VizieR

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VizieR

  
J/A+A/527/A134
  Fe abundances for 28 XMM galaxy clusters (Matsushita, 2011)
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img(gal)
1.J/A+A/527/A134/table2Results of spectral fitting of annular spectra (130 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. ((unassigned);meta.version;arith.diff;phys.veloc)
  Cluster (char) Cluster name ((unassigned);(unassigned);(unassigned);spect.line.veloc;arith)
  rl  Lower value of radius interval, in units of r180 ((unassigned);(unassigned);(unassigned);(unassigned);instr.offset)
  ru  Upper value of radius interval, in units of r180 (phot.color;em.IR.60-100um;arith.factor;(unassigned);instr.offset)
  kT keV Best-fit ICM temperature derived from the 1T model fits ((unassigned);instr.det.noise;stat.min;em)
  e_kT keV 1{sigma} statistical error on kT ((unassigned);(unassigned);arith;em)
  FeA [Sun] Best-fit Fe abundance using the ICM temperature derived from the 1T model fits (from FFeHeK/F3.5–6) ((unassigned);meta.version;arith.diff;phys.reflectance;src.orbital.inclination)
  e_FeA [Sun] 1{sigma} statistical error on FeA (Note 1)   ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  DFeA [Sun] Difference in the derived FeA abundances using the best-fit multi-T model and the 1T model ((unassigned);meta.version;arith.diff;time.obs.end;src.orbital.meanAnomaly)
  FeB [Sun] (n) Best-fit Fe abundance using the ICM temperature derived from the 1T model fits (for FFeHK/F3.5–6) ((unassigned);(unassigned);(unassigned);phys.reflectance;src.orbital.inclination)
  e_FeB [Sun] (n) 1{sigma} statistical error on FeB (Note 1)   ((unassigned);meta.version;arith.diff;time.age;meta.main)
  DFeB [Sun] (n) Difference in the derived FeB abundances using the best-fit multi-T model and the 1T model ((unassigned);meta.version;arith.diff;time.obs.end;src.orbital.meanAnomaly)

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