| J/ApJ/801/97/goodss | GOODS-S & UDS stellar mass catalogs from CANDELS (Santini+, 2015) GOODS-S field stellar masses and other physical parameters (tables 4a and 5a) (34930 rows) | recno=3816 |
| Column | Value | Explain (UCD) | |
| _RAJ2000 | 03 32 33.59987 | "h:m:s" | Right ascension (FK5, Equinox=J2000.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra) |
| _DEJ2000 | -27 52 42.3870 | "d:m:s" | Declination (FK5, Equinox=J2000.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec) |
| _RAB1950 | 03 30 28.12661 | "h:m:s" | Right ascension (FK4, Equinox=B1950.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra) |
| _DEB1950 | -28 02 47.2708 | "d:m:s" | Declination (FK4, Equinox=B1950.0) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec) |
| _Glon | 223.69760959 | deg | Galactic longitude (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lon) |
| _Glat | -54.42739726 | deg | Galactic latitude (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lat) |
| 3816recno | 3816 | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) | |
| Seq | 3816 | [1/35932] Designation (Note G1) (meta.id;meta.main) | |
| RAJ2000 | 053.139999 | deg | (i) Right ascension in decimal degrees (J2000) (pos.eq.ra;meta.main) |
| DEJ2000 | -27.878441 | deg | (i) Declination in decimal degrees (J2000) (pos.eq.dec;meta.main) |
| Hmag | 20.73 | mag | [12.7/32.1] Observed magnitude in WFC3 F160W filter (phot.mag;em.UV.100-200nm) |
| SNR | 344.30 | [0/9999] H-band Signal-to-noise ratio (Note 1) (stat.snr) | |
| qph | 0 | [0/18] Photometry flag; 0=ok, >0=bad photometry (meta.code.qual) | |
| Star | 0 | [0/1] Spectroscopic star (1=spec. star) (src.class) | |
| S/G | 0.00 | [0/1] SExtractor stellarity index on F160W band (1=star) (src.class.starGalaxy) | |
| AGN | 0 | [0/1] Xray AGN from Xue et al. 2011; J/ApJS/195/10 (src.class) | |
| zbest | 0.1410 | [0/9.92] Redshift (Note 2) (src.redshift;pos.heliocentric) | |
| zsp | 0.1474 | [0/6.7] Spectroscopic redshift (src.redshift) | |
| q_zsp | 2 | [1/4] Quality of spectroscopic redshift; 1=good, 2=intermediate, 3=uncertain (meta.code.qual) | |
| r_zsp | 112 | Reference spectroscopic survey (see refs.dat file) (meta.ref;pos.frame) | |
| zph | 0.141 | [0.009/9.92] Photometric redshift (Note 3) (src.redshift) | |
| b_zph | 0.09 | Lower zph 68% confidence limit (stat.fit.param) | |
| B_zph | 0.18 | Upper zph 68% confidence limit (stat.fit.param) | |
| b_zph2 | 0.05 | Lower zph 95% confidence limit (stat.fit.param) | |
| B_zph2 | 0.23 | Upper zph 95% confidence limit (stat.fit.param) | |
| zAGN | -99.000 | 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) | |
| M | 3.85e+08 | Msun | CANDELS reference median stellar mass Mmed (Note 4) (phys.mass) |
| e_M | 1.21e+08 | Msun | Standard deviation on Mmed (Note 5) (stat.error) |
| Mneb | 4.02e+08 | Msun | Median stellar mass including nebular component Mneb (Note 6) (phys.mass) |
