VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/ApJ/801/97
  GOODS-S & UDS stellar mass catalogs from CANDELS (Santini+, 2015)
ReadMe+ftp
2015ApJ...801...97S
Similar Catalogs
filter
Post annotation 		img(gal)
1.J/ApJ/801/97/table2(c)Magellan/IMACS Redshift Catalog (502 rows)
2.J/ApJ/801/97/goodss(c)GOODS-S field stellar masses and other physical parameters (tables 4a and 5a) (34930 rows)
3.J/ApJ/801/97/uds(c)UDS field stellar masses and other physical parameters (tables 4b and 5b) (35932 rows)
4.J/ApJ/801/97/fig12Filter curves (figure 12) [filter](Plot) (29247 rows)
5.J/ApJ/801/97/refsReferences (111 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortJoin tables
more join
Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)ID   [10011963/30136160] Object identifier (Note 1)   (meta.id;meta.main)
  (1+2+3)RAJ2000 deg (i) Right Ascension in decimal degrees (J2000) (Note 1)   (pos.eq.ra;meta.main)
  (1+2+3)DEJ2000 deg (i) Declination in decimal degrees (J2000) (Note 1)   (pos.eq.dec;meta.main)
  (1)Rmag mag [18/23.5] The R band AB magnitude (Note 1)   (phot.mag;em.opt.R)
  (1)Mask (char) IMACS slitmask name (meta.id;instr)
  (1)Slit   [1/134] IMACS slitmask slit number corresponding to object (meta.note)
  (1)MJD d Modified Julian Date of observation (time.epoch)
  (1)z  (n) [-0.001/2.81] Spectroscopic redshift (src.redshift)
  (1)q_z   [-2/4] Quality code on z (3 or 4 = secure) (Note 2)   (meta.code.qual;src.redshift)
  (1)zHelio  (n) [-0.0011/2.81] Heliocentric-frame redshift (src.redshift;pos.heliocentric)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)Seq   [1/35932] Designation (Note G1)   (meta.id;meta.main)
  (2+3)Hmag mag (n) [12.7/32.1] Observed magnitude in WFC3 F160W filter (phot.mag;em.UV.100-200nm)
  (2+3)SNR   [0/9999] H-band Signal-to-noise ratio (Note 1)   (stat.snr)
  (2+3)qph   [0/18] Photometry flag; 0=ok, >0=bad photometry (meta.code.qual)
  (2+3)Star   [0/1] Spectroscopic star (1=spec. star) (src.class)
  (2+3)S/G   [0/1] SExtractor stellarity index on F160W band (1=star) (src.class.starGalaxy)
  (2+3)AGN   [0/1] Xray AGN from Xue et al. 2011; J/ApJS/195/10 (src.class)
  (2+3)zbest   [0/9.92] Redshift (Note 2)   (src.redshift;pos.heliocentric)
  (2+3)zsp  (n) [0/6.7] Spectroscopic redshift (src.redshift)
  (2+3)q_zsp  (n) [1/4] Quality of spectroscopic redshift; 1=good, 2=intermediate, 3=uncertain (meta.code.qual)
   (2+3)r_zsp (char) Reference spectroscopic survey (see refs.dat file) (meta.ref;pos.frame)
  (2+3)zph   [0.009/9.92] Photometric redshift (Note 3)   (src.redshift)
  (2+3)b_zph  (n) Lower zph 68% confidence limit (stat.fit.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)B_zph  (n) Upper zph 68% confidence limit (stat.fit.param)
  (2+3)b_zph2  (n) Lower zph 95% confidence limit (stat.fit.param)
  (2+3)B_zph2  (n) Upper zph 95% confidence limit (stat.fit.param)
  (2+3)zAGN  (n) Photometric redshift for AGNs from Hsu et al 2014ApJ...796...60H; where ?=-99 for non AGN sources (only for table4a.dat) (src.redshift;pos.heliocentric)
  (2+3)M Msun (n) CANDELS reference median stellar mass Mmed (Note 4)   (phys.mass)
  (2+3)e_M Msun (n) Standard deviation on Mmed (Note 5)   (stat.error)
