J/ApJS/262/15ivo://CDS.VizieR/J/ApJS/262/15CDSZou F.Brandt W.N.Chen C.-T.Leja J.Ni Q.Yan W.Yang G.Zhu S.,Luo B.Nyland K.Vito F.Xue Y.2025-06-02T07:05:25Z2025-05-21T15:23:14ZCDS support team

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

cds-question@unistra.frgalaxiescatalogssurveystwo-color-diagramsultraviolet-astronomyvisible-astronomyinfrared-astronomyactive-galactic-nucleix-ray-sourcesredshiftedW-CDF-S, ELAIS-S1, and XMM-LSS will be three Deep-Drilling Fields (DDFs) of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), but their extensive multiwavelength data have not been fully utilized as done in the COSMOS field, another LSST DDF. To prepare for future science, we fit source spectral energy distributions (SEDs) from X-ray to far-infrared in these three fields mainly to derive galaxy stellar masses and star formation rates. We use CIGALE v2022.0, a code that has been regularly developed and evaluated, for the SED fitting. Our catalog includes 0.8 million sources covering 4.9deg^2^ in W-CDF-S, 0.8 million sources covering 3.4deg^2^ in ELAIS-S1, and 1.2 million sources covering 4.9deg^2^ in XMM-LSS. Besides fitting normal galaxies, we also select candidates that may host active galactic nuclei (AGNs) or are experiencing recent star formation variations and use models specifically designed for these sources to fit their SEDs; this increases the utility of our catalog for various projects in the future. We calibrate our measurements by comparison with those in well-studied smaller regions and briefly discuss the implications of our results. We also perform detailed tests of the completeness and purity of SED-selected AGNs. Our data can be retrieved from a public website.2022ApJS..262...15Zhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/15CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/317 : The CFHTLS Survey (T0007 release) (Hudelot+ 2012)III/334 : VISTA Deep Extragalactic Observations (VIDEO) (Jarvis+, 2013)II/335 : Revised cat. of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)I/350 : Gaia EDR3 (Gaia Collaboration, 2020)II/371 : The Dark Energy Survey (DES): Data Release 2 (Abbott+, 2021)VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)J/A+A/451/881 : ESIS BVR catalog, ELAIS-S1 (Berta+, 2006)J/AJ/133/186 : Opt. spectroscopy of 77 luminous AGNs and QSOs (Lacy+, 2007)J/ApJS/187/560 : Photometric redshifts of the 2Ms CDF-S (Luo+, 2010)J/ApJ/759/139 : Herschel + MIPS phot. of GOODS sources (Kirkpatrick+, 2012)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/790/54 : AGN models according to a UV to Mid-IR study (Chung+, 2014)J/ApJ/807/129 : X-ray to MIR luminosities relation of AGNs (Stern, 2015)J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)J/ApJ/825/7 : Evolution of ~6Ms CDF-S galaxies (Lehmer+, 2016)J/ApJS/228/2 : Chandra Deep Field-South survey: 7Ms sources (Luo+, 2017)J/ApJS/230/9 : Improved multi-band photometry from SERVS (Nyland+, 2017)J/MNRAS/478/2132 : XMM-LSS field. New XMM-Newton PSC (Cheng+, 2018)J/ApJ/868/99 : Post-starburst galaxies from surveys (French+, 2018)J/ApJS/236/48 : The Chandra UDS survey (X-UDS) (Kocevski+, 2018)J/MNRAS/480/1022 : Black-hole growth and cosmic environment (Yang+, 2018)J/ApJ/877/5 : Chandra