J/ApJS/243/22ivo://CDS.VizieR/J/ApJS/243/22doi:10.26093/cds/vizier.22430022CDSBarro G.Perez-Gonzalez P.G.Cava A.Brammer G.Pandya V.,Eliche Moral C.Esquej P.Dominguez-Sanchez H.Pampliega B.A.Guo Y.,Koekemoer A.M.Trump J.R.Ashby M.L.N.Cardiel N.Castellano M.,Conselice C.J.Dickinson M.E.Dolch T.Donley J.L.Briones N.E.,Faber S.M.Fazio G.G.Ferguson H.Finkelstein S.Fontana A.,Galametz A.Gardner J.P.Gawiser E.Giavalisco M.Grazian A.,Grogin N.A.Hathi N.P.Hemmati S.Hernan-Caballero A.Kocevski D.,Koo D.C.Kodra D.Lee K.-S.Lin L.Lucas R.A.Mobasher B.,McGrath E.J.Nandra K.Nayyeri H.Newman J.A.Pforr J.Peth M.,Rafelski M.Rodriguez-Munoz L.Salvato M.Stefanon M.van der Wel A.,Willner S.P.Wiklind T.Wuyts S.2023-05-26T08:52:16Z2023-03-27T14:26:08ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesultraviolet-photometryinfrared-photometryredshiftedvisible-astronomyspectroscopyabsolute-magnitudeinterstellar-reddeningline-intensitiesWe present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts, and stellar parameters derived from the analysis of the multiwavelength data. The catalog contains 35445 sources over the 171arcmin^2^ of the CANDELS F160W mosaic. The 5{sigma} detection limits (within an aperture of radius 0.17") of the mosaic range between H=27.8, 28.2, and 28.7 in the wide, intermediate, and deep regions, which span approximately 50%, 15%, and 35% of the total area. The multiwavelength photometry includes broadband data from the UV (U band from KPNO and LBC), optical (HST/ACS F435W, F606W, F775W, F814W, and F850LP), near-to-mid IR (HST/WFC3 F105W, F125W, F140W, and F160W; Subaru/MOIRCS Ks; CFHT/Megacam K; and Spitzer/IRAC 3.6, 4.5, 5.8, and 8.0{mu}m), and far-IR (Spitzer/MIPS 24{mu}m, HERSCHEL/PACS 100 and 160{mu}m, SPIRE 250, 350 and 500{mu}m) observations. In addition, the catalog also includes optical medium-band data (R~50) in 25 consecutive bands, {lambda}=500-950nm, from the SHARDS survey and WFC3 IR spectroscopic observations with the G102 and G141 grisms (R~210 and 130). The use of higher spectral resolution data to estimate photometric redshifts provides very high, and nearly uniform, precision from z=0-2.5. The comparison to 1485 good-quality spectroscopic redshifts up to z~3 yields {Delta}z/(1+z_spec_)=0.0032 and an outlier fraction of {eta}=4.3%. In addition to the multiband photometry, we release value-added catalogs with emission-line fluxes, stellar masses, dust attenuations, UV- and IR-based star formation rates, and rest-frame colors.2019ApJS..243...22Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/243/22CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)III/88 : Stellar Spectrophotometric Atlas (Gunn+ 1983)II/261 : GOODS initial results (Giavalisco+, 2004)VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)J/AJ/120/2206 : NTT, HDF-S and HDF-N photometric redshifts (Fontana+, 2000)J/A+A/377/442 : Chandra Deep Field South: R-band photometry (Wolf+, 2001)J/AJ/126/539 : The Chandra Deep Fields North and South (Alexander+, 2003)J/AJ/127/180 : The Hawaii Hubble Deep Field North (Capak+, 2004)J/AJ/127/3137 : Hawaii redshifts in the ACS-GOODS region (Cowie+, 2004)J/AJ/127/3121 : TKRS catalog of GOODS-North Field (Wirth+, 2004)J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)J/ApJ/653/1004 : Galaxies at 1.4<~z<~3.0 in GOODS-North Field (Reddy+, 2006)J/ApJ/689/687 : GOODS-N spectroscopic survey (Barger+, 2008)J/ApJ/675/234 : Mass functions for 0<z<4 galaxies (Perez-Gonzalez+, 2008)J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008)J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)J/ApJ/706/158 : Early-type galaxies in PEARS (Ferreras+, 2009)J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009)J/ApJ/692/556 : Star forming galaxy templates (Rieke+, 2009)J/ApJ/709/572 : COSMOS 70um sources (Kartaltepe+, 2010)J/ApJS/193/30 : UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011)J/ApJS/193/14 : DEEP3 Galaxy Redshift Survey: GOODS-N field (Cooper+, 2011)J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)J/PASJ/63/S379 : MOIRCS Deep Survey deep and wide catalogs (Kajisawa+, 2011)J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)J/A+A/545/A141 : UV selected sources in the GOODS-S field (Buat+, 2012)J/ApJS/203/24 : Structural param. of gal. in CANDELS (van der Wel+, 2012)J/ApJ/769/80 : Spitzer/IRAC observations of five deep fields (Ashby+, 2013)J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)J/ApJS/207/24 : GOODS-S CANDELS multiwavelength catalog (Guo+, 2013)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/762/46 : SHARDS: GOODS-N spectrophot. survey (Perez-Gonzalez+, 2013)J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)J/ApJS/218/33 : Spitzer-CANDELS catalog within 5 deep fields (Ashby+, 2015)J/ApJ/810/71 : UV mag of cand. galaxies at 3~<z~<8.5 (Finkelstein+, 2015)J/ApJ/801/97 : GOODS-S & UDS stellar masses from CANDELS (Santini+, 2015)J/ApJ/812/114 : Grism Lens-Amplified Survey from Space. I. (Treu+, 2015)J/AJ/150/153 : Team Keck Redshift Survey 2 (TKRS2) (Wirth+, 2015)J/ApJS/225/27 : 3D-HST Survey: grism spectra master cat. (Momcheva+, 2016)J/MNRAS/459/1626 : HST Frontier Fields Herschel sources (Rawle+, 2016)J/ApJ/820/83 : ALMA galaxies in the COSMOS survey field (Scoville+, 2016)J/ApJ/830/51 : FourStar gal. evolution survey (ZFOURGE) (Straatman+, 2016)J/ApJS/228/7 : Multi-wavelength data in CANDELS COSMOS (Nayyeri+, 2017)http://archive.stsci.edu/hlsp/candels : CANDELS home page on MASThttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/243/22https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/243/22http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/243/22https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/243/22https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/243/22http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/243/22GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/243/22/phot1 (CANDELS GOODS-N photometric catalog; part 1 (see Table 4))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/243/22/phot1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/243/22/phot1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/243/22/phot1?GETtext/xml+votable180.050000true189.1521617862.091777640.0055555555555555566/112523.2031150387835462e-22 5.922712285419815e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/243/22?format=asciiUVOpticalInfrareddefaultJ/ApJS/243/22/phot1CANDELS GOODS-N photometric catalog; part 1 (see Table 4)ID[1/35451] Identifiermeta.id;meta.mainintprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCANDELSCANDELS GDN name based on coordinates (JHHMMSS.s+DDMMSS.s) (IAU_Name)meta.idcharRAJ2000[188.9/189.6] Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000[62/62.4] Declination (J2000) (DEC)degpos.eq.dec;meta.mainindexedFlag[0/2] SExtractor F160W flag used to designate suspicious sources that fall in contaminated regions (FLAGS)meta.code.errorintF140W[0.0009/9187]? HST/WFC3 F140W flux density (WFC3_F140W_FLUX) (1)uJyphot.flux.density;em.IRdoublenullablee_F140W[0.002/3]? F140W uncertainty (WFC3_F140W_FLUXERR)uJystat.errordoublenullableF160W[0.007/48735]? HST/WFC3 F160W flux density (WFC3_F160W_FLUX) (1)uJyphot.flux.density;em.IR.Hdoublenullablee_F160W[0.003/24]? F160W uncertainty (WFC3_F160W_FLUXERR)uJystat.errordoublenullableFK-MOIRCS[0.0019/132325]? Subaru/MOIRCS Ks-band flux density (MOIRCS_K_FLUX) (1)uJyphot.mag;em.IR.Kdoublenullablee_FK-MOIRCS[0/2709]? KFluxMOIRCS uncertainty (MOIRCS_K_FLUXERR)uJystat.errordoublenullableFK-CFHT[0.007/11357]? CFHT/Megacam K-band flux density (CFHT_Ks_FLUX) (1)uJyphot.mag;em.IR.Kdoublenullablee_FK-CFHT[0.05/8]? KsFluxCFHT uncertainty (CFHT_Ks_FLUXERR)uJystat.errordoublenullableF3.6um[0.005/16513]? Spitzer/IRAC 3.6um flux density (IRAC_CH1_SCANDELS_FLUX) (1)uJyphot.mag;em.IR.3-4umdoublenullablee_F3.6um[0.04/7]? 3.6Flux uncertainty (IRAC_CH1_SCANDELS_FLUXERR)uJystat.errordoublenullableF4.5um[0.0048/10540]? Spitzer/IRAC 4.5um flux density (IRAC_CH2_SCANDELS_FLUX) (1)uJyphot.mag;em.IR.4-8umdoublenullablee_F4.5um[0.03/3]? 4.5Flux uncertainty (IRAC_CH2_SCANDELS_FLUXERR)uJystat.errordoublenullablee_F5.8um[0.4/30]? 5.8Flux uncertainty (IRAC_CH3_FLUXERR)uJystat.errordoublenullableF8.0um[0.048/6133]? Spitzer/IRAC 8.0um flux density (IRAC_CH4_FLUX) (1)uJyphot.flux.density;em.IR.8-15umdoublenullablee_F8.0um[0.4/42]? 8.0Flux uncertainty (IRAC_CH4_FLUXERR)uJystat.errordoublenullableH19Display data from Hsu+ 2019, J/ApJ/871/233 within 0.5"meta.ref.urlintnullableA15Display data from Ashby+ 2015, J/ApJS/218/33 within 0.5"meta.ref.urlintnullableS/G[0/1] SExtractor CLASS_STAR parameter in the F160W band (CLASS_STAR)src.class.starGalaxyintXray[1]?