| e_Mneb | 1.16e+08 | Msun | Standard deviation on Mneb (Note 5) (stat.error) |
| dMz | 0.223 | Relative uncertainty due to model degeneracy and zphot scatter (Note 7) (stat.error) | |
| M2at | 8.56 | [Msun] | Stellar mass from Method 2aτ (Note 8) (phys.mass) |
| M2dt | 8.76 | [Msun] | Stellar mass from Method 2dτ (Note 8) (phys.mass) |
| M6at | 8.81 | [Msun] | Stellar mass from Method 6aτ (Note 8) (phys.mass) |
| M10c | 8.36 | [Msun] | Stellar mass from Method 10c (Note 8) (phys.mass) |
| M11at | 8.59 | [Msun] | Stellar mass from Method 11aτ (Note 8) (phys.mass) |
| M12a | 8.72 | [Msun] | Stellar mass from Method 12a (Note 8) (phys.mass) |
| M13at | 8.58 | [Msun] | Stellar mass from Method 13aτ (Note 8) (phys.mass) |
| M14a | 8.46 | [Msun] | Stellar mass from Method 14a (Note 8) (phys.mass) |
| M15a | 8.54 | [Msun] | Stellar mass from Method 15a (Note 8) (phys.mass) |
| M6atNEB | 8.71 | [Msun] | Stellar mass from Method 6aτNEB (Note 8) (phys.mass) |
| M6adt | 8.78 | [Msun] | Stellar mass from Method 6adelτ (Note 8) (phys.mass) |
| M6ainvt | 8.81 | [Msun] | Stellar mass from Method 6ainvτ (Note 8) (phys.mass) |
| M10cdust | 8.58 | [Msun] | Stellar mass from Method 10cdust (Note 8) (phys.mass) |
| M12at | 8.72 | [Msun] | Stellar mass from Method 12aτ (Note 8) (phys.mass) |
| M14acst | 8.73 | [Msun] | Stellar mass from Method 14aconst (Note 9) (phys.mass) |
| M14alin | 8.64 | [Msun] | Stellar mass from Method 14alin (Note 9) (phys.mass) |
| M14adt | 8.46 | [Msun] | Stellar mass from Method 14adelτ (Note 9) (phys.mass) |
| M14at | 8.46 | [Msun] | Stellar mass from Method 14aτ (Note 9) (phys.mass) |
| age2at | 9.1 | [yr] | Age from Method 2aτ (Note 2) (time.age) |
| tau2at | 0.300 | Gyr | τ from Method 2aτ (Note 2) (time.scale) |
| Av2at | 0.1 | mag | Av from Method 2aτ (Note 2) (phys.absorption) |
| SFR2at | 3.600e-02 | Msun/yr | SFR from Method 2aτ (Note 2) (phys.SFR) |
| X2.2at | 1.49e+02 | Reduced chi2 from Method 2aτ (Note 2) (stat.fit.chi2) | |
| age2dt | [yr] | Age from Method 2dτ (Note 2) (time.age) | |
| tau2dt | 0.000 | Gyr | τ from Method 2dτ (Note 2) (time.scale) |
| Av2dt | 0.0 | mag | Av from Method 2dτ (Note 2) (phys.absorption) |
| met2dt | 1.000 | Sun | Gas metallicity from Method 2dτ (Note 2) (phys.abund) |
| age4b | [yr] | Age from Method 4b (table5b only) (Note 2) (time.age) | |
| EBV4b | mag | E(B-V) from Method 4b (table5b only) (Note 2) (phot.color.excess) | |
| Ml6at | 8.61 | [Msun] | Lower stellar mass 68% confidence limit from Method 6aτ (Note 2) (phys.mass) |
| Mu6at | 8.96 | [Msun] | Upper stellar mass 68% confidence limit from Method 6aτ (Note 2) (phys.mass) |
| age6at | 9.70 | [yr] | Age from Method 6aτ (Note 2) (time.age) |
| tau6at | 2.0 | Gyr | τ from Method 6aτ (Note 2) (time.scale) |
| EBV6at | 0.03 | mag | E(B-V) from Method 6aτ (Note 2) (phot.color.excess) |
