J/A+A/648/A4ivo://CDS.VizieR/J/A+A/648/A4doi:10.26093/cds/vizier.36480004CDSDuncan K.J.Kondapally R.Brown M.J.I.Bonato M.Best P.N.,Roettgering H.J.A.Bondi M.Bowler R.A.A.Cochrane R.K.Guerkan G.,Hardcastle M.J.Jarvis M.J.Kunert-Bajraszewska M.Leslie S.K.Malek K.,Morabito L.K.O'Sullivan S.P.Prandoni I.Sabater J.Shimwell T.W.,Smith D.J.B.Wang L.Wolowska A.2021-09-16T09:59:48Z2021-04-07T12:50:29ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryradio-galaxiesredshiftedThe Low Frequency Array (LOFAR) Two-metre Sky Survey (LoTSS) is a sensitive, high-resolution 120-168MHz survey split across multiple tiers over the northern sky. The first LoTSS Deep Fields data release consists of deep radio continuum imaging at 150 MHz of the Bootes, European Large Area Infrared Space Observatory Survey-North 1 (ELAIS-N1), and Lockman Hole fields, down to rms sensitivities of ~32, 20, and 22 muJy/beam, respectively. In this paper we present consistent photometric redshift (photo-z) estimates for the optical source catalogues in all three fields - totalling over 7 million sources (~5 million after limiting to regions with the best photometric coverage). Our photo-z estimation uses a hybrid methodology that combines template fitting and machine learning and is optimised to produce the best possible performance for the radio continuum selected sources and the wider optical source population. Comparing our results with spectroscopic redshift samples, we find a robust scatter ranging from 1.6 to 2% for galaxies and 6.4 to 7% for identified optical, infrared, or X-ray selected active galactic nuclei (AGN). Our estimated outlier fractions (|z_phot-z_spec|/(1+z_spec)>0.15) for the corresponding subsets range from 1.5 to 1.8% and 18 to 22%, respectively. Replicating trends seen in analyses of previous wide-area radio surveys, we find no strong trend in photo-$z$ quality as a function of radio luminosity for a fixed redshift. We exploit the broad wavelength coverage available within each field to produce galaxy stellar mass estimates for all optical sources at z<1.5. Stellar mass functions derived for each field are used to validate our mass estimates, with the resulting estimates in good agreement between each field and with published results from the literature.2021A&A...648A...4Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/648/A4CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/648/A2 : LOFAR Two-metre Sky Survey Deep Fields DR1 (Sabater+, 2021)J/A+A/648/A3 : LOFAR Two-metre Sky Survey Deep Fields DR1 (Kondapally+, 2021)J/A+A/648/A9 : Lockman Hole Apertif map at 1.4GHz (Morganti+, 2021)https://lofar-surveys.org/releases.html : LOFAR Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/648/A4https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/648/A4http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/648/A4https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/648/A4https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/648/A4http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/648/A4GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/648/A4/bootes (Bootes Field Photometric redshift catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/648/A4/bootes?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/648/A4/bootes?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/648/A4/bootes?GETtext/xml+votable180.050000true216.47386332.28259630.005555555555555556Cone search capability for table J/A+A/648/A4/en1 (ELAIS-N1 Photometric redshift catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/648/A4/en1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/648/A4/en1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/648/A4/en1?GETtext/xml+votable180.050000true242.80436433930653.154941701475010.005555555555555556Cone search capability for table J/A+A/648/A4/lockman (Lockman Hole photometric redshift catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/648/A4/lockman?