  (2+3)Mneb Msun (n) Median stellar mass including nebular component Mneb (Note 6)   (phys.mass)
  (2+3)e_Mneb Msun (n) Standard deviation on Mneb (Note 5)   (stat.error)
  (2+3)dMz  (n) Relative uncertainty due to model degeneracy and zphot scatter (Note 7)   (stat.error)
  (2+3)M2at [Msun] (n) Stellar mass from Method 2a{tau} (Note 8)   (phys.mass)
  (2+3)M2dt [Msun] (n) Stellar mass from Method 2d{tau} (Note 8)   (phys.mass)
  (2+3)M6at [Msun] (n) Stellar mass from Method 6a{tau} (Note 8)   (phys.mass)
  (2+3)M10c [Msun] (n) Stellar mass from Method 10c (Note 8)   (phys.mass)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)M11at [Msun] (n) Stellar mass from Method 11a{tau} (Note 8)   (phys.mass)
  (2+3)M12a [Msun] (n) Stellar mass from Method 12a (Note 8)   (phys.mass)
  (2+3)M13at [Msun] (n) Stellar mass from Method 13a{tau} (Note 8)   (phys.mass)
  (2+3)M14a [Msun] (n) Stellar mass from Method 14a (Note 8)   (phys.mass)
  (2+3)M15a [Msun] (n) Stellar mass from Method 15a (Note 8)   (phys.mass)
  (2+3)M6atNEB [Msun] (n) Stellar mass from Method 6a{tau}NEB (Note 8)   (phys.mass)
  (2+3)M6adt [Msun] (n) Stellar mass from Method 6adel{tau} (Note 8)   (phys.mass)
  (2+3)M6ainvt [Msun] (n) Stellar mass from Method 6ainv{tau} (Note 8)   (phys.mass)
  (2+3)M10cdust [Msun] (n) Stellar mass from Method 10cdust (Note 8)   (phys.mass)
  (2+3)M12at [Msun] (n) Stellar mass from Method 12a{tau} (Note 8)   (phys.mass)
  (2+3)M14acst [Msun] (n) Stellar mass from Method 14aconst (Note 9)   (phys.mass)
  (2+3)M14alin [Msun] (n) Stellar mass from Method 14alin (Note 9)   (phys.mass)
  (2+3)M14adt [Msun] (n) Stellar mass from Method 14adel{tau} (Note 9)   (phys.mass)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)M14at [Msun] (n) Stellar mass from Method 14a{tau} (Note 9)   (phys.mass)
  (2+3)age2at [yr] (n) Age from Method 2a{tau} (Note 2)   (time.age)
  (2+3)tau2at Gyr (n) {tau} from Method 2a{tau} (Note 2)   (time.scale)
  (2+3)Av2at mag (n) Av from Method 2a{tau} (Note 2)   (phys.absorption)
  (2+3)SFR2at Msun/yr (n) SFR from Method 2a{tau} (Note 2)   (phys.SFR)
  (2+3)X2.2at  (n) Reduced chi2 from Method 2a{tau} (Note 2)   (stat.fit.chi2)
  (2+3)age2dt [yr] (n) Age from Method 2d{tau} (Note 2)   (time.age)
  (2+3)tau2dt Gyr (n) {tau} from Method 2d{tau} (Note 2)   (time.scale)
  (2+3)Av2dt mag (n) Av from Method 2d{tau} (Note 2)   (phys.absorption)
  (2+3)met2dt Sun (n) Gas metallicity from Method 2d{tau} (Note 2)   (phys.abund)
  (2+3)age4b [yr] (n) Age from Method 4b (table5b only) (Note 2)   (time.age)
  (2+3)EBV4b mag (n) E(B-V) from Method 4b (table5b only) (Note 2)   (phot.color.excess)
  (2+3)Ml6at [Msun] (n) Lower stellar mass 68% confidence limit from Method 6a{tau} (Note 2)   (phys.mass)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)Mu6at [Msun] (n) Upper stellar mass 68% confidence limit from Method 6a{tau} (Note 2)   (phys.mass)
  (2+3)age6at [yr] (n) Age from Method 6a{tau} (Note 2)   (time.age)
  (2+3)tau6at Gyr (n) {tau} from Method 6a{tau} (Note 2)   (time.scale)
  (2+3)EBV6at mag (n) E(B-V) from Method 6a{tau} (Note 2)   (phot.color.excess)