| SFR6at | 5.000e-02 | Msun/yr | SFR from Method 6aτ (Note 2) (phys.SFR) |
| met6at | 0.20 | Sun | Gas metallicity from Method 6aτ (Note 2) (phys.abund) |
| el6at | 1 | [1/2] Extinction law from Method 6aτ; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2) (phys.absorption) | |
| X2.6at | 9.99e-01 | Reduced chi2 from Method 6aτ (Note 2) (stat.fit.chi2) | |
| L1.6at | 6.11e+26 | 10-7W/Hz | Rest-frame luminosity at 140nm Lν(140nm) from Method 6aτ; erg/s/Hz (Note 2) (phys.luminosity;em.UV.100-200nm) |
| L2.6at | 7.72e+26 | 10-7W/Hz | Rest-frame luminosity at 270nm Lν(270nm) from Method 6aτ; erg/s/Hz (Note 2) (phys.luminosity;em.UV.200-300nm) |
| UM6at | -16.26 | mag | AB rest-frame magnitude in U band from Method 6aτ (Note 2) (phys.magAbs) |
| BM6at | -17.14 | mag | AB rest-frame magnitude in B band from Method 6aτ (Note 2) (phys.magAbs) |
| VM6at | -17.59 | mag | AB rest-frame magnitude in V band from Method 6aτ (Note 2) (phys.magAbs) |
| RM6at | -17.80 | mag | AB rest-frame magnitude in R band from Method 6aτ (Note 2) (phys.magAbs) |
| IM6at | -18.01 | mag | AB rest-frame magnitude in I band from Method 6aτ (Note 2) (phys.magAbs) |
| JM6at | -18.22 | mag | AB rest-frame magnitude in J band from Method 6aτ (Note 2) (phys.magAbs) |
| KM6at | -17.97 | mag | AB rest-frame magnitude in K band from Method 6aτ (Note 2) (phys.magAbs) |
| age10c | 8.557 | [yr] | Age from Method 10c (Note 2) (time.age) |
| SFH10c | 3 | Star formation history from Method 10c (2) (Note 3) (meta.code) | |
| tau10c | 0.1 | Gyr | τ from Method 10c (Note 2) (time.scale) |
| met10c | 0.5 | Sun | Gas metallicity from Method 10c (Note 2) (phys.abund) |
| Ml11at | 8.38 | [Msun] | Lower stellar mass 99% confidence limit from Method 11aτ (Note 2) (phys.mass) |
| Mu11at | 8.83 | [Msun] | Upper stellar mass 99% confidence limit from Method 11aτ (Note 2) (phys.mass) |
| age11at | 9.722 | [yr] | Age from Method 11aτ (Note 2) (time.age) |
| SFR11at | 5.000e-02 | Msun/yr | SFR from Method 11aτ (Note 2) (phys.SFR) |
| Ml12a | 8.40 | [Msun] | Lower stellar mass 68% confidence limit from Method 12a (Note 2) (phys.mass) |
| Mu12a | 8.90 | [Msun] | Upper stellar mass 68% confidence limit from Method 12a (Note 2) (phys.mass) |
| M2l12a | 8.32 | [Msun] | Lower stellar mass 95% confidence limit from Method 12a (Note 2) (phys.mass) |
| M2u12a | 8.97 | [Msun] | Upper stellar mass 95% confidence limit from Method 12a (Note 2) (phys.mass) |
| age12a | 9.477 | [yr] | Age from Method 12a (Note 2) (time.age) |
| tau12a | 0.6 | Gyr | τ from Method 12a (Note 2) (time.scale) |
| EBV12a | 0.050 | mag | E(B-V) from Method 12a (Note 2) (phot.color.excess) |
| met12a | 0.2 | Sun | Gas metallicity from Method 12a (Note 2) (phys.abund) |
| Lb12a | 9.32 | [Lsun] | Stellar bolometric luminosity corrected for dust extinction from Method 12a (2) (Note 4) (phys.luminosity) |
| X2.12a | 2.00e-01 | Reduced chi2 from Method 12a (Note 2) (stat.fit.chi2) | |
