VizieR

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

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

  
J/MNRAS/360/782
  X-ray-selected normal galaxies (Georgantopoulos+, 2005)
Post annotation
img(gal)
1.J/MNRAS/360/782/table2The candidate normal galaxy sample (28 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)
  [GGK2005]  Identification number (meta.id;meta.main)
  RAJ2000 "h:m:s" (i) X-ray Right ascension (J2000) (pos.eq.ra;meta.main)
  DEJ2000 "d:m:s" (i) X-ray Declination (J2000) (pos.eq.dec;meta.main)
  rmag mag SDSS r optical magnitude (phot.mag;em.opt.R)
  l_Prob (char) Limit flag on Prob (meta.code.error)
  Prob % Probability the optical counterpart is a spurious alignment (stat.value)
  DXO arcsec X-ray/optical position offset (pos.angDistance)
  FX 10-17W/m2Absorbed X-ray flux in the 0.5-8keV spectral band (phot.flux;em.X-ray)
  e_FX 10-17W/m2rms uncertainty on FX (stat.error)
  l_HR (char) Limit flag on HR (meta.code.error)
  HR  Hardness ratio derived in the 0.5-2 and 2-8keV bands (phot.flux;em.X-ray.medium)
  e_HR  (n) rms uncertainty on HR (stat.error)
  log(FX/Fo)  X-ray-to-optical flux ratio (phot.flux;arith.ratio)
  z  Spectroscopic or photometric redshift (src.redshift)
  n_z (char) [bc ] Note on z (Note 1)   (meta.note)
  logLX 10+34W Logarithmic 0.5-8keV X-ray luminosity (phys.luminosity;em.X-ray)
  Sp (char) Spectral features (Note 2)   (meta.note)
  u_Sp (char) [*] * denotes ambiguous SDSS spectral classification (meta.code.error;src.spType)
  SDSS  Display the SDSS data (meta.ref.url)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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usage  Display UCD1+    UCD1  
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