J/ApJS/229/32ivo://CDS.VizieR/J/ApJS/229/32doi:10.26093/cds/vizier.22290032CDSStefanon M.Yan H.Mobasher B.Barro G.Donley J.L.Fontana A.,Hemmati S.Koekemoer A.M.Lee B.Lee S.-K.Nayyeri H.Peth M.,Pforr J.Salvato M.Wiklind T.Wuyts S.Ashby M.L.N.Castellano M.,Conselice C.J.Cooper M.C.Cooray A.R.Dolch T.Ferguson H.,Galametz A.Giavalisco M.Guo Y.Willner S.P.Dickinson M.E.,Faber S.M.Fazio G.G.Gardner J.P.Gawiser E.Grazian A.Grogin N.A.,Kocevski D.Koo D.C.Lee K.-S.Lucas R.A.McGrath E.J.Nandra K.,Newman J.A.Van Der Wel A.2021-11-03T09:14:43Z2021-02-18T09:21:40ZCDS support team

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

cds-question@unistra.frinfrared-photometryvisible-astronomybroad-band-photometryredshiftedWe present a 0.4-8{mu}m multi-wavelength photometric catalog in the Extended Groth Strip (EGS) field. This catalog is built on the Hubble Space Telescope (HST) WFC3 and ACS data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), and it incorporates the existing HST data from the All-wavelength Extended Groth strip International Survey (AEGIS) and the 3D-HST program. The catalog is based on detections in the F160W band reaching a depth of F160W=26.62 AB (90% completeness, point sources). It includes the photometry for 41457 objects over an area of ~206arcmin^2^ in the following bands: HST/ACS F606W and F814W; HST WFC3 F125W, F140W, and F160W; Canada-France-Hawaii Telescope (CFHT)/Megacam u*, g' , r', i' and z'; CFHT/WIRCAM J, H, and K_S_; Mayall/NEWFIRM J1, J2, J3, H1, H2, and K; Spitzer IRAC 3.6, 4.5, 5.8, and 8.0{mu}m. We are also releasing value-added catalogs that provide robust photometric redshifts and stellar mass measurements.2017ApJS..229...32Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/229/32CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIII/268 : DEEP2 Redshift Survey, Data Release 4 (Matthews+ 2013)II/301 : The DEEP2-DR1 Photometric Catalog (Coil+ 2004)II/261 : GOODS initial results (Giavalisco+, 2004)J/ApJS/228/7 : Multi-wavelength data in CANDELS COSMOS field (Nayyeri+, 2017)J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016)J/ApJS/220/10 : AEGIS-X Deep survey of EGS (AEGIS-XD) (Nandra+, 2015)J/ApJ/810/71 : UV mag of candidate galaxies at 3~<z~<8.5 (Finkelstein+, 2015)J/ApJS/218/33 : Spitzer-CANDELS catalog within 5 deep fields (Ashby+, 2015)J/ApJ/803/34 : z~4-10 galaxies from HST legacy fields (Bouwens+, 2015)J/ApJ/801/97 : GOODS-S+UDS stellar masses from CANDELS (Santini+, 2015)J/ApJ/796/60 : ECDFS galaxies phot. redshifts + counterparts (Hsu+, 2014)J/ApJ/793/101 : CANDELS z~2 galaxy properties (Trump+, 2014)J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)J/ApJS/212/18 : An atlas of UV-to-MIR galaxy SEDs (Brown+, 2014)J/ApJS/207/24 : GOODS-S CANDELS multiwavelength catalog (Guo+, 2013)J/ApJ/771/85 : Dynamical masses of z~2 quiescent gal. (van de Sande+, 2013)J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)J/ApJ/769/80 : Spitzer/IRAC observations of five deep fields (Ashby+, 2013)J/ApJ/751/50 : Galaxy groups from DEEP2 Redshift Survey (Gerke+ 2012)J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)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/ApJS/193/13 : Spitzer/IRAC sources in