=-99 In Alexander+ (2003, J/AJ/126/539) X-ray catalog (<[ABB2003] CDFN NNN> in Simbad)meta.codeintnullableF5.8um[0.047/11578]? Spitzer/IRAC 5.8um flux density (IRAC_CH3_FLUX) (1)uJyphot.flux.density;em.IR.4-8umdoublenullableFU-KPNO[0.001/1992]? KPNO/Mosaic U-band flux density (KPNO_U_FLUX) (1)uJyphot.flux.density;em.opt.Udoublenullablee_FU-KPNO[0.01/1]? UFluxKPNO uncertainty (KPNO_U_FLUXERR)uJystat.errordoublenullableFU-LBC[0.00039/4914]? LBT/LBC U'-band flux density (LBC_U_FLUX) (1)uJyphot.flux.density;em.opt.Udoublenullablee_FU-LBC[0.003/1]? UFluxLBC uncertainty (LBC_U_FLUXERR)uJystat.errordoublenullableF435W[0.0003/6466]? HST/ACS F435W flux density (ACS_F435W_FLUX) (1)uJyphot.mag;em.opt.Bdoublenullablee_F435W[0.001/6.3]? F435W uncertainty (ACS_F435W_FLUXERR)uJystat.errordoublenullableF606W[0.0003/3549]? HST/ACS F606W flux density (ACS_F606W_FLUX) (1)uJyphot.mag;em.opt.Rdoublenullablee_F606W[0.001/8]? F606W uncertainty (ACS_F606W_FLUXERR)uJystat.errordoublenullableF775W[0.00049/6460]? HST/ACS F775W flux density (ACS_F775W_FLUX) (1)uJyphot.mag;em.opt.Idoublenullablee_F775W[0.001/15]? F775W uncertainty (ACS_F775W_FLUXERR)uJystat.errordoublenullableF814W[0.0002/6595]? HST/ACS F814W flux density (ACS_F814W_FLUX) (1)uJyphot.mag;em.opt.Idoublenullablee_F814W[0.001/35]? F814W uncertainty (ACS_F814W_FLUXERR)uJystat.errordoublenullableF850LP[0.0006/17959]? HST/ACS F850LP flux density (ACS_F850LP_FLUX) (1)uJyphot.mag;em.opt.Idoublenullablee_F850LP[0.002/17]? F850LP uncertainty (ACS_F850LP_FLUXERR)uJystat.errordoublenullableF105W[0.00039/8604]? HST/WFC3 F105W flux density (WFC3_F105W_FLUX) (1)uJyphot.mag;em.IR.Jdoublenullablee_F105W[0.002/4]? F105W uncertainty (WFC3_F105W_FLUXERR)uJystat.errordoublenullableF125W[0.00049/8052]? HST/WFC3 F125W flux density (WFC3_F125W_FLUX) (1)uJyphot.flux.density;em.IR.Jdoublenullablee_F125W[0.001/2]? F125W uncertainty (WFC3_F125W_FLUXERR)uJystat.errordoublenullableJ/ApJS/243/22/phot3CANDELS GOODS-N photometric catalog; part 3 (see Table 4)FWHMF850LPaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F850LParcsecphys.angSizecharFWHMF098MaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F098Marcsecphys.angSizecharFWHMF105WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F105Warcsecphys.angSizecharFWHMF125WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F125Warcsecphys.angSizecharFWHMF160WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F160Warcsecphys.angSizecharKRadaF160W band Kron radius from SExtractor in arcsec (col. pix*0.06)arcsecphys.angSize;srccharPRadaF160W band Petrosian radius from SExtractor in arcsec (col. pix*0.06)arcsecphys.angSize;srccharFWHMF435WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F435Warcsecphys.angSizecharFWHMF606WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F606Warcsecphys.angSizecharFWHMF775WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F775Warcsecphys.angSizecharFWHMF814WaFWHM of the image of an object in units of arcsec (col. pix*0.06) in HST F814Warcsecphys.angSizecharFR2F606W[-4859/38410] RADIUS_2 with the 0.5 fraction of light in HST F606W (FLUX_RADIUS_2_F606W)arcsecphys.size.radius;em.optdoubleFR2F775W[-18720/11278] RADIUS_2 with the 0.5 fraction of light in HST F775W (FLUX_RADIUS_2_F775W)arcsecphys.size.radius;em.optdoubleFR2F814W[-5920/20655] RADIUS_2 with the 0.5 fraction of light in HST F814W (FLUX_RADIUS_2_F814W)arcsecphys.size.radius;em.IRdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintXImg[989/19101] Object position along x (X_IMAGE)pixpos;instr.detdoubleYImg[1413/19226] Object position along y (Y_IMAGE)pixpos;instr.detdoubleXPkImg[988/19101] X coordinate of the brightest pixel (XPEAK_IMAGE)pixpos.cartesian.xintYPkImg[1414/19226] Y coordinate of the brightest pixel (YPEAK_IMAGE)pixpos.cartesian.yintXminImg[988/19099] Minimum x coordinate among detected pixels (XMIN_IMAGE)pixpos.cartesian.x;stat.minintYminImg[1412/19218] Minimum y coordinate among detected pixels (YMIN_IMAGE)pixpos.cartesian.y;stat.minintXmaxImg[994/19103] Maximum x coordinate among detected pixels (XMAX_IMAGE)pixpos.cartesian.x;stat.maxintYmaxImg[1416/19233] Maximum y coordinate among detected pixels (YMAX_IMAGE)pixpos.cartesian.y;stat.maxintX2Img[0.13/2930] Variance along x (X2_IMAGE)pixel**2stat.variancedoubleY2Img[0.14/3112] Variance along y (Y2_IMAGE)pixel**2stat.variancedoubleXYImg[-2742/1019] Covariance between x and y (XY_IMAGE)pixel**2stat.covariancedoubleCXXImg[0.00035/8.2] Cxx object ellipse parameter (CXX_IMAGE)pixel**-2stat.correlationdoubleCYYImg[0.00048/9.3] Cyy object ellipse parameter (CYY_IMAGE)pixel**-2stat.correlationdoubleAreaF814W[0/72544] SExtractor isophotal area (filtered) above detection threshold in HST F814W (ISOAREA_IMAGE_F814W)pixel**2instr.sensitivitydoubleAreaF850LP[0/91033] SExtractor isophotal area (filtered) above detection threshold in HST F850LP (ISOAREA_IMAGE_F850LP)pixel**2instr.sensitivitydoubleAreaF098M[0/68598] SExtractor isophotal area (filtered) above detection threshold in HST F098M (ISOAREA_IMAGE_F098M)pixel**2instr.sensitivitydoubleAreaF105W[0/50581] SExtractor isophotal area (filtered) above detection threshold in HST F105W (ISOAREA_IMAGE_F105W)pixel**2instr.sensitivitydoubleAreaF125W[0/28611] SExtractor isophotal area (filtered) above detection threshold in HST F125W (ISOAREA_IMAGE_F125W)pixel**2instr.sensitivitydoubleID[1/35451] Identifiermeta.id;meta.mainintprimaryCXYImg[-4.8/7.4] Cxy object ellipse parameter (CXY_IMAGE)pixel**-2stat.correlationdoubleAImg[0.6/76] F160W profile rms along major axis (A_IMAGE)pixstat.stdevfloatBImg[0.3/46] F160W profile rms along minor axis (B_IMAGE)pixstat.stdevfloate_AImg[0.0009/1.5] AImg uncertainty (ERRA_IMAGE)pixstat.errorfloate_BImg[0.0009/0.6] BImg uncertainty (ERRB_IMAGE)pixstat.errorfloatPAImg[-90/90] F160W position angle (THETA_IMAGE)degpos.posAngfloate_PAImg[-90/90] PAImg uncertainty (ERRTHETA_IMAGE)degstat.errorfloatIsoAImg[5/152234] SExtractor F160W isophotal area (filtered) above detection threshold (ISOAREAF_IMAGE)pixel**2instr.sensitivityintAreaF435W[0/49919] SExtractor isophotal area (filtered) above detection threshold in HST F435W (ISOAREA_IMAGE_F435W)pixel**2instr.sensitivitydoubleAreaF606W[0/71904] SExtractor isophotal area (filtered) above detection threshold in HST F606W (ISOAREA_IMAGE_F606W)pixel**2instr.sensitivitydoubleAreaF775W[0/72460] SExtractor isophotal area (filtered) above detection threshold in HST F775W (ISOAREA_IMAGE_F775W)pixel**2instr.sensitivitydoubleBkgF098M[-0.5/0.5] Background at centroid position in HST F098M (BACKGROUND_F098M)instr.backgrounddoubleBkgF105W[-0.003/0.006] Background at centroid position in HST F105W (BACKGROUND_F105W)instr.backgrounddoubleBkgF125W[-0.03/0.009] Background at centroid position in HST F125W (BACKGROUND_F125W)instr.backgrounddoubleBkgF160W[-0.003/0.008] Background at centroid position in HST F160W (BACKGROUND_F160W)instr.backgrounddoubleFR1F435W[-19760/33247] RADIUS_1 with the 0.2 fraction of light in HST F435W (FLUX_RADIUS_1_F435W)arcsecphys.size.radius;em.optdoubleFR1F606W[-1944/15364] RADIUS_1 with the 0.2 fraction of light in HST F606W (FLUX_RADIUS_1_F606W)arcsecphys.size.radius;em.optdoubleFR1F775W[-7488/4511] RADIUS_1 with the 0.2 fraction of light in HST F775W (FLUX_RADIUS_1_F775W)arcsecphys.size.radius;em.optdoubleFR1F814W[-2368/8262] RADIUS_1 with the 0.2 fraction of light in HST F814W (FLUX_RADIUS_1_F814W)arcsecphys.size.radius;em.IRdoubleFR1F850LP[-2584/3645] RADIUS_1 with the 0.2 fraction of light in HST F850LP (FLUX_RADIUS_1_F850LP)arcsecphys.size.radius;em.IRdoubleFR1F098M[-1536/39849] RADIUS_1 with the 0.2 fraction of light in HST F098M (FLUX_RADIUS_1_F098M)arcsecphys.size.radius;em.IRdoubleFR1F105W[-2007/1188] RADIUS_1 with the 0.2 fraction of light in HST F105W (FLUX_RADIUS_1_F105W)arcsecphys.size.radius;em.IRdoubleFR1F125W[-1915/713] RADIUS_1 with the 0.2 fraction of light in HST F125W (FLUX_RADIUS_1_F125W)arcsecphys.size.radius;em.IRdoubleFR1F160W[-36/43] RADIUS_1 with the 0.2 fraction of light in HST F160W (FLUX_RADIUS_1_F160W)arcsecphys.size.radius;em.IRfloatFR2F435W[-49400/83116] RADIUS_2 with the 0.5 fraction of light in HST F435W (FLUX_RADIUS_2_F435W)arcsecphys.size.radius;em.optdoubleFR2F850LP[-6458/9113] RADIUS_2 with the 0.5 fraction of light in HST F850LP (FLUX_RADIUS_2_F850LP)arcsecphys.size.radius;em.IRdoubleFR2F098M[-3838/99621] RADIUS_2 with the 0.5 fraction of light in HST