| age13at | 9.0 | [yr] | Age from Method 13aτ (Note 2) (time.age) |
| tau13at | 0.316 | Gyr | τ from Method 13aτ (Note 2) (time.scale) |
| Av13at | 0.4 | mag | Av from Method 13aτ (Note 2) (phys.absorption) |
| SFR13at | 8.510e-02 | Msun/yr | SFR from Method 13aτ (Note 2) (phys.SFR) |
| X2.13at | 7.40e-01 | Reduced chi2 from Method 13aτ (Note 2) (stat.fit.chi2) | |
| age14a | 9.139 | [yr] | Age from Method 14a (Note 2) (time.age) |
| SFH14a | 4 | Star formation history from Method 14a (2) (Note 5) (meta.code) | |
| tau14a | 0.315 | Gyr | τ from Method 14a (Note 2) (time.scale) |
| EBV14a | 0.024 | mag | E(B-V) from Method 14a (Note 2) (phot.color.excess) |
| SFR14a | 1.900e-02 | Msun/yr | SFR from Method 14a (2) (Note 5) (phys.SFR) |
| q14a | 1 | [1/3] Quality of the fit from Method 14a; 1:best; 2:good; others:bad (Note 2) (meta.code.qual) | |
| age15a | 9.230 | [yr] | Age from Method 15a (table5a only) (Note 2) (time.age) |
| tau15a | 0.3 | Gyr | τ from Method 15a (table5a only) (Note 2) (time.scale) |
| EBV15a | 0.075 | mag | E(B-V) from Method 15a (table5a only) (Note 2) (phot.color.excess) |
| met15a | 0.2 | Sun | Gas metallicity from Method 15a (table5a only) (Note 2) (phys.abund) |
| age6atNEB | 9.60 | [yr] | Age from Method 6aτNEB (Note 2) (time.age) |
| tau6atNEB | 3.0 | Gyr | τ from Method 6aτNEB (Note 2) (time.scale) |
| EBV6atNEB | 0.15 | mag | E(B-V) from Method 6aτNEB (Note 2) (phot.color.excess) |
| SFR6atNEB | 1.100e-01 | Msun/yr | SFR from Method 6aτNEB (Note 2) (phys.SFR) |
| met6atNEB | 0.20 | Sun | Gas metallicity from Method 6aτNEB (Note 2) (phys.abund) |
| el6atNEB | 2 | [1/2] Extinction law from Method 6aτNEB; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2) (phys.absorption) | |
| X2.6atNEB | 8.63e-01 | Reduced chi2 from Method 6aτNEB (Note 2) (stat.fit.chi2) | |
| L1.6atNEB | 2.44e+26 | 10-7W/Hz | Rest-frame luminosity at 140nm Lν(140nm) from Method 6aτNEB; erg/s/Hz (Note 2) (phys.luminosity;em.UV.100-200nm) |
| L2.6atNEB | 7.55e+26 | 10-7W/Hz | Rest-frame luminosity at 270nm Lν(270nm) from Method 6aτNEB; erg/s/Hz (Note 2) (phys.luminosity;em.UV.200-300nm) |
| UM6atNEB | -16.30 | mag | AB rest-frame magnitude in U band from Method 6aτNEB (Note 2) (phys.magAbs) |
| BM6atNEB | -17.12 | mag | AB rest-frame magnitude in B band from Method 6aτNEB (Note 2) (phys.magAbs) |
| VM6atNEB | -17.57 | mag | AB rest-frame magnitude in V band from Method 6aτNEB (Note 2) (phys.magAbs) |
| RM6atNEB | -17.77 | mag | AB rest-frame magnitude in R band from Method 6aτNEB (Note 2) (phys.magAbs) |
| IM6atNEB | -17.96 | mag | AB rest-frame magnitude in I band from Method 6aτNEB (Note 2) (phys.magAbs) |
| JM6atNEB | -18.23 | mag | AB rest-frame magnitude in J band from Method 6aτNEB (Note 2) (phys.magAbs) |
| KM6atNEB | -18.01 | mag | AB rest-frame magnitude in K band from Method 6aτNEB (Note 2) (phys.magAbs) |