the EGS I. SEDs (Barro+, 2011)J/ApJS/189/270 : MUSYC optical imaging in ECDF-S (Cardamone+, 2010)J/MNRAS/393/1275 : STAGES master catalog (Gray+, 2009)J/ApJS/180/102 : AEGIS-X: Chandra deep survey (Laird+, 2009)J/ApJS/177/431 : Mid-IR sources in EGS (Barmby+, 2008)J/ApJ/675/234 : Stellar mass functions for gal. 0<z<4 (Perez-Gonzalez+, 2008)J/ApJS/174/136 : GEMS survey data and catalog (Caldwell+, 2008)J/AJ/132/2159 : IRAC counterparts of 6cm galaxies in EGS (Willner+, 2006)J/A+A/449/951 : GOODS-MUSIC sample: multicolour catalog (Grazian+, 2006)J/MNRAS/356/568 : Deep Chandra survey of the Groth Strip (Nandra+, 2005)J/AJ/125/1107 : Ultra-deep near-IR observation in HDF-S (Labbe+, 2003)J/ApJ/513/34 : HDF photometric redshifts catalog (Fernandez-Soto+, 1999)http://candels.ucolick.org/ : CANDELS home pagehttp://www.mpe.mpg.de/XraySurveys/AEGIS-X/ : AEGIS-X home pagehttp://3dhst.research.yale.edu/Data.php : 3D-HST home pagehttp://deep.ps.uci.edu/deep3/home.html : DEEP3 galaxy redshift surveyhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/229/32https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/229/32http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/229/32https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/229/32https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/229/32http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/229/32GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/229/32/table6 (Photometric catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/229/32/table6?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/229/32/table6?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/229/32/table6?GETtext/xml+votable180.050000true215.301153.051206110.005555555555555556Cone search capability for table J/ApJS/229/32/table8 (Stellar mass catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/229/32/table8?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/229/32/table8?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/229/32/table8?GETtext/xml+votable180.050000true215.301153.051206110.0055555555555555566/114252.0616683193919197e-20 5.500300350312679e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/229/32?format=asciiOpticalInfrareddefaultJ/ApJS/229/32/table6Photometric catalogSimbadNameSimbad column added by the CDSmeta.idcharnullableSEDSED plot of this objectmeta.ref.urlchare_8.0flux? Uncertainty in 8.0flux (5)uJystat.errordoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential identifier number (<[SYM2017] NNNNN> in Simbad) (1)meta.idintprimaryNameIAU designation (<CANDELS EGS F160W JHHMMSS.s+DDMMSS.s> in Simbad)meta.id;meta.maincharRAJ2000Right Ascension (J2000) (2)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (2)degpos.eq.dec;meta.mainindexedRALdegL08 Right Ascension (J2000) (3)degpos.eq.raDELdegL08 Declination (J2000) (3)degpos.eq.decFlag[0/11]? Quality flag (0=good) (4)meta.code.errorintnullableS/GSExtractor CLASS_STAR parameter from F160W mosaic (0=galaxy)src.class.starGalaxyfloatufluxC[-0.5/3906] CFHT/MegaCam u* band flux densityuJyphot.flux.density;em.opt.Udoublee_ufluxC? Uncertainty in ufluxC (5)uJystat.errordoublenullablegfluxC[-0.9/3235] CFHT/MegaCam g' band flux