F098M (FLUX_RADIUS_2_F098M)arcsecphys.size.radius;em.IRdoubleFR2F105W[-5018/2969] RADIUS_2 with the 0.5 fraction of light in HST F105W (FLUX_RADIUS_2_F105W)arcsecphys.size.radius;em.IRdoubleFR2F125W[-2282/1782] RADIUS_2 with the 0.5 fraction of light in HST F125W (FLUX_RADIUS_2_F125W)arcsecphys.size.radius;em.IRdoubleFR2F160W[-90/91] RADIUS_2 with the 0.5 fraction of light in HST F160W (FLUX_RADIUS_2_F160W)arcsecphys.size.radius;em.IRfloatFR3F435W[-79040/132985] RADIUS_3 with the 0.8 fraction of light in HST F435W (FLUX_RADIUS_3_F435W)arcsecphys.size.radius;em.optdoubleFR3F606W[-68930/61456] RADIUS_3 with the 0.8 fraction of light in HST F660W (FLUX_RADIUS_3_F606W)arcsecphys.size.radius;em.optdoubleFR3F775W[-29952/18044] RADIUS_3 with the 0.8 fraction of light in HST F775W (FLUX_RADIUS_3_F775W)arcsecphys.size.radius;em.optdoubleFR3F814W[-9471/33047] RADIUS_3 with the 0.8 fraction of light in HST F814W (FLUX_RADIUS_3_F814W)arcsecphys.size.radius;em.IRdoubleFR3F850LP[-10333/14580] RADIUS_3 with the 0.8 fraction of light in HST F850LP (FLUX_RADIUS_3_F850LP)arcsecphys.size.radius;em.IRdoubleFR3F098M[-6141/159393] RADIUS_3 with the 0.8 fraction of light in HST F098M (FLUX_RADIUS_3_F098M)arcsecphys.size.radius;em.IRdoubleFR3F105W[-8028/4750] RADIUS_3 with the 0.8 fraction of light in HST F105W (FLUX_RADIUS_3_F105W)arcsecphys.size.radius;em.IRdoubleFR3F125W[-3142/2851] RADIUS_3 with the 0.8 fraction of light in HST F125W (FLUX_RADIUS_3_F125W)arcsecphys.size.radius;em.IRdoubleFR3F160W[-659/218] RADIUS_3 with the 0.8 fraction of light in HST F160W (FLUX_RADIUS_3_F160W)arcsecphys.size.radius;em.IRdoubleAreaF160W[0/73541] SExtractor isophotal area (filtered) above detection threshold in HST F160W (ISOAREA_IMAGE_F160W)pixel**2instr.sensitivitydoubleBkgF435W[-0.002/0.002] Background at centroid position in HST F435W (BACKGROUND_F435W)instr.backgrounddoubleBkgF606W[-0.0012/0.006] Background at centroid position in HST F606W (BACKGROUND_F606W)instr.backgrounddoubleBkgF775W[-0.002/0.005] Background at centroid position in HST F775W (BACKGROUND_F775W)instr.backgrounddoubleBkgF814W[-0.003/0.009] Background at centroid position in HST F814W (BACKGROUND_F814W)instr.backgrounddoubleBkgF850LP[-0.0014/0.004] Background at centroid position in HST F850LP (BACKGROUND_F850LP)instr.backgrounddoubleFWHMF435W[-28/250] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F435W (FWHM_IMAGE_F435W)pixphys.angSizefloatFWHMF606W[-5/250] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F606W (FWHM_IMAGE_F606W)pixphys.angSizefloatFWHMF775W[-5/250] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F775W (FWHM_IMAGE_F775W)pixphys.angSizefloatFWHMF814W[-5/250] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F814W (FWHM_IMAGE_F814W)pixphys.angSizefloatFWHMF850LP[-5/249] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F850LP (FWHM_IMAGE_F850LP)pixphys.angSizefloatFWHMF098M[-5/250] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F098M (FWHM_IMAGE_F098M)pixphys.angSizefloatFWHMF105W[-3/250] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F105W (FWHM_IMAGE_F105W)pixphys.angSizefloatFWHMF125W[-4/245] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F125W (FWHM_IMAGE_F125W)pixphys.angSizefloatFWHMF160W[-5/147] FWHM of the image of an object, in units of pixel (1pix=0.06") in HST F160W (FWHM_IMAGE_F160W)pixphys.angSizefloatKRad[0/10.6] F160W band Kron radius from SExtractor (in unit of A_IMAGE or B_IMAGE) (KRON_RADIUS)pixphys.size.radiusfloatPRad[0/11] F160W band Petrosian radius from SExtractor (in unit of A_IMAGE or B_IMAGE) (PETRO_RADIUS)pixphys.size.radiusfloatJ/ApJS/243/22/shardsSHARDS photometry for the CANDELS catalog (see Table 5)l_F704Upper limit flag on F704meta.code.errorcharl_F500Upper limit flag on F500meta.code.errorcharl_F602Upper limit flag on F602meta.code.errorcharl_F755Upper limit flag on F755meta.code.errorcharF883[0.0005/697]? Flux density in F883W35 (Flux_f883w35)uJyphot.flux.density;em.IRdoublenullablee_F883[0.004/3]? F883 uncertainty (Flux_err_f883w35)uJystat.errorfloatnullableF500[0.005/747]? Flux density in F500W17 (Flux_f500w17)uJyphot.flux.density;em.optdoublenullablee_F500[0.01/0.3]? F500 uncertainty (Flux_err_f500w17)uJystat.errorfloatnullablelamF517[510.4/520] Central effective wavelength in F517W17 filter (Eff_wav_f517w17) (1)nmem.wl.centralfloatF517[0.007/655]? Flux density in F517W17 (Flux_f517w17)uJyphot.flux.density;em.optdoublenullablee_F517[0.01/0.4]? F517 uncertainty (Flux_err_f517w17)uJystat.errorfloatnullablelamF534[528/538.3] Central effective wavelength in F534W17 filter (Eff_wav_f534w17) (1)nmem.wl.centralfloatl_F534Upper limit flag on F534meta.code.errorcharF534[0.003/413]? Flux density in F534W17 (Flux_f534w17)uJyphot.flux.density;em.optdoublenullablee_F534[0.007/0.2]? F534 uncertainty (Flux_err_f534w17)uJystat.errorfloatnullablelamF551[541/554.8] Central effective wavelength in F551W17 filter (Eff_wav_f551w17) (1)nmem.wl.centralfloatl_F551Upper limit flag on F551meta.code.errorcharF551[0.005/754]? Flux density in F551W17 (Flux_f551w17)uJyphot.flux.density;em.optdoublenullablee_F551[0.008/0.7]? F551 uncertainty (Flux_err_f551w17)uJystat.errorfloatnullablelamF568[557.5/572] Central effective wavelength in F568W17 filter (Eff_wav_f568w17) (1)nmem.wl.centralfloatl_F568Upper limit flag on F568meta.code.errorcharF568[0.004/382]? Flux density in F568W17 (Flux_f568w17)uJyphot.flux.density;em.optdoublenullablee_F568[0.01/0.8]? F568 uncertainty (Flux_err_f568w17)uJystat.errorfloatnullablelamF585[574.3/588.6] Central effective wavelength in F585W17 filter (Eff_wav_f585w17) (1)nmem.wl.centralfloate_F585[0.007/0.4]? F585 uncertainty (Flux_err_f585w17)uJystat.errorfloatnullablelamF602[590.8/606] Central effective wavelength in F602W17 filter (Eff_wav_f602w17)nmem.wl.centralfloatF602[0.01/382]? Flux density in F602W17 (Flux_f602w17)uJyphot.flux.density;em.optdoublenullablee_F602[0.006/0.2]? F602 uncertainty (Flux_err_f602w17)uJystat.errorfloatnullablelamF619[607.6/623] Central effective wavelength in F619W17 filter (Eff_wav_f619w17) (1)nmem.wl.centralfloatl_F619Upper limit flag on F619meta.code.errorcharF619[0.002/595]? Flux density in F619W17 (Flux_f619w17)uJyphot.flux.density;em.optdoublenullablee_F619[0.009/0.2]? F619 uncertainty (Flux_err_f619w17)uJystat.errorfloatnullablelamF636[625.3/641.3] Central effective wavelength in F636W17 filter (Eff_wav_f636w17) (1)nmem.wl.centralfloatl_F636Upper limit flag on F636meta.code.errorcharF636[0.01/370]? Flux density in F636W17 (Flux_f636w17)uJyphot.flux.density;em.optdoublenullablee_F636[0.01/0.3]? F636 uncertainty (Flux_err_f636w17)uJystat.errorfloatnullablelamF653[639.8/656] Central effective wavelength in F653W17 filter (Eff_wav_f653w17) (1)nmem.wl.centralfloatl_F653Upper limit flag on F653meta.code.errorcharF653[0.006/388]? Flux density in F653W17 (Flux_f653w17)uJyphot.flux.density;em.optdoublenullablee_F653[0.008/0.4]? F653 uncertainty (Flux_err_f653w17)uJystat.errorfloatnullablelamF670[655/672] Central effective wavelength in F670W17 filter (Eff_wav_f670w17) (1)nmem.wl.centralfloatl_F670Upper limit flag on F670meta.code.errorcharF670[0.005/556]? Flux density in F670W17 (Flux_f670w17)uJyphot.flux.density;em.optdoublenullablee_F670[0.005/0.3]? F670 uncertainty (Flux_err_f670w17)uJystat.errorfloatnullablelamF687[673.2/691] Central effective wavelength in F687W17 filter (Eff_wav_f687w17) (1)nmem.wl.centralfloatl_F687Upper limit flag on F687meta.code.errorcharF755[0.003/593]? Flux density in F755W17 (Flux_f755w17)uJyphot.flux.density;em.IRdoublenullablee_F755[0.01/0.4]? F755 uncertainty (Flux_err_f755w17)uJystat.errorfloatnullablelamF772[756.8/774.6] Central effective wavelength in F772W17 filter (Eff_wav_f772w17) (1)nmem.wl.centralfloatl_F772Upper limit flag on F772meta.code.errorcharF772[0.004/470]? Flux density in F772W17 (Flux_f772w17)uJyphot.flux.density;em.IRdoublenullablee_F772[0.01/0.3]? F772 uncertainty (Flux_err_f772w17)uJystat.errorfloatnullablelamF789[772.2/791.2] Central effective wavelength in F789W17 filter (Eff_wav_f789w17)nmem.wl.centralfloatF789[0.02/716]? Flux density in F789W17 (Flux_f789w17)uJyphot.flux.density;em.IRdoublenullablee_F789[0.01/1]? F789 uncertainty (Flux_err_f789w17)uJystat.errorfloatnullablelamF806[789.9/809.3] Central effective wavelength in F806W17 filter (Eff_wav_f806w17) (1)nmem.wl.centralfloatl_F806Upper limit flag on F806meta.code.errorcharF806[0.02/1392]? Flux density in F806W17 (Flux_f806w17)uJyphot.flux.density;em.IRdoublenullablee_F806[0.01/0.7]? F806 uncertainty (Flux_err_f806w17)uJystat.errorfloatnullablelamF823[809.5/829.1] Central effective wavelength in F823W17 filter (Eff_wav_f823w17)nmem.wl.centralfloatl_F823Upper limit flag on F823meta.code.errorcharF823[0.002/1285]? Flux density in F823W17 (Flux_f823w17)uJyphot.flux.density;em.IRdoublenullablee_F823[0.01/0.5]? F823 uncertainty (Flux_err_f823w17)uJystat.errorfloatnullablelamF840[823/843.3] Central effective wavelength in F840W17 filter (Eff_wav_f840w17) (1)nmem.wl.centralfloatl_F840Upper limit flag on F840meta.code.errorcharF840[0.01/1238]? Flux density in F840W17 (Flux_f840w17)uJyphot.flux.density;em.IRdoublenullablee_F840[0.01/0.5]? F840 uncertainty (Flux_err_f840w17)uJystat.errorfloatnullablelamF857[840.7/859.7] Central effective wavelength in F857W17 filter (Eff_wav_f857w17) (1)nmem.wl.centralfloatl_F857Upper limit flag on F857meta.code.errorcharF857[0.01/513]? Flux density in F857W17 (Flux_f857w17)uJyphot.flux.density;em.IRdoublenullablee_F857[0.007/0.8]? F857 uncertainty (Flux_err_f857w17)uJystat.errorfloatnullablelamF883[865.3/885.1] Central effective wavelength in F883W35 filter (Eff_wav_f883w35) (1)nmem.wl.centralfloatl_F883Upper limit flag on F883meta.code.errorcharlamF913[889.6/913.6] Central effective wavelength in F913W25 filter (Eff_wav_f913w25) (1)nmem.wl.centralfloatl_F913Upper limit flag on F913meta.code.errorcharF913[0.01/676]? Flux density in F913W25 (Flux_f913w25)uJyphot.flux.density;em.IRdoublenullablee_F913[0.006/0.2]? F913 uncertainty (Flux_err_f913w25)uJystat.errorfloatnullablelamF941[920.6/943.7] Central effective wavelength in F941W33 filter (Eff_wav_f941w33) (1)nmem.wl.centralfloatl_F941Upper limit flag on F941meta.code.errorcharF941[0.006/1900]? Flux density in F941W33 (Flux_f941w33)uJyphot.flux.density;em.IRdoublenullablee_F941[0.02/6.3]? F941 uncertainty (Flux_err_f941w33)uJystat.errorfloatnullablel_F585Upper limit flag on F585meta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/35451] Identifiermeta.id;meta.mainintprimarylamF500[494/503.2] Central effective wavelength in F500W17 filter (Eff_wav_f500w17) (1)nmem.wl.centralfloatl_F517Upper limit flag on F517meta.code.errorcharF585[0.005/434]? Flux density in F585W17 (Flux_f585w17)uJyphot.flux.density;em.optdoublenullablel_F789Upper limit flag on F789meta.code.errorchare_F738[0.01/0.3]? F738 uncertainty (Flux_err_f738w17)uJystat.errorfloatnullableF687[0.01/386]? Flux density in F687W17 (Flux_f687w17)uJyphot.flux.density;em.optdoublenullablee_F687[0.007/0.2]? F687 uncertainty (Flux_err_f687w17)uJystat.errorfloatnullablelamF704[690.3/707.6] Central effective wavelength in F704W17 filter (Eff_wav_f704w17) (1)nmem.wl.centralfloatF704[0.01/483]? Flux density in F704W17 (Flux_f704w17)mJyphot.flux.density;em.IRdoublenullablee_F704[0.01/0.5]? F704 uncertainty (Flux_err_f704w17)mJystat.errorfloatnullablelamF721[705.4/723.2] Central effective wavelength in F721W17 filter (Eff_wav_f721w17) (1)nmem.wl.centralfloatl_F721Upper limit flag on F721meta.code.errorcharF721[0.01/483]? Flux density in F721W17 (Flux_f721w17)uJyphot.flux.density;em.IRdoublenullablee_F721[0.02/0.3]? F721 uncertainty (Flux_err_f721w17)uJystat.errorfloatnullablelamF738[724.6/741.4] Central effective wavelength in F738W17 filter (Eff_wav_f738w17) (1)nmem.wl.centralfloatl_F738Upper limit flag on F738meta.code.errorcharF738[0.0007/503]? Flux density in F738W17 (Flux_f738w17)uJyphot.flux.density;em.IRdoublenullablelamF755[740.5/757.7] Central effective wavelength in F755W17 filter (Eff_wav_f755w17) (1)nmem.wl.centralfloatJ/ApJS/243/22/zcatPhotometric redshift catalog (see Table 7)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzspec[0/99] Spectroscopic redshiftsrc.redshiftfloatq_zspec[0/5] Flag on zspec (1=most reliable) (zspecflag) (1)meta.code.qualintr_zspecOriginal reference for the spectroscopic redshift (zref) (2)meta.ref;pos.framecharztier[0/10] Best photometric redshift from the three-tiered estimatesrc.redshift.photfloate_ztier[0/4.6] ztier uncertainty computed from the 68% confidence region of the PDFz (ztier_err)stat.errorfloatf_ztier[1/3] Classification flag of ztier (ztier_class) (3)meta.codeintzbest[0/10] Best redshift estimate from zspec, if available and with q_zspec<3, or ztiersrc.redshift;pos.heliocentricfloatID[1/35451] Identifiermeta.id;meta.mainintprimaryJ/ApJS/243/22/fastStellar population properties catalog from FAST (see Table 9)ID[1/35451] Identifiermeta.id;meta.mainintprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbest[0.0001/10] zbest from Table 7 (z)src.redshift;pos.heliocentricfloatlogtau[8.5/10.1] log of tau (ltau)log(yr)time.scalefloatMetal[0.02] Metallicity (fixed to 0.020)phys.abund.ZfloatlogAge[7.6/10.1] log of Age (lage)log(yr)time.agefloatAv[0/4] Dust reddeningmagphys.absorptionfloatlogMass[-1.5/13.4] log of Mass (lmass)log(solMass)phys.massfloatlogSFR[-19.4/4.8] log of SFR (lsfr)log(solMass.yr**-1)phys.SFRfloatlogsSFR[-25.5/-7.5] log of specific SFR (lssfr)log(yr**-1)phys.SFRfloatAge/tau[-2.5/1.6] log of Age to {tau} (la2t)time.agefloatChi2[0.008/9.4e+6] Minimum {chi}^2^stat.fit.chi2;stat.mindoubleUMag[-54/2.1]? Absolute magnitude in Johnson U (M_U)magphys.magAbs;em.opt.UdoublenullableVMag[-56.4/0.6]? Absolute magnitude in Johnson V (M_V)magphys.magAbs;em.opt.VdoublenullableJMag[-57.6/-1.6]? Absolute magnitude in 2MASS J (M_J)magphys.magAbs;em.IR.JdoublenullableJ/ApJS/243/22/g102*Emission-line catalog based on the G102 spectra (see Table 11)ID[1/35451] Identifiermeta.id;meta.mainintprimaryFHd[-28/1532]? H{delta} 4102.9{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Hd_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHd[0.3/373]? FHd uncertainty (Hd_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableEWOIIIx[-4890/2.1e+29]? [OIII]4364.4{AA} equivalent width in {AA} (OIIIx_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOIIIx[1/2.5e+15]? EWOIIIx uncertainty (OIIIx_EQW_ERR)0.1nmstat.errordoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHmag[14.28/24]? H-band AB magnitude (h_mag)magphot.mag;em.IR.Hfloatnullableztier[0/3.1]? Grism redshift used in the emission-line fit, identical to ztier in the redshift catalog (z_max_grism)src.redshift.photdoublenullables0[-101193/37756] s0 valuestat.fit.paramdoublee_s0[0.001/6.3e+11]? s0 uncertainty (s0_err)stat.errordoublenullables1[-24154/226742] s1 valuestat.fit.paramdoublee_s1[0.004/2e+9]? s1 uncertainty (s1_err)stat.errordoublenullableScHd[0.01/9e+9]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Hd_SCALE)arith.factordoublenullableEWHd[-2820/2.1e+14]? H{delta} 4102.9{AA} equivalent width in {AA} (Hd_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHd[2/2.1e+26]? EWHd uncertainty (Hd_EQW_ERR)0.1nmstat.errordoublenullableFHg[-14/2761]? H{gamma} 4341.7{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Hg_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHg[0.3/792]? FHg uncertainty (Hg_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScHg[0.007/1.4e+8]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Hg_SCALE)arith.factordoublenullableEWHg[-2550/9e+12]? H{gamma} 4341.7{AA} equivalent width in {AA} (Hg_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHg[2/2.4e+30]? EWHg uncertainty (Hg_EQW_ERR)0.1nmstat.errordoublenullableFHeII[-46/1152]? HeII 4687.5{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (HeII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHeII[0.6/468]? FHeII uncertainty (HeII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScHeII[0.006/503000]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (HeII_SCALE)arith.factordoublenullableEWHeII[-9720/2e+9]? HeII 4687.5{AA} equivalent width in {AA} (HeII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHeII[0.8/9.8e+11]? EWHeII uncertainty (HeII_EQW_ERR)0.1nmstat.errordoublenullableFHb[-39/710]? H{beta} 4862.7{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Hb_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHb[0.5/233]? FHb uncertainty (Hb_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScHb[0.007/9.7e+30]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Hb_SCALE)arith.factordoublenullableEWHb[-10700/2.2e+25]? H{beta} 4862.7{AA} equivalent width in {AA} (Hb_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHb[0.5/4.8e+9]? EWHb uncertainty (Hb_EQW_ERR)0.1nmstat.errordoublenullableScSIII[0.008/7.6e+27]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (SIII_SCALE)arith.factordoublenullableEWSIII[-83/1.6e+7]? SIII{lambda}{lambda}9068.6,9530.6 equivalent width in {AA} (SIII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWSIII[0/6e+27]? EWSIII uncertainty (SIII_EQW_ERR)0.1nmstat.errordoublenullableFHeI[-19/859]? HeI 5877.2{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (HeI_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHeI[0.5/104]? FHeI uncertainty (HeI_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScNeIII[0.015/7e+6]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (NeIII_SCALE)arith.factordoublenullableFMgII[-3.7/4898]? MgII 2799.1{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (MgII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FMgII[0.3/362]? FMgII uncertainty (MgII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScMgII[0.05/3.8e+21]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (MgII_SCALE)arith.factordoublenullableEWMgII[-3.9e+8/1.1e+26]? MgII 2799.1{AA} equivalent width in {AA} (MgII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWMgII[0.04/8.5e+37]? EWMgII uncertainty (MgII_EQW_ERR)0.1nmstat.errordoublenullableFOII[-6/7797]? 