DF obscured & Compton-thick AGNs. I. (Li+, 2019)J/ApJS/240/5 : SHELA. II. DECam and IRAC multiwavelength cat. (Wold+, 2019)J/ApJ/878/11 : Type 1 vs 2 X-ray COSMOS AGNs & environment (Zou+, 2019)J/MNRAS/492/1887 : Physical properties of the CDFS X-ray sources (Guo+, 2020)J/MNRAS/495/1853 : SED-selected AGN in the VIPERS field (Pouliasis+, 2020)J/MNRAS/496/245 : L_x_-L_uv_-L_radio_ relation in radio-loud QSOs (Zhu+, 2020)J/A+A/654/A93 : Polar dust obscuration in broad-line AGN (Buat+, 2021)J/ApJS/256/21 : XMM-SERVS survey: W-CDF-S & ELAIS-S1 (Ni+, 2021)J/MNRAS/503/2583 : Survey for z< 0.04 CLAGNs (Senarath+, 2021)J/MNRAS/509/2150 : MIGHTEE catalogues of COSMOS/XMM-LSS fields (Heywood+, 2022)J/MNRAS/510/687 : Viewing angle in AGN SED models (Ramos Padilla+, 2022)J/ApJS/258/11 : The COSMOS2020 catalog (Weaver+, 2022)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/262/15https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/262/15http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/262/15https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/262/15https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/262/15http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/262/15GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/262/15/es1_v1 (*ELAIS-S1 SED-fitting results)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/262/15/es1_v1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/262/15/es1_v1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/262/15/es1_v1?GETtext/xml+votable180.050000true9.7101806-44.03439070.005555555555555556Cone search capability for table J/ApJS/262/15/wcdfs_v1 (*W-CDF-S SED-fitting results)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/262/15/wcdfs_v1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/262/15/wcdfs_v1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/262/15/wcdfs_v1?GETtext/xml+votable180.050000true53.8470039-28.72562790.005555555555555556Cone search capability for table J/ApJS/262/15/xmmlss_v1 (*XMM-LSS SED-fitting results)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/262/15/xmmlss_v1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/262/15/xmmlss_v1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/262/15/xmmlss_v1?GETtext/xml+votable180.050000true36.9227295-5.47579050.0055555555555555565/4422 8847 8983 8989 6/17677 17679 17681-17683 17686 17692-17694 17712-17713 35379-35380 35382-35383 35385 35387 35473 35476 35931 35953 36104 36106 36128https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/262/15?format=asciiX-rayUVOpticalInfrareddefaultJ/ApJS/262/15/es1_v1*ELAIS-S1 SED-fitting resultsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordinte_SFRagn[2.3e-08/2950]? SFRagn uncertainty (SFR_agn_err)solMass/yrstat.error;phys.SFRdoublenullableU-Vgal[-0.31/4.5]? Rest-frame U-V color using the galaxy templates (U_V_gal)magstat.error;phot.color;em.optfloatnullablee_U-Vgal[6.5e-06/1.7]? U-Vgal uncertainty (U_V_gal_err)magstat.error;phot.color;em.opt.UdoublenullablefracAGN[0/0.99]? AGN fractions (fracagn) (G13)meta.numberdoublenullableID[644246429973/644247287328] Unique source identifier (Tractor_ID) (G1)meta.id;meta.mainindexedRAJ2000[8.37/10.54] Right ascension (J2000) (RA) (G2)degpos.eq.ra;meta.mainindexedDEJ2000[-45.15/-42.8] Declination (J2000) (DEC) (G2)degpos.eq.dec;meta.mainindexedz[0/5.961]? Redshift (redshift)src.redshiftfloatnullableb_zphot[-1/5.87]? 