densityuJyphot.flux.density;em.opt.Rdoublee_gfluxC? Uncertainty in gfluxC (5)uJystat.errordoublenullablerfluxC[-0.8/3004] CFHT/MegaCam r' band flux densityuJyphot.flux.density;em.opt.Rdoublee_rfluxC? Uncertainty in rfluxC (5)uJystat.errordoublenullableifluxC[-0.9/2058] CFHT/MegaCam i' band flux densityuJyphot.flux.density;em.opt.Idoublee_ifluxC? Uncertainty in ifluxC (5)uJystat.errordoublenullablezfluxC[-3.2/6484] CFHT/MegaCam z' band flux densityuJyphot.flux.density;em.opt.Idoublee_zfluxC? Uncertainty in zfluxC (5)uJystat.errordoublenullableF606W[-1.3/1016]? HST/ACS F606W band flux densityuJyphot.mag;em.opt.Rdoublenullablee_F606W? Uncertainty in F606Wflux (5)uJystat.errordoublenullableF814W[-1.5/1744]? HST/ACS F814W band flux densityuJyphot.mag;em.opt.Idoublenullablee_F814W? Uncertainty in F814Wflux (5)uJystat.errordoublenullableF125W[-1.2/2891]? HST/WFC3 F125W band flux densityuJyphot.flux.density;em.IR.Jdoublenullablee_F125W? Uncertainty in F125Wflux (5)uJystat.errordoublenullableF140W[-13.1/3181]? HST/WFC3 F140W band flux densityuJyphot.flux.density;em.IR.Hdoublenullablee_F140W? Uncertainty in F140Wflux (5)uJystat.errordoublenullableF160W[-1.3/38710]? HST/WFC3 F160W band flux densityuJyphot.flux.density;em.IR.Hdoublenullablee_F160W? Uncertainty in F160Wflux (5)uJystat.errordoublenullableJfluxW[-2.8/13430] CFHT/WIRCAM J band flux densityuJyphot.flux.density;em.IR.Jdoublee_JfluxW? Uncertainty in JfluxW (5)uJystat.errordoublenullableHfluxW[-6.7/22490] CFHT/WIRCAM H band flux densityuJyphot.flux.density;em.IR.Hdoublee_HfluxW? Uncertainty in HfluxW (5)uJystat.errordoublenullableKfluxW[-2.6/15020] CFHT/WIRCAM Ks band flux densityuJyphot.mag;em.IR.Kdoublee_KfluxW? Uncertainty in KfluxW (5)uJystat.errordoublenullableJ1flux[-31960/13750]? NEWFIRM J1 band flux densityuJyphot.flux.density;em.IR.Jdoublenullablee_J1flux? Uncertainty in J1flux (5)uJystat.errordoublenullableJ2flux[-3863/11750]? NEWFIRM J2 band flux densityuJyphot.flux.density;em.IR.Jdoublenullablee_J2flux? Uncertainty in J2flux (5)uJystat.errordoublenullableJ3flux[-7181/9168]? NEWFIRM J3 band flux densityuJyphot.flux.density;em.IR.Jdoublenullablee_J3flux? Uncertainty in J3flux (5)uJystat.errordoublenullableH1flux[-8008/80980]? NEWFIRM H1 band flux densityuJyphot.flux.density;em.IR.Hdoublenullablee_H1flux? Uncertainty in H1flux (5)uJystat.errordoublenullableH2flux[-6297/16840]? NEWFIRM H2 band flux densityuJyphot.flux.density;em.IR.Hdoublenullablee_H2flux? Uncertainty in H2flux (5)uJystat.errordoublenullableKflux[-8047/21860]? NEWFIRM K band flux densityuJyphot.mag;em.IR.Kdoublenullablee_Kflux? Uncertainty in Kflux (5)uJystat.errordoublenullable3.6flux[-16110/19490]? Spitzer/IRAC 3.6um band flux densityuJyphot.mag;em.IR.3-4umdoublenullablee_3.6flux? Uncertainty in 3.6flux (5)uJystat.errordoublenullable4.5flux[-17480/19790]? Spitzer/IRAC 4.5um band flux densityuJyphot.mag;em.IR.4-8umdoublenullablee_4.5flux? Uncertainty in 4.5flux (5)uJystat.errordoublenullable5.8flux[-38/6383]? Spitzer/IRAC 5.8um band flux densityuJyphot.flux.density;em.IR.4-8umdoublenullablee_5.8flux? Uncertainty in 5.8flux (5)uJystat.errordoublenullable8.0flux[-101/3273]? Spitzer/IRAC 8.0um band flux