| Show | Sort | Column | Constraint | Explain (UCD) |
| | | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | | Name | (char) | Source name (B2 HHMM+DDA or 3C NNN.N) (meta.id;meta.main) (ID_MAIN) |
| | | logM | [Msun] | Galaxy mass (phys.mass) (PHYS_MASS_MISC) |
| | | Age | 10+9yr | Galaxy age (time.age) (TIME_AGE) |
| | | C1g | [Msun] | (n) 2nd galaxy component logM for a (young) galaxy model (phys.mass) (PHYS_MASS_MISC) |
| | | C2g | yr | (n) 2nd component Age for a (young) galaxy model (pos.cartesian) (TIME_AGE) |
| | | g | (char) | [g] g for galaxy model (meta.code) (CODE_MISC) |
| | | C1p | [10Lsun/nm] | (n) 2nd galaxy component luminosity density (in L_☉/Å), at the reference point λ=2000Å, Lp.l2000Å, for a power law (phys.luminosity) (PHYS_LUMINOSITY_GENERAL) |
| | | C2p | | (n) 2nd galaxy component slope of power-law (lambda–alpha), for a power law (spect.index) (SPECT_SP-INDEX) |
| | | p | (char) | [p] p for power law (meta.code) (CODE_MISC) |
| | | chi2min | | Reduced minimum chi2 value (stat.fit.chi2) (FIT_CHI2) |
ALL cols | | | |
| | | n_chi2min | (char) | [cd] Note on chi2min (Note 1)
(meta.note) (NOTE) |
| | | logP | [-] | (n) Total power at 1.4GHz (phys.luminosity;em.radio.750-1500MHz) (SPECT_LUMINOSITY) |
| | | FR | | (n) FR type (Note 2)
(meta.code.class) (CLASS_CODE) |
| | | SpCode | | (n) [0/4] Spectral type code (Note 3)
(meta.code.class) (CLASS_CODE) |
| | | Class | (char) | Classification of the spectral type according to the emission line ratios determined here (Note 4)
(meta.code.class) (CLASS_CODE) |
| | | l_LHa | (char) | Limit flag on LHa (meta.code.error) (CODE_LIMIT) |
| | | LHa | 10+33W | (n) Luminosity of Hα emission (phys.luminosity;em.line.Halpha) (PHYS_LUMINOSITY_HALPHA) |
| | | XUV | mag | (n) Ultraviolet excess (phot.color.excess) (PHOT_COLOR_EXCESS) |
| | | e_XUV | mag | (n) rms uncertainty on XUV (stat.error) (ERROR) |
| | | logRw | [-] | (n) Logarithm of the ratio of the two near-IR (W1 plus W2) and the two MIR (W3 and W4) WISE luminosities, log[L(W1+W2)/L(W3+W4)] (phys.luminosity;arith.ratio) (PHYS_LUMINOSITY_RATIO) |
| | | logMBH | [Msun] | (n) Black hole mass (phys.mass) (PHYS_MASS_MISC) |
| | | r_logMBH | (char) | [efg] reference for logMBH (Note 5)
(meta.ref;pos.frame) (REFER_CODE) |
ALL cols | | | |