  (2+3)SFR6at Msun/yr (n) SFR from Method 6a{tau} (Note 2)   (phys.SFR)
  (2+3)met6at Sun (n) Gas metallicity from Method 6a{tau} (Note 2)   (phys.abund)
  (2+3)el6at  (n) [1/2] Extinction law from Method 6a{tau}; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2)   (phys.absorption)
  (2+3)X2.6at  (n) Reduced chi2 from Method 6a{tau} (Note 2)   (stat.fit.chi2)
  (2+3)L1.6at 10-7W/Hz (n) Rest-frame luminosity at 140nm L{nu}(140nm) from Method 6a{tau}; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.100-200nm)
  (2+3)L2.6at 10-7W/Hz (n) Rest-frame luminosity at 270nm L{nu}(270nm) from Method 6a{tau}; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.200-300nm)
  (2+3)UM6at mag (n) AB rest-frame magnitude in U band from Method 6a{tau} (Note 2)   (phys.magAbs)
  (2+3)BM6at mag (n) AB rest-frame magnitude in B band from Method 6a{tau} (Note 2)   (phys.magAbs)
  (2+3)VM6at mag (n) AB rest-frame magnitude in V band from Method 6a{tau} (Note 2)   (phys.magAbs)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)RM6at mag (n) AB rest-frame magnitude in R band from Method 6a{tau} (Note 2)   (phys.magAbs)
  (2+3)IM6at mag (n) AB rest-frame magnitude in I band from Method 6a{tau} (Note 2)   (phys.magAbs)
  (2+3)JM6at mag (n) AB rest-frame magnitude in J band from Method 6a{tau} (Note 2)   (phys.magAbs)
  (2+3)KM6at mag (n) AB rest-frame magnitude in K band from Method 6a{tau} (Note 2)   (phys.magAbs)
  (2+3)age10c [yr] (n) Age from Method 10c (Note 2)   (time.age)
  (2+3)SFH10c  (n) Star formation history from Method 10c (2) (Note 3)   (meta.code)
  (2+3)tau10c Gyr (n) {tau} from Method 10c (Note 2)   (time.scale)
  (2+3)met10c Sun (n) Gas metallicity from Method 10c (Note 2)   (phys.abund)
  (2+3)Ml11at [Msun] (n) Lower stellar mass 99% confidence limit from Method 11a{tau} (Note 2)   (phys.mass)
  (2+3)Mu11at [Msun] (n) Upper stellar mass 99% confidence limit from Method 11a{tau} (Note 2)   (phys.mass)
  (2+3)age11at [yr] (n) Age from Method 11a{tau} (Note 2)   (time.age)
  (2+3)SFR11at Msun/yr (n) SFR from Method 11a{tau} (Note 2)   (phys.SFR)
  (2+3)Ml12a [Msun] (n) Lower stellar mass 68% confidence limit from Method 12a (Note 2)   (phys.mass)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)Mu12a [Msun] (n) Upper stellar mass 68% confidence limit from Method 12a (Note 2)   (phys.mass)
  (2+3)M2l12a [Msun] (n) Lower stellar mass 95% confidence limit from Method 12a (Note 2)   (phys.mass)
  (2+3)M2u12a [Msun] (n) Upper stellar mass 95% confidence limit from Method 12a (Note 2)   (phys.mass)
  (2+3)age12a [yr] (n) Age from Method 12a (Note 2)   (time.age)
  (2+3)tau12a Gyr (n) {tau} from Method 12a (Note 2)   (time.scale)
  (2+3)EBV12a mag (n) E(B-V) from Method 12a (Note 2)   (phot.color.excess)
  (2+3)met12a Sun (n) Gas metallicity from Method 12a (Note 2)   (phys.abund)
  (2+3)Lb12a [Lsun] (n) Stellar bolometric luminosity corrected for dust extinction from Method 12a (2) (Note 4)   (phys.luminosity)
  (2+3)X2.12a  (n) Reduced chi2 from Method 12a (Note 2)   (stat.fit.chi2)
  (2+3)age13at [yr] (n) Age from Method 13a{tau} (Note 2)   (time.age)
  (2+3)tau13at Gyr (n) {tau} from Method 13a{tau} (Note 2)   (time.scale)