densityuJyphot.flux.density;em.IR.8-15umdoublenullableF606Wv08[-0.6/4769]? AEGIS HST/ACS F606W band flux densityuJyphot.mag;em.opt.Rdoublenullablee_F606Wv08? Uncertainty in F606Wfluxv08uJystat.errordoublenullableF814Wv08[-0.4/7766]? AEGIS HST/ACS F814W band flux densityuJyphot.mag;em.opt.Idoublenullablee_F814Wv08? Uncertainty in F814Wfluxv08uJystat.errordoublenullableF125Wv08[-3.5/8426]? AEGIS HST/WFC3 F125W band flux densityuJyphot.flux.density;em.IR.Jdoublenullablee_F125Wv08? Uncertainty in F125Wfluxv08uJystat.errordoublenullableF160Wv08[-1.8/34070]? AEGIS HST/WFC3 F160W band flux densityuJyphot.flux.density;em.IR.Hdoublenullablee_F160Wv08? Uncertainty in F160Wfluxv08uJystat.errordoublenullable5.8v08[-9262/10640]? Spitzer/IRAC 5.8um band flux density (6)uJyphot.flux.density;em.IR.4-8umdoublenullablee_5.8v08? Uncertainty in 5.8fluxv08uJystat.errordoublenullable8.0v08[-5470/6051]? Spitzer/IRAC 8.0um band flux density (6)uJyphot.flux.density;em.IR.4-8umdoublenullablee_8.0v08? Uncertainty in 8.0fluxv08uJystat.errordoublenullableF606WPHZ[-0.5/1016]? HST/ACS F606W band flux density (7)uJyphot.mag;em.opt.Rdoublenullablee_F606WPHZ? Uncertainty in F606WPHZuJystat.errordoublenullableF814WPHZ[-1.5/1744]? HST/ACS F814W band flux density (7)uJyphot.mag;em.opt.Idoublenullablee_F814WPHZ? Uncertainty in F814WPHZuJystat.errordoublenullableF125WPHZ[-0.3/2891]? HST/WFC3 F125W band flux density (7)uJyphot.flux.density;em.IR.Jdoublenullablee_F125WPHZ? Uncertainty in F125WPHZuJystat.errordoublenullableF140WPHZ[0.0002/11700]? HST/WFC3 F140W band flux density (7)uJyphot.flux.density;em.IR.Hdoublenullablee_F140WPHZ? Uncertainty in F140WPHZuJystat.errordoublenullableF160WPHZ[-1.3/3410]? HST/WFC3 F160W band flux density (7)uJyphot.flux.density;em.IR.Hdoublenullablee_F160WPHZ? Uncertainty in F160WPHZuJystat.errordoublenullablezspec[-1/3.5]? DEEP2/3 spectroscopic redshift (8)src.redshiftdoublenullableJ/ApJS/229/32/table7Photometric redshift catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential identifier number (<[SYM2017] NNNNN> in Simbad)meta.id;meta.mainintprimary<photz>[0/9.9] Median of photometric redshift measurementssrc.redshift.photfloatphotz-S[0.03/10]? Salvato photometric redshift (1)src.redshift.photfloatnullablephotz-M[0/9.6] Mobasher photometric redshift (1)src.redshift.photfloatphotz-F[0/10] Finkelstein photometric redshift (1)src.redshift.photfloatphotz-B[0.03/10]? Barro photometric redshift (1)src.redshift.photfloatnullablephotz-Wi[0.01/10] Wiklind photometric redshift (1)src.redshift.photfloatphotz-Wu[0/10]? Wuyts photometric redshift (1)src.redshift.photfloatnullableD95[0.01/7.4] Accuracy of photometric redshifts (2)stat.errorfloatspecz[-0.001/2.3]? Spectroscopic redshift of control sample (3)src.redshift;pos.heliocentricdoublenullablephotzl68Lower 68% confidence interval on <photz>src.redshift.photfloatphotzu68Upper 68% confidence interval on <photz>src.redshift.photfloatphotzl95Lower 95% confidence interval on <photz>src.redshift.photfloatphotzu95Upper 95% confidence interval on <photz>src.redshift.photfloatJ/ApJS/229/32/table8Stellar mass catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential identifier number (<[SYM2017] NNNNN> in Simbad) (1)meta.id;meta.mainintprimaryRAJ2000Right Ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainindexedHmag[12.4/32.7]? HST/WFC3 F160W band magnitude (2)magphot.mag;em.opt.RfloatnullablePFlag[0/11] Photometric catalog flagmeta.code.error;meta.tableintS/GSExtractor CLASS_STAR parameter (0=galaxy)stat.paramfloatAGNNandra+ 2015, J/ApJS/220/10 counterpart flag (0=no counterpart)meta.codeintzphot[0.001/9.9] Photometric redshiftsrc.redshiftfloatzspec[-0.001/2.3]? DEEP3 catalog spectroscopic redshiftsrc.redshiftdoublenullableq_zspec[-99/1] Quality flag on zspec (1=good) (3)meta.code.qualintr_zspec[-99/2] zspec reference: 1=DEEP2/3 (See Cooper+, 2011, J/ApJS/193/14)meta.ref;pos.frameintzbest[0.001/9.9] Best redshift measurement (4)src.redshift;pos.heliocentricfloatzbestl68Lower 68% confidence interval on zbest (5)stat.errorfloatzbestu68Upper 68% confidence interval on zbest (5)stat.errorfloatzbestl95Lower 95% confidence interval on zbest (5)stat.errorfloatzbestu95Upper 95% confidence interval on zbest (5)stat.errorfloatzAGN[0.09/6]? Nandra+ 2015, J/ApJS/220/10 X-ray catalog photometric redshift (6)src.redshift.photfloatnullablelogM*N[4.2/12.4] Log stellar mass (7)log(solMass)phys.massdoublee_logM*N? Uncertainty in logM*Nlog(solMass)stat.errordoublenullablelogM*[4.2/12.3] Log stellar mass (8)log(solMass)phys.massdoublee_logM*? Uncertainty in logM*log(solMass)stat.errordoublenullablelogM*1[6.3/12]? M_14a_cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*2[3.3/12.4]? M_11a_tau stellar mass (G1)log(solMass)phys.massfloatnullablelogM*3[3.5/12.4]? M_6a_tau^NEB cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*4? M_13a_tau cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*5[4/12.5] M_12a_cons stellar mass (G1)log(solMass)phys.massfloatlogM*6? M_6a_tau cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*7[0/15.3]? M_2a_tau cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*8[3.7/12.4]? M_15a_cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*9[1.2/12.5]? M_10c_cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*10? M_14a_lin cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*11? M_14a_deltau cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*12? M_14a_tau cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*13? M_14a_inctau cons stellar mass (G1)log(solMass)phys.massfloatnullablelogM*14[6.3/11.7]? M_14a stellar mass (G1)log(solMass)phys.massfloatnullablelogM*Nml[3.5/12.4] Log stellar mass (9)log(solMass)phys.massdoublee_logM*Nml[0.0002/246]? Uncertainty in logM*Nmllog(solMass)stat.errordoublenullablelogM*ml[4.3/13.2] Log stellar mass (10)log(solMass)phys.massdoublee_logM*ml? Uncertainty in logM*mllog(solMass)stat.errordoublenullableJ/ApJS/229/32/table9Physical parameters catalogElaw-6ad[1/2] Extinction law method 6a_del_meta.codeinttau-12a[0/2] The {tau} from method 12a (G1)Gyrtime.agefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential identifier number (1)meta.id;meta.mainintprimarylogA-2a[7.6/10.1] Log age from method 2alog(yr)time.agefloattau-2a[0.3/12.6] The {tau} from method 2a (G1)Gyrtime.agefloatAv-2a[0/4] A_V_ from method 2amagphys.absorptionfloatSFR-2aStar formation rate from method 2asolMass/yrphys.SFRdoublechi2-2a? Reduced {chi}^2^ from method 