J/ApJ/801/97ivo://CDS.VizieR/J/ApJ/801/97doi:10.26093/cds/vizier.18010097CDSSantini P.Ferguson H.C.Fontana A.Mobasher B.Barro G.,Castellano M.Finkelstein S.L.Grazian A.Hsu L.T.Lee B.Lee S.-K.,Pforr J.Salvato M.Wiklind T.Wuyts S.Almaini O.Cooper M.C.,Galametz A.Weiner B.Amorin R.Boutsia K.Conselice C.J.Dahlen T.,Dickinson M.E.Giavalisco M.Grogin N.A.Guo Y.Hathi N.P.,Kocevski D.Koekemoer A.M.Kurczynski P.Merlin E.Mortlock A.,Newman J.A.Paris D.Pentericci L.Simons R.Willner S.P.2017-06-19T07:57:56Z2015-09-17T08:17:41ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsredshiftedstellar-massesstellar-agessurveysspectroscopyWe present the public release of the stellar mass catalogs for the GOODS-S and UDS fields obtained using some of the deepest near-IR images available, achieved as part of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey project. We combine the effort from 10 different teams, who computed the stellar masses using the same photometry and the same redshifts. Each team adopted their preferred fitting code, assumptions, priors, and parameter grid. The combination of results using the same underlying stellar isochrones reduces the systematics associated with the fitting code and other choices. Thanks to the availability of different estimates, we can test the effect of some specific parameters and assumptions on the stellar mass estimate. The choice of the stellar isochrone library turns out to have the largest effect on the galaxy stellar mass estimates, resulting in the largest distributions around the median value (with a semi interquartile range larger than 0.1dex). On the other hand, for most galaxies, the stellar mass estimates are relatively insensitive to the different parameterizations of the star formation history. The inclusion of nebular emission in the model spectra does not have a significant impact for the majority of galaxies (less than a factor of 2 for ~80% of the sample). Nevertheless, the stellar mass for the subsample of young galaxies (age <100Myr), especially in particular redshift ranges (e.g., 2.2<z<2.4, 3.2<z<3.6, and 5.5<z<6.5), can be seriously overestimated (by up to a factor of 10 for <20Myr sources) if nebular contribution is ignored.2015ApJ...801...97Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/801/97CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIII/268 : DEEP2 Redshift Survey, Data Release 4 (Matthews+ 2013)II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)II/261 : GOODS initial results (Giavalisco+, 2004)J/ApJS/207/24 : GOODS-S CANDELS multiwavelength catalog (Guo+, 2013)J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)J/ApJ/769/80 : Spitzer/IRAC observations of five deep fields (Ashby+, 2013)J/MNRAS/428/3089 : X-ray properties of BzK-selected galaxies (Rangel+, 2013)J/MNRAS/425/2116 : Arizona CDFS Environment Survey, ACES (Cooper+, 2012)J/ApJ/756/164 : UV galaxies in CANDELS from z=8 to z=4 (Finkelstein+, 2012)J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 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/ApJ/708/137 : Broad-line AGNs in zCOSMOS survey (Merloni+, 2010)J/ApJS/179/124 : Subaru/XMM-Newton deep survey (SXDS) III. (Ueda+, 2008)J/ApJS/176/1 : Subaru/XMM-Newton deep survey (SXDS). II. (Furusawa+, 2008)J/ApJ/675/234 : Stellar mass functions for 0<z<4 gal (Perez-Gonzalez+, 2008)J/MNRAS/381/1369 : Redshifts in Subaru/XMM Deep Field (Geach+, 2007)J/MNRAS/372/741 : SXDF 100{mu}Jy catalogue (Simpson+, 2006)J/ApJS/157/1 : Red-Sequence Cluster Survey (Gladders+, 2005)J/AJ/127/3121 : TKRS catalog of GOODS-North Field (Wirth+, 2004)J/A+A/401/1063 : Evolutionary synthesis models. III. (Anders+, 2003)J/AJ/120/2206 : NTT, HDF-S and HDF-N photometric redshifts (Fontana+, 2000)http://candels.ucolick.org/data_access/GOODS-S.html : CANDELS GOODS-S home pagehttp://candels.ucolick.org/data_access/UDS.html : CANDELS UDS home pagehttp://archive.stsci.edu/prepds/candels/ : CANDELS on MASThttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/801/97https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/801/97http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/801/97https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/801/97https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/801/97http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/801/97GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/801/97/goodss (GOODS-S field stellar masses and other physical parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/801/97/goodss?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/801/97/goodss?