VizieR

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

VizieR

  
J/MNRAS/511/214
  Study of CSS/GPS/MPS radio sources (Nascimento+, 2022)
ReadMe+ftp
2022MNRAS.511..214N
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/511/214/table4Stellar Population Synthesis Results for MPS sources in our sample (14 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Source (char) Source object name (Object) (meta.id;meta.main)
  FC % Percentage contribution of Featureless Continuum to SSPs (FC) (stat.fit.param)
  xy % Percentage xy(t ≤ 50 Myr) Light-weighted young age contribution to SSPs (xy) (stat.fit.param)
  xi % Percentage xi(50 Myr ≤ t ≤ 2 Gyr) Light-weighted intermediate age contribution to SSPs (xi) (stat.fit.param)
  xo % Percentage xo(t > 2 Gyr) Light-weighted old age contribution to SSPs (xo) (stat.fit.param)
  my % Percentage my(t ≤ 50 Myr) Mass-weighted young age contribution to SSPs (my) (stat.fit.param)
  mi % Percentage mi(50 Myr ≤ t ≤ 2 Gyr) Mass-weighted intermediate age contribution to SSPs (mi) (stat.fit.param)
  mo % Percentage mo(t > 2 Gyr) Mass-weighted old age contribution to SSPs (mo) (stat.fit.param)
  Av mag Dust extinction in V band (AV) (phys.absorption)
  logt*L [yr] The light-weighted mean age (<logt*>L) (Note G3)   (time.age;stat.mean)
  logt*M [yr] The mass-weighted mean age ( (<logt*>M) (Note G3)   (time.age;stat.mean)
  Z*L  The light-weighted mean metallicity (<Z*>L) (Note G3)   (phys.abund.Z;stat.mean)
  Z*M  The mass-weighted mean metallicity (<Z*>M) (Note G3)   (phys.abund.Z;stat.mean)
  logM* [Msun] Logarithm of the present stellar mass of the galaxy (M*) (Note G4)   (phys.mass)
  SFR* Msun/yr Logarithm of the Star formation rate over the last 50 Myr (SFR*) (Note G4)   (phys.SFR)
  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)
  MType (char) Morphology type determined visually from SDSS images (Morph) (Note 1)   (src.morph.type)

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