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

  SDSS/3XMM X-ray-selected LINERs (Nisbet+, 2016)
Post annotation
1.J/MNRAS/455/2551/tablea1Full sample of 576 LINERs (576 rows)

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)
  Id  Identifier in this sample of LINERs (
  Plate  Plate identifier for the SDSS source in the SDSS-DR7 catalogue (;instr.plate)
  MJD d MJD identifier for the SDSS source in the SDSS-DR7 catalogue (;time.epoch)
  Fibre  Fibre identifier for the SDSS source in the SDSS-DR7 catalogue (;meta.main)
  RAJ2000 deg (i) Right ascension for the SDSS source (J2000) (pos.eq.ra;meta.main)
  DEJ2000 deg (i) Declination for the SDSS source (J2000) (pos.eq.dec;meta.main)
  z  Redshift derived from the SDSS spectra (src.redshift)
  sigma km/s Stellar velocity dispersion of the galaxy bulge, derived from SDSS data (src.class.starGalaxy)
  MBH [Msun] log10 black hole mass (Note 1)   (phys.mass)
  M* Msun log10 stellar mass derived from the SDSS data (phys.mass)
  3XMM  Identifier of X-ray source in the 3XMM-DR4 catalogue (
  FX mW/m2 X-ray flux in the 2.0-12.0keV band (phot.flux;em.X-ray)
  logLX [10-7W] log10 X-ray luminosity corresponding to the flux in the 2.0-10.0keV band (phys.luminosity;em.X-ray)
  S1.4GHz Jy Radio flux density at an observing frequency of 1.4GHz (phot.flux.density;
  l_logL1.4GHz (char) [L] Limit flag on logL1.4GHz (Note 2)   (meta.code.error)
  logL1.4GHz [10-7W] log10 radio luminosity from an observing frequency of 1.4GHz (Note 2)   (phys.luminosity;
  Sloan  Display the SDSS data for this galaxy (meta.ref.url)
  SimbadName (char) Designation understandable by the Simbad data-base (

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