| age-6adt | 9.85 | [yr] | Age from Method 6adelτ (Note 2) (time.age) |
| tau-6adt | 1.5 | Gyr | τ from Method 6adelτ (Note 2) (time.scale) |
| EBV-6adt | 0.10 | mag | E(B-V) from Method 6adelτ (Note 2) (phot.color.excess) |
| SFR-6adt | 9.000e-02 | Msun/yr | SFR from Method 6adelτ (Note 2) (phys.SFR) |
| met-6adt | 0.20 | Sun | Gas metallicity from Method 6adelτ (Note 2) (phys.abund) |
| el6ad | 2 | Extinction law from Method 6adelτ; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2) (phys.absorption) | |
| X2.6adt | 1.02e+00 | Reduced chi2 from Method 6adelτ (Note 2) (stat.fit.chi2) | |
| L1.6adt | 3.69e+26 | 10-7W/Hz | Rest-frame luminosity at 140nm Lν(140nm) from Method 6adelτ; erg/s/Hz (Note 2) (phys.luminosity;em.UV.100-200nm) |
| L2.6adt | 7.91e+26 | 10-7W/Hz | Rest-frame luminosity at 270nm Lν(270nm) from Method 6adelτ; erg/s/Hz (Note 2) (phys.luminosity;em.UV.200-300nm) |
| UM6adt | -16.25 | mag | AB rest-frame magnitude in U band from Method 6adelτ (Note 2) (phys.magAbs) |
| BM6adt | -17.12 | mag | AB rest-frame magnitude in B band from Method 6adelτ (Note 2) (phys.magAbs) |
| VM6adt | -17.56 | mag | AB rest-frame magnitude in V band from Method 6adelτ (Note 2) (phys.magAbs) |
| RM6adt | -17.77 | mag | AB rest-frame magnitude in R band from Method 6adelτ (Note 2) (phys.magAbs) |
| IM6adt | -17.99 | mag | AB rest-frame magnitude in I band from Method 6adelτ (Note 2) (phys.magAbs) |
| JM6adt | -18.24 | mag | AB rest-frame magnitude in J band from Method 6adelτ (Note 2) (phys.magAbs) |
| KM6adt | -18.00 | mag | AB rest-frame magnitude in K band from Method 6adelτ (Note 2) (phys.magAbs) |
| age6ainvt | 10.05 | [yr] | Age from Method 6ainvτ (Note 2) (time.age) |
| tau6ainvt | 15.0 | Gyr | τ from Method 6ainvτ (Note 2) (time.scale) |
| EBV6ainvt | 0.15 | mag | E(B-V) from Method 6ainvτ (Note 2) (phot.color.excess) |
| SFR6ainvt | 1.500e-01 | Msun/yr | SFR from Method 6ainvτ (Note 2) (phys.SFR) |
| met6ainvt | 0.20 | Sun | Gas metallicity from Method 6ainvτ (Note 2) (phys.abund) |
| el6ainvt | 2 | [1/2] Extinction law from Method 6ainvτ; 1: Calzetti et al. 2000ApJ...533..682C; 2: SMC (Note 2) (phys.absorption) | |
| X2.6ainvt | 1.29e+00 | Reduced chi2 from Method 6ainvτ (Note 2) (stat.fit.chi2) | |
| L1.6ainvt | 3.13e+26 | 10-7W/Hz | Rest-frame luminosity at 140nm Lν(140nm) from Method 6ainvτ; erg/s/Hz (Note 2) (phys.luminosity;em.UV.100-200nm) |
| L2.6ainvt | 8.75e+26 | 10-7W/Hz | Rest-frame luminosity at 270nm Lν(270nm) from Method 6ainvτ; erg/s/Hz (Note 2) (phys.luminosity;em.UV.200-300nm) |
| UM6ainvt | -16.29 | mag | AB rest-frame magnitude in U band from Method 6ainvτ (Note 2) (phys.magAbs) |
| BM6ainvt | -17.13 | mag | AB rest-frame magnitude in B band from Method 6ainvτ (Note 2) (phys.magAbs) |
| VM6ainvt | -17.53 | mag | AB rest-frame magnitude in V band from Method 6ainvτ (Note 2) (phys.magAbs) |
