| Show | Sort | Join tables | Column | Constraint | Explain (UCD) |
| | | (ALL) | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | |  (ALL) | Source | (char) | Source object name (Source) (meta.id;meta.main) (ID_MAIN) |
| | | (1+2) | n_Source | (char) | Note on typical source objects (Note G1)
(meta.note) (NOTE) |
| | | (1+2) | RAJ2000 | "h:m:s" | (i) Right ascension (J2000) (pos.eq.ra;meta.main) (POS_EQ_RA_MAIN) |
| | | (1+2) | DEJ2000 | "d:m:s" | (i) Declination (J2000) (pos.eq.dec;meta.main) (POS_EQ_DEC_MAIN) |
| | | (1+2) | z | | Redshift (z) (src.redshift) (REDSHIFT_HC) |
| | | (1+2) | S1.4 | mJy/beam | (n) Peak flux per beam area derived by fitting an elliptical Gaussian model to the source from FIRST survey at 1.4 GHz in the L-band (PeakFlux) (Note G2)
(phot.flux.density;em.radio.750-1500MHz) (PHOT_FLUX_RADIO_1.4G) |
| | | (1+2) | I1.4 | mJy | (n) Intensity flux derived by fitting an elliptical Gaussian model to the source from FIRST survey at 1.4 GHz in the L-band (Int.Flux) (Note G2)
(phot.flux.density;em.radio.750-1500MHz) (PHOT_FLUX_RADIO_1.4G) |
| | | (1+2) | W1-W2 | mag | WISE colours from MIR centered at 3.4 µm and 4.6 µm (W1-W2) (phot.color;em.IR;em.IR) (PHOT_CI_IR) |
| | | (1+2) | W2-W3 | mag | (n) WISE colours from MIR centered at 4.6 µm and 12 µm (W2-W3) (phot.color;em.IR;em.IR) (PHOT_CI_IR) |
| | | (1+2) | AGN | (char) | [S W] AGN classification of the source according to the position in the WISE colour diagram see section 6 MID-Infrared photometry (AGNclass) (Note 1)
(src.class) (CLASS_MISC) |
ALL cols | | | |
| | | (1+2) | SimbadName | (char) | (n)Designation understandable by the Simbad data-base (meta.id) (ID_ALTERNATIVE) |
| | | (3+4) | FC | % | Percentage contribution of Featureless Continuum to SSPs (FC) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | xy | % | Percentage xy(t ≤ 50 Myr) Light-weighted young age contribution to SSPs (xy) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | xi | % | Percentage xi(50 Myr ≤ t ≤ 2 Gyr) Light-weighted intermediate age contribution to SSPs (xi) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | xo | % | Percentage xo(t > 2 Gyr) Light-weighted old age contribution to SSPs (xo) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | my | % | Percentage my(t ≤ 50 Myr) Mass-weighted young age contribution to SSPs (my) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | mi | % | Percentage mi(50 Myr ≤ t ≤ 2 Gyr) Mass-weighted intermediate age contribution to SSPs (mi) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | mo | % | Percentage mo(t > 2 Gyr) Mass-weighted old age contribution to SSPs (mo) (stat.fit.param) (STAT_PARAM) |
| | | (3+4) | Av | mag | Dust extinction in V band (AV) (phys.absorption) (PHOT_EXTINCTION_ISM) |
| | | (3+4) | logt*L | [yr] | The light-weighted mean age (<logt*>L) (Note G3)
(time.age;stat.mean) (TIME_AGE) |
| | | (3+4) | logt*M | [yr] | The mass-weighted mean age ( (<logt*>M) (Note G3)
(time.age;stat.mean) (TIME_AGE) |
| | | (3+4) | Z*L | | The light-weighted mean metallicity (<Z*>L) (Note G3)
(phys.abund.Z;stat.mean) (PHYS_ABUND_Z) |
| | | (3+4) | Z*M | | The mass-weighted mean metallicity (<Z*>M) (Note G3)
(phys.abund.Z;stat.mean) (PHYS_ABUND_Z) |
ALL cols | | | |
| | | (3+4) | logM* | [Msun] | Logarithm of the present stellar mass of the galaxy (M*) (Note G4)
(phys.mass) (PHYS_MASS_MISC) |
| | | (3+4) | SFR* | Msun/yr | Logarithm of the Star formation rate over the last 50 Myr (SFR*) (Note G4)
(phys.SFR) (PHYS_STAR-FORM_RATE) |
| | | (3+4) | logL1.4 | [W/Hz] | Radio uminosity estimated assuming H0 = 69.8 km/s/Mpc as proposed by Freedman et al. 2019ApJ...882...34F Hubble Program (LogLR) (phot.flux.density;em.radio.750-1500MHz) (PHOT_FLUX_RADIO_1.4G) |
| | | (3+4) | MType | (char) | Morphology type determined visually from SDSS images (Morph) (Note 1)
(src.morph.type) (MORPH_TYPE) |
ALL cols | | | |