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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

  
J/A+A/527/A134
  Fe abundances for 28 XMM galaxy clusters (Matsushita, 2011)
Post annotation
img(gal)
1.J/A+A/527/A134/clusters(c)Clusters studied (from table 1 of paper) (28 rows)
2.J/A+A/527/A134/table1Cluster samples in the XMM-Newton archival data (118 rows)
3.J/A+A/527/A134/table2Results of spectral fitting of annular spectra (130 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)Cluster (char) (i) Cluster name (meta.id;meta.main)
  (1)OName (char) Other name of cluster (meta.id)
  (1)z  Redshift (src.redshift)
  (1)<kT> keV Adopted average temperature of ICM used to calculate the virial radius r180 (phys.temperature)
  (1)NH 10+20cm-2Galactic value of the hydrogen column density (Dickey & Lockman, 1990ARA&A..28..215D) (phys.columnDensity;pos.galactic)
  (1)Type (char) Type of cluster: cD or non-cD (Note G1)   (src.class)
  (1)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)
  (1)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (1)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (2)ObsID  XMM Obs ID (meta.id;obs)

ALL cols
    
 (i)indexed column
  (2)ExpPN ks Exposure time of PN camera (Note 2)   (time.duration;obs.exposure)
  (2)ExpMOS1 ks Exposure time of MOS1 camera (Note 2)   (time.duration;obs.exposure)
  (2)ExpMOS2 ks Exposure time of MOS2 camera (Note 2)   (time.duration;obs.exposure)
  (3)rl  Lower value of radius interval, in units of r180 (phys.size.radius;arith.ratio)
  (3)ru  Upper value of radius interval, in units of r180 (phys.size.radius;arith.ratio)
  (3)kT keV Best-fit ICM temperature derived from the 1T model fits (phys.temperature)
  (3)e_kT keV 1σ statistical error on kT (phys.temperature)
  (3)FeA [Sun] Best-fit Fe abundance using the ICM temperature derived from the 1T model fits (from FFeHeK/F3.5–6) (phys.abund.Fe;meta.modelled)
  (3)e_FeA [Sun] 1σ statistical error on FeA (Note 1)   (stat.error)
  (3)DFeA [Sun] Difference in the derived FeA abundances using the best-fit multi-T model and the 1T model (stat.param;meta.modelled)
  (3)FeB [Sun] (n) Best-fit Fe abundance using the ICM temperature derived from the 1T model fits (for FFeHK/F3.5–6) (phys.abund.Fe;meta.modelled)
  (3)e_FeB [Sun] (n) 1σ statistical error on FeB (Note 1)   (stat.error)
  (3)DFeB [Sun] (n) Difference in the derived FeB abundances using the best-fit multi-T model and the 1T model (stat.param;meta.modelled)

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