3729.9{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FOII[0.4/485]? FOII uncertainty (OII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScOII[0.04/1066]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OII_SCALE)arith.factordoublenullableEWOII[-2249/10179]? 3729.9{AA} equivalent width in {AA} (OII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOII[0.2/7.8e+10]? EWOII uncertainty (OII_EQW_ERR)0.1nmstat.errordoublenullableFOIIIx[-49/2117]? 4364.4{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OIIIx_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FOIIIx[0.2/1055]? FOIIIx uncertainty (OIIIx_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScOIIIx[0.002/9.6e+7]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OIIIx_SCALE)arith.factordoublenullableFOIII[-20/3497]? {lambda}{lambda}5008.2,4960.3{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OIII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FOIII[0.7/60]? FOIII uncertainty (OIII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScOIII[0.006/1.1e+36]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OIII_SCALE)arith.factordoublenullableEWOIII[-4500/7.2e+13]? [OIII]{lambda}{lambda}5008.2,4960.3{AA} equivalent width in {AA} (OIII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOIII[1/1.2e+10]? EWOIII uncertainty (OIII_EQW_ERR)0.1nmstat.errordoublenullableFHa[-3.6/1206]? H{alpha} 6564.6{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Ha_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHa[0/117]? FHa uncertainty (Ha_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScHa[0.01/1.1e+37]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Ha_SCALE)arith.factordoublenullableEWHa[-266/8e+9]? H{alpha} 6564.6{AA} equivalent width in {AA} (Ha_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHa[0/2e+32]? EWHa uncertainty (Ha_EQW_ERR)0.1nmstat.errordoublenullableFSII[-8.2/252]? {lambda}{lambda}6718.3,6732.7 emission-line flux in units of 10^-17^ergs/s/cm^2^ (SII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FSII[0/287]? FSII uncertainty (SII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScSII[0.02/373000]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (SII_SCALE)arith.factordoublenullableEWSII[-29300/4e+7]? [SII]{lambda}{lambda}6718.3,6732.7 equivalent width in {AA} (SII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWSII[0/2.3e+32]? EWSII uncertainty (SII_EQW_ERR)0.1nmstat.errordoublenullableFSIII[-1/1448]? SIII{lambda}{lambda}9068.6,9530.6 emission-line flux in units of 10^-17^ergs/s/cm^2^ (SIII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FSIII[0/1.2e+11]? FSIII uncertainty (SIII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableEWNeIII[-1420/2.5e+8]? [NeIII] 3869{AA} equivalent width in {AA} (NeIII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWNeIII[2/4.8e+26]? EWNeIII uncertainty (NeIII_EQW_ERR)0.1nmstat.errordoublenullableFNeV[-20/14343]? NeV 3346.8{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (NeV_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FNeV[0.4/1349]? FNeV uncertainty (NeV_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScNeV[0.07/1.1e+32]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (NeV_SCALE)arith.factordoublenullableEWNeV[-3.2e+10/3.5e+23]? NeV 3346.8{AA} equivalent width in {AA} (NeV_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWNeV[0.08/1.6e+35]? EWNeV uncertainty (NeV_EQW_ERR)0.1nmstat.errordoublenullableFNeVI[-17/7018]? NeVI 3426.85{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (NeVI_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FNeVI[0.4/510]? FNeVI uncertainty (NeVI_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScNeVI[0.08/2.5e+25]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (NeVI_SCALE)arith.factordoublenullableEWNeVI[-374000/9.6e+20]? NeVI 3426.85{AA} equivalent width in {AA} (NeVI_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWNeVI[0.1/5.2e+17]? EWNeVI uncertainty (NeVI_EQW_ERR)0.1nmstat.errordoublenullableFOI[-4/227]? 6302{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OI_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FOI[0.4/57]? FOI uncertainty (OI_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScOI[0.009/2.6e+6]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OI_SCALE)arith.factordoublenullableEWOI[-996/3.6e+37]? [OI] 6302{AA} equivalent width in {AA} (OI_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOI[0.1/3.4e+34]? EWOI uncertainty (OI_EQW_ERR)0.1nmstat.errordoublenullableGrismIDGrism number ("-99" if no grism data) (grism_id)meta.idcharScHeI[0.04/10700]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (HeI_SCALE)arith.factordoublenullableEWHeI[-1710/3.3e+6]? HeI 5877.2{AA} equivalent width in {AA} (HeI_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHeI[0.16/8.8e+12]? EWHeI uncertainty (HeI_EQW_ERR)0.1nmstat.errordoublenullableFHeIb[-12.2/1721]? HeI 3889.5{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (HeIb_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHeIb[0.2/271]? FHeIb uncertainty (HeIb_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScHeIb[0.015/8.3e+6]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (HeIb_SCALE)arith.factordoublenullableEWHeIb[-859/7.5e+8]? HeI 3889.5{AA} equivalent width in {AA} (HeIb_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHeIb[1.6/4e+32]? EWHeIb uncertainty (HeIb_EQW_ERR)0.1nmstat.errordoublenullableFNeIII[-23/567]? 3869{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (NeIII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FNeIII[0.2/468]? FNeIII uncertainty (NeIII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableJ/ApJS/243/22/g141*Emission-line catalog based on the G141 spectra (see Table 11)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintztier[0.3/3.6]? Grism redshift used in the emission-line fit, identical to ztier in the redshift catalog (z_max_grism)src.redshift.photdoublenullablee_s0[0/6.7e+15]? s0 uncertainty (s0_err)stat.errordoublenullables1[-249727/592044]? s1 valuestat.fit.paramdoublenullablee_s1[0.003/1.5e+14]? s1 uncertainty (s1_err)stat.errordoublenullableFMgII[-17.7/24816]? MgII 2799.1{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (MgII_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FMgII[0.4/46361]? FMgII uncertainty (MgII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScMgII[0.04/4.5e+7]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (MgII_SCALE)arith.factordoublenullableEWMgII[-17934/387215]? MgII 2799.1{AA} equivalent width in {AA} (MgII_EQW)0.1nmspect.line.eqWidthdoublenullableEWOII[-4.1e+12/3.2e+11]? 