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/648/A4/lockman?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/648/A4/lockman?GETtext/xml+votable180.050000true164.48053950361955.880103208947010.0055555555555555564/379 5/1522 1528 2286-2287 2537-2539 2628-2629 2880 6/6045-6047 6082 6120-6122 7441 7443-7446 9135 9194 9983 10145-10147 10162 10501 10521 10524 10560 11349 11351 11524-11526https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/648/A4?format=asciiRadiodefaultJ/A+A/648/A4/bootesBootes Field Photometric redshift catalogueXrayAGN[0/1] Source has X-ray counterpartmeta.codeintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDUnique object identifier for multi-wavelength catalogue in this fieldmeta.id;meta.mainintIDOptIdentifier for the optical-NIR detected chi2 catalogue (ID_OPTICAL)meta.idintIDSpitzer? Identifier for the Spitzer detected chi2 catalogue (ID_SPITZER)meta.idintnullableRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (DEC)degpos.eq.dec;meta.mainindexedE(B-V)E(B-V) galactic extinction for the source based on its position and Schlegel+(1998ApJ...500..525S)phot.color.excessfloatClassStellarity Parameter (CLASSSTAR)src.class.starGalaxydoubleoverlap[0/1] Bit flag indicating the multi-wavelength coverage (FLAGOVERLAP)meta.codeintclean[0/3] 3-valued flag indicating bright star masking (FLAGCLEAN)meta.codeintzbestBest available redshift estimate (Z_BEST)phot.mag;em.optdoublef_zbest[0/1] Source of z_best, 0 = photometric, 1 = spectroscopic (Z_BEST_SOURCE)meta.codeintzspec? Literature Spectroscopic Redshift (Z_SPEC)src.redshiftdoublenullabler_zspec? Source of the spectroscopic redshift (Z_SOURCE)meta.ref;pos.frameintnullableq_zspec? Spectroscopic redshift quality: flag Q=3 means probable, Q>=4 means reliable (Z_QUAL)meta.code.qualintnullablez1medMedian of the primary redshift peak above 80% HPD CI (z1_median)phot.mag;em.optdoublez1minLower bound of the primary 80% HPD CI peak (z1_min)phot.mag;em.optdoublez1maxUpper bound of the primary 80% HPD CI peak (z1_max)phot.mag;em.optdoublez1areaIntegrated area of the primary 80% HPD CI peak (z1_area)phys.area;instrdoublez2medMedian of the secondary redshift peak (if present) above 80% HPD CI (z2_median)phot.mag;em.optdoublez2minLower bound of the secondary 80% HPD CI peak (z2_min)phot.mag;em.optdoublez2maxUpper bound of the secondary 80% HPD CI peak (z2_max)phot.mag;em.optdoublez2areaIntegrated area of the secondary 80% HPD CI peak (z2_area)phys.area;instrdoublenfiltEazy? Number of filters included in EAZY template fit (nfilt_eazy) (G1)meta.numberintnullablenfiltAtl? Number of filters included in Atlas+AGN template fit (nfilt_atlas) (G2)meta.numberintnullablenfiltAna? Number of filters included in Ananna+ template fit (nfilt_ananna) (G3)meta.numberintnullablechirBest? Chi^2 / nfilt for best-fit galaxy/AGN template (any library) (chi_r_best)stat.fit.chi2doublenullablechirStelR? Chi^2 / nfilt for best-fit stellar template (chi_r_stellar)stat.fit.chi2doublenullableStelTypeStellar type of best-fit stellar template (stellar_type)meta.code.classcharAGN[0/1] Sources flagged by any one of optAGN/IRAGN/XrayAGNmeta.codeintoptAGN[0/1] Source is included in Million Quasar Catalog (Flesch 2015PASA...32...10F) compilation or spectroscopically identified AGNmeta.codeintIRAGN[0/1] Source satisfies Donley et al. (2012ApJ...748..142D) IR AGN