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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

  WARPS-II Cluster catalog. VII. (Horner+, 2008)
Post annotation
1.J/ApJS/176/374/warpsWARPS-II catalog, with additional clusters and candidates (tables 2 and 3 of paper) (125 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)
  f_WARPS (char) A for additional and candidate clusters (table3); non-flagged clusters represent a statistically complete, flux-limited sample (meta.code)
  WARPS (char) (i) Assigned cluster name (JHHMM.m+DDMMW) (Note G1)   (;meta.main)
  n_WARPS (char) * indicates other names for the cluster in table4 (meta.ref.url)
  RAJ2000 deg (i) Right ascension in decimal degrees (J2000) (pos.eq.ra;meta.main)
  DEJ2000 deg (i) Declination in decimal degrees (J2000) (pos.eq.dec;meta.main)
  nH 10+20/cm2Hydrogen column density from Dickey & Lockman, 1990ARA&A..28..215D (phys.columnDensity)
  Flux 10-17W/m2Unabsorbed source flux in the 0.5-2.0keV band, in 10–14erg/cm2/s (Note 1)   (phot.flux;em.X-ray)
  logLX [10-7W] Log of the rest-frame source luminosity in the 0.5-2.0keV band derived as the flux (Note 2)   (phys.luminosity;em.X-ray)
  logLX2 [10-7W] Luminosity calculated using a H0=70, ΩM=0.3, ΩΛ=0.7 cosmology. (phys.luminosity;em.X-ray)
  z  Redshift of the cluster (src.redshift)
  o_z  (n) Number of galaxy redshifts used to derive the cluster redshift (meta.number)
  u_z (char) [.5? ] Uncertain number of valid redshifts (meta.code.error;src.redshift)
  Rad arcsec (n) Estimated core radius of the cluster (phys.angSize;src)
  Com (char) Comments (See section 3.2 for more details) (meta.note)

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