VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/AJ/169/172
  Derived parameters & abundances of metal-poor stars (Mittal+, 2025)
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2025AJ....169..172M
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1.J/AJ/169/172/table4Derived local thermodynamic equilibrium (LTE) abundances (311 rows)
Abundances derived from O I, Na I, Mg I, Si I, K I, Fe I, and Fe II lines have been corrected for NLTE. Their LTE abundances are presented in this Table for reference, but we recommend adopting the NLTE-corrected abundances presented in Table 5.

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)
  Name (char) (i) Stellar identifier (meta.id;meta.main)
  nFeI   [19/138] Number of FeI LTE lines used (Note 1)   (meta.number)
  loge(FeI) [-] [3.38/6.46] Log epsilon mean abundance of FeI (phys.abund;stat.mean)
  [FeI/H] [-] [-4.12/-1.04] FeI abundance relative to H (phys.abund.Fe)
  e_[FeI/H] [-] [0.03/0.1] Total uncertainty in [FeI/H] (stat.error;phys.abund.Fe)
  nFeII  (n) [1/13] Number of FeII LTE lines used (Note 1)   (meta.number)
  loge(FeII) [-] (n) [3.41/6.52] Log epsilon mean abundance of FeII (phys.abund;stat.mean)
  [FeII/H] [-] (n) [-4.09/-0.98] FeII abundance relative to H (phys.abund.Fe)
  e_[FeII/H] [-] (n) [0.12/0.6] Total uncertainty in [FeII/H] (stat.error;phys.abund.Fe)
  nOI  (n) [1/4] Number of OI LTE lines used (Note 1)   (meta.number)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  loge(OI) [-] (n) [6.55/8.72] Log epsilon mean abundance of OI (phys.abund;stat.mean)
  [OI/Fe] [-] (n) [0.26/2.85] OI abundance relative to FeI (phys.abund;arith.ratio)
  e_[OI/Fe] [-] (n) [0.09/0.31] Total uncertainty in [OI/Fe] (stat.error;phys.abund;arith.ratio)
  nNaI  (n) [1/4] Number of NaI LTE lines used (Note 1)   (meta.number)
  loge(NaI) [-] (n) [2.42/5.33] Log epsilon mean abundance of NaI (phys.abund;stat.mean)
  [NaI/Fe] [-] (n) [-0.56/1.63] NaI abundance relative to FeI (phys.abund;arith.ratio)
  e_[NaI/Fe] [-] (n) [0.12/0.28] Total uncertainty in [NaI/Fe] (stat.error;phys.abund;arith.ratio)
  nMgI   [1/9] Number of MgI LTE lines used (Note 1)   (meta.number)
  loge(MgI) [-] [3.81/7.18] Log epsilon mean abundance of MgI (phys.abund;stat.mean)
  [MgI/Fe] [-] [-0.36/1.51] MgI abundance relative to FeI (phys.abund;arith.ratio)
  e_[MgI/Fe] [-] [0.08/0.22] Total uncertainty in [MgI/Fe] (stat.error;phys.abund;arith.ratio)
  nSiI  (n) [1/4] Number of SiI LTE lines used (Note 1)   (meta.number)
  loge(SiI) [-] (n) [3.63/6.87] Log epsilon mean abundance of SiI (phys.abund;stat.mean)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  [SiI/Fe] [-] (n) [-0.34/1.14] SiI abundance relative to FeI (phys.abund;arith.ratio)
  e_[SiI/Fe] [-] (n) [0.09/0.55] Total uncertainty in [SiI/Fe] (stat.error;phys.abund;arith.ratio)
  nKI  (n) [1/2] Number of KI LTE lines used (Note 1)   (meta.number)
  loge(KI) [-] (n) [1.51/4.74] Log epsilon mean abundance of KI (phys.abund;stat.mean)
  [KI/Fe] [-] (n) [-0.08/0.88] KI abundance relative to FeI (phys.abund;arith.ratio)
  e_[KI/Fe] [-] (n) [0.11/0.21] Total uncertainty in [KI/Fe] (stat.error;phys.abund;arith.ratio)
  nCaI   [3/14] Number of CaI LTE lines used (meta.number)
  loge(CaI) [-] [2.45/5.58] Log epsilon mean abundance of CaI (phys.abund;stat.mean)
  [CaI/Fe] [-] [-0.32/0.54] CaI abundance relative to FeI (phys.abund;arith.ratio)
  e_[CaI/Fe] [-] [0.06/0.24] Total uncertainty in [CaI/Fe] (stat.error;phys.abund;arith.ratio)
  nTiI  (n) [1/19] Number of TiI LTE lines used (meta.number)
  loge(TiI) [-] (n) [1.21/4.21] Log epsilon mean abundance of TiI (phys.abund;stat.mean)
  [TiI/Fe] [-] (n) [-0.35/1.16] TiI abundance relative to FeI (phys.abund;arith.ratio)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  e_[TiI/Fe] [-] (n) [0.05/0.52] Total uncertainty in [TiI/Fe] (stat.error;phys.abund;arith.ratio)
  nTiII   [2/34] Number of TiII LTE lines used (meta.number)
  loge(TiII) [-] [1.31/4.4] Log epsilon mean abundance of TiII (phys.abund;stat.mean)
  [TiII/Fe] [-] [-0.14/1.04] TiII abundance relative to FeI (phys.abund;arith.ratio)
  e_[TiII/Fe] [-] [0.09/0.32] Total uncertainty in [TiII/Fe] (stat.error;phys.abund;arith.ratio)
  nCrI   [1/13] Number of CrI LTE lines used (meta.number)
  loge(CrI) [-] [1.03/4.53] Log epsilon mean abundance of CrI (phys.abund;stat.mean)
  [CrI/Fe] [-] [-0.67/0.3] CrI abundance relative to FeI (phys.abund;arith.ratio)
  e_[CrI/Fe] [-] [0.06/0.4] Total uncertainty in [CrI/Fe] (stat.error;phys.abund;arith.ratio)
  nCrII  (n) [1/4] Number of CrII LTE lines used (meta.