criteriameta.codeintXrayFlux? XBootes Soft X-ray Flux (XrayFlux_0.5-2)W.m**-2phot.flux;em.X-raydoublenullableHRX? XBootes X-ray Hardness Ratiophot.flux;arith.ratiodoublenullableaptmz? Estimated z-band total flux correction from Legacy Surveys model flux (z) (ap_to_model_z)arith.factor;phot.fluxdoublenullablee_aptmz? Statistical uncertainty on tot_z (ap_to_model_err_z)stat.errordoublenullableaptmzS? Estimated z-band total flux correction from Legacy Surveys model flux (z_Subaru) (ap_to_model_z_Subaru)arith.factor;phot.fluxdoublenullablee_aptmzS? Statistical uncertainty on tot_z_Subaru (ap_to_model_err_z_Subaru)stat.errordoublenullablezmodel? Model grid redshift used in stellar mass fitstat.paramdoublenullablechibest? Minimum Chi^2 in stellar mass fit (for Z_BEST) (chi_best)stat.fit.chi2;phys.mass;stat.mindoublenullableMassmed? 50th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_median)log(solMass)phys.massdoublenullableMassl68? 16th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_l68)log(solMass)phys.massdoublenullableMassu68? 84th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_u68)log(solMass)phys.massdoublenullableNfilts? Number of bands included in stellar mass fitmeta.numberintnullableumag? Rest-frame u-band magnitude for best-fit SED (for Z_BEST) (u_rest)magphot.mag;em.opt.UdoublenullableBwmag? Rest-frame Bw-band magnitude for best-fit SED (for Z_BEST) (Bw_rest)magphot.mag;em.opt.BdoublenullableRmag? Rest-frame R-band magnitude for best-fit SED (for Z_BEST) (R_rest)magphot.mag;em.opt.Rdoublenullableimag? Rest-frame I-band magnitude for best-fit SED (for Z_BEST) (I_rest)magphot.mag;em.opt.Idoublenullablezmag? Rest-frame z-band magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.mag;em.opt.IdoublenullablezSmag? Rest-frame z_Subaru-band magnitude for best-fit SED (for Z_BEST) (z_Subaru_rest)magphot.mag;em.opt.Idoublenullableymag? Rest-frame y-band magnitude for best-fit SED (for Z_BEST) (y_rest)magphot.mag;em.IR.JdoublenullableJmag? Rest-frame J-band magnitude for best-fit SED (for Z_BEST) (J_rest)magphot.mag;em.IR.JdoublenullableHmag? Rest-frame H-band magnitude for best-fit SED (for Z_BEST) (H_rest)magphot.mag;em.IR.HdoublenullableKmag? Rest-frame K-band magnitude for best-fit SED (for Z_BEST) (K_rest)magphot.mag;em.IR.KdoublenullableKsmag? Rest-frame Ks-band magnitude for best-fit SED (for Z_BEST) (Ks_rest)magphot.mag;em.IR.KdoublenullableIRAC1? Rest-frame IRAC 3.6micron magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.mag;em.IR.3-4umdoublenullableIRAC2? Rest-frame IRAC 4.5micron magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.mag;em.IR.4-8umdoublenullableIRAC3? Rest-frame IRAC 5.8micron magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.flux.density;em.IR.4-8umdoublenullableIRAC4? Rest-frame IRAC 8.0micron magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.flux.density;em.IR.8-15umdoublenullableJ/A+A/648/A4/en1ELAIS-N1 Photometric redshift catalogueXrayAGN[0/1] Source has X-ray counterpartmeta.codeintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDUnique object identifier for multi-wavelength catalogue in this fieldmeta.id;meta.mainintIDOptIdentifier for the optical-NIR detected chi2 catalogue (ID_OPTICAL)meta.idintIDSpitzer? Identifier for the Spitzer detected chi2 catalogue (ID_SPITZER)meta.idintnullableRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (DEC)degpos.eq.dec;meta.mainindexedE(B-V)E(B-V) galactic extinction for the source based on its position and Schlegel et al. (1998ApJ...500..525S)magphot.color.excessfloatClassStellarity Parametersrc.class.starGalaxyfloatoverlap[0/7] Bit flag indicating the multi-wavelength coveragemeta.codeintclean[1/3] 