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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/ApJ/682/821
  Spectral fits of galaxy clusters in X-ray (Cavagnolo+, 2008)
Post annotation
img(gal)
1.J/ApJ/682/821/table1(c)Summary of sample (244 rows)
2.J/ApJ/682/821/fitsSummary of spectral fits (tables 2 and 3 of the paper) (358 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)Name (char) (i) Cluster name (Note 1)   (meta.id;meta.main)
  (1)f_Name (char) [di] Note on cluster (Note 2)   (meta.code)
  (1)ObsID  Chandra observation identification number (meta.id;obs.param;obs)
  (1)RAJ2000 "h:m:s" (i) Cluster center hour of Right Ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Cluster center degree of Declination (J2000) (pos.eq.dec;meta.main)
  (1)ExpT ks Exposure time (time.duration;obs.exposure)
  (1)Mode (char) Observing mode (instr.setup)
  (1)ACIS (char) ACIS CCD location of centroid (instr.setup)
  (1)z  Redshift taken from Horner, 2001PhDT........88H (all redshifts confirmed with NED) (src.redshift)
  (1)Lbol 10+37W Bolometric luminosity in units of 10+44erg/s (phys.luminosity)

ALL cols
    
 (i)indexed column
  (1)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)
  (1)NED (char) ask the NED data-base about this object
  (2)n_Name (char) [*] Indicates multiple observations (meta.note)
  (2)Rc kpc Excluded core region size (phys.angSize;obs.field)
  (2)R  (n)Cluster density relative to Universe critical density (2500 or 5000) (phys.density;arith.ratio)
  (2)Rad kpc Cluster radius (Note 2)   (phys.angSize;src)
  (2)NHI 10+20/cm2Galactic neutral hydrogen column density (phys.columnDensity;pos.galactic)
  (2)E_NHI 10+20/cm2(n) Upper limit uncertainty in NHI (stat.error;stat.max)
  (2)e_NHI 10+20/cm2(n) Lower limit uncertainty in NHI (stat.error)
  (2)T77 keV Best fit 0.7-7keV MeKaL temperature (phys.temperature)
  (2)E_T77 keV Upper limit uncertainty in T77 (stat.error;stat.max)
  (2)e_T77 keV Lower limit uncertainty in T77 (stat.error)
  (2)T27 keV Best fit 2-7keV MeKaL temperature (phys.temperature)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)E_T27 keV Upper limit uncertainty in T27 (stat.error;stat.max)
  (2)e_T27 keV Lower limit uncertainty in T27 (stat.error)
  (2)THBR  The T77/T22 ratio (phys.temperature)
  (2)E_THBR  Upper limit uncertainty in THBR (stat.error;stat.max)
  (2)e_THBR  Lower limit uncertainty in THBR (stat.error)
  (2)Z77 Sun Best-fit 0.7-7keV MeKaL abundance (phys.abund)
  (2)E_Z77 Sun Upper limit uncertainty in Z77 (stat.error;stat.max)
  (2)e_Z77 Sun Lower limit uncertainty in Z77 (stat.error)
  (2)chi77  Reduced χ2 for best-fit 0.7-7keV model (stat.fit.chi2)
  (2)chi27  Reduced χ2 for best-fit 2-7keV model (stat.fit.chi2)
  (2)Src % Percentage of emission attributable to source (meta.note)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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