 70micron bandJystat.error;phot.flux.density;em.IR.60-100umDOUBLEprincipalflux_P100Total flux measured in Herschel-PACS 100micron bandJyphot.flux.density;em.IR.FIRDOUBLEprincipalflux_err_P100Error on total flux measured in Herschel-PACS 100micron bandJystat.error;phot.flux.density;em.IR.FIRDOUBLEprincipalflux_P160Total flux measured in Herschel-PACS 160micron bandJyphot.flux.density;em.IR.FIRDOUBLEprincipalflux_err_P160Error on total flux measured in Herschel-PACS 160micron bandJystat.error;phot.flux.density;em.IR.FIRDOUBLEprincipalflux_S250Total flux measured in Herschel-SPIRE 250micron bandJyphot.flux.density;em.IR.FIRDOUBLEprincipalflux_err_S250Error on total flux measured in Herschel-SPIRE 250micron bandJystat.error;phot.flux.density;em.IR.FIRDOUBLEprincipalflux_S350Total flux measured in Herschel-SPIRE 350micron bandJyphot.flux.density;em.IR.FIRDOUBLEprincipalflux_err_S350Error on total flux measured in Herschel-SPIRE 350micron bandJystat.error;phot.flux.density;em.IR.FIRDOUBLEprincipalflux_S500Total flux measured in Herschel-SPIRE 500micron bandJyphot.flux.density;em.IR.FIRDOUBLEprincipalflux_err_S500Error on total flux measured in Herschel-SPIRE 500micron bandJystat.error;phot.flux.density;em.IR.FIRDOUBLEprincipalflux_FUV_cColour-optimised flux measured in GALEX FUV bandJyphot.flux.density;em.UV.100-200nmDOUBLEprincipalflux_err_FUV_cError on colour-optimised flux measured in GALEX FUV bandJystat.error;phot.flux.density;em.UV.100-200nmDOUBLEprincipalflux_NUV_cColour-optimised flux measured in GALEX NUV bandJyphot.flux.density;em.UV.200-300nmDOUBLEprincipalflux_err_NUV_cError on colour-optimised flux measured in GALEX NUV bandJystat.error;phot.flux.density;em.UV.200-300nmDOUBLEprincipalflux_u_cColour-optimised flux measured in CFHT-MEGAcam u band (D02/D10) or VST-OmegaCam u band (D03)Jyphot.flux.density;em.opt.uDOUBLEprincipalflux_err_u_cError on colour-optimised flux measured in CFHT-MEGAcam u band (D02/D10) or VST-OmegaCam u band (D03)Jystat.error;phot.flux.density;em.opt.uDOUBLEprincipalflux_g_cColour-optimised flux measured in Subaru-HSC g band (D02/D10) or VST-OmegaCam g band (D03)Jyphot.flux.density;em.opt.gDOUBLEprincipalflux_err_g_cError on colour-optimised flux measured in Subaru-HSC g band (D02/D10) or VST-OmegaCam g band (D03)Jystat.error;phot.flux.density;em.opt.gDOUBLEprincipalflux_r_cColour-optimised flux measured in Subaru-HSC r band (D02/D10) or VST-OmegaCam r band (D03)Jyphot.flux.density;em.opt.rDOUBLEprincipalflux_err_r_cError on colour-optimised flux measured in Subaru-HSC r band (D02/D10) or VST-OmegaCam r band (D03)Jystat.error;phot.flux.density;em.opt.rDOUBLEprincipalflux_i_cColour-optimised flux measured in Subaru-HSC i band (D02/D10) or VST-OmegaCam i band (D03)Jyphot.flux.density;em.opt.iDOUBLEprincipalflux_err_i_cError on colour-optimised flux measured in Subaru-HSC i band (D02/D10) or VST-OmegaCam i band (D03)Jystat.error;phot.flux.density;em.opt.iDOUBLEprincipalflux_z_cColour-optimised flux measured in