2ameta.notedoublenullablelogA-4b[7/10.1] Log age from method 4blog(yr)time.agefloatE(B-V)-4b[0/0.8] The (B-V) color excess from method 4bmagphot.color.excessfloatlogA-6a[7/10.2]? Log age from method 6a_{tau}_log(yr)time.agefloatnullabletau-6a[0.1/15]? The {tau} from method 6a_{tau}_ (G1)Gyrtime.agefloatnullableE(B-V)-6a[0/1.1]? The (B-V) color excess from method 6a_{tau}_magphot.color.excessfloatnullableSFR-6a[0/11430]? Star formation rate from method 6a_{tau}_solMass/yrphys.SFRdoublenullableZ-6a[0.02/2.5]? Gass metallicity from method 6a_{tau}_Sunphys.abund.ZfloatnullableElaw-6aExtinction law method 6a_{tau}_ (2)meta.codeintchi2-6a[0.05/220]? Reduced {chi}^2^ from method 6a_{tau}_meta.notedoublenullableL1400-6a? Rest-frame luminosity at 1400{AA} from method 6a_{tau}_ (3)1e-07W.Hz**-1phys.luminositydoublenullableL2700-6a? Rest-frame luminosity at 2700{AA} from method 6a_{tau}_ (3)1e-07W.Hz**-1phys.luminositydoublenullableUMag-6a[-26.2/-4.8]? U rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullableBMag-6a[-26.3/-5.5]? B rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullableVMag-6a[-26.1/-5.9]? V rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullableRMag-6a[-26.2/-6.1]? R rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullableIMag-6a[-26.5/-6.3]? I rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullableJMag-6a[-27/-6.7]? J rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullableKMag-6a[-27/-6.3]? K rest-frame AB magnitude from method 6a_{tau}_magphys.magAbsfloatnullablelogA-10c[8/10.2]? Log age from method 10clog(yr)time.agefloatnullableSFH-10cStar formation history method 10c (4)meta.codeinttau-10c[0.1/1]? The {tau} from method 10c (5)Gyrtime.agefloatnullableZ-10c[0/0.04]? Gas metallicity from method 10cSunphys.abund.ZfloatnullableMl99-11a[7/12.4]? Log lower 99% confidence stellar mass interval from method 11a_{tau}_log(solMass)stat.errorfloatnullableMu99-11a[7/12.5]? Log upper 99% confidence stellar mass interval from method 11a_{tau}_log(solMass)stat.errorfloatnullablelogA-11a[7/10.1]? Log age from method 11a_{tau}_log(yr)time.agefloatnullableSFR-11a[0/3267] Log star formation rate for method 11a_{tau}_ (8)log(solMass.yr**-1)meta.iddoubleMl68-12a? Log lower 68% confidence stellar mass interval from method 12alog(solMass)stat.errorfloatnullableMu68-12a? Log upper 68% confidence stellar mass interval from method 12alog(solMass)stat.errorfloatnullableMl95-12a? Log lower 95% confidence stellar mass interval from method 12alog(solMass)stat.errorfloatnullableMu95-12a? Log upper 95% confidence stellar mass interval from method 12alog(solMass)stat.errorfloatnullablelogA-12a[7.3/9.9] Log age from method 12alog(yr)time.agefloatE(B-V)-12aThe (B-V) color excess from method 12amagphot.color.excessfloatZ-12a[0/0.05] Gas metallicity form method 12aSunphys.abund.ZfloatLbol-12a[6/13.8] Log bolometric luminosity from method 12alog(solLum)phys.luminosityfloatchi2-12a[0/999] Reduced {chi}^2^ from method 12ameta.notedoublelogA-13a[7.7/10.1] Log age from method 13a_{tau}_log(yr)time.agefloattau-13a[0.3/10] The {tau} from method 13a_{tau}_ (G1)Gyrtime.agefloatAv-13a[0/4] V band extinction from method 13a_{tau}_magphys.absorptionfloatSFR-13a[0/30200] Star