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J/MNRAS/514/4816
  50 giant cluster stars abund. study (Katime Santrich+, 2022)
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2022MNRAS.514.4816K
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1.J/MNRAS/514/4816/table5Stellar atmospheric parameters calculated from our spectroscopic analysis work (43 rows)

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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Star (char) Star identification name as ClusterName-NNNNN (Star) (meta.id;meta.main)
  Teff K Mean effective temperature derived from SAP spectroscopic analysis (Teff) (Note 1)   (phys.temperature.effective;stat.mean)
  e_Teff K Standard deviation/error of the Teff derived from SAP spectroscopic analysis (σTeff) (stat.error;phys.temperature.effective)
  logg [cm/s2] Logarithm of the surface gravity derived from SAP spectroscopic analysis (logg) (Note 2)   (phys.gravity)
  e_logg [cm/s2] Standard deviation/error of the logg (σlogg) (stat.error)
  vt km/s Microturbulence velocity derived from SAP spectroscopic analysis (Ξ) (Note 3)   (phys.veloc.microTurb)
  e_vt km/s Standard deviation/error of the vt (σvt) (stat.error)
  [Fe/H] [Sun] Iron to hydrogen abundance ratio ([Fe/H]) (Note 4)   (phys.abund.Fe;arith.ratio)
  e_[Fe/H] [Sun] Standard deviation/error of the [Fe/H] (σ[Fe/H]) (stat.error;phys.abund.Fe)
  NFeI  The number of Fe I lines used in the spectroscopic analysis (#1) (meta.number;spect.line)
  NFeII  The number of Fe II lines used in the spectroscopic analysis (#2) (meta.number;spect.line)

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