  (2+3)Av13at mag (n) Av from Method 13a{tau} (Note 2)   (phys.absorption)
  (2+3)SFR13at Msun/yr (n) SFR from Method 13a{tau} (Note 2)   (phys.SFR)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)X2.13at  (n) Reduced chi2 from Method 13a{tau} (Note 2)   (stat.fit.chi2)
  (2+3)age14a [yr] (n) Age from Method 14a (Note 2)   (time.age)
  (2+3)SFH14a  (n) Star formation history from Method 14a (2) (Note 5)   (meta.code)
  (2+3)tau14a Gyr (n) {tau} from Method 14a (Note 2)   (time.scale)
  (2+3)EBV14a mag (n) E(B-V) from Method 14a (Note 2)   (phot.color.excess)
  (2+3)SFR14a Msun/yr (n) SFR from Method 14a (2) (Note 5)   (phys.SFR)
  (2+3)q14a  (n) [1/3] Quality of the fit from Method 14a; 1:best; 2:good; others:bad (Note 2)   (meta.code.qual)
  (2+3)age15a [yr] (n) Age from Method 15a (table5a only) (Note 2)   (time.age)
  (2+3)tau15a Gyr (n) {tau} from Method 15a (table5a only) (Note 2)   (time.scale)
  (2+3)EBV15a mag (n) E(B-V) from Method 15a (table5a only) (Note 2)   (phot.color.excess)
  (2+3)met15a Sun (n) Gas metallicity from Method 15a (table5a only) (Note 2)   (phys.abund)
  (2+3)age6atNEB [yr] (n) Age from Method 6a{tau}NEB (Note 2)   (time.age)
  (2+3)tau6atNEB Gyr (n) {tau} from Method 6a{tau}NEB (Note 2)   (time.scale)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)EBV6atNEB mag (n) E(B-V) from Method 6a{tau}NEB (Note 2)   (phot.color.excess)
  (2+3)SFR6atNEB Msun/yr (n) SFR from Method 6a{tau}NEB (Note 2)   (phys.SFR)
  (2+3)met6atNEB Sun (n) Gas metallicity from Method 6a{tau}NEB (Note 2)   (phys.abund)
  (2+3)el6atNEB  (n) [1/2] Extinction law from Method 6a{tau}NEB; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2)   (phys.absorption)
  (2+3)X2.6atNEB  (n) Reduced chi2 from Method 6a{tau}NEB (Note 2)   (stat.fit.chi2)
  (2+3)L1.6atNEB 10-7W/Hz (n) Rest-frame luminosity at 140nm L{nu}(140nm) from Method 6a{tau}NEB; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.100-200nm)
  (2+3)L2.6atNEB 10-7W/Hz (n) Rest-frame luminosity at 270nm L{nu}(270nm) from Method 6a{tau}NEB; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.200-300nm)
  (2+3)UM6atNEB mag (n) AB rest-frame magnitude in U band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)
  (2+3)BM6atNEB mag (n) AB rest-frame magnitude in B band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)
  (2+3)VM6atNEB mag (n) AB rest-frame magnitude in V band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)
  (2+3)RM6atNEB mag (n) AB rest-frame magnitude in R band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)
  (2+3)IM6atNEB mag (n) AB rest-frame magnitude in I band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)
  (2+3)JM6atNEB mag (n) AB rest-frame magnitude in J band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)KM6atNEB mag (n) AB rest-frame magnitude in K band from Method 6a{tau}NEB (Note 2)   (phys.magAbs)
  (2+3)age-6adt [yr] (n) Age from Method 6adel{tau} (Note 2)   (time.age)
  (2+3)tau-6adt Gyr (n) {tau} from Method 6adel{tau} (Note 2)   (time.scale)
  (2+3)EBV-6adt mag (n) E(B-V) from Method 6adel{tau} (Note 2)   (phot.color.excess)