3729.9{AA} equivalent width in {AA} (OII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOII[0.3/3.1e+25]? EWOII uncertainty (OII_EQW_ERR)0.1nmstat.errordoublenullableFHd[-2300/7.6e+8]? H{delta} 4102.9{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Hd_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FHd[0.3/5.9e+16]? FHd uncertainty (Hd_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScHd[0.015/3.5e+15]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Hd_SCALE)arith.factordoublenullableEWHd[-4.2e+23/1.4e+14]? H{delta} 4102.9{AA} equivalent width in {AA} (Hd_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHd[0.4/1.6e+26]? EWHd uncertainty (Hd_EQW_ERR)0.1nmstat.errordoublenullableFHg[-537/8.5e+8]? H{gamma} 4341.7{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Hg_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FHg[0.3/6.4e+16]? FHg uncertainty (Hg_FLUX_ERR)1e-20W.m**-2stat.errordoublenullablee_FHb[0.2/3e+15]? FHb uncertainty (Hb_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScHb[0.002/10e+14]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Hb_SCALE)arith.factordoublenullableEWHb[-13500/5.6e+13]? H{beta} 4862.7{AA} equivalent width in {AA} (Hb_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHb[0.3/2.6e+26]? EWHb uncertainty (Hb_EQW_ERR)0.1nmstat.errordoublenullableFOIII[-4115/10892]? {lambda}{lambda}5008.2,4960.3{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OIII_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FOIII[0.3/1.9e+14]? FOIII uncertainty (OIII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScOIII[0.001/1.3e+29]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OIII_SCALE)arith.factordoublenullableEWOIII[-1.6e+13/2e+17]? {lambda}{lambda}5008.2,4960.3{AA} equivalent width in {AA} (OIII_EQW)0.1nmspect.line.eqWidthdoublenullableEWNeIII[-58000/1.6e+14]? 3869{AA} equivalent width in {AA} (NeIII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWNeIII[0.1/2.1e+15]? EWNeIII uncertainty (NeIII_EQW_ERR)0.1nmstat.errordoublenullableFNeV[-7.1e+8/51100]? NeV 3346.8{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (NeV_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FNeV[0.3/6e+16]? FNeV uncertainty (NeV_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScNeV[0.003/4.9e+8]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (NeV_SCALE)arith.factordoublenullablee_EWNeVI[1.6/9.1e+32]? EWNeVI uncertainty (NeVI_EQW_ERR)0.1nmstat.errordoublenullableFOI[-10/3256]? 6302{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OI_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FOI[0.3/387]? FOI uncertainty (OI_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScOI[0.02/6.5e+14]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OI_SCALE)arith.factordoublenullableEWOI[-2e+10/3.5e+12]? 6302{AA} equivalent width in {AA} (OI_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOI[1/4.3e+26]? EWOI uncertainty (OI_EQW_ERR)0.1nmstat.errordoublenullableID[1/35451] Identifiermeta.id;meta.mainintprimaryGrismIDGrism number ("-99" if no grism data) (grism_id)meta.idcharHmag[14/25]? H-band AB magnitude (h_mag)magphot.mag;em.IR.HfloatnullableScHg[0.01/9.8e+29]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Hg_SCALE)arith.factordoublenullableEWHg[-8.8e+13/1.8e+12]? H{gamma} 4341.7{AA} equivalent width in {AA} (Hg_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHg[0.3/8.9e+14]? EWHg uncertainty (Hg_EQW_ERR)0.1nmstat.errordoublenullableFOIIIx[-987/5.5e+8]? 4364.4{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OIIIx_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FOIIIx[0.2/4.2e+16]? FOIIIx uncertainty (OIIIx_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScOIIIx[0.009/2.3e+31]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OIIIx_SCALE)arith.factordoublenullableEWOIIIx[-4.6e+7/4.8e+15]? 4364.4{AA} equivalent width in {AA} (OIIIx_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWOIIIx[0.19/1.2e+26]? EWOIIIx uncertainty (OIIIx_EQW_ERR)0.1nmstat.errordoublenullableFHeII[-3.5e+8/8680]? HeII 4687.5{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (HeII_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FHeII[0.3/2.1e+16]? FHeII uncertainty (HeII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScHeII[0.003/5.9e+10]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (HeII_SCALE)arith.factordoublenullableEWHeII[-4.8e+54/2.9e+13]? HeII 4687.5{AA} equivalent width in {AA} (HeII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHeII[0.1/1.4e+29]? EWHeII uncertainty (HeII_EQW_ERR)0.1nmstat.errordoublenullableFHb[-3318/21853]? H{beta} 4862.7{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Hb_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_EWSII[0.1/1.6e+29]? EWSII uncertainty (SII_EQW_ERR)0.1nmstat.errordoublenullableFSIII[-66/1282]? SIII{lambda}{lambda}9068.6,9530.6 emission-line flux in units of 10^-17^ergs/s/cm^2^ (SIII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FSIII[0.3/1461]? FSIII uncertainty (SIII_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScSIII[0.01/1.6e+18]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (SIII_SCALE)arith.factordoublenullableEWSIII[-184000/1.7e+37]? SIII{lambda}{lambda}9068.6,9530.6 equivalent width in {AA} (SIII_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWSIII[0.01/5.2e+30]? EWSIII uncertainty (SIII_EQW_ERR)0.1nmstat.errordoublenullableFHeI[-4387/7505]? HeI 5877.2{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (HeI_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FHeI[0.3/5.1e+12]? FHeI uncertainty (HeI_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScHeI[0.01/2.7e+10]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (HeI_SCALE)arith.factordoublenullablee_EWHeI[0.1/1.4e+29]? EWHeI uncertainty (HeI_EQW_ERR)0.1nmstat.errordoublenullableEWNeV[-5260/8.9e+8]? NeV 3346.8{AA} equivalent width in {AA} (NeV_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWNeV[1/5.1e+24]? EWNeV uncertainty (NeV_EQW_ERR)0.1nmstat.errordoublenullableFNeVI[-21.4/3e+8]? NeVI 3426.85{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (NeVI_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FNeVI[0.4/2.3e+16]? FNeVI uncertainty (NeVI_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScNeVI[0.005/2.2e+6]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (NeVI_SCALE)arith.factordoublenullableEWNeVI[-4440/1.1e+9]? NeVI 3426.85{AA} equivalent width in {AA} (NeVI_EQW)0.1nmspect.line.eqWidthdoublenullables0[-395000/8.9e+7]? s0 valuestat.fit.paramdoublenullablee_EWMgII[13/1.5e+15]? EWMgII uncertainty (MgII_EQW_ERR)0.1nmstat.errordoublenullableFOII[-2.8e+8/5630]? 3729.9{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (OII_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FOII[0.3/1.7e+16]? FOII uncertainty (OII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScOII[0.016/2e+9]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (OII_SCALE)arith.factordoublenullablee_EWOIII[0.1/1.5e+14]? EWOIII uncertainty (OIII_EQW_ERR)0.1nmstat.errordoublenullableFHa[-19/1789]? H{alpha} 6564.6{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (Ha_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FHa[0.3/1029]? FHa uncertainty (Ha_FLUX_ERR)1e-20W.m**-2stat.errorfloatnullableScHa[0.03/5.1e+16]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (Ha_SCALE)arith.factordoublenullableEWHa[-28200/5e+16]? H{alpha} 6564.6{AA} equivalent width in {AA} (Ha_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHa[0.7/9.8e+29]? EWHa uncertainty (Ha_EQW_ERR)0.1nmstat.errordoublenullableFSII[-39.3/1533]? {lambda}{lambda}6718.3,6732.7 emission-line flux in units of 10^-17^ergs/s/cm^2^ (SII_FLUX)1e-20W.m**-2phot.fluxfloatnullablee_FSII[0.3/4.6e+13]? FSII uncertainty (SII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScSII[0.03/1.1e+23]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (SII_SCALE)arith.factordoublenullableEWSII[-1.2e+7/9.4e+35]? {lambda}{lambda}6718.3,6732.7 equivalent width in {AA} (SII_EQW)0.1nmspect.line.eqWidthdoublenullableEWHeI[-1.3e+6/3.5e+29]? HeI 5877.2{AA} equivalent width in {AA} (HeI_EQW)0.1nmspect.line.eqWidthdoublenullableFHeIb[-9.3e+8/13100]? HeI 3889.5{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (HeIb_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FHeIb[0.3/7.1e+16]? FHeIb uncertainty (HeIb_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScHeIb[0.02/1.8e+9]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (HeIb_SCALE)arith.factordoublenullableEWHeIb[-24200/7.4e+12]? HeI 3889.5{AA} equivalent width in {AA} (HeIb_EQW)0.1nmspect.line.eqWidthdoublenullablee_EWHeIb[0.04/3.2e+29]? EWHeIb uncertainty (HeIb_EQW_ERR)0.1nmstat.errordoublenullableFNeIII[-639/8e+7]? 