Subaru-HSC z band (D02/D10) or VISTA-VIRCAM Z band (D03)Jyphot.flux.density;em.opt.zDOUBLEprincipalflux_err_z_cError on colour-optimised flux measured in Subaru-HSC z bandJystat.error;phot.flux.density;em.opt.zDOUBLEprincipalflux_HY_cColour-optimised flux measured in Subaru-HSC Y bandJyphot.flux.density;em.IR.YDOUBLEprincipalflux_err_HY_cError on colour-optimised flux measured in Subaru-HSC Y bandJystat.error;phot.flux.density;em.IR.YDOUBLEprincipalflux_Y_cColour-optimised flux measured in VISTA-VIRCAM Y bandJyphot.flux.density;em.IR.YDOUBLEprincipalflux_err_Y_cError on colour-optimised flux measured in VISTA-VIRCAM Y bandJystat.error;phot.flux.density;em.IR.YDOUBLEprincipalflux_J_cColour-optimised flux measured in VISTA-VIRCAM J bandJyphot.flux.density;em.IR.JDOUBLEprincipalflux_err_J_cError on colour-optimised flux measured in VISTA-VIRCAM J bandJystat.error;phot.flux.density;em.IR.JDOUBLEprincipalflux_H_cColour-optimised flux measured in VISTA-VIRCAM H bandJyphot.flux.density;em.IR.HDOUBLEprincipalflux_err_H_cError on colour-optimised flux measured in VISTA-VIRCAM H bandJystat.error;phot.flux.density;em.IR.HDOUBLEprincipalflux_Ks_cColour-optimised flux measured in VISTA-VIRCAM Ks bandJyphot.flux.density;em.IR.KsDOUBLEprincipalflux_err_Ks_cError on colour-optimised flux measured in VISTA-VIRCAM Ks bandJystat.error;phot.flux.density;em.IR.KsDOUBLEprincipalflux_S36_cColour-optimised flux measured in Spitzer-IRAC 3.6micron bandJyphot.flux.density;em.IR.3-4umDOUBLEprincipalflux_err_S36_cError on colour-optimised flux measured in Spitzer-IRAC 3.6micron bandJystat.error;phot.flux.density;em.IR.3-4umDOUBLEprincipalflux_S45_cColour-optimised flux measured in Spitzer-IRAC 4.5micron bandJyphot.flux.density;em.IR.4-8umDOUBLEprincipalflux_err_S45_cError on colour-optimised flux measured in Spitzer-IRAC 4.5micron bandJystat.error;phot.flux.density;em.IR.4-8umDOUBLEprincipalflux_S58_cColour-optimised flux measured in Spitzer-IRAC 5.8micron bandJyphot.flux.density;em.IR.4-8umDOUBLEprincipalflux_err_S58_cError on colour-optimised flux measured in Spitzer-IRAC 5.8micron bandJystat.error;phot.flux.density;em.IR.4-8umDOUBLEprincipalflux_S80_cColour-optimised flux measured in Spitzer-IRAC 8.0micron bandJyphot.flux.density;em.IR.4-8umDOUBLEprincipalflux_err_S80_cError on colour-optimised flux measured in Spitzer-IRAC 8.0micron bandJystat.error;phot.flux.density;em.IR.4-8umDOUBLEprincipaldevils_dr1.D10MasterRedshiftsAvailable redshifts for sources in the DEVILS D10 region down to the DEVILS spectroscopic limit (Y<21.2). Compiled from various spectroscopic, grism and photometric campaigns/analyses. Where possible, all possible redshifts are provided for each source. A "best" redshift is also providide and should be used in most cases. Davies et al in prepMIGHTEEtmp_u68No error provided for MIGHTEEtmp PhotoZ (COS_Master_hatfield_GPz_V1.fits).stat.error;src.redshiftDOUBLEprincipalMIGHTEEtmp_typeMIGHTEEtmp redshift typemeta.idVARCHARprincipalzBestBest Redshift for