68% lower limit of photo-z (-1 if zspec) (zphot_lowlim)stat.min;src.redshift.photdoublenullableB_zphot[-1/5.96]? 68% upper limit of photo-z (-1 if zspec) (zphot_upplim)stat.max;src.redshift.photdoublenullableStar[0/1] 1:the source is a star; or "0" (flag_star)meta.codeintxAGN[-1/1] 1: the source is an X-ray AGN (flag_Xrayagn) (G3)meta.codeintirAGNS05[-1/1] IR AGN satisfying S05 criteria (flag_IRagn_S05) (G4)meta.codeintirAGNL07[-1/1] IR AGN satisfying L07 criteria (flag_IRagn_L07) (G5)meta.codeintirAGND12[-1/1] IR AGN satisfying D12 criteria (flag_IRagn_D12) (G6)meta.codeintAGN[0/1] Whether this source is a reliable SED AGN (flag_reliablesedagn) (G7)meta.codeintdelB1agn[-9.8/432.4]? {Delta}BIC_1_ (AGN) (detBIC1_agn) (G8)stat.fit.chi2doublenullabledelB2agn[-226/378.3]? {Delta}BIC_2_ (AGN) (detBIC2_agn) (G8)stat.fit.chi2doublenullabledelB1bqg[-11.4/281.4]? {Delta}BIC_1_ (BQ) (detBIC1_bqgal) (G9)stat.fit.chi2doublenullabledelB2bqg[-41/79]? {Delta}BIC_2_ (BQ) (detBIC2_bqgal) (G9)stat.fit.chi2doublenullablerchi2gal[1e-05/40]? Best-fit {chi}_r_^2^ values using normal-galaxy templates (redchi2_gal)stat.fit.chi2doublenullablerchi2agn[0.03/38.2]? Best-fit {chi}_r_^2^ values using AGN templates (redchi2_agn) (G10)stat.fit.chi2floatnullablerchi2bqg[0.001/38.5]? Best-fit {chi}_r_^2^ values using BQ-galaxy templates (redchi2_agn) (redchi2_bqgal)stat.fit.chi2floatnullablerchi2best[1e-05/36]? Adopted best-fit {chi}_r_^2^ values, see Section 3.5 (redchi2_best)stat.fit.chi2doublenullableMsgal[196/1.7e+14]? Stellar mass using normal-galaxy templates (Mstar_gal)solMassphys.massdoublenullablee_Msgal[272/1.2e+16]? Msgal uncertainty (Mstar_gal_err)solMassstat.error;phys.massdoublenullableMsagn[989/2.7e+13]? Stellar mass using AGN templates (Mstar_agn)solMassphys.massdoublenullablee_Msagn[786/6.7e+15]? Msagn uncertainty (Mstar_agn_err)solMassstat.error;phys.massdoublenullableMsbqg[280/1.6e+14]? Stellar mass using BQ-galaxy templates (Mstar_bqgal)solMassphys.massdoublenullablee_Msbqg[186/7.7e+15]? Msbqg uncertainty (Mstar_bqgal_err)solMassstat.error;phys.massdoublenullableMsbest[280/2.7e+13]? Adopted best-fit stellar mass (Mstar_best)solMassphys.massdoublenullablee_Msbest[186/1.2e+16]? Msbest uncertainty (Mstar_best_err)solMassstat.error;phys.massdoublenullablelogMserr[0/40784]? Additional error of logM* from photo-z uncertainties, see Section 4.9 (logMstar_err_from_zphot) (G11)solMassphys.massdoublenullablelogMsnew[4.8/17.5]? The corrected logM_*_ derived from Equation 23 (logMstar_new) (G12)solMassphys.massfloatnullableSFRgal[9.9e-11/131879]? Star formation rate using normal-galaxy templates (SFR_gal)solMass/yrphys.SFRdoublenullablee_SFRgal[5.6e-09/87206]? SFRgal uncertainty (SFR_gal_err)solMass/yrstat.error;phys.SFRdoublenullableSFRagn[1.5e-07/4601]? Star formation rate using AGN templates (SFR_agn)solMass/yrphys.SFRdoublenullableSFRbqg[1.8e-11/51137]? Star formation rate using BQ-galaxy templates (SFR_bqgal)solMass/yrphys.SFRdoublenullablee_SFRbqg[1.3e-08/34763]? SFRbqg uncertainty (SFR_bqgal_err)solMass/yrstat.error;phys.SFRdoublenullableSFRbest[6.9e-09/17178]? Adopted