3869{AA} emission-line flux in units of 10^-17^ergs/s/cm^2^ (NeIII_FLUX)1e-20W.m**-2phot.fluxdoublenullablee_FNeIII[0.3/7.8e+15]? FNeIII uncertainty (NeIII_FLUX_ERR)1e-20W.m**-2stat.errordoublenullableScNeIII[0.01/1.8e+9]? Multiplicative scaling factor to correct the flux of the emission line to the photometry (NeIII_SCALE)arith.factordoublenullableJ/ApJS/243/22/sfrgdnThe GOODS-N SFR catalog (see Table 17)e_F160um[1848/1969]? F160um uncertainty (only for COSMOS) (Flux_Err_MIPS160)uJystat.errorfloatnullablee_F100umP[142/16007]? F100um uncertainty (Flux_Err_PACS_100)uJystat.errordoublenullablee_F160umP[204/17311]? F160um uncertainty (Flux_Err_PACS_160)uJystat.errordoublenullablee_F250um[580/7680]? F250um uncertainty (Flux_Err_SPIRE_250)uJystat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbest[0/10.01]? Photometric redshift used in the IR SED fitting, corresponds to zbest in the redshift catalogsrc.redshift;pos.heliocentricfloatnullableF24um[14/9639]? Spitzer/MIPS 24um flux (Flux_MIPS24) (1)uJyphot.flux.density;em.IR.15-30umdoublenullableF70um[980/153570]? Spitzer/MIPS 70um flux (Flux_MIPS70)uJyphot.flux.density;em.IR.30-60umdoublenullableF160um[26790/31244]? Spitzer/MIPS 160um flux (only for COSMOS) (Flux_MIPS160)uJyphot.flux.density;em.mm.1500-3000GHzfloatnullableF100umP[203/207880]? Herschel/PACS 100um flux (Flux_PACS_100)uJyphot.flux.density;em.IR.60-100umdoublenullableF160umP[687/224810]? Herschel/PACS 160um flux (Flux_PACS_160)uJyphot.flux.density;em.mm.1500-3000GHzdoublenullableF250um[2309/130160]? Herschel/SPIRE 250um flux (Flux_SPIRE_250)uJyphot.flux.density;em.mm.750-1500GHzdoublenullableF350um[1631/68809]? Herschel/SPIRE 350um flux (Flux_SPIRE_350)uJyphot.flux.density;em.mm.750-1500GHzfloatnullableF500um[1327/53735]? Herschel/SPIRE 500um flux (Flux_SPIRE_500)uJyphot.flux.density;em.mm.400-750GHzfloatnullablee_F24um[4/280]? F24um uncertainty (Flux_Err_MIPS24)uJystat.errordoublenullablee_F350um[492/5712]? F350um uncertainty (Flux_Err_SPIRE_350)uJystat.errorfloatnullablee_F500um[374/4807]? F500um uncertainty (Flux_Err_SPIRE_500)uJystat.errorfloatnullableSFRtot[-1.1e+17/2.6e+43]? Best estimate of the total SFR (SFR_ladder_total) (2)solMass/yrphys.SFRdoublenullableLType[1/3] Type of SFR indicators used in SFRtot (SFR_ladder_type) (3)meta.codeintUVcor[-1.1e+17/2.6e+43]? UV-based star formation rate corrected for extinction (SFR_UV_corr) (4)solMass/yrphys.SFRdoublenullablee_UVcor[2.1e-8/3.7e+43]? UVcor uncertainty (SFR_UV_corr_Error)solMass/yrstat.errordoublenullableSFR-IR[-2020/15562] IR-based star formation rate (5)solMass/yrphys.SFRdoubleSFR-UV160[-6.9e+16/8.7e+17]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 160nm (SFR_UV_obs_160)solMass/yrphys.SFRdoublenullableSFR-UV280[-1.5e+17/1.8e+18]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 280nm (SFR_UV_obs_280)solMass/yrphys.SFRdoublenullablebeta[-2.5/81.7]? UV slope, {beta}_UV_stat.fit.paramdoublenullableAuv160[0.08/97]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV160 (A_UV_160)magphys.absorptionfloatnullableAuv280[0.06/71]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV280 (A_UV_280)magphys.absorptionfloatnullableAv[0.03/40]? Optical attenuation in the V-band (A_V) (6)magphys.absorptionfloatnullableSFR-UVc160[-6.9e+16/5.2e+43]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 160nm (SFR_UV_corr_160)solMass/yrphys.SFRdoublenullableSFR-UVc280[-1.5e+17/3.6e+33]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 280nm (SFR_UV_corr_280)solMass/yrphys.SFRdoublenullableSFR-IRw11[-2019/23460] IR-based star formation rate derived from the MIPS 24um flux following Calzetti+ (2000ApJ...533..682C) (SFR_IR_W11)solMass/yrphys.SFRdoubleID[1/41457] Identifiermeta.id;meta.mainintprimarye_F70um[305/4915]? F70um uncertainty (Flux_Err_MIPS70)uJystat.errorfloatnullableJ/ApJS/243/22/sfrgdsThe GOODS-S SFR catalog (see Appendix D)SFR-UVc280[-1.5e+17/3.6e+33]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 280nm (SFR_UV_corr_280)solMass/yrphys.SFRdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/41457] Identifiermeta.id;meta.mainintzbest[0/10.01]? Photometric redshift used in the IR SED fitting, corresponds to zbest in the redshift catalogsrc.redshift;pos.heliocentricfloatnullableF24um[14/9639]? Spitzer/MIPS 24um flux (Flux_MIPS24) (1)uJyphot.flux.density;em.IR.15-30umdoublenullableF70um[980/153570]? Spitzer/MIPS 70um flux (Flux_MIPS70)uJyphot.flux.density;em.IR.30-60umdoublenullableF160um[26790/31244]? Spitzer/MIPS 160um flux (only for COSMOS) (Flux_MIPS160)uJyphot.flux.density;em.mm.1500-3000GHzfloatnullableF100umP[203/207880]? Herschel/PACS 100um flux (Flux_PACS_100)uJyphot.flux.density;em.IR.60-100umdoublenullableF160umP[687/224810]? Herschel/PACS 160um flux (Flux_PACS_160)uJyphot.flux.density;em.mm.1500-3000GHzdoublenullableF250um[2309/130160]? Herschel/SPIRE 250um flux (Flux_SPIRE_250)uJyphot.flux.density;em.mm.750-1500GHzdoublenullableF350um[1631/68809]? Herschel/SPIRE 350um flux (Flux_SPIRE_350)uJyphot.flux.density;em.mm.750-1500GHzfloatnullableF500um[1327/53735]? Herschel/SPIRE 500um flux (Flux_SPIRE_500)uJyphot.flux.density;em.mm.400-750GHzfloatnullablee_F24um[4/280]? F24um uncertainty (Flux_Err_MIPS24)uJystat.errordoublenullablee_F70um[305/4915]? F70um uncertainty (Flux_Err_MIPS70)uJystat.errorfloatnullablee_F160um[1848/1969]? F160um uncertainty (only for COSMOS) (Flux_Err_MIPS160)uJystat.errorfloatnullablee_F250um[580/7680]? F250um uncertainty (Flux_Err_SPIRE_250)uJystat.errorfloatnullablee_F100umP[142/16007]? F100um uncertainty (Flux_Err_PACS_100)uJystat.errordoublenullablee_F160umP[204/17311]? F160um uncertainty (Flux_Err_PACS_160)uJystat.errordoublenullablee_F350um[492/5712]? F350um uncertainty (Flux_Err_SPIRE_350)uJystat.errorfloatnullablee_F500um[374/4807]? F500um uncertainty (Flux_Err_SPIRE_500)uJystat.errorfloatnullableSFRtot[-1.1e+17/2.6e+43]? Best estimate of the total SFR (SFR_ladder_total) (2)solMass/yrphys.SFRdoublenullableLType[1/3] Type of SFR indicators used in SFRtot (SFR_ladder_type) (3)meta.codeintUVcor[-1.1e+17/2.6e+43]? UV-based star formation rate corrected for extinction (SFR_UV_corr) (4)solMass/yrphys.SFRdoublenullablee_UVcor[2.1e-8/3.7e+43]? UVcor uncertainty (SFR_UV_corr_Error)solMass/yrstat.errordoublenullableSFR-IR[-2020/15562] IR-based star formation rate (5)solMass/yrphys.SFRdoubleSFR-UV160[-6.9e+16/8.7e+17]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 160nm (SFR_UV_obs_160)solMass/yrphys.SFRdoublenullableSFR-UV280[-1.5e+17/1.8e+18]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 280nm (SFR_UV_obs_280)solMass/yrphys.SFRdoublenullablebeta[-2.5/81.7]? UV slope, {beta}_UV_stat.fit.paramdoublenullableAuv160[0.08/97]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV160 (A_UV_160)magphys.absorptionfloatnullableAuv280[0.06/71]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV280 (A_UV_280)magphys.absorptionfloatnullableAv[0.03/40]? Optical attenuation in the V-band (A_V) (6)magphys.absorptionfloatnullableSFR-UVc160[-6.9e+16/5.2e+43]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 160nm (SFR_UV_corr_160)solMass/yrphys.SFRdoublenullableSFR-IRw11[-2019/23460] IR-based star formation rate derived from the MIPS 24um flux following Calzetti+ (2000ApJ...533..682C) (SFR_IR_W11)solMass/yrphys.SFRdoubleJ/ApJS/243/22/sfrcosThe COSMOS SFR catalog (see Appendix D)ID[1/41457] Identifiermeta.id;meta.mainintzbest[0/10.01]? Photometric redshift used in the IR SED fitting, corresponds to zbest in the redshift catalogsrc.redshift;pos.heliocentricfloatnullableSFRtot[-1.1e+17/2.6e+43]? Best estimate of the total SFR (SFR_ladder_total) (2)solMass/yrphys.SFRdoublenullableLType[1/3] Type of SFR indicators used in SFRtot (SFR_ladder_type) (3)meta.codeintUVcor[-1.1e+17/2.6e+43]? UV-based star formation rate corrected for extinction (SFR_UV_corr) (4)solMass/yrphys.SFRdoublenullablee_UVcor[2.1e-8/3.7e+43]? UVcor uncertainty (SFR_UV_corr_Error)solMass/yrstat.errordoublenullableSFR-IR[-2020/15562] IR-based star formation rate (5)solMass/yrphys.SFRdoubleSFR-UV160[-6.9e+16/8.7e+17]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 160nm (SFR_UV_obs_160)solMass/yrphys.SFRdoublenullableSFR-UV280[-1.5e+17/1.8e+18]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 280nm (SFR_UV_obs_280)solMass/yrphys.SFRdoublenullablebeta[-2.5/81.7]? UV slope, {beta}_UV_stat.fit.paramdoublenullableAuv160[0.08/97]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV160 (A_UV_160)magphys.absorptionfloatnullableAuv280[0.06/71]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV280 (A_UV_280)magphys.absorptionfloatnullableAv[0.03/40]? Optical attenuation in the V-band (A_V) (6)magphys.absorptionfloatnullableSFR-UVc160[-6.9e+16/5.2e+43]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 160nm (SFR_UV_corr_160)solMass/yrphys.SFRdoublenullableSFR-UVc280[-1.5e+17/3.6e+33]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 280nm (SFR_UV_corr_280)solMass/yrphys.SFRdoublenullableSFR-IRw11[-2019/23460] IR-based star formation rate derived from the MIPS 24um flux following Calzetti+ (2000ApJ...533..682C) (SFR_IR_W11)solMass/yrphys.SFRdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintF24um[14/9639]? Spitzer/MIPS 24um flux (Flux_MIPS24) (1)uJyphot.flux.density;em.IR.15-30umdoublenullableF70um[980/153570]? Spitzer/MIPS 70um flux (Flux_MIPS70)uJyphot.flux.density;em.IR.30-60umdoublenullableF160um[26790/31244]? Spitzer/MIPS 160um flux (only for COSMOS) (Flux_MIPS160)uJyphot.flux.density;em.mm.1500-3000GHzfloatnullableF100umP[203/207880]? Herschel/PACS 100um flux (Flux_PACS_100)uJyphot.flux.density;em.IR.60-100umdoublenullableF160umP[687/224810]? Herschel/PACS 160um flux (Flux_PACS_160)uJyphot.flux.density;em.mm.1500-3000GHzdoublenullableF250um[2309/130160]? Herschel/SPIRE 250um flux (Flux_SPIRE_250)uJyphot.flux.density;em.mm.750-1500GHzdoublenullableF350um[1631/68809]? Herschel/SPIRE 350um flux (Flux_SPIRE_350)uJyphot.flux.density;em.mm.750-1500GHzfloatnullableF500um[1327/53735]? Herschel/SPIRE 500um flux (Flux_SPIRE_500)uJyphot.flux.density;em.mm.400-750GHzfloatnullablee_F24um[4/280]? F24um uncertainty (Flux_Err_MIPS24)uJystat.errordoublenullablee_F70um[305/4915]? F70um uncertainty (Flux_Err_MIPS70)uJystat.errorfloatnullablee_F160um[1848/1969]? F160um uncertainty (only for COSMOS) (Flux_Err_MIPS160)uJystat.errorfloatnullablee_F100umP[142/16007]? F100um uncertainty (Flux_Err_PACS_100)uJystat.errordoublenullablee_F160umP[204/17311]? F160um uncertainty (Flux_Err_PACS_160)uJystat.errordoublenullablee_F250um[580/7680]? F250um uncertainty (Flux_Err_SPIRE_250)uJystat.errorfloatnullablee_F350um[492/5712]? F350um uncertainty (Flux_Err_SPIRE_350)uJystat.errorfloatnullablee_F500um[374/4807]? F500um uncertainty (Flux_Err_SPIRE_500)uJystat.errorfloatnullableJ/ApJS/243/22/sfregsThe EGS SFR catalog (see Appendix D)SFR-UVc160[-6.9e+16/5.2e+43]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 160nm (SFR_UV_corr_160)solMass/yrphys.SFRdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzbest[0/10.01]? Photometric redshift used in the IR SED fitting, corresponds to zbest in the redshift catalogsrc.redshift;pos.heliocentricfloatnullableF24um[14/9639]? Spitzer/MIPS 24um flux (Flux_MIPS24) (1)uJyphot.flux.density;em.IR.15-30umdoublenullableF70um[980/153570]? Spitzer/MIPS 70um flux (Flux_MIPS70)uJyphot.flux.density;em.IR.30-60umdoublenullableF160um[26790/31244]? Spitzer/MIPS 160um flux (only for COSMOS) (Flux_MIPS160)uJyphot.flux.density;em.mm.1500-3000GHzfloatnullableF100umP[203/207880]? Herschel/PACS 100um flux (Flux_PACS_100)uJyphot.flux.density;em.IR.60-100umdoublenullableF160umP[687/224810]? Herschel/PACS 160um flux (Flux_PACS_160)uJyphot.flux.density;em.mm.1500-3000GHzdoublenullableF250um[2309/130160]? Herschel/SPIRE 250um flux (Flux_SPIRE_250)uJyphot.flux.density;em.mm.750-1500GHzdoublenullableF350um[1631/68809]? Herschel/SPIRE 350um flux (Flux_SPIRE_350)uJyphot.flux.density;em.mm.750-1500GHzfloatnullableF500um[1327/53735]? Herschel/SPIRE 500um flux (Flux_SPIRE_500)uJyphot.flux.density;em.mm.400-750GHzfloatnullablee_F24um[4/280]? F24um uncertainty (Flux_Err_MIPS24)uJystat.errordoublenullablee_F70um[305/4915]? F70um uncertainty (Flux_Err_MIPS70)uJystat.errorfloatnullablee_F160um[1848/1969]? F160um uncertainty (only for COSMOS) (Flux_Err_MIPS160)uJystat.errorfloatnullablee_F100umP[142/16007]? F100um uncertainty (Flux_Err_PACS_100)uJystat.errordoublenullablee_F160umP[204/17311]? F160um uncertainty (Flux_Err_PACS_160)uJystat.errordoublenullablee_F250um[580/7680]? F250um uncertainty (Flux_Err_SPIRE_250)uJystat.errorfloatnullablee_F350um[492/5712]? F350um uncertainty (Flux_Err_SPIRE_350)uJystat.errorfloatnullablee_F500um[374/4807]? F500um uncertainty (Flux_Err_SPIRE_500)uJystat.errorfloatnullableSFRtot[-1.1e+17/2.6e+43]? Best estimate of the total SFR (SFR_ladder_total) (2)solMass/yrphys.SFRdoublenullableLType[1/3] Type of SFR indicators used in SFRtot (SFR_ladder_type) (3)meta.codeintID[1/41457] Identifiermeta.id;meta.mainintSFR-UV160[-6.9e+16/8.7e+17]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 160nm (SFR_UV_obs_160)solMass/yrphys.SFRdoublenullableSFR-UV280[-1.5e+17/1.8e+18]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 280nm (SFR_UV_obs_280)solMass/yrphys.SFRdoublenullablebeta[-2.5/81.7]? UV slope, {beta}_UV_stat.fit.paramdoublenullableAuv160[0.08/97]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV160 (A_UV_160)magphys.absorptionfloatnullableAuv280[0.06/71]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV280 (A_UV_280)magphys.absorptionfloatnullableAv[0.03/40]? Optical attenuation in the V-band (A_V) (6)magphys.absorptionfloatnullableUVcor[-1.1e+17/2.6e+43]? UV-based star formation rate corrected for extinction (SFR_UV_corr) (4)solMass/yrphys.SFRdoublenullablee_UVcor[2.1e-8/3.7e+43]? UVcor uncertainty (SFR_UV_corr_Error)solMass/yrstat.errordoublenullableSFR-IR[-2020/15562] IR-based star formation rate (5)solMass/yrphys.SFRdoubleSFR-UVc280[-1.5e+17/3.6e+33]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 280nm (SFR_UV_corr_280)solMass/yrphys.SFRdoublenullableSFR-IRw11[-2019/23460] IR-based star formation rate derived from the MIPS 24um flux following Calzetti+ (2000ApJ...533..682C) (SFR_IR_W11)solMass/yrphys.SFRdoubleJ/ApJS/243/22/sfrudsThe UDS SFR catalog (see Appendix D)Auv280[0.06/71]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV280 (A_UV_280)magphys.absorptionfloatnullableAv[0.03/40]? Optical attenuation in the V-band (A_V) (6)magphys.absorptionfloatnullableF350um[1631/68809]? Herschel/SPIRE 350um flux (Flux_SPIRE_350)uJyphot.flux.density;em.mm.750-1500GHzfloatnullableF500um[1327/53735]? Herschel/SPIRE 500um flux (Flux_SPIRE_500)uJyphot.flux.density;em.mm.400-750GHzfloatnullablee_F24um[4/280]? F24um uncertainty (Flux_Err_MIPS24)uJystat.errordoublenullablee_F70um[305/4915]? F70um uncertainty (Flux_Err_MIPS70)uJystat.errorfloatnullablee_F160um[1848/1969]? F160um uncertainty (only for COSMOS) (Flux_Err_MIPS160)uJystat.errorfloatnullablee_F100umP[142/16007]? F100um uncertainty (Flux_Err_PACS_100)uJystat.errordoublenullablee_F160umP[204/17311]? F160um uncertainty (Flux_Err_PACS_160)uJystat.errordoublenullablee_F250um[580/7680]? F250um uncertainty (Flux_Err_SPIRE_250)uJystat.errorfloatnullablee_F350um[492/5712]? F350um uncertainty (Flux_Err_SPIRE_350)uJystat.errorfloatnullablee_F500um[374/4807]? F500um uncertainty (Flux_Err_SPIRE_500)uJystat.errorfloatnullableSFRtot[-1.1e+17/2.6e+43]? Best estimate of the total SFR (SFR_ladder_total) (2)solMass/yrphys.SFRdoublenullablebeta[-2.5/81.7]? UV slope, {beta}_UV_stat.fit.paramdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/41457] Identifiermeta.id;meta.mainintzbest[0/10.01]? Photometric redshift used in the IR SED fitting, corresponds to zbest in the redshift catalogsrc.redshift;pos.heliocentricfloatnullableF24um[14/9639]? Spitzer/MIPS 24um flux (Flux_MIPS24) (1)uJyphot.flux.density;em.IR.15-30umdoublenullableF70um[980/153570]? Spitzer/MIPS 70um flux (Flux_MIPS70)uJyphot.flux.density;em.IR.30-60umdoublenullableF160um[26790/31244]? Spitzer/MIPS 160um flux (only for COSMOS) (Flux_MIPS160)uJyphot.flux.density;em.mm.1500-3000GHzfloatnullableF100umP[203/207880]? Herschel/PACS 100um flux (Flux_PACS_100)uJyphot.flux.density;em.IR.60-100umdoublenullableF160umP[687/224810]? Herschel/PACS 160um flux (Flux_PACS_160)uJyphot.flux.density;em.mm.1500-3000GHzdoublenullableF250um[2309/130160]? Herschel/SPIRE 250um flux (Flux_SPIRE_250)uJyphot.flux.density;em.mm.750-1500GHzdoublenullableLType[1/3] Type of SFR indicators used in SFRtot (SFR_ladder_type) (3)meta.codeintUVcor[-1.1e+17/2.6e+43]? UV-based star formation rate corrected for extinction (SFR_UV_corr) (4)solMass/yrphys.SFRdoublenullablee_UVcor[2.1e-8/3.7e+43]? UVcor uncertainty (SFR_UV_corr_Error)solMass/yrstat.errordoublenullableSFR-IR[-2020/15562] IR-based star formation rate (5)solMass/yrphys.SFRdoubleSFR-UV160[-6.9e+16/8.7e+17]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 160nm (SFR_UV_obs_160)solMass/yrphys.SFRdoublenullableSFR-UV280[-1.5e+17/1.8e+18]? UV-based star formation rate not corrected for extinction determined from the UV luminosity at 280nm (SFR_UV_obs_280)solMass/yrphys.SFRdoublenullableAuv160[0.08/97]? UV attenuation derived from the IRX-{beta}_UV_ calibration for SFR-UV160 (A_UV_160)magphys.absorptionfloatnullableSFR-UVc160[-6.9e+16/5.2e+43]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 160nm (SFR_UV_corr_160)solMass/yrphys.SFRdoublenullableSFR-UVc280[-1.5e+17/3.6e+33]? UV-based star formation rate corrected for extinction using the IRX-{beta}_UV_ relations determined from the UV luminosity at 280nm (SFR_UV_corr_280)solMass/yrphys.SFRdoublenullableSFR-IRw11[-2019/23460] IR-based star formation rate derived from the MIPS 24um flux following Calzetti+ (2000ApJ...533..682C) (SFR_IR_W11)solMass/yrphys.SFRdouble