| RM6ainvt | -17.75 | mag | AB rest-frame magnitude in R band from Method 6ainvτ (Note 2) (phys.magAbs) |
| IM6ainvt | -17.97 | mag | AB rest-frame magnitude in I band from Method 6ainvτ (Note 2) (phys.magAbs) |
| JM6ainvt | -18.24 | mag | AB rest-frame magnitude in J band from Method 6ainvτ (Note 2) (phys.magAbs) |
| KM6ainvt | -18.02 | mag | AB rest-frame magnitude in K band from Method 6ainvτ (Note 2) (phys.magAbs) |
| age10cdust | 8.357 | [yr] | Age from Method 10cdust (Note 2) (time.age) |
| SFH10cdust | 3 | Star formation history from Method 10cdust (2) (Note 3) (meta.code) | |
| tau10cdust | 0.1 | Gyr | τ from Method 10cdust (Note 2) (time.scale) |
| met10cdust | 0.5 | Sun | Gas metallicity from Method 10cdust (Note 2) (phys.abund) |
| age12at | 9.398 | [yr] | Age from Method 12aτ (Note 2) (time.age) |
| tau12at | 0.8 | Gyr | τ from Method 12aτ (Note 2) (time.scale) |
| EBV12at | 0.050 | mag | E(B-V) from Method 12aτ (Note 2) (phot.color.excess) |
| met12at | 0.2 | Sun | Gas metallicity from Method 12aτ (Note 2) (phys.abund) |
| Lb12at | 9.32 | [Lsun] | Stellar bolometric luminosity corrected for dust extinction from Method 12a (2) (Note 4) (phys.luminosity) |
| X2.12at | 1.86e-01 | Reduced chi2 from Method 12aτ (Note 2) (stat.fit.chi2) | |
| age14acst | 9.990 | [yr] | Age from Method 14aconst (Note 2) (time.age) |
| EBV14acst | 0.110 | mag | E(B-V) from Method 14aconst (Note 2) (phot.color.excess) |
| SFR14acst | 1.000e-01 | Msun/yr | SFR from Method 14aconst (Note 2) (phys.SFR) |
| q14acst | 1 | [1/3] Quality of the fit from Method 14aconst; 1:best; 2:good; others:bad (Note 2) (meta.code.qual) | |
| age14alin | 10.023 | [yr] | Age from Method 14alin (Note 2) (time.age) |
| EBV14alin | 0.163 | mag | E(B-V) from Method 14alin (Note 2) (phot.color.excess) |
| SFR14alin | 1.450e-01 | Msun/yr | SFR from Method 14alin (Note 2) (phys.SFR) |
| q14alin | 1 | [1/3] Quality of the fit from Method 14alin; 1:best; 2:good; others:bad (Note 2) (meta.code.qual) | |
| age14adt | 9.195 | [yr] | Age from Method 14adelτ (Note 2) (time.age) |
| tau14adt | 0.234 | Gyr | τ from Method 14adelτ (Note 2) (time.scale) |
| EBV14adt | 0.024 | mag | E(B-V) from Method 14adelτ (Note 2) (phot.color.excess) |
| SFR14adt | 1.700e-02 | Msun/yr | SFR from Method 14adelτ (Note 2) (phys.SFR) |
| q14adt | 1 | [1/3] Quality of the fit from Method 14adelτ; 1:best; 2:good; others:bad (Note 2) (meta.code.qual) | |
| age14at | 9.139 | [yr] | Age from Method 14aτ (Note 2) (time.age) |
| tau14at | 0.315 | Gyr | τ from Method 14aτ (Note 2) (time.scale) |
| EBV14at | 0.024 | mag | E(B-V) from Method 14aτ (Note 2) (phot.color.excess) |
| SFR14at | 1.900e-02 | Msun/yr | SFR from Method 14aτ (Note 2) (phys.SFR) |
| q14at | 1 | [0/3] Quality of fit from Method 14a_τ; 1=best; 2=good; others=bad (Note 2) (meta.code.qual) | |
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