3-valued flag indicating bright star maskingmeta.codeintzbestBest available redshift estimate (Z_BEST)phot.mag;em.optdoublef_zbest[0/1] Source of z_best, 0 = photometric, 1 = spectroscopic (Z_BEST_SOURCE)meta.codeintzspec? Literature Spectroscopic Redshift (Z_SPEC)src.redshiftdoublenullablee_zspec? Source of the spectroscopic redshift (Z_SOURCE)stat.errorintnullableq_zspec? Spectroscopic redshift quality: flag Q=3 means probable, Q>=4 means reliable (Z_QUAL)meta.code.qualintnullablez1medMedian of the primary redshift peak above 80% HPD CI (z1_median)phot.mag;em.optdoublez1minLower bound of the primary 80% HPD CI peak (z1_min)phot.mag;em.optdoublez1maxUpper bound of the primary 80% HPD CI peak (z1_max)phot.mag;em.optdoublez1areaIntegrated area of the primary 80% HPD CI peak (z1_area)phys.area;instrdoublez2medMedian of the secondary redshift peak (if present) above 80% HPD CI (z2_median)phot.mag;em.optdoublez2minLower bound of the secondary 80% HPD CI peak (z2_min)phot.mag;em.optdoublez2maxUpper bound of the secondary 80% HPD CI peak (z2_max)phot.mag;em.optdoublez2areaIntegrated area of the secondary 80% HPD CI peak (z2_area)phys.area;instrdoublenfiltEazy? Number of filters included in EAZY template fit (nfilt_eazy) (G1)meta.numberintnullablenfiltAtl? Number of filters included in Atlas+AGN template fit (nfilt_atlas) (G2)meta.numberintnullablenfiltAna? Number of filters included in Ananna+ template fit (nfilt_ananna) (G3)meta.numberintnullablechirBest? Chi^2 / nfilt for best-fit galaxy/AGN template (any library) (chi_r_best)stat.fit.chi2doublenullablechirStel? Chi^2 / nfilt for best-fit stellar template (chi_r_stellar)stat.fit.chi2doublenullableStelTypeStellar type of best-fit stellar template (stellar_type)meta.code.classcharAGN[0/1] Sources flagged by any one of optAGN/IRAGN/XrayAGNmeta.codeintoptAGN[0/1] Source is included in Million Quasar Catalog (Flesch 2015PASA...32...10F) compilation or spectroscopically identified AGNmeta.codeintIRAGN[0/1] Source satisfies Donley et al. (2012ApJ...748..142D) IR AGN criteriameta.codeint2RXSID? ID for 2RXS X-ray Catalog counterpart (G4)meta.idcharXMMSL2ID? ID for XMMSL2 X-ray Catalog counterpart (G4)meta.idcharaptmg? Estimated g-band total flux correction from Legacy Surveys model flux (g) (ap_to_model_g)arith.factor;phot.fluxdoublenullablee_aptmg? Statistical uncertainty on atpmg (ap_to_model_err_g)stat.errordoublenullableaptmr? Estimated r-band total flux correction from Legacy Surveys model flux (r) (ap_to_model_r)arith.factor;phot.fluxdoublenullablee_aptmr? Statistical uncertainty on atpmg (ap_to_model_err_r)stat.errordoublenullableaptmz? Estimated z-band total flux correction from Legacy Surveys model flux (z) (ap_to_model_z)arith.factor;phot.fluxdoublenullablee_aptmz? Statistical uncertainty on atpmg (ap_to_model_err_z)stat.errordoublenullablezmodel? Model grid redshift used in stellar mass fitstat.paramdoublenullablechibest? Minimum Chi^2 in stellar mass fit (for Z_BEST) (chi_best)stat.fit.chi2;phys.mass;stat.mindoublenullableMassmed? 50th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_median)log(solMass)phys.massdoublenullableMassl68? 16th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_l68)log(solMass)phys.massdoublenullableMassu68? 