  (2+3)SFR-6adt Msun/yr (n) SFR from Method 6adel{tau} (Note 2)   (phys.SFR)
  (2+3)met-6adt Sun (n) Gas metallicity from Method 6adel{tau} (Note 2)   (phys.abund)
  (2+3)el6ad  (n) Extinction law from Method 6adel{tau}; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2)   (phys.absorption)
  (2+3)X2.6adt  (n) Reduced chi2 from Method 6adel{tau} (Note 2)   (stat.fit.chi2)
  (2+3)L1.6adt 10-7W/Hz (n) Rest-frame luminosity at 140nm L{nu}(140nm) from Method 6adel{tau}; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.100-200nm)
  (2+3)L2.6adt 10-7W/Hz (n) Rest-frame luminosity at 270nm L{nu}(270nm) from Method 6adel{tau}; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.200-300nm)
  (2+3)UM6adt mag (n) AB rest-frame magnitude in U band from Method 6adel{tau} (Note 2)   (phys.magAbs)
  (2+3)BM6adt mag (n) AB rest-frame magnitude in B band from Method 6adel{tau} (Note 2)   (phys.magAbs)
  (2+3)VM6adt mag (n) AB rest-frame magnitude in V band from Method 6adel{tau} (Note 2)   (phys.magAbs)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)RM6adt mag (n) AB rest-frame magnitude in R band from Method 6adel{tau} (Note 2)   (phys.magAbs)
  (2+3)IM6adt mag (n) AB rest-frame magnitude in I band from Method 6adel{tau} (Note 2)   (phys.magAbs)
  (2+3)JM6adt mag (n) AB rest-frame magnitude in J band from Method 6adel{tau} (Note 2)   (phys.magAbs)
  (2+3)KM6adt mag (n) AB rest-frame magnitude in K band from Method 6adel{tau} (Note 2)   (phys.magAbs)
  (2+3)age6ainvt [yr] (n) Age from Method 6ainv{tau} (Note 2)   (time.age)
  (2+3)tau6ainvt Gyr (n) {tau} from Method 6ainv{tau} (Note 2)   (time.scale)
  (2+3)EBV6ainvt mag (n) E(B-V) from Method 6ainv{tau} (Note 2)   (phot.color.excess)
  (2+3)SFR6ainvt Msun/yr (n) SFR from Method 6ainv{tau} (Note 2)   (phys.SFR)
  (2+3)met6ainvt Sun (n) Gas metallicity from Method 6ainv{tau} (Note 2)   (phys.abund)
  (2+3)el6ainvt  (n) [1/2] Extinction law from Method 6ainv{tau}; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2)   (phys.absorption)
  (2+3)X2.6ainvt  (n) Reduced chi2 from Method 6ainv{tau} (Note 2)   (stat.fit.chi2)
  (2+3)L1.6ainvt 10-7W/Hz (n) Rest-frame luminosity at 140nm L{nu}(140nm) from Method 6ainv{tau}; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.100-200nm)
  (2+3)L2.6ainvt 10-7W/Hz (n) Rest-frame luminosity at 270nm L{nu}(270nm) from Method 6ainv{tau}; erg/s/Hz (Note 2)   (phys.luminosity;em.UV.200-300nm)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)UM6ainvt mag (n) AB rest-frame magnitude in U band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)BM6ainvt mag (n) AB rest-frame magnitude in B band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)VM6ainvt mag (n) AB rest-frame magnitude in V band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)RM6ainvt mag (n) AB rest-frame magnitude in R band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)IM6ainvt mag (n) AB rest-frame magnitude in I band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)JM6ainvt mag (n) AB rest-frame magnitude in J band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)KM6ainvt mag (n) AB rest-frame magnitude in K band from Method 6ainv{tau} (Note 2)   (phys.magAbs)