best-fit SFR (SFR_best)solMass/yrphys.SFRdoublenullablee_SFRbest[2.6e-08/4677]? SFRbest uncertainty (SFR_best_err)solMass/yrstat.error;phys.SFRdoublenullablelogSFRerr[0/0.93]? Additional error of SFR from photo-z uncertainties, see Section 4.9 (logSFR_err_from_zphot)solMass/yrphys.SFRfloatnullablelogSFRnew[-3.03/27.85]? The corrected SFR derived from Equation 23 (logSFR_new) (G11)solMass/yrphys.SFRfloatnullableSFRfir[0.007/54014]? The original, uncorrected FIR-based SFRs (SFR_FIR)solMass/yrphys.SFRdoublenullableSFRfirnew[-26201/24918]? The corrected FIR-based SFRs based on Equation (25) (SFR_FIR_new)solMass/yrphys.SFRdoublenullableV-Jgal[-0.62/5]? Rest-frame V-J color using the galaxy templates (V_J_gal)magphot.color;em.opt.V;em.IR.Jfloatnullablee_V-Jgal[4.4e-06/2.6]? V-Jgal uncertainty (V_J_gal_err)magstat.error;phot.color;em.opt.VdoublenullableFUV-Vgal[-0.8/12.8]? Rest-frame FUV-V color using the galaxy templates (FUV_V_gal)magphot.color;em.UV.100-200nm;em.opt.Vfloatnullablee_FUV-Vgal[3.9e-05/5.2]? FUV-Vgal uncertainty (FUV_V_gal_err)magstat.error;phot.color;em.UV.100-200nmdoublenullablee_fracAGN[0/0.5]? fracAGN uncertainty (fracagn_err)stat.error;meta.numberdoublenullablelogL6um[40/47]? The decomposed best-fit AGN rest-frame 6um luminosity (logL_6um_AGN)log(1e-07W)phys.luminosity;em.IR.4-8umfloatnullablerSFR[3.5e-09/97.2] Reduced SFR in Equation 21 (rSFR) (G14)solMass/yrphys.SFRdoublee_rSFR[0.0002/46.2]? rSFR uncertainty (rSFR_err)solMass/yrstat.error;phys.SFRfloatnullableNgood[0/27]? The number of bands with S/N>5, as defined in Section 4.8 (ngoodband)meta.numberfloatnullablen_zType of the redshift ("zphot" or "zspec") (ztype)meta.notecharJ/ApJS/262/15/wcdfs_v1*W-CDF-S SED-fitting resultsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/804420] Unique source identifier (Tractor_ID) (G1)meta.id;meta.mainintindexedRAJ2000[51.68/54.63] Right ascension (J2000) (RA) (G2)degpos.eq.ra;meta.mainindexedDEJ2000[-29.24/-26.96] Declination (J2000) (DEC) (G2)degpos.eq.dec;meta.mainindexedz[0/5.961]? Redshift (redshift)src.redshiftfloatnullableb_zphot[-1/5.869]? 68% lower limit of photo-z (-1 if zspec) (zphot_lowlim)stat.min;src.redshift.photdoublenullableB_zphot[-1/5.955]? 68% upper limit of photo-z (-1 if zspec) (zphot_upplim)stat.max;src.redshift.photdoublenullableStar[0/1] 1:the source is a star; or "0" (flag_star)meta.codeintxAGN[-1/1] 1: the source is an X-ray AGN (flag_Xrayagn) (G3)meta.codeintirAGNS05[-1/1] IR AGN satisfying S05 criteria (flag_IRagn_S05) (G4)meta.codeintirAGNL07[-1/1] IR AGN satisfying L07 criteria (flag_IRagn_L07) (G5)meta.codeintirAGND12[-1/1] IR AGN satisfying D12 criteria (flag_IRagn_D12) (G6)meta.codeintAGN[0/1] Whether this source is a reliable SED AGN (flag_reliablesedagn) (G7)meta.codeintdelB1agn[-9.7/399.1]? {Delta}BIC_1_ (AGN) (detBIC1_agn) (G8)stat.fit.chi2doublenullabledelB2agn[-389.5/355.7]? {Delta}BIC_2_ (AGN) (detBIC2_agn) (G8)stat.fit.chi2doublenullabledelB1bqg[-13.92/154.2]? {Delta}BIC_1_ (BQ) (detBIC1_bqgal) (G9)stat.fit.chi2doublenullabledelB2bqg[-40.9/167.8]? {Delta}BIC_2_ (BQ) (detBIC2_bqgal) (G9)stat.fit.chi2doublenullablerchi2gal[0/47.1]? Best-fit {chi}_r_^2^ values using normal-galaxy templates (redchi2_gal)stat.fit.chi2doublenullablerchi2agn[0.005/50.6]? Best-fit {chi}_r_^2^ values using AGN templates (redchi2_agn) (G10)stat.fit.chi2floatnullablerchi2bqg[0.0027/39]? Best-fit {chi}_r_^2^ values using BQ-galaxy templates (redchi2_agn) (redchi2_bqgal)stat.fit.chi2floatnullablerchi2best[0/51]? Adopted best-fit {chi}_r_^2^ values, see Section 3.5 (redchi2_best)stat.fit.chi2doublenullableMsgal[1.4/6.9e+14]? Stellar mass using normal-galaxy templates (Mstar_gal)solMassphys.massdoublenullablee_Msgal[3.5/1.2e+14]? Msgal uncertainty (Mstar_gal_err)solMassstat.error;phys.massdoublenullableMsagn[1180/5.1e+14]? Stellar mass using AGN templates (Mstar_agn)solMassphys.massdoublenullablee_Msagn[2447/3.1e+13]? Msagn uncertainty (Mstar_agn_err)solMassstat.error;phys.massdoublenullableMsbqg[1690/7.5e+14]? Stellar mass using BQ-galaxy templates (Mstar_bqgal)solMassphys.massdoublenullablee_Msbqg[1421/1.7e+14]? Msbqg uncertainty (Mstar_bqgal_err)solMassstat.error;phys.massdoublenullableMsbest[364.8/3.5e+13]? Adopted best-fit stellar mass (Mstar_best)solMassphys.massdoublenullablee_Msbest[713/6.92e+12]? Msbest uncertainty (Mstar_best_err)solMassstat.error;phys.massdoublenullablelogMserr[0/1.93]? Additional error of logM* from photo-z uncertainties, see Section 4.9 (logMstar_err_from_zphot) (G11)solMassphys.massdoublenullablelogMsnew[5/17.67]? The corrected logM_*_ derived from Equation 23 (logMstar_new) (G12)solMassphys.massfloatnullableSFRgal[1.3e-11/652867]? Star formation rate using normal-galaxy templates (SFR_gal)solMass/yrphys.SFRdoublenullablee_SFRgal[4.5e-10/95148]? SFRgal uncertainty (SFR_gal_err)solMass/yrstat.error;phys.SFRdoublenullableSFRagn[3.6e-09/20810]? Star formation rate using AGN templates (SFR_agn)solMass/yrphys.SFRdoublenullablee_SFRagn[1.9e-07/5759]? SFRagn uncertainty (SFR_agn_err)solMass/yrstat.error;phys.SFRdoublenullableSFRbqg[9.1e-13/662750]? Star formation rate using BQ-galaxy templates (SFR_bqgal)solMass/yrphys.SFRdoublenullablee_SFRbqg[2.5e-09/87330]? SFRbqg uncertainty (SFR_bqgal_err)solMass/yrstat.error;phys.SFRdoublenullableSFRbest[9.19e-13/72905]? Adopted best-fit SFR (SFR_best)solMass/yrphys.SFRdoublenullablee_SFRbest[5e-07/21405]? SFRbest uncertainty (SFR_best_err)solMass/yrstat.error;phys.SFRdoublenullablelogSFRerr[0/4.91]? Additional error of SFR from photo-z uncertainties, see Section 4.9 (logSFR_err_from_zphot)solMass/yrphys.SFRfloatnullablelogSFRnew[-4.96/283]? The corrected SFR derived from Equation 23 (logSFR_new) (G11)solMass/yrphys.SFRdoublenullableSFRfir[0.003/13869]? The original, uncorrected FIR-based SFRs (SFR_FIR)solMass/yrphys.SFRdoublenullableSFRfirnew[-4551/11366]? The corrected FIR-based SFRs based on Equation (25) (SFR_FIR_new)solMass/yrphys.SFRdoublenullableV-Jgal[-0.62/5.7]? Rest-frame V-J color using the galaxy templates (V_J_gal)magphot.color;em.opt.V;em.IR.Jfloatnullablee_V-Jgal[3.1e-08/3]? V-Jgal uncertainty (V_J_gal_err)magstat.error;phot.color;em.opt.VdoublenullableU-Vgal[-0.31/5.5]? Rest-frame U-V color using the galaxy templates (U_V_gal)magstat.error;phot.color;em.optfloatnullablee_U-Vgal[6.6e-08/2.6]? U-Vgal uncertainty (U_V_gal_err)magstat.error;phot.color;em.opt.UdoublenullableFUV-Vgal[-0.8/14.7]? Rest-frame FUV-V color using the