source from all availble redshifts (see README)src.redshiftDOUBLEprincipalzBestSourceSurvey from which best redshift comes, identifier in column namesmeta.idVARCHARprincipalzBestTypeType of redshift: spec, grism, photozmeta.idVARCHARprincipalC3R2_typeC3R2 redshift typemeta.idVARCHARprincipalHST3D_IDHST3D grism ID taken from HST3D catalogue cosmos_3dhst.v4.1.5.zbest.fits - Momcheva+ 2015 - we take only sources with use_zgrism=1meta.idINTEGERprincipalHST3D_RAHST3D grism RA taken from HST3D catalogue (cosmos_3dhst.v4.1.5.zbest.fits)degpos.eq.raDOUBLEprincipalHST3D_DECHST3D grism DEC taken from HST3D catalogue (cosmos_3dhst.v4.1.5.zbest.fits)degpos.eq.decDOUBLEprincipalHST3D_zHST3D grism redshift taken from HST3D catalogue (cosmos_3dhst.v4.1.5.zbest.fits)src.redshiftDOUBLEprincipalHST3D_l68HST3D grism 1sigma lower confidence boundary taken from HST3D catalogue (cosmos_3dhst.v4.1.5.zbest.fits).stat.error;src.redshiftDOUBLEprincipalHST3D_typeHST3D redshift typemeta.idVARCHARprincipalUIDUID based on feild, RA, DEC taken from DEVILS profound photometry catalogue - UID<-as.numeric(paste("field number", round(RAmax*1000000), abs(round(DECmax*1000000)), sep=""))meta.idBIGINTprincipalRAcenRight assecention position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.raDOUBLEprincipalDECcenDeclination position of the ProFound segment centre in the VISTA Y-band imagedegpos.eq.decDOUBLEprincipalRAmaxRight assecention position of the brightest pixel in the ProFound segment in the VISTA Y-band imagedegpos.eq.raDOUBLEprincipalDECmaxDeclination position of the brightest pixel in the ProFound segment in the VISTA Y-band imagedegpos.eq.decDOUBLEprincipalmaskMask flag to identify is segement falls in a masked region. 0=not masked, 1=maskedmeta.idINTEGERprincipalartefactFlagArtefact flag to identify if a segment is deemd to be an artefact (see description paper). 0=Not artefact, >0=artefactmeta.idINTEGERprincipalstarFlagStar/galaxy classifier. 0=galaxy, 1=starmeta.idINTEGERprincipalmag_YTotal magnitude measured in VISTA Y bandmagphot.mag;em.IR.YDOUBLEprincipalDEVILS_IDDEVILS spectroscopic ID taken from DMCat (DMCat2020-03-25)meta.idVARCHARprincipalDEVILS_RADEVILS spectroscopic RA taken from DMCat (DMCat2020-03-25 - Davies et al)degpos.eq.raDOUBLEprincipalDEVILS_DECDEVILS spectroscopic DEC taken from DMCat (DMCat2020-03-25)degpos.eq.decDOUBLEprincipalDEVILS_zDEVILS current best spectroscopic redshift taken from DMCat (DMCat2020-03-25)src.redshiftDOUBLEprincipalDEVILS_probDEVILS current best spectroscopic redshift probability taken from DMCat. 