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J/A+A/527/A134
  Fe abundances for 28 XMM galaxy clusters (Matsushita, 2011)
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2011A&A...527A.134M
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Post annotation 		img(gal)
1.J/A+A/527/A134/table2Results of spectral fitting of annular spectra (130 rows)

Simple ConstraintList Of Constraints
 
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)
  Cluster (char) Cluster name (meta.id;meta.main)
  rl  Lower value of radius interval, in units of r180 (phys.size.radius;arith.ratio)
  ru  Upper value of radius interval, in units of r180 (phys.size.radius;arith.ratio)
  kT keV Best-fit ICM temperature derived from the 1T model fits (phys.temperature)
  e_kT keV 1σ statistical error on kT (phys.temperature)
  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)
  e_FeA [Sun] 1σ statistical error on FeA (Note 1)   (stat.error)
  DFeA [Sun] Difference in the derived FeA abundances using the best-fit multi-T model and the 1T model (stat.param;meta.modelled)
  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)
  e_FeB [Sun] (n) 1σ statistical error on FeB (Note 1)   (stat.error)
  DFeB [Sun] (n) Difference in the derived FeB abundances using the best-fit multi-T model and the 1T model (stat.param;meta.modelled)

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