  (2+3)age10cdust [yr] (n) Age from Method 10cdust (Note 2)   (time.age)
  (2+3)SFH10cdust  (n) Star formation history from Method 10cdust (2) (Note 3)   (meta.code)
  (2+3)tau10cdust Gyr (n) {tau} from Method 10cdust (Note 2)   (time.scale)
  (2+3)met10cdust Sun (n) Gas metallicity from Method 10cdust (Note 2)   (phys.abund)
  (2+3)age12at [yr] (n) Age from Method 12a{tau} (Note 2)   (time.age)
  (2+3)tau12at Gyr (n) {tau} from Method 12a{tau} (Note 2)   (time.scale)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)EBV12at mag (n) E(B-V) from Method 12a{tau} (Note 2)   (phot.color.excess)
  (2+3)met12at Sun (n) Gas metallicity from Method 12a{tau} (Note 2)   (phys.abund)
  (2+3)Lb12at [Lsun] (n) Stellar bolometric luminosity corrected for dust extinction from Method 12a (2) (Note 4)   (phys.luminosity)
  (2+3)X2.12at  (n) Reduced chi2 from Method 12a{tau} (Note 2)   (stat.fit.chi2)
  (2+3)age14acst [yr] (n) Age from Method 14aconst (Note 2)   (time.age)
  (2+3)EBV14acst mag (n) E(B-V) from Method 14aconst (Note 2)   (phot.color.excess)
  (2+3)SFR14acst Msun/yr (n) SFR from Method 14aconst (Note 2)   (phys.SFR)
  (2+3)q14acst  (n) [1/3] Quality of the fit from Method 14aconst; 1:best; 2:good; others:bad (Note 2)   (meta.code.qual)
  (2+3)age14alin [yr] (n) Age from Method 14alin (Note 2)   (time.age)
  (2+3)EBV14alin mag (n) E(B-V) from Method 14alin (Note 2)   (phot.color.excess)
  (2+3)SFR14alin Msun/yr (n) SFR from Method 14alin (Note 2)   (phys.SFR)
  (2+3)q14alin  (n) [1/3] Quality of the fit from Method 14alin; 1:best; 2:good; others:bad (Note 2)   (meta.code.qual)
  (2+3)age14adt [yr] (n) Age from Method 14adel{tau} (Note 2)   (time.age)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)tau14adt Gyr (n) {tau} from Method 14adel{tau} (Note 2)   (time.scale)
  (2+3)EBV14adt mag (n) E(B-V) from Method 14adel{tau} (Note 2)   (phot.color.excess)
  (2+3)SFR14adt Msun/yr (n) SFR from Method 14adel{tau} (Note 2)   (phys.SFR)
  (2+3)q14adt  (n) [1/3] Quality of the fit from Method 14adel{tau}; 1:best; 2:good; others:bad (Note 2)   (meta.code.qual)
  (2+3)age14at [yr] (n) Age from Method 14a{tau} (Note 2)   (time.age)
  (2+3)tau14at Gyr (n) {tau} from Method 14a{tau} (Note 2)   (time.scale)
  (2+3)EBV14at mag (n) E(B-V) from Method 14a{tau} (Note 2)   (phot.color.excess)
  (2+3)SFR14at Msun/yr (n) SFR from Method 14a{tau} (Note 2)   (phys.SFR)
  (2+3)q14at   [0/3] Quality of fit from Method 14a_{tau}; 1=best; 2=good; others=bad (Note 2)   (meta.code.qual)
  (4)F (char) Filter (UBVRI or JK) (meta.code;instr.filter)
  (4)lambda 0.1nm [2000/30000] Wavelength; Angstroms (em.wl)
  (4)Trans   [0/1] Normalized transmission value (phys.transmission;instr.filter)
  (5)Ref (char) Reference code (meta.note)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)f_Ref (char) Flag on Ref (Note 1)   (meta.code)
  (5)BibCode (char) Bibcode of the main reference (meta.bib.bibcode)
  (5)Aut (char) Author's name(s) of the main reference (meta.bib.author)
  (5)Comm (char) Comment (Note 2)   (meta.note)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
Adapt form
 Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0