0-1. Good redshifts have DEVILS_prob>0.9 (~Q3), very good have DEVILS_prob>0.95 (~Q4) (DMCat2020-03-25)stat.probability;src.redshiftDOUBLEprincipalDEVILS_zPlusDEVILS spectroscopic redshifts weighted by matches exisiting redshift information (see Davies et al 2023 for more info)src.redshiftDOUBLEprincipalDEVILS_probPlusDEVILS weighted probability. DEVILS_prob +1 (if consistent with photo-z) & +2 (if consistent with grism redshift) & + 4 (if consistent with spec redshift). Numbers are adative, such that 7.xxx means redshift is consistent with existing photo-z, grism-z and spec-zstat.probability;src.redshiftDOUBLEprincipalDEVILS_typeDEVILS redshift type (DMCat2020-03-25)meta.idVARCHARprincipalzCOSMOS_IDzCOSMOS spectroscopic ID taken from zCOSMOS Bright DR3 catalogue (zcosbrightspec20k_dr3_catalog_1595990782.csv - Lily et al)meta.idINTEGERprincipalzCOSMOS_RAzCOSMOS spectroscopic RA taken from zCOSMOS Bright DR3 catalogue (zcosbrightspec20k_dr3_catalog_1595990782.csv)degpos.eq.raDOUBLEprincipalzCOSMOS_DECzCOSMOS spectroscopic DEC taken from zCOSMOS Bright DR3 catalogue (zcosbrightspec20k_dr3_catalog_1595990782.csv)degpos.eq.decDOUBLEprincipalzCOSMOS_zzCOSMOS spectroscopic redshift taken from zCOSMOS Bright DR3 catalogue (zcosbrightspec20k_dr3_catalog_1595990782.csv)src.redshiftDOUBLEprincipalzCOSMOS_probzCOSMOS spectroscopic confidence taken from zCOSMOS Bright DR3 catalogue (zcosbrightspec20k_dr3_catalog_1595990782.csv). 4=very secure, 3=secure, 2=probable, 1=insecure, 9=single line, 18=single line BL AGN. Other things are added. It gets quite complicated - see www.eso.org/sci/observing/phase3/data_releases/zcosmos_dr3_b2.pdfmeta.idDOUBLEprincipalzCOSMOS_typezCOSMOS redshift typemeta.idVARCHARprincipalDESI_IDDESI spectroscopic ID taken from DESI EDR catalogue (zall-pix-edr-vac.fits - DESI collaboration et al 2023)meta.idBIGINTprincipalDESI_RADESI spectroscopic RA taken from DESI EDR catalogue (zall-pix-edr-vac.fits)degpos.eq.raDOUBLEprincipalDESI_DECDESI spectroscopic DEC taken from DESI EDR catalogue (zall-pix-edr-vac.fits)degpos.eq.decDOUBLEprincipalDESI_zDESI spectroscopic redshift taken from DESI EDR catalogue (zall-pix-edr-vac.fits)src.redshiftDOUBLEprincipalDESI_probDESI spectroscopic confidence taken from DELTACHI2 in the DESI EDR catalogue (zall-pix-edr-vac.fits).Values >9 are classed as secure.meta.idDOUBLEprincipalDESI_typeDESI redshift typemeta.idVARCHARprincipalhCOSMOS_IDhCOSMOS spectroscopic ID generated for hCOSMOS catalogue (seq using row order from hcosmosNew.cat.txt - Damjanov+ 2018)meta.idINTEGERprincipalhCOSMOS_RAhCOSMOS spectroscopic RA taken from hCOSMOS catalogue (hcosmosNew.cat.txt)degpos.eq.raDOUBLEprincipalhCOSMOS_DEChCOSMOS spectroscopic DEC taken from hCOSMOS catalogue (hcosmosNew.cat.txt)degpos.eq.decDOUBLEprincipalhCOSMOS_zhCOSMOS spectroscopic redshift taken from hCOSMOS catalogue (hcosmosNew.cat.txt)src.redshiftDOUBLEprincipalhCOSMOS_probhCOSMOS spectroscopic error taken from hCOSMOS catalogue (hcosmosNew.cat.txt). Actual Delta_zstat.error;src.redshiftDOUBLEprincipalhCOSMOS_typehCOSMOS redshift typemeta.idVARCHARprincipalDEIMOS_IDDEIMOS spectroscopic ID taken from DEIMOS catalogue COSMOS_DEIMOS.csv - Hasinger+ 2018)meta.idVARCHARprincipalDEIMOS_RADEIMOS spectroscopic RA taken from DEIMOS catalogue (COSMOS_DEIMOS.csv)degpos.eq.raDOUBLEprincipalDEIMOS_DECDEIMOS spectroscopic DEC taken from DEIMOS catalogue (COSMOS_DEIMOS.csv)degpos.eq.decDOUBLEprincipalDEIMOS_zDEIMOS spectroscopic redshift taken from DEIMOS catalogue (COSMOS_DEIMOS.csv)src.redshiftDOUBLEprincipalDEIMOS_probDEIMOS spectroscopic quality flag taken from DEIMOS catalogue (COSMOS_DEIMOS.csv). 