galaxy templates (FUV_V_gal)magphot.color;em.UV.100-200nm;em.opt.Vfloatnullablee_FUV-Vgal[1.4e-07/6.7]? FUV-Vgal uncertainty (FUV_V_gal_err)magstat.error;phot.color;em.UV.100-200nmdoublenullablefracAGN[0/0.99]? AGN fractions (fracagn) (G13)meta.numberdoublenullablee_fracAGN[0/0.5]? fracAGN uncertainty (fracagn_err)stat.error;meta.numberdoublenullablelogL6um[39.96/47.3]? The decomposed best-fit AGN rest-frame 6um luminosity (logL_6um_AGN)log(1e-07W)phys.luminosity;em.IR.4-8umfloatnullablerSFR[5.7e-14/98.1] Reduced SFR in Equation 21 (rSFR) (G14)solMass/yrphys.SFRdoublee_rSFR[0/47.2]? rSFR uncertainty (rSFR_err)solMass/yrstat.error;phys.SFRfloatnullableNgood[0/25]? The number of bands with S/N>5, as defined in Section 4.8 (ngoodband)meta.numberfloatnullablen_zType of the redshift ("zphot" or "zspec") (ztype)meta.notecharJ/ApJS/262/15/xmmlss_v1*XMM-LSS SED-fitting resultsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/1247954] Unique source identifier (Tractor_ID) (G1)meta.id;meta.mainintindexedRAJ2000[33.9/37.2] Right ascension (J2000) (RA) (G2)degpos.eq.ra;meta.mainindexedDEJ2000[-5.7/-3.98] Declination (J2000) (DEC) (G2)degpos.eq.dec;meta.mainindexedz[0/9.999]? Redshift (redshift)src.redshiftfloatnullableb_zphot[-99/5.869]? 68% lower limit of photo-z (-1 if zspec) (zphot_lowlim)stat.min;src.redshift.photfloatnullableB_zphot[-99/5.955]? 68% upper limit of photo-z (-1 if zspec) (zphot_upplim)stat.max;src.redshift.photfloatnullableStar[0/1] 1:the source is a star; or "0" (flag_star)meta.codeintxAGN[-1/1] 1: the source is an X-ray AGN (flag_Xrayagn) (G3)meta.codeintirAGNS05[-1/1] IR AGN satisfying S05 criteria (flag_IRagn_S05) (G4)meta.codeintirAGNL07[-1/1] IR AGN satisfying L07 criteria (flag_IRagn_L07) (G5)meta.codeintirAGND12[-1/1] IR AGN satisfying D12 criteria (flag_IRagn_D12) (G6)meta.codeintAGN[0/1] Whether this source is a reliable SED AGN (flag_reliablesedagn) (G7)meta.codeintdelB1agn[-10/424]? {Delta}BIC_1_ (AGN) (detBIC1_agn) (G8)stat.fit.chi2doublenullabledelB2agn[-454/362]? {Delta}BIC_2_ (AGN) (detBIC2_agn) (G8)stat.fit.chi2doublenullabledelB1bqg[-21.13/622]? {Delta}BIC_1_ (BQ) (detBIC1_bqgal) (G9)stat.fit.chi2doublenullabledelB2bqg[-57/199]? {Delta}BIC_2_ (BQ) (detBIC2_bqgal) (G9)stat.fit.chi2doublenullablerchi2gal[0/55]? Best-fit {chi}_r_^2^ values using normal-galaxy templates (redchi2_gal)stat.fit.chi2doublenullablerchi2agn[0.009/41]? Best-fit {chi}_r_^2^ values using AGN templates (redchi2_agn) (G10)stat.fit.chi2floatnullablerchi2bqg[0.0002/34]? Best-fit {chi}_r_^2^ values using BQ-galaxy templates (redchi2_agn) (redchi2_bqgal)stat.fit.chi2floatnullablerchi2best[0/55]? Adopted best-fit {chi}_r_^2^ values, see Section 3.5 (redchi2_best)stat.fit.chi2doublenullableMsgal[0.19/1.94e+15]? Stellar mass using normal-galaxy templates (Mstar_gal)solMassphys.massdoublenullablee_Msgal[0.02/3.3e+17]? Msgal uncertainty (Mstar_gal_err)solMassstat.error;phys.massdoublenullableMsagn[3.4/5e+14]? Stellar mass using AGN templates (Mstar_agn)solMassphys.massdoublenullablee_Msagn[0.17/9.9e+16]? Msagn uncertainty (Mstar_agn_err)solMassstat.error;phys.massdoublenullableMsbqg[35.68/6.6e+14]? Stellar mass using BQ-galaxy templates (Mstar_bqgal)solMassphys.massdoublenullablee_Msbqg[8/2.95e+17]? Msbqg