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/801/97/goodss?GETtext/xml+votable180.050000true53.09299472-27.954536390.005555555555555556Cone search capability for table J/ApJ/801/97/uds (UDS field stellar masses and other physical parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/801/97/uds?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/801/97/uds?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/801/97/uds?GETtext/xml+votable180.050000true34.2237625-5.278052780.005555555555555556Cone search capability for table J/ApJ/801/97/table2 (Magellan/IMACS Redshift Catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/801/97/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/801/97/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/801/97/table2?GETtext/xml+votable180.050000true34.21204194-5.206258330.0055555555555555566/17679 17688 17690 359352.762881831355591e-19 1.3189343879298211e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/801/97?format=asciiOpticaldefaultJ/ApJ/801/97/goodssGOODS-S field stellar masses and other physical parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/35932] Designation (G1)meta.id;meta.mainintRAJ2000Right ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainindexedHmag[12.7/32.1]? Observed magnitude in WFC3 F160W filtermagphot.mag;em.UV.100-200nmfloatnullableSNR[0/9999] H-band Signal-to-noise ratio (1)stat.snrfloatqph[0/18] Photometry flag; 0=ok, >0=bad photometrymeta.code.qualintStar[0/1] Spectroscopic star (1=spec. star)src.classintS/G[0/1] SExtractor stellarity index on F160W band (1=star)src.class.starGalaxyfloatAGN[0/1] Xray AGN from Xue et al. 2011; J/ApJS/195/10src.classintzbest[0/9.92] Redshift (2)src.redshift;pos.heliocentricfloatzsp[0/6.7]? Spectroscopic redshiftsrc.redshiftdoublenullableq_zsp[1/4]? Quality of spectroscopic redshift; 1=good, 2=intermediate, 3=uncertainmeta.code.qualintnullabler_zspReference spectroscopic survey (see refs.dat file)meta.ref;pos.framecharzph[0.009/9.92] Photometric redshift (3)src.redshiftfloatb_zph? Lower zph 68% confidence limitstat.fit.paramfloatnullableB_zph? Upper zph 68% confidence limitstat.fit.paramfloatnullableb_zph2? Lower zph 95% confidence limitstat.fit.paramfloatnullableB_zph2? Upper zph 95% confidence limitstat.fit.paramfloatnullablezAGN? Photometric redshift for AGNs from Hsu et al 2014ApJ...796...60H; where ?=-99 for non AGN sources (only for table4a.dat)src.redshift;pos.heliocentricfloatnullableM? CANDELS reference median stellar mass M_med_ (4)solMassphys.massdoublenullablee_M? Standard deviation on M_med_ (5)solMassstat.errordoublenullableMneb? Median stellar mass including nebular component M^neb^ (6)solMassphys.massdoublenullablee_Mneb? Standard deviation on M^neb^ (5)solMassstat.errordoublenullabledMz? Relative uncertainty due to model degeneracy and zphot scatter (7)stat.errorfloatnullableM2at? Stellar mass from Method 2a_{tau}_ (8)log(solMass)phys.massfloatnullableM2dt? Stellar mass from Method 2d_{tau}_ (8)log(solMass)phys.massfloatnullableM6at? Stellar mass from Method 6a_{tau}_ (8)log(solMass)phys.massfloatnullableM10c? Stellar mass from Method 10c (8)log(solMass)phys.massfloatnullableM11at? Stellar mass from Method 11a_{tau}_ (8)log(solMass)phys.massfloatnullableM12a? Stellar mass from Method 12a (8)log(solMass)phys.massfloatnullableM13at? Stellar mass from Method 13a_{tau}_ (8)log(solMass)phys.massfloatnullableM14a? Stellar mass from Method 14a (8)log(solMass)phys.massfloatnullableM15a? Stellar mass from Method 15a (8)log(solMass)phys.massfloatnullableM6atNEB? Stellar mass from Method 6a_{tau}_^NEB^ (8)log(solMass)phys.massfloatnullableM6adt? Stellar mass from Method 6a_del{tau}_ (8)log(solMass)phys.massfloatnullableM6ainvt? Stellar mass from Method 6a_inv{tau}_(8)log(solMass)phys.massfloatnullableM10cdust? Stellar mass from Method 10c^dust^ (8)log(solMass)phys.massfloatnullableM12at? Stellar mass from Method 12a_{tau}_ (8)log(solMass)phys.massfloatnullableM14acst? Stellar mass from Method 14a_const_ (9)log(solMass)phys.massfloatnullableM14alin? Stellar mass from Method 14a_lin_ (9)log(solMass)phys.massfloatnullableM14adt? Stellar mass from Method 14a_del{tau}_(9)log(solMass)phys.massfloatnullableM14at? Stellar mass from Method 14a_{tau}_ (9)log(solMass)phys.massfloatnullableage2at? Age from Method 2a_{tau}_ (2)log(yr)time.agefloatnullabletau2at? {tau} from Method 2a_{tau}_ (2)Gyrtime.scalefloatnullableAv2at? Av from Method 2a_{tau}_ (2)magphys.absorptionfloatnullableSFR2at? SFR from Method 2a_{tau}_ (2)solMass/yrphys.SFRdoublenullableX2.2at? Reduced chi2 from Method 2a_{tau}_ (2)stat.fit.chi2doublenullableage2dt? Age from Method 2d_{tau}_ (2)log(yr)time.agefloatnullabletau2dt? {tau} from Method 2d_{tau}_ (2)Gyrtime.scalefloatnullableAv2dt? A_v_ from Method 2d_{tau}_ (2)magphys.absorptionfloatnullablemet2dt? Gas metallicity from Method 2d_{tau}_ (2)Sunphys.abundfloatnullableage4b? Age from Method 4b (table5b only) (2)log(yr)time.agefloatnullableEBV4b? E(B-V) from Method 4b (table5b only) (2)magphot.color.excessfloatnullableMl6at? Lower stellar mass 68% confidence limit from Method 6a_{tau}_ (2)log(solMass)phys.massfloatnullableMu6at? Upper stellar mass 68% confidence limit from Method 6a_{tau}_ (2)log(solMass)phys.massfloatnullableage6at? Age from Method 6a_{tau}_ (2)log(yr)time.agefloatnullabletau6at? {tau} from Method 6a_{tau}_ (2)Gyrtime.scalefloatnullableEBV6at? E(B-V) from Method 6a_{tau}_ (2)magphot.color.excessfloatnullableSFR6at? SFR from Method 6a_{tau}_ (2)solMass/yrphys.SFRdoublenullablemet6at? Gas metallicity from Method 6a_{tau}_ (2)Sunphys.abundfloatnullableel6at[1/2]? Extinction law from Method 6a_{tau}_; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6at? Reduced chi2 from Method 6a_{tau}_ (2)stat.fit.chi2doublenullableL1.6at? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6at? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6at? AB rest-frame magnitude in U band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableBM6at? AB rest-frame magnitude in B band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableVM6at? AB rest-frame magnitude in V band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableRM6at? AB rest-frame magnitude in R band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableIM6at? AB rest-frame magnitude in I band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableJM6at? AB rest-frame magnitude in J band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableKM6at? AB rest-frame magnitude in K band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableage10c? Age from Method 10c (2)log(yr)time.agefloatnullableSFH10c? Star formation history from Method 10c (2)(3)meta.codeintnullabletau10c? {tau} from Method 10c (2)Gyrtime.scalefloatnullablemet10c? Gas metallicity from Method 10c (2)Sunphys.abundfloatnullableMl11at? Lower stellar mass 99% confidence limit from Method 11a_{tau}_ (2)log(solMass)phys.massfloatnullableMu11at? Upper stellar mass 99% confidence limit from Method 11a_{tau}_ (2)log(solMass)phys.massfloatnullableage11at? Age from Method 11a_{tau}_ (2)log(yr)time.agefloatnullableSFR11at? SFR from Method 11a_{tau}_ (2)solMass/yrphys.SFRdoublenullableMl12a? Lower stellar mass 68% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableMu12a? Upper stellar mass 68% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableM2l12a? Lower stellar mass 95% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableM2u12a? Upper stellar mass 95% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableage12a? Age from Method 12a (2)log(yr)time.agefloatnullabletau12a? {tau} from Method 12a (2)Gyrtime.scalefloatnullableEBV12a? E(B-V) from Method 12a (2)magphot.color.excessfloatnullablemet12a? Gas metallicity from Method 12a (2)Sunphys.abundfloatnullableLb12a? Stellar bolometric luminosity corrected for dust extinction from Method 12a (2)(4)log(solLum)phys.luminosityfloatnullableX2.12a? Reduced chi2 from Method 12a (2)stat.fit.chi2doublenullableage13at? Age from Method 13a_{tau}_ (2)log(yr)time.agefloatnullabletau13at? {tau} from Method 13a_{tau}_ (2)Gyrtime.scalefloatnullableAv13at? Av from Method 13a_{tau}_ (2)magphys.absorptionfloatnullableSFR13at? SFR from Method 13a_{tau}_ (2)solMass/yrphys.SFRdoublenullableX2.13at? Reduced chi2 from Method 13a_{tau}_(2)stat.fit.chi2doublenullableage14a? Age from Method 14a (2)log(yr)time.agefloatnullableSFH14a? Star formation history from Method 14a (2)(5)meta.codeintnullabletau14a? {tau} from Method 14a (2)Gyrtime.scalefloatnullableEBV14a? E(B-V) from Method 14a (2)magphot.color.excessfloatnullableSFR14a? SFR from Method 14a (2)(5)solMass/yrphys.SFRdoublenullableq14a[1/3]? Quality of the fit from Method 14a; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage15a? Age from Method 15a (table5a only) (2)log(yr)time.agefloatnullabletau15a? {tau} from Method 15a (table5a only) (2)Gyrtime.scalefloatnullableEBV15a? E(B-V) from Method 15a (table5a only) (2)magphot.color.excessfloatnullablemet15a? Gas metallicity from Method 15a (table5a only) (2)Sunphys.abundfloatnullableage6atNEB? Age from Method 6a_{tau}_^NEB^ (2)log(yr)time.agefloatnullabletau6atNEB? {tau} from Method 6a_{tau}_^NEB^ (2)Gyrtime.scalefloatnullableEBV6atNEB? E(B-V) from Method 6a_{tau}_^NEB^ (2)magphot.color.excessfloatnullableSFR6atNEB? SFR from Method 6a_{tau}_^NEB^ (2)solMass/yrphys.SFRdoublenullablemet6atNEB? Gas metallicity from Method 6a_{tau}_^NEB^ (2)Sunphys.abundfloatnullableel6atNEB[1/2]? Extinction law from Method 6a_{tau}_^NEB^; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6atNEB? Reduced chi2 from Method 6a_{tau}_^NEB^ (2)stat.fit.chi2doublenullableL1.6atNEB? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_{tau}_^NEB^; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6atNEB? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_{tau}_^NEB^; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6atNEB? AB rest-frame magnitude in U band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableBM6atNEB? AB rest-frame magnitude in B band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableVM6atNEB? AB rest-frame magnitude in V band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableRM6atNEB? AB rest-frame magnitude in R band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableIM6atNEB? AB rest-frame magnitude in I band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableJM6atNEB? AB rest-frame magnitude in J band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableKM6atNEB? AB rest-frame magnitude in K band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableage-6adt? Age from Method 6a_del{tau}_ (2)log(yr)time.agefloatnullabletau-6adt? {tau} from Method 6a_del{tau}_ (2)Gyrtime.scalefloatnullableEBV-6adt? E(B-V) from Method 6a_del{tau}_ (2)magphot.color.excessfloatnullableSFR-6adt? SFR from Method 6a_del{tau}_ (2)solMass/yrphys.SFRdoublenullablemet-6adt? Gas metallicity from Method 6a_del{tau}_ (2)Sunphys.abundfloatnullableel6ad? Extinction law from Method 6a_del{tau}_; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6adt? Reduced chi2 from Method 6a_del{tau}_ (2)stat.fit.chi2doublenullableL1.6adt? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_del{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6adt? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_del{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6adt? AB rest-frame magnitude in U band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableBM6adt? AB rest-frame magnitude in B band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableVM6adt? AB rest-frame magnitude in V band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableRM6adt? AB rest-frame magnitude in R band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableIM6adt? AB rest-frame magnitude in I band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableJM6adt? AB rest-frame magnitude in J band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableKM6adt? AB rest-frame magnitude in K band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableage6ainvt? Age from Method 6a_inv{tau}_ (2)log(yr)time.agefloatnullabletau6ainvt? {tau} from Method 6a_inv{tau}_ (2)Gyrtime.scalefloatnullableEBV6ainvt? E(B-V) from Method 6a_inv{tau}_ (2)magphot.color.excessdoublenullableSFR6ainvt? SFR from Method 6a_inv{tau}_ (2)solMass/yrphys.SFRdoublenullablemet6ainvt? Gas metallicity from Method 6a_inv{tau}_ (2)Sunphys.abundfloatnullableel6ainvt[1/2]? Extinction law from Method 6a_inv{tau}_; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6ainvt? Reduced chi2 from Method 6a_inv{tau}_ (2)stat.fit.chi2doublenullableL1.6ainvt? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_inv{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6ainvt? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_inv{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6ainvt? AB rest-frame magnitude in U band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableBM6ainvt? AB rest-frame magnitude in B band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableVM6ainvt? AB rest-frame magnitude in V band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableRM6ainvt? AB rest-frame magnitude in R band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableIM6ainvt? AB rest-frame magnitude in I band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableJM6ainvt? AB rest-frame magnitude in J band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableKM6ainvt? AB rest-frame magnitude in K band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableage10cdust? Age from Method 10c^dust^ (2)log(yr)time.agefloatnullableSFH10cdust? Star formation history