2=Reliable, 1.5=uncertain but agrees with photo-z, 1=uncertainmeta.idDOUBLEprincipalDEIMOS_typeDEIMOS redshift typemeta.idVARCHARprincipalComparatOII_IDComparatOII spectroscopic ID generated from ComparatOII catalogue Comparat_catalog.dat - Comparat+ 2015)meta.idINTEGERprincipalComparatOII_RAComparatOII spectroscopic RA taken from ComparatOII catalogue (Comparat_catalog.dat)degpos.eq.raDOUBLEprincipalComparatOII_DECComparatOII spectroscopic DEC taken from ComparatOII catalogue (Comparat_catalog.dat)degpos.eq.decDOUBLEprincipalComparatOII_zComparatOII OII-derived spectroscopic Redshift taken from ComparatOII catalogue (Comparat_catalog.dat)src.redshiftDOUBLEprincipalComparatOII_prob**NOTE: ComparatOII catalogue does not contain quality flagsmeta.idDOUBLEprincipalComparatOII_typeComparatOII redshift typemeta.idVARCHARprincipalFMOS_IDFMOS spectroscopic ID taken from FMOS catalogue FMOS_COSMOS_v1.0.fits - Silverman+ 2015)meta.idVARCHARprincipalFMOS_RAFMOS spectroscopic RA taken from FMOS catalogue (FMOS_COSMOS_v1.0.fit)degpos.eq.raDOUBLEprincipalFMOS_DECFMOS spectroscopic DEC taken from FMOS catalogue (FMOS_COSMOS_v1.0.fit)degpos.eq.decDOUBLEprincipalFMOS_zFMOS spectroscopic redshift taken from FMOS catalogue (FMOS_COSMOS_v1.0.fit)src.redshiftDOUBLEprincipalFMOS_probFMOS spectroscopic quality flag taken from FMOS catalogue (FMOS_COSMOS_v1.0.fit). 4=Very secure, 3=secure, 2=probable, 1=not secure, 0=nothingmeta.idDOUBLEprincipalFMOS_typeFMOS redshift typemeta.idVARCHARprincipalMOSDEF_IDMOSDEF spectroscopic ID (ID_V4) taken from MOSDEF catalogue mosdef_zcat.final.fits - Kriek+ 2015)meta.idINTEGERprincipalMOSDEF_RAMOSDEF spectroscopic RA taken from MOSDEF catalogue (mosdef_zcat.final.fits)degpos.eq.raDOUBLEprincipalMOSDEF_DECMOSDEF spectroscopic DEC taken from MOSDEF catalogue (mosdef_zcat.final.fits)degpos.eq.decDOUBLEprincipalMOSDEF_zMOSDEF spectroscopic redshift taken from MOSDEF catalogue (mosdef_zcat.final.fits)src.redshiftDOUBLEprincipalMOSDEF_probMOSDEF spectroscopic quality flag taken from MOSDEF catalogue (mosdef_zcat.final.fits)meta.idDOUBLEprincipalMOSDEF_typeMOSDEF redshift typemeta.idVARCHARprincipalC3R2_IDC3R2 spectroscopic ID taken from C3R2 catalogue c3r2_DR1+DR2_2019april11.txt - Masters+ 2017, 2019)meta.idVARCHARprincipalC3R2_RAC3R2 spectroscopic RA taken from C3R2 catalogue (c3r2_DR1+DR2_2019april11.txt)degpos.eq.raDOUBLEprincipalC3R2_DECC3R2 spectroscopic DEC taken from C3R2 catalogue (c3r2_DR1+DR2_2019april11.txt)degpos.eq.decDOUBLEprincipalC3R2_zC3R2 spectroscopic redshift taken from C3R2 catalogue (c3r2_DR1+DR2_2019april11.txt)src.redshiftDOUBLEprincipalC3R2_probC3R2 spectroscopic quality flag taken from C3R2 catalogue (c3r2_DR1+DR2_2019april11.txt). 