uncertainty (Mstar_bqgal_err)solMassstat.error;phys.massdoublenullableMsbest[1.38/2.6e+14]? Adopted best-fit stellar mass (Mstar_best)solMassphys.massdoublenullablee_Msbest[0.06/2.7e+15]? Msbest uncertainty (Mstar_best_err)solMassstat.error;phys.massdoublenullablelogMserr[0/716]? Additional error of logM* from photo-z uncertainties, see Section 4.9 (logMstar_err_from_zphot) (G11)solMassphys.massdoublenullablelogMsnew[-2.1/33.6]? The corrected logM_*_ derived from Equation E2 (logMstar_new) (G12)solMassphys.massfloatnullableSFRgal[5.4e-16/123460]? Star formation rate using normal-galaxy templates (SFR_gal)solMass/yrphys.SFRdoublenullablee_SFRgal[8.2e-15/3.2e+06]? SFRgal uncertainty (SFR_gal_err)solMass/yrstat.error;phys.SFRdoublenullableSFRagn[1.5e-17/64130]? Star formation rate using AGN templates (SFR_agn)solMass/yrphys.SFRdoublenullablee_SFRagn[3.7e-15/1.5e+06]? SFRagn uncertainty (SFR_agn_err)solMass/yrstat.error;phys.SFRdoublenullableSFRbqg[9.2e-15/30804]? Star formation rate using BQ-galaxy templates (SFR_bqgal)solMass/yrphys.SFRdoublenullablee_SFRbqg[1.9e-11/3.8e+06]? SFRbqg uncertainty (SFR_bqgal_err)solMass/yrstat.error;phys.SFRdoublenullableSFRbest[6e-16/16407]? Adopted best-fit SFR (SFR_best)solMass/yrphys.SFRdoublenullablee_SFRbest[8.2e-15/796004]? SFRbest uncertainty (SFR_best_err)solMass/yrstat.error;phys.SFRdoublenullablelogSFRerr[0/398]? Additional error of SFR from photo-z uncertainties, see Section 4.9 (logSFR_err_from_zphot)solMass/yrphys.SFRdoublenullablelogSFRnew[-5.4/108]? The corrected SFR derived from Equation E2 (logSFR_new) (G13)solMass/yrphys.SFRdoublenullableSFRfir[8.9e-11/106350]? The original, uncorrected FIR-based SFRs (SFR_FIR)solMass/yrphys.SFRdoublenullableSFRfirnew[-4277/28087]? The corrected FIR-based SFRs based on Equation (25) (SFR_FIR_new)solMass/yrphys.SFRdoublenullableV-Jgal[-0.9/5.7]? Rest-frame V-J color using the galaxy templates (V_J_gal)magphot.color;em.opt.V;em.IR.Jfloatnullablee_V-Jgal[0/2.1]? V-Jgal uncertainty (V_J_gal_err)magstat.error;phot.color;em.opt.VdoublenullableU-Vgal[-0.2/5.4]? Rest-frame U-V color using the galaxy templates (U_V_gal)magstat.error;phot.color;em.optfloatnullablee_U-Vgal[0/1.8]? U-Vgal uncertainty (U_V_gal_err)magstat.error;phot.color;em.opt.UdoublenullableFUV-Vgal[-0.6/14.1]? Rest-frame FUV-V color using the galaxy templates (FUV_V_gal)magphot.color;em.UV.100-200nm;em.opt.Vfloatnullablee_FUV-Vgal[0/5.2]? FUV-Vgal uncertainty (FUV_V_gal_err)magstat.error;phot.color;em.UV.100-200nmdoublenullablefracAGN[0/0.99]? AGN fractions (fracagn) (G13)meta.numberdoublenullablee_fracAGN[0/0.5]? fracAGN uncertainty (fracagn_err)stat.error;meta.numberdoublenullablelogL6um[40/47.3]? The decomposed best-fit AGN rest-frame 6um luminosity (logL_6um_AGN)log(1e-07W)phys.luminosity;em.IR.4-8umfloatnullablerSFR[3e-44/100] Reduced SFR in Equation 21 (rSFR) (G14)solMass/yrphys.SFRdoublee_rSFR[0/48]? rSFR uncertainty (rSFR_err)solMass/yrstat.error;phys.SFRfloatnullableNgood[0/28]? The number of bands with S/N>5, as defined in Section 4.8 (ngoodband)meta.numberfloatnullableC18Display data from Cheng+ 2018, J/MNRAS/478/2132 within 0.5" if anymeta.ref.urlintnullablen_zType of the redshift ("zphot" or "zspec") (ztype)meta.notechar