84th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_u68)log(solMass)phys.massdoublenullableNfilts? Number of bands included in stellar mass fitmeta.numberintnullableumag? Rest-frame u-band magnitude for best-fit SED (for Z_BEST) (u_rest)magphot.mag;em.opt.Udoublenullablegmag? Rest-frame g-band magnitude for best-fit SED (for Z_BEST) (g_rest)magphot.mag;em.opt.Bdoublenullablermag? Rest-frame r-band magnitude for best-fit SED (for Z_BEST) (r_rest)magphot.mag;em.opt.Rdoublenullableimag? Rest-frame i-band magnitude for best-fit SED (for Z_BEST) (i_rest)magphot.mag;em.opt.Idoublenullablezmag? Rest-frame z-band magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.mag;em.opt.Idoublenullableymag? Rest-frame y-band magnitude for best-fit SED (for Z_BEST) (y_rest)magphot.mag;em.IR.JdoublenullableJmag? Rest-frame J-band magnitude for best-fit SED (for Z_BEST) (J_rest)magphot.mag;em.IR.JdoublenullableKmag? Rest-frame K-band magnitude for best-fit SED (for Z_BEST) (K_rest)magphot.mag;em.IR.KdoublenullableIRAC1vs? Rest-frame IRAC 3.6micron magnitude for best-fit SED (for Z_BEST) (ch1_servs_rest)magphot.mag;em.IR.3-4umdoublenullableIRAC2vs? Rest-frame IRAC 4.5micron magnitude for best-fit SED (for Z_BEST) (ch2_servs_rest)magphot.mag;em.IR.4-8umdoublenullableIRAC1sw? Rest-frame IRAC 3.6micron magnitude for best-fit SED (for Z_BEST) (ch1_swire_rest)magphot.mag;em.IR.3-4umdoublenullableIRAC2sw? Rest-frame IRAC 4.5micron magnitude for best-fit SED (for Z_BEST) (ch2_swire_rest)magphot.mag;em.IR.4-8umdoublenullableIRAC3sw? Rest-frame IRAC 5.8micron magnitude for best-fit SED (for Z_BEST) (ch3_swire_rest)magphot.flux.density;em.IR.4-8umdoublenullableIRAC4sw? Rest-frame IRAC 8.0micron magnitude for best-fit SED (for Z_BEST) (ch4_swire_rest)magphot.flux.density;em.IR.8-15umdoublenullableJ/A+A/648/A4/lockmanLockman Hole photometric redshift catalogueRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDUnique object identifier for multi-wavelength catalogue in this fieldmeta.id;meta.mainintIDOptIdentifier for the optical-NIR detected chi2 catalogue (ID_OPTICAL)meta.idintIDSpitzer? Identifier for the Spitzer detected chi2 catalogue (ID_SPITZER)meta.idintnullableDEJ2000Declination (J2000) (DEC)degpos.eq.dec;meta.mainindexedE(B-V)E(B-V) galactic extinction for the source based on its position and Schlegel et al. (1998ApJ...500..525S)magphot.color.excessfloatClassStellarity Parameter (CLASSSTAR)src.class.starGalaxyfloatclean[1/3] 3-valued flag indicating bright star masking (FLAGCLEAN)meta.codeintzbest? Best available redshift estimate (Z_BEST)phot.mag;em.optdoublenullablef_zbest[0/1] Source of z_best, 0 = photometric, 1 = spectroscopic (Z_BEST_SOURCE)meta.codeintzspec? Literature Spectroscopic Redshift (Z_SPEC)src.redshiftdoublenullablez1med? Median of the primary redshift peak above 80% HPD CI (z1_median)phot.mag;em.optdoublenullablez1min? Lower bound of the primary 80% HPD CI peak (z1_min)phot.mag;em.optdoublenullablez1max? Upper bound of the primary 80% HPD CI peak (z1_max)phot.mag;em.optdoublenullablez1area? Integrated area of the primary 80% HPD CI peak (z1_area)phys.area;instrdoublenullablez2med? Median of the secondary redshift peak (if present) above 80% HPD CI (z2_median)phot.mag;em.optdoublenullablez2min? Lower bound of the secondary 80% HPD CI peak (z2_min)phot.mag;em.optdoublenullablez2max? Upper bound of the secondary 80% HPD CI peak (z2_max)phot.mag;em.optdoublenullablez2area? Integrated area of the secondary 80% HPD CI peak (z2_area)phys.area;instrdoublenullablenfiltEazy? Number of filters included in EAZY template fit (nfilt_eazy) (G1)meta.numberintnullablenfiltAtl? Number of filters included in Atlas+AGN template fit (nfilt_atlas) (G2)meta.numberintnullablenfiltAna? Number of filters included in Ananna+ template fit (nfilt_ananna) (G3)meta.numberintnullablechirBest? Chi^2 / nfilt for best-fit galaxy/AGN template (any library) (chi_r_best)stat.fit.chi2doublenullablechirStel? Chi^2 / nfilt for best-fit stellar template (chi_r_stellar)stat.fit.chi2doublenullableStelTypeStellar type of best-fit stellar