from Method 10c^dust^ (2)(3)meta.codeintnullabletau10cdust? {tau} from Method 10c^dust^ (2)Gyrtime.scalefloatnullablemet10cdust? Gas metallicity from Method 10c^dust^ (2)Sunphys.abundfloatnullableage12at? Age from Method 12a_{tau}_ (2)log(yr)time.agefloatnullabletau12at? {tau} from Method 12a_{tau}_ (2)Gyrtime.scalefloatnullableEBV12at? E(B-V) from Method 12a_{tau}_ (2)magphot.color.excessfloatnullablemet12at? Gas metallicity from Method 12a_{tau}_ (2)Sunphys.abundfloatnullableLb12at? Stellar bolometric luminosity corrected for dust extinction from Method 12a (2)(4)log(solLum)phys.luminosityfloatnullableX2.12at? Reduced chi2 from Method 12a_{tau}_(2)stat.fit.chi2doublenullableage14acst? Age from Method 14a_const_ (2)log(yr)time.agefloatnullableEBV14acst? E(B-V) from Method 14a_const_ (2)magphot.color.excessdoublenullableSFR14acst? SFR from Method 14a_const_ (2)solMass/yrphys.SFRdoublenullableq14acst[1/3]? Quality of the fit from Method 14a_const_; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage14alin? Age from Method 14a_lin_ (2)log(yr)time.agefloatnullableEBV14alin? E(B-V) from Method 14a_lin_ (2)magphot.color.excessdoublenullableSFR14alin? SFR from Method 14a_lin_ (2)solMass/yrphys.SFRdoublenullableq14alin[1/3]? Quality of the fit from Method 14a_lin_; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage14adt? Age from Method 14a_del{tau}_ (2)log(yr)time.agefloatnullabletau14adt? {tau} from Method 14a_del{tau}_ (2)Gyrtime.scalefloatnullableEBV14adt? E(B-V) from Method 14a_del{tau}_ (2)magphot.color.excessdoublenullableSFR14adt? SFR from Method 14a_del{tau}_ (2)solMass/yrphys.SFRdoublenullableq14adt[1/3]? Quality of the fit from Method 14a_del{tau}_; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage14at? Age from Method 14a_{tau}_ (2)log(yr)time.agefloatnullabletau14at? {tau} from Method 14a_{tau}_ (2)Gyrtime.scalefloatnullableEBV14at? E(B-V) from Method 14a_{tau}_ (2)magphot.color.excessdoublenullableSFR14at? SFR from Method 14a_{tau}_ (2)solMass/yrphys.SFRdoublenullableq14at[0/3] Quality of fit from Method 14a_{tau}; 1=best; 2=good; others=bad (2)meta.code.qualintJ/ApJ/801/97/udsUDS field stellar masses and other physical parametersSeq[1/35932] Designation (G1)meta.id;meta.mainintB_zph? Upper zph 68% confidence limitstat.fit.paramfloatnullableage2at? Age from Method 2a_{tau}_ (2)log(yr)time.agefloatnullableEBV6at? E(B-V) from Method 6a_{tau}_ (2)magphot.color.excessfloatnullabletau2at? {tau} from Method 2a_{tau}_ (2)Gyrtime.scalefloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainindexedHmag[12.7/32.1]? Observed magnitude in WFC3 F160W filtermagphot.mag;em.UV.100-200nmfloatnullableSNR[0/9999] H-band Signal-to-noise ratio (1)stat.snrfloatqph[0/18] Photometry flag; 0=ok, >0=bad photometrymeta.code.qualintStar[0/1] Spectroscopic star (1=spec. star)src.classintS/G[0/1] SExtractor stellarity index on F160W band (1=star)src.class.starGalaxyfloatAGN[0/1] Xray AGN from Xue et al. 2011; J/ApJS/195/10src.classintzbest[0/9.92] Redshift (2)src.redshift;pos.heliocentricfloatzsp[0/6.7]? Spectroscopic redshiftsrc.redshiftdoublenullableq_zsp[1/4]? Quality of spectroscopic redshift; 1=good, 2=intermediate, 3=uncertainmeta.code.qualintnullabler_zspReference spectroscopic survey (see refs.dat file)meta.ref;pos.framecharzph[0.009/9.92] Photometric redshift (3)src.redshiftfloatb_zph? Lower zph 68% confidence limitstat.fit.paramfloatnullableb_zph2? Lower zph 95% confidence limitstat.fit.paramfloatnullableB_zph2? Upper zph 95% confidence limitstat.fit.paramfloatnullablezAGN? Photometric redshift for AGNs from Hsu et al 2014ApJ...796...60H; where ?=-99 for non AGN sources (only for table4a.dat)src.redshift;pos.heliocentricfloatnullableM? CANDELS reference median stellar mass M_med_ (4)solMassphys.massdoublenullablee_M? Standard deviation on M_med_ (5)solMassstat.errordoublenullableMneb? Median stellar mass including nebular component M^neb^ (6)solMassphys.massdoublenullablee_Mneb? Standard deviation on M^neb^ (5)solMassstat.errordoublenullabledMz? Relative uncertainty due to model degeneracy and zphot scatter (7)stat.errorfloatnullableM2at? Stellar mass from Method 2a_{tau}_ (8)log(solMass)phys.massfloatnullableM2dt? Stellar mass from Method 2d_{tau}_ (8)log(solMass)phys.massfloatnullableM6at? Stellar mass from Method 6a_{tau}_ (8)log(solMass)phys.massfloatnullableM10c? Stellar mass from Method 10c (8)log(solMass)phys.massfloatnullableM11at? Stellar mass from Method 11a_{tau}_ (8)log(solMass)phys.massfloatnullableM12a? Stellar mass from Method 12a (8)log(solMass)phys.massfloatnullableM13at? Stellar mass from Method 13a_{tau}_ (8)log(solMass)phys.massfloatnullableM14a? Stellar mass from Method 14a (8)log(solMass)phys.massfloatnullableM15a? Stellar mass from Method 15a (8)log(solMass)phys.massfloatnullableM6atNEB? Stellar mass from Method 6a_{tau}_^NEB^ (8)log(solMass)phys.massfloatnullableM6adt? Stellar mass from Method 6a_del{tau}_ (8)log(solMass)phys.massfloatnullableM6ainvt? Stellar mass from Method 6a_inv{tau}_(8)log(solMass)phys.massfloatnullableM10cdust? Stellar mass from Method 10c^dust^ (8)log(solMass)phys.massfloatnullableM12at? Stellar mass from Method 12a_{tau}_ (8)log(solMass)phys.massfloatnullableM14acst? Stellar mass from Method 14a_const_ (9)log(solMass)phys.massfloatnullableM14alin? Stellar mass from Method 14a_lin_ (9)log(solMass)phys.massfloatnullableM14adt? Stellar mass from Method 14a_del{tau}_(9)log(solMass)phys.massfloatnullableM14at? Stellar mass from Method 14a_{tau}_ (9)log(solMass)phys.massfloatnullableAv2at? Av from Method 2a_{tau}_ (2)magphys.absorptionfloatnullableSFR2at? SFR from Method 2a_{tau}_ (2)solMass/yrphys.SFRdoublenullableX2.2at? Reduced chi2 from Method 2a_{tau}_ (2)stat.fit.chi2doublenullableage2dt? Age from Method 2d_{tau}_ (2)log(yr)time.agefloatnullabletau2dt? {tau} from Method 2d_{tau}_ (2)Gyrtime.scalefloatnullableAv2dt? A_v_ from Method 2d_{tau}_ (2)magphys.absorptionfloatnullablemet2dt? Gas metallicity from Method 2d_{tau}_ (2)Sunphys.abundfloatnullableage4b? Age from Method 4b (table5b only) (2)log(yr)time.agefloatnullableEBV4b? E(B-V) from Method 4b (table5b only) (2)magphot.color.excessfloatnullableMl6at? Lower stellar mass 68% confidence limit from Method 6a_{tau}_ (2)log(solMass)phys.massfloatnullableMu6at? Upper stellar mass 68% confidence limit from Method 6a_{tau}_ (2)log(solMass)phys.massfloatnullableage6at? Age from Method 6a_{tau}_ (2)log(yr)time.agefloatnullabletau6at? {tau} from Method 6a_{tau}_ (2)Gyrtime.scalefloatnullableSFR6at? SFR from Method 6a_{tau}_ (2)solMass/yrphys.SFRdoublenullablemet6at? Gas metallicity from Method 6a_{tau}_ (2)Sunphys.abundfloatnullableel6at[1/2]? Extinction law from Method 6a_{tau}_; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6at? Reduced chi2 from Method 6a_{tau}_ (2)stat.fit.chi2doublenullableL1.6at? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6at? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6at? AB rest-frame magnitude in U band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableBM6at? AB rest-frame magnitude in B band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableVM6at? AB rest-frame magnitude in V band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableRM6at? AB rest-frame magnitude in R band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableIM6at? AB rest-frame magnitude in I band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableJM6at? AB rest-frame magnitude in J band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableKM6at? AB rest-frame magnitude in K band from Method 6a_{tau}_ (2)magphys.magAbsfloatnullableage10c? Age from Method 10c (2)log(yr)time.agefloatnullableSFH10c? Star formation history from Method 10c (2)(3)meta.codeintnullabletau10c? {tau} from Method 10c (2)Gyrtime.scalefloatnullablemet10c? Gas metallicity from Method 10c (2)Sunphys.abundfloatnullableMl11at? Lower stellar mass 99% confidence limit from Method 11a_{tau}_ (2)log(solMass)phys.massfloatnullableMu11at? Upper stellar mass 99% confidence limit from Method 11a_{tau}_ (2)log(solMass)phys.massfloatnullableage11at? Age from Method 11a_{tau}_ (2)log(yr)time.agefloatnullableSFR11at? SFR from Method 11a_{tau}_ (2)solMass/yrphys.SFRdoublenullableMl12a? Lower stellar mass 68% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableMu12a? Upper stellar mass 68% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableM2l12a? Lower stellar mass 95% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableM2u12a? Upper stellar mass 95% confidence limit from Method 12a (2)log(solMass)phys.massfloatnullableage12a? Age from Method 12a (2)log(yr)time.agefloatnullabletau12a? {tau} from Method 12a (2)Gyrtime.scalefloatnullableEBV12a? E(B-V) from Method 12a (2)magphot.color.excessfloatnullablemet12a? Gas metallicity from Method 12a (2)Sunphys.abundfloatnullableLb12a? Stellar bolometric luminosity corrected for dust extinction from Method 12a (2)(4)log(solLum)phys.luminosityfloatnullableX2.12a? Reduced chi2 from Method 12a (2)stat.fit.chi2doublenullableage13at? Age from Method 13a_{tau}_ (2)log(yr)time.agefloatnullabletau13at? {tau} from