4=certain, 3.5=very high confidence, 3=high confidencemeta.idDOUBLEprincipalLRIS_IDLRIS spectroscopic ID taken from LRIS catalogue cl2017_valueadded_release_20171009.txt - Lee+ 2015)meta.idVARCHARprincipalLRIS_RALRIS spectroscopic RA taken from LRIS catalogue (cl2017_valueadded_release_20171009.txt)degpos.eq.raDOUBLEprincipalLRIS_DECLRIS spectroscopic DEC taken from LRIS catalogue (c3r2_DR1+DR2_2019april11.txt)degpos.eq.decDOUBLEprincipalLRIS_zLRIS spectroscopic redshift taken from LRIS catalogue (c3r2_DR1+DR2_2019april11.txt)src.redshiftDOUBLEprincipalLRIS_probLRIS spectroscopic quality flag taken from LRIS catalogue (c3r2_DR1+DR2_2019april11.txt). 4=high confidence, 3=reasonable confidence, 2=low-confidence, 1=guessmeta.idDOUBLEprincipalLRIS_typeLRIS redshift typemeta.idVARCHARprincipalVIS3COSMOS_IDVIS3COSMOS spectroscopic ID taken from VIS3COSMOS catalogue VIS3COSMOS_tableb1.dat - Paulino-Afonso+ 2018)meta.idVARCHARprincipalVIS3COSMOS_RAVIS3COSMOS spectroscopic RA taken from VIS3COSMOS catalogue (VIS3COSMOS_tableb1.dat)degpos.eq.raDOUBLEprincipalVIS3COSMOS_DECVIS3COSMOS spectroscopic DEC taken from VIS3COSMOS catalogue (VIS3COSMOS_tableb1.dat)degpos.eq.decDOUBLEprincipalVIS3COSMOS_zVIS3COSMOS spectroscopic redshift taken from VIS3COSMOS catalogue (VIS3COSMOS_tableb1.dat)src.redshiftDOUBLEprincipalVIS3COSMOS_probVIS3COSMOS catalogue (VIS3COSMOS_tableb1.dat) has no quality flagmeta.idDOUBLEprincipalVIS3COSMOS_typeVIS3COSMOS redshift typemeta.idVARCHARprincipalLEGA_C_IDLEGA_C spectroscopic ID taken from LEGA_C catalogue ADP.2018-06-13T13:17:01.234.fits - van der Wel+ 2016)meta.idINTEGERprincipalLEGA_C_RALEGA_C spectroscopic RA taken from LEGA_C catalogue (ADP.2018-06-13T13:17:01.234.fits)degpos.eq.raDOUBLEprincipalLEGA_C_DECLEGA_C spectroscopic DEC taken from LEGA_C catalogue (ADP.2018-06-13T13:17:01.234.fits)degpos.eq.decDOUBLEprincipalLEGA_C_zLEGA_C spectroscopic redshift taken from LEGA_C catalogue (ADP.2018-06-13T13:17:01.234.fits)src.redshiftDOUBLEprincipalLEGA_C_probLEGA_C catalogue redshift quality flag (ADP.2018-06-13T13:17:01.234.fits). 0=good redshift, 1=bad redshiftmeta.idDOUBLEprincipalLEGA_C_typeLEGA_C redshift typemeta.idVARCHARprincipalVVDS_IDVVDS spectroscopic ID taken from VVDS catalogue VVDS_COSMOS.csv - Le Fèvre+, 2013)meta.idVARCHARprincipalVVDS_RAVVDS spectroscopic RA taken from VVDS catalogue (VVDS_COSMOS.csv)degpos.eq.raDOUBLEprincipalVVDS_DECVVDS spectroscopic DEC taken from VVDS catalogue (VVDS_COSMOS.csv)degpos.eq.decDOUBLEprincipalVVDS_zVVDS spectroscopic redshift taken from VVDS catalogue (VVDS_COSMOS.csv)src.redshiftDOUBLEprincipalVVDS_probVVDS spectroscopic quality flag taken from VVDS catalogue (VVDS_COSMOS.csv). 