formation rate from method 13a_{tau}_ (8)solMass/yrphys.SFRdoublechi2-13a[0.07/1250] Reduced {chi}^2^ from method 13a_{tau}_meta.notedoublelogA-14a[8/9.2]? Log age from method 14alog(yr)time.agefloatnullableSFH-14aStar formation history method 14a (6)meta.codeinttau-14a[0.1/7]? {tau} from method 14a (G1)Gyrtime.agefloatnullableE(B-V)-14a[0.01/1]? The (B-V) color excess from method 14amagphot.color.excessfloatnullableSFR-14a[0.0004/1579]? Star formation rate from method 14asolMass/yrphys.SFRdoublenullableq-14a[1/3] Fit quality from method 14a (7)meta.code.qualintlogA-6at[7/10.2]? Log age from method 6a_{tau}_^NEB^log(yr)time.agefloatnullabletau-6at[0.1/15]? The {tau} from method 6a_{tau}_^NEB^ (G1)Gyrtime.agefloatnullableE(B-V)-6at[0/1.1]? The (B-V) color excess from method 6a_{tau}_^NEB^magphot.color.excessfloatnullableSFR-6at[0/6174]? Star formation rate from method 6a_{tau}_^NEB^solMass/yrphys.SFRdoublenullableZ-6at[0.02/2.5]? Gas metallicity from method 6a_{tau}_^NEB^Sunphys.abund.ZfloatnullableElaw-6at[1/2] Extintion law from method 6a_{tau}_^NEB^meta.codeintchi2-6at[0.05/208]? Reduced {chi}^2^ from method 6a_{tau}_^NEB^meta.notedoublenullableL1400-6at? Rest-frame luminosity at 1400{AA} from method 6a_{tau}_^NEB^ (3)1e-07W.Hz**-1phys.luminositydoublenullableL2700-6at? Rest-frame luminosity at 2700{AA} from method 6a_{tau}_^NEB^ (3)1e-07W.Hz**-1phys.luminositydoublenullableUMag-6at[-26.4/-4.8]? U rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullableBMag-6at[-26.5/-5.5]? B rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullableVMag-6at[-26.7/-5.9]? V rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullableRMag-6at[-26.6/-6.1]? R rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullableIMag-6at[-26.5/-6.3]? I rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullableJMag-6at[-27/-6.7]? J rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullableKMag-6at[-27/-6.6]? K rest-frame AB magnitude from method 6a_{tau}_^NEB^magphys.magAbsfloatnullablelogA-6ad[7/10.2]? Log Age from method 6a_del_log(yr)time.agefloatnullabletau-6ad[0.1/2]? The {tau} from method 6a_del_ (G1)Gyrtime.agefloatnullableE(B-V)-6ad[0/1.1]? The (B-V) color excess from method 6a_del_magphot.color.excessfloatnullableSFR-6ad[0/58910]? Star formation rate from method 6a_del_solMass/yrphys.SFRdoublenullableZ-6ad[0.02/2.5]? Gas metallicity from method 6a_del_Sunphys.abund.Zfloatnullablechi2-6ad? Reduced {chi}^2^ from method 6a_del_meta.notedoublenullableL1400-6ad? Rest-frame luminosity at 1400{AA} from method 6a_del_ (3)1e-07W.Hz**-1phys.luminositydoublenullableL2700-6ad? Rest-frame luminosity at 2700{AA} from method 6a_del_ (3)1e-07W.Hz**-1phys.luminositydoublenullableUMag-6ad[-26.6/-4.8]? U rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullableBMag-6ad[-26.7/-5.6]? B rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullableVMag-6ad[-26.4/-5.3]? V rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullableRMag-6ad[-26.3/-5.2]? R rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullableIMag-6ad[-26.1/-4.9]? I rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullableJMag-6ad[-26.4/-4.4]? J rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullableKMag-6ad[-26.4/-3.5]? K rest-frame AB magnitude from method 6a_del_magphys.magAbsfloatnullablelogA-6ai[7/10.1]? Log age from method 6a_inv_log(yr)time.agefloatnullabletau-6ai[0.1/15]? {tau} from method 6a_inv_ (G1)Gyrtime.agefloatnullableE(B-V)-6ai[0/1.1]? The (B-V) color excess from method 6a_inv_magphot.color.excessfloatnullableSFR-6ai[5e-6/15950]? Star formation rate from method 6a_inv_solMass/yrphys.SFRdoublenullableZ-6ai[0.02/2.5]? Gas metallicity from method 6a_inv_Sunphys.abund.ZfloatnullableElaw-6aiExtinction law method 6a_inv_meta.codeintchi2-6ai[0.05/191]? Reduced {chi}^2^ from method 6a_inv_meta.notedoublenullableL1400-6ai? Rest-frame luminosity at 1400{AA} from method 6a_inv_ (3)1e-07W.Hz**-1phys.luminositydoublenullableL2700-6ai? Rest-frame luminosity at 2700{AA} from method 6a_inv_ (3)1e-07W.Hz**-1phys.luminositydoublenullableUMag-6ai[-26.3/-4.7]? U rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableBMag-6ai[-26.3/-5.6]? B rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableVMag-6ai[-26.2/-5.9]? V rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableRMag-6ai[-26/-6.1]? R rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableIMag-6ai[-26.2/-6.3]? I rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableJMag-6ai[-26.8/-6.7]? J rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableKMag-6ai[-27.3/-6.6]? K rest-frame AB magnitude from method 6a_inv_magphys.magAbsfloatnullableage-10cd[8/11]? Log age from method 10c^dust^log(yr)time.agefloatnullableSFH-10cdStar formation history from method 10c^dust^ (4)meta.codeinttau-10cd? The {tau} from method 10c^dust^ (5)Gyrtime.agefloatnullableZ-10cd[0/0.04]? Gas metallicity from method 10c^dust^Sunphys.abund.Zfloatnullableage-14ac[8/9.3]? Log age from method 14a_const_log(yr)time.agefloatnullableE(B-V)-14ac[0.01/1]? The (B-V) color excess from method 14a_const_magphot.color.excessfloatnullableSFR-14ac[0.006/2099]? Star formation rate from method 14a_const_solMass/yrphys.SFRdoublenullableq-14ac[1/3] Fit quality from method 14a_const_ (7)meta.code.qualintlogA-14al[8/9.5]? Log age from method 14a_lin_log(yr)time.agefloatnullableE(B-V)-14al[0.01/1]? The (B-V) color excess from method 14a_lin_magphot.color.excessfloatnullableSFR-14al[0.01/4497]? Star formation rate from method 14a_lin_solMass/yrphys.SFRdoublenullableq-14alFit quality from method 14a_lin_ (7)meta.code.qualintlogA-14ad[8/9.1]? Log age from method 14a_del_log(yr)time.agefloatnullabletau-14ad? The {tau} from method 14a_del_ (G1)Gyrtime.agefloatnullableE(B-V)-14ad[0.01/1]? The (B-V) color excess from method 14a_del_magphot.color.excessfloatnullableSFR-14ad[0.001/4454]? Star formation rate from method 14a_del_solMass/yrphys.SFRdoublenullableq-14adFit quality from method 14a_del_ (7)meta.code.qualintlogA-14at[8/10]? Log age from method 14a_{tau}_log(yr)time.agefloatnullabletau-14at? {tau} from method 14a_{tau}_ (G1)Gyrtime.agefloatnullableE(B-V)-14at[0.01/1]? The (B-V) color excess from method 14a_{tau}_magphot.color.excessfloatnullableSFR-14at[0.0004/2052]? Star formation rate from method 14a_{tau}_solMass/yrphys.SFRdoublenullableq-14at[1/3] Fit quality from method 14a_{tau}_ (7)meta.code.qualint