Method 13a_{tau}_ (2)Gyrtime.scalefloatnullableAv13at? Av from Method 13a_{tau}_ (2)magphys.absorptionfloatnullableSFR13at? SFR from Method 13a_{tau}_ (2)solMass/yrphys.SFRdoublenullableX2.13at? Reduced chi2 from Method 13a_{tau}_(2)stat.fit.chi2doublenullableage14a? Age from Method 14a (2)log(yr)time.agefloatnullableSFH14a? Star formation history from Method 14a (2)(5)meta.codeintnullabletau14a? {tau} from Method 14a (2)Gyrtime.scalefloatnullableEBV14a? E(B-V) from Method 14a (2)magphot.color.excessfloatnullableSFR14a? SFR from Method 14a (2)(5)solMass/yrphys.SFRdoublenullableq14a[1/3]? Quality of the fit from Method 14a; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage15a? Age from Method 15a (table5a only) (2)log(yr)time.agefloatnullabletau15a? {tau} from Method 15a (table5a only) (2)Gyrtime.scalefloatnullableEBV15a? E(B-V) from Method 15a (table5a only) (2)magphot.color.excessfloatnullablemet15a? Gas metallicity from Method 15a (table5a only) (2)Sunphys.abundfloatnullableage6atNEB? Age from Method 6a_{tau}_^NEB^ (2)log(yr)time.agefloatnullabletau6atNEB? {tau} from Method 6a_{tau}_^NEB^ (2)Gyrtime.scalefloatnullableEBV6atNEB? E(B-V) from Method 6a_{tau}_^NEB^ (2)magphot.color.excessfloatnullableSFR6atNEB? SFR from Method 6a_{tau}_^NEB^ (2)solMass/yrphys.SFRdoublenullablemet6atNEB? Gas metallicity from Method 6a_{tau}_^NEB^ (2)Sunphys.abundfloatnullableel6atNEB[1/2]? Extinction law from Method 6a_{tau}_^NEB^; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6atNEB? Reduced chi2 from Method 6a_{tau}_^NEB^ (2)stat.fit.chi2doublenullableL1.6atNEB? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_{tau}_^NEB^; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6atNEB? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_{tau}_^NEB^; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6atNEB? AB rest-frame magnitude in U band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableBM6atNEB? AB rest-frame magnitude in B band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableVM6atNEB? AB rest-frame magnitude in V band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableRM6atNEB? AB rest-frame magnitude in R band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableIM6atNEB? AB rest-frame magnitude in I band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableJM6atNEB? AB rest-frame magnitude in J band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableKM6atNEB? AB rest-frame magnitude in K band from Method 6a_{tau}_^NEB^ (2)magphys.magAbsfloatnullableage-6adt? Age from Method 6a_del{tau}_ (2)log(yr)time.agefloatnullabletau-6adt? {tau} from Method 6a_del{tau}_ (2)Gyrtime.scalefloatnullableEBV-6adt? E(B-V) from Method 6a_del{tau}_ (2)magphot.color.excessfloatnullableSFR-6adt? SFR from Method 6a_del{tau}_ (2)solMass/yrphys.SFRdoublenullablemet-6adt? Gas metallicity from Method 6a_del{tau}_ (2)Sunphys.abundfloatnullableel6ad? Extinction law from Method 6a_del{tau}_; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6adt? Reduced chi2 from Method 6a_del{tau}_ (2)stat.fit.chi2doublenullableL1.6adt? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_del{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6adt? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_del{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6adt? AB rest-frame magnitude in U band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableBM6adt? AB rest-frame magnitude in B band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableVM6adt? AB rest-frame magnitude in V band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableRM6adt? AB rest-frame magnitude in R band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableIM6adt? AB rest-frame magnitude in I band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableJM6adt? AB rest-frame magnitude in J band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableKM6adt? AB rest-frame magnitude in K band from Method 6a_del{tau}_ (2)magphys.magAbsfloatnullableage6ainvt? Age from Method 6a_inv{tau}_ (2)log(yr)time.agefloatnullabletau6ainvt? {tau} from Method 6a_inv{tau}_ (2)Gyrtime.scalefloatnullableEBV6ainvt? E(B-V) from Method 6a_inv{tau}_ (2)magphot.color.excessdoublenullableSFR6ainvt? SFR from Method 6a_inv{tau}_ (2)solMass/yrphys.SFRdoublenullablemet6ainvt? Gas metallicity from Method 6a_inv{tau}_ (2)Sunphys.abundfloatnullableel6ainvt[1/2]? Extinction law from Method 6a_inv{tau}_; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (2)phys.absorptionintnullableX2.6ainvt? Reduced chi2 from Method 6a_inv{tau}_ (2)stat.fit.chi2doublenullableL1.6ainvt? Rest-frame luminosity at 140nm L_{nu}_(140nm) from Method 6a_inv{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.100-200nmdoublenullableL2.6ainvt? Rest-frame luminosity at 270nm L_{nu}_(270nm) from Method 6a_inv{tau}_; erg/s/Hz (2)1e-07W.Hz**-1phys.luminosity;em.UV.200-300nmdoublenullableUM6ainvt? AB rest-frame magnitude in U band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableBM6ainvt? AB rest-frame magnitude in B band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableVM6ainvt? AB rest-frame magnitude in V band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableRM6ainvt? AB rest-frame magnitude in R band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableIM6ainvt? AB rest-frame magnitude in I band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableJM6ainvt? AB rest-frame magnitude in J band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableKM6ainvt? AB rest-frame magnitude in K band from Method 6a_inv{tau}_ (2)magphys.magAbsfloatnullableage10cdust? Age from Method 10c^dust^ (2)log(yr)time.agefloatnullableSFH10cdust? Star formation history from Method 10c^dust^ (2)(3)meta.codeintnullabletau10cdust? {tau} from Method 10c^dust^ (2)Gyrtime.scalefloatnullablemet10cdust? Gas metallicity from Method 10c^dust^ (2)Sunphys.abundfloatnullableage12at? Age from Method 12a_{tau}_ (2)log(yr)time.agefloatnullabletau12at? {tau} from Method 12a_{tau}_ (2)Gyrtime.scalefloatnullableEBV12at? E(B-V) from Method 12a_{tau}_ (2)magphot.color.excessfloatnullablemet12at? Gas metallicity from Method 12a_{tau}_ (2)Sunphys.abundfloatnullableLb12at? Stellar bolometric luminosity corrected for dust extinction from Method 12a (2)(4)log(solLum)phys.luminosityfloatnullableX2.12at? Reduced chi2 from Method 12a_{tau}_(2)stat.fit.chi2doublenullableage14acst? Age from Method 14a_const_ (2)log(yr)time.agefloatnullableEBV14acst? E(B-V) from Method 14a_const_ (2)magphot.color.excessdoublenullableSFR14acst? SFR from Method 14a_const_ (2)solMass/yrphys.SFRdoublenullableq14acst[1/3]? Quality of the fit from Method 14a_const_; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage14alin? Age from Method 14a_lin_ (2)log(yr)time.agefloatnullableEBV14alin? E(B-V) from Method 14a_lin_ (2)magphot.color.excessdoublenullableSFR14alin? SFR from Method 14a_lin_ (2)solMass/yrphys.SFRdoublenullableq14alin[1/3]? Quality of the fit from Method 14a_lin_; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage14adt? Age from Method 14a_del{tau}_ (2)log(yr)time.agefloatnullabletau14adt? {tau} from Method 14a_del{tau}_ (2)Gyrtime.scalefloatnullableEBV14adt? E(B-V) from Method 14a_del{tau}_ (2)magphot.color.excessdoublenullableSFR14adt? SFR from Method 14a_del{tau}_ (2)solMass/yrphys.SFRdoublenullableq14adt[1/3]? Quality of the fit from Method 14a_del{tau}_; 1:best; 2:good; others:bad (2)meta.code.qualintnullableage14at? Age from Method 14a_{tau}_ (2)log(yr)time.agefloatnullabletau14at? {tau} from Method 14a_{tau}_ (2)Gyrtime.scalefloatnullableEBV14at? E(B-V) from Method 14a_{tau}_ (2)magphot.color.excessdoublenullableSFR14at? SFR from Method 14a_{tau}_ (2)solMass/yrphys.SFRdoublenullableq14at[0/3] Quality of fit from Method 14a_{tau}; 1=best; 2=good; others=bad (2)meta.code.qualintJ/ApJ/801/97/table2Magellan/IMACS Redshift CatalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[10011963/30136160] Object identifier (1)meta.id;meta.mainintRAJ2000Right Ascension in decimal degrees (J2000) (1)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000) (1)degpos.eq.dec;meta.mainRmag[18/23.5] The R band AB magnitude (1)magphot.mag;em.opt.RfloatMaskIMACS slitmask namemeta.id;instrcharSlit[1/134] IMACS slitmask slit number corresponding to objectmeta.noteintMJDModified Julian Date of observationdtime.epochfloatz[-0.001/2.81]? Spectroscopic redshiftsrc.redshiftdoublenullableq_z[-2/4] Quality code on z (3 or 4 = secure) (2)meta.code.qual;src.redshiftintzHelio[-0.0011/2.81]? Heliocentric-frame redshiftsrc.redshift;pos.heliocentricdoublenullableJ/ApJ/801/97/refsReferencesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharf_RefFlag on Ref (1)meta.codecharBibCodeBibcode of the main referencemeta.bib.bibcodecharAutAuthor's name(s) of the main referencemeta.bib.authorcharCommComment (2)meta.notecharJ/ApJ/801/97/fig12Filter curves (figure 12)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFFilter (UBVRI or JK)meta.code;instr.filtercharlambda[2000/30000] Wavelength; Angstroms0.1nmem.wldoubleTrans[0/1] Normalized transmission valuephys.transmission;instr.filterdouble