4=high confidence, 3=reasonable confidence, 2=low-confidence, 1=guessmeta.idDOUBLEprincipalVVDS_typeVVDS redshift typemeta.idVARCHARprincipalVUDS_IDVUDS spectroscopic ID taken from OzDES master catalogue OzDES_GRC_2017_08_30.csv - Le Fèvre+, 2013)meta.idVARCHARprincipalVUDS_RAVUDS spectroscopic RA taken from VUDS catalogue (OzDES_GRC_2017_08_30.csv)degpos.eq.raDOUBLEprincipalVUDS_DECVUDS spectroscopic DEC taken from VUDS catalogue (OzDES_GRC_2017_08_30.csv)degpos.eq.decDOUBLEprincipalVUDS_zVUDS spectroscopic redshift taken from VUDS catalogue (OzDES_GRC_2017_08_30.csv)src.redshiftDOUBLEprincipalVUDS_probVUDS spectroscopic quality flag taken from VUDS catalogue (OzDES_GRC_2017_08_30.csv). reliable = 1.5,2,3,4,9meta.idDOUBLEprincipalVUDS_typeVUDS redshift typemeta.idVARCHARprincipalPRIMUS_IDPRIMUS grism ID taken from PRIMUS catalogue PRIMUS_2013_zcat_v1.fits - Coil+ 2011)meta.idVARCHARprincipalPRIMUS_RAPRIMUS grism RA taken from PRIMUS catalogue (PRIMUS_2013_zcat_v1.fits)degpos.eq.raDOUBLEprincipalPRIMUS_DECPRIMUS grism DEC taken from PRIMUS catalogue (PRIMUS_2013_zcat_v1.fits)degpos.eq.decDOUBLEprincipalPRIMUS_zPRIMUS grism redshift taken from PRIMUS catalogue (PRIMUS_2013_zcat_v1.fits)src.redshiftDOUBLEprincipalPRIMUS_probPRIMUS grism quality flag taken from PRIMUS catalogue (PRIMUS_2013_zcat_v1.fits). 4=high quality (dz/(1+z)~0.003), 3=good quality dz/(1+z)~0.015), 2=probable dz/(1+z)~0.03, -1=starmeta.idDOUBLEprincipalPRIMUS_typePRIMUS redshift typemeta.idVARCHARprincipalHST3D_u68HST3D grism 1sigma upper confidence boundary taken from HST3D catalogue (cosmos_3dhst.v4.1.5.zbest.fits).stat.error;src.redshiftDOUBLEprincipalPAU_IDPAU PhotoZ ID taken from PAU catalogue pau_cosmos_photoz_v0_4_c.fits - Alarcon et al. 2020.meta.idINTEGERprincipalPAU_RAPAU PhotoZ RA taken from PAU catalogue (pau_cosmos_photoz_v0_4_c.fits)degpos.eq.raDOUBLEprincipalPAU_DECPAU PhotoZ DEC taken from PAU catalogue (pau_cosmos_photoz_v0_4_c.fits)degpos.eq.decDOUBLEprincipalPAU_zPAU PhotoZ redshift taken from PAU catalogue (pau_cosmos_photoz_v0_4_c.fits)src.redshiftDOUBLEprincipalPAU_l68PAU PhotoZ catalogue has no error boundstat.error;src.redshiftDOUBLEprincipalPAU_u68PAU PhotoZ catalogue has no error boundstat.error;src.redshiftDOUBLEprincipalPAU_typePAU redshift typemeta.idVARCHARprincipalCOSMOS2015_IDCOSMOS2015 PhotoZ ID (ID2013) taken from COSMOS2015 catalogue COSMOS2015_Laigle+_v1.1.fits - Laigle+ 2016meta.idINTEGERprincipalCOSMOS2015_RACOSMOS2015 PhotoZ RA taken from COSMOS2015 catalogue (COSMOS2015_Laigle+_v1.1.fits)degpos.eq.raDOUBLEprincipalCOSMOS2015_DECCOSMOS2015 PhotoZ DEC taken from COSMOS2015 catalogue (COSMOS2015_Laigle+_v1.1.fits)degpos.eq.decDOUBLEprincipalCOSMOS2015_zCOSMOS2015 PhotoZ (ZPDF) redshift taken from COSMOS2015 catalogue (COSMOS2015_Laigle+_v1.1.fits)src.redshiftDOUBLEprincipalCOSMOS2015_l68COSMOS2015 PhotoZ 1sigma lower confidence boundary taken from COSMOS2015 catalogue (COSMOS2015_Laigle+_v1.1.fits).stat.error;src.redshiftDOUBLEprincipalCOSMOS2015_u68COSMOS2015 PhotoZ 1sigma upper confidence boundary taken from COSMOS2015 catalogue (COSMOS2015_Laigle+_v1.1.fits).stat.error;src.redshiftDOUBLEprincipalCOSMOS2015_typeCOSMOS2015 redshift typemeta.idVARCHARprincipalGpZ_IDGpZ PhotoZ ID taken from GpZ catalogue COS_Master_hatfield_GPz_V1.fits - Hatfield+ in prepmeta.idINTEGERprincipalGpZ_RAGpZ PhotoZ RA taken from GpZ catalogue (COS_Master_hatfield_GPz_V1.fits)degpos.eq.raDOUBLEprincipalGpZ_DECGpZ PhotoZ DEC taken from GpZ catalogue (COS_Master_hatfield_GPz_V1.fits)degpos.eq.decDOUBLEprincipalGpZ_zGpZ PhotoZ (Z_GPz_all) redshift taken from GpZ catalogue (COS_Master_hatfield_GPz_V1.fits)src.redshiftDOUBLEprincipalGpZ_l68GpZ PhotoZ 1sigma lower confidence boundary taken from GpZ catalogue as Z_GPz_all-Z_GPz_all_err (COS_Master_hatfield_GPz_V1.fits).stat.error;src.redshiftDOUBLEprincipalGpZ_u68GpZ PhotoZ 1sigma upper confidence boundary taken from GpZ catalogue as Z_GPz_all-Z_GPz_all_err (COS_Master_hatfield_GPz_V1.fits).stat.error;src.redshiftDOUBLEprincipalGpZ_typeGpZ redshift typemeta.idVARCHARprincipalMIGHTEEtmp_IDMIGHTEEtmp PhotoZ ID taken from MIGHTEEtmp catalogue COS_Master_hatfield_GPz_V1.fits - Hatfield+ in prepmeta.idINTEGERprincipalMIGHTEEtmp_RAMIGHTEEtmp PhotoZ RA taken from MIGHTEEtmp catalogue (COS_Master_hatfield_GPz_V1.fits)degpos.eq.raDOUBLEprincipalMIGHTEEtmp_DECMIGHTEEtmp PhotoZ DEC taken from MIGHTEEtmp catalogue (COS_Master_hatfield_GPz_V1.fits)degpos.eq.decDOUBLEprincipalMIGHTEEtmp_zMIGHTEEtmp PhotoZ (Z_GPz_all) redshift taken from MIGHTEEtmp catalogue (COS_Master_hatfield_GPz_V1.fits)src.redshiftDOUBLEprincipalMIGHTEEtmp_l68No error provided for MIGHTEEtmp PhotoZ (COS_Master_hatfield_GPz_V1.fits).stat.error;src.redshiftDOUBLEprincipal2dflens_fdr2dFLenS is a southern-hemisphere spectroscopic redshift survey using the 2dF-AAOmega multi-fibre spectroscopic system at the Anglo-Australian Telescope. Its purpose was to extend the coverage of spectroscopic-redshift observations that overlap with deep optical imaging surveys performed to measure weak gravitational lensing.2dflens_fdr.redshift_catalogueThe final catalogue of 70,028 good-quality spectroscopic redshifts obtained by 2dFLenS (after 51 duplicates were removed from the original catalogue with 70,079 sources). The catalogue lists the galaxy equatorial coordinate, the redshift, the quality flag, the target type, the (u,g,r,i,z) VST-ATLAS magnitudes, and the W1 WISE magnitude.raRight ascension of the sourcedegpos.eq.ra;meta.mainDOUBLEindexedprincipaldecDeclination of the sourcedegpos.eq.dec;meta.mainDOUBLEindexedprincipalzRedshift of the sourcesrc.redshiftDOUBLEprincipalqualQuality flag (see documentation)meta.code.qualINTEGERprincipaltargetTarget type (see documentation)meta.code.class;src.classINTEGERprincipalumagPhotometric magnitude in VST-ATLAS u-bandmagphot.mag;em.opt.UDOUBLEprincipalgmagPhotometric magnitude in VST-ATLAS g-bandmagphot.mag;em.opt.BDOUBLEprincipalrmagPhotometric magnitude in VST-ATLAS r-bandmagphot.mag;em.opt.RDOUBLEprincipalimagPhotometric magnitude in VST-ATLAS i-bandmagphot.mag;em.opt.IDOUBLEprincipalzmagPhotometric magnitude in VST-ATLAS z-bandmagphot.mag;em.opt.IDOUBLEprincipalw1magPhotometric magnitude in WISE W1 channelmagphot.mag;em.IR.3-4umDOUBLEprincipaldc_idAAO Data Central assigned IDmeta.id;meta.mainBIGINTindexedprincipal