VizieR

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VizieR

  
J/AJ/169/172
  Derived parameters & abundances of metal-poor stars (Mittal+, 2025)
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1.J/AJ/169/172/table5Derived non-local thermodynamic equilibrium (NLTE) abundances (311 rows)
The number of lines listed here refers to the number of lines for which NLTE corrections were calculated using the procedure explained in Section 4.3. For O I, Na I, Mg I, Si I, K I, Fe I, and Fe II, we recommend adopting the abundances presented here.

 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Name (char) (i) Stellar identifier (meta.id;meta.main)
  nFeI-NLTE   [7/32] Number of FeI NLTE lines used (Note 1)   (meta.number)
  loge(FeI)-NLTE [-] [3.56/6.5] Log epsilon mean abundance of FeI (phys.abund;stat.mean)
  [FeI/H]-NLTE [-] [-3.94/-1.0] FeI abundance relative to H (phys.abund.Fe)
  e_[FeI/H]-NLTE [-] [0.06/0.18] Total uncertainty in [FeI/H]-NLTE (stat.error;phys.abund.Fe)
  nFeII-NLTE  (n) [1/13] Number of FeII NLTE lines used (Note 1)   (meta.number)
  loge(FeII)-NLTE [-] (n) [3.42/6.5] Log epsilon mean abundance of FeII (phys.abund;stat.mean)
  [FeII/H]-NLTE [-] (n) [-4.08/-1.0] FeII abundance relative to H (phys.abund.Fe)
  e_[FeII/H]-NLTE [-] (n) [0.13/0.6] Total uncertainty in [FeII/H]-NLTE (stat.error;phys.abund.Fe)
  nOI-NLTE  (n) [1/4] Number of OI NLTE lines used (Note 1)   (meta.number)

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(n) indicates a possible blank or NULL column(i)indexed column
  loge(OI)-NLTE [-] (n) [6.55/8.72] Log epsilon mean abundance of OI (phys.abund;stat.mean)
  [OI/Fe]-NLTE [-] (n) [0.1/2.85] OI abundance relative to FeI (phys.abund;arith.ratio)
  e_[OI/Fe]-NLTE [-] (n) [0.13/0.33] Total uncertainty in [OI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)
  nNaI-NLTE  (n) [1/4] Number of NaI NLTE lines used (Note 1)   (meta.number)
  loge(NaI)-NLTE [-] (n) [2.38/5.22] Log epsilon mean abundance of NaI (phys.abund;stat.mean)
  [NaI/Fe]-NLTE [-] (n) [-0.63/1.53] NaI abundance relative to FeI (phys.abund;arith.ratio)
  e_[NaI/Fe]-NLTE [-] (n) [0.16/0.31] Total uncertainty in [NaI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)
  nMgI-NLTE   [1/9] Number of MgI NLTE lines used (Note 1)   (meta.number)
  loge(MgI)-NLTE [-] [4.02/7.18] Log epsilon mean abundance of MgI (phys.abund;stat.mean)
  [MgI/Fe]-NLTE [-] [-0.36/1.58] MgI abundance relative to FeI (phys.abund;arith.ratio)
  e_[MgI/Fe]-NLTE [-] [0.1/0.26] Total uncertainty in [MgI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)
  nSiI-NLTE  (n) [1/4] Number of SiI NLTE lines used (Note 1)   (meta.number)
  loge(SiI)-NLTE [-] (n) [3.63/6.86] Log epsilon mean abundance of SiI (phys.abund;stat.mean)
  [SiI/Fe]-NLTE [-] (n) [-0.29/1.14] SiI abundance relative to FeI (phys.abund;arith.ratio)
  e_[SiI/Fe]-NLTE [-] (n) [0.13/0.56] Total uncertainty in [SiI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)
  nKI-NLTE  (n) [1/2] Number of KI NLTE lines used (Note 1)   (meta.number)
  loge(KI)-NLTE [-] (n) [1.43/4.21] Log epsilon mean abundance of KI (phys.abund;stat.mean)
  [KI/Fe]-NLTE (char) [-] KI abundance relative to FeI (phys.abund;arith.ratio)
  e_[KI/Fe]-NLTE [-] (n) [0.17/0.26] Total uncertainty in [KI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)

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