template (stellar_type)meta.code.classcharAGN[0/1] Sources flagged by any one of optAGN/IRAGN/XrayAGNmeta.codeintoptAGN[0/1] Source is included in Million Quasar Catalog (Flesch 2015PASA...32...10F) compilation or spectroscopically identified AGNmeta.codeintIRAGN[0/1] Source satisfies Donley et al. (2012ApJ...748..142D) IR AGN criteriameta.codeintXrayAGN? Source has X-ray counterpartmeta.codeintnullable2RXSID? ID for 2RXS X-ray Catalog counterpartmeta.idcharXMMSL2ID? ID for XMMSL2 X-ray Catalog counterpartmeta.idcharaptmg? Estimated g-band total flux correction from Legacy Surveys model flux (g) (ap_to_model_g)arith.factor;phot.fluxdoublenullablee_aptmg? Statistical uncertainty on atpmg (ap_to_model_err_g)stat.errordoublenullableaptmr? Estimated r-band total flux correction from Legacy Surveys model flux (r) (ap_to_model_r)arith.factor;phot.fluxdoublenullablee_aptmr? Statistical uncertainty on atpmr (ap_to_model_err_r)stat.errordoublenullableaptmz? Estimated z-band total flux correction from Legacy Surveys model flux (z) (ap_to_model_z)arith.factor;phot.fluxdoublenullablee_aptmz? Statistical uncertainty on atpmz (ap_to_model_err_z)stat.errordoublenullablezmodel? Model grid redshift used in stellar mass fitstat.paramdoublenullablechibest? Minimum Chi^2 in stellar mass fit (for Z_BEST) (chi_best)stat.fit.chi2;phys.mass;stat.mindoublenullableMassmed? 50th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_median)log(solMass)phys.massdoublenullableMassl68? 16th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_l68)log(solMass)phys.massdoublenullableMassu68? 84th percentile of the marginalised stellar mass posterior (for Z_BEST) (Mass_u68)log(solMass)phys.massdoublenullableNfilts? Number of bands included in stellar mass fitmeta.numberintnullableumag? Rest-frame u-band magnitude for best-fit SED (for Z_BEST) (u_rest)magphot.mag;em.opt.Udoublenullablegmag? Rest-frame g-band magnitude for best-fit SED (for Z_BEST) (g_rest)magphot.mag;em.opt.Bdoublenullablermag? Rest-frame r-band magnitude for best-fit SED (for Z_BEST) (r_rest)magphot.mag;em.opt.Rdoublenullablezmag? Rest-frame z-band magnitude for best-fit SED (for Z_BEST) (z_rest)magphot.mag;em.opt.Idoublenullablegrcsmag? Rest-frame g_rcs-band magnitude for best-fit SED (for Z_BEST) (g_rcs_rest)magphot.mag;em.opt.Bdoublenullablerrcsmag? Rest-frame r_rcs-band magnitude for best-fit SED (for Z_BEST) (r_rcs_rest)magphot.mag;em.opt.Rdoublenullableircsmag? Rest-frame i_rcs-band magnitude for best-fit SED (for Z_BEST) (i_rcs_rest)magphot.mag;em.opt.Idoublenullablezrcsmag? Rest-frame z_rcs-band magnitude for best-fit SED (for Z_BEST) (z_rcs_rest)magphot.mag;em.opt.IdoublenullableJmag? Rest-frame J-band magnitude for best-fit SED (for Z_BEST) (J_rest)magphot.mag;em.IR.JdoublenullableKmag? Rest-frame K-band magnitude for best-fit SED (for Z_BEST) (K_rest)magphot.mag;em.IR.KdoublenullableIRAC1sv? Rest-frame IRAC 3.6micron magnitude for best-fit SED (for Z_BEST) (ch1_servs_rest)magphot.mag;em.IR.3-4umdoublenullableIRAC2sv? Rest-frame IRAC 4.5micron magnitude for best-fit SED (for Z_BEST) (ch2_servs_rest)magphot.mag;em.IR.4-8umdoublenullableIRAC1sw? Rest-frame IRAC 3.6micron magnitude for best-fit SED (for Z_BEST) (ch1_swire_rest)magphot.mag;em.IR.3-4umdoublenullableIRAC2sw? Rest-frame IRAC 4.5micron magnitude for best-fit SED (for Z_BEST) (ch2_swire_rest)magphot.mag;em.IR.4-8umdoublenullableIRAC3sw? Rest-frame IRAC 5.8micron magnitude for best-fit SED (for Z_BEST) (ch3_swire_rest)magphot.flux.density;em.IR.4-8umdoublenullableIRAC4sw? Rest-frame IRAC 8.0micron magnitude for best-fit SED (for Z_BEST) (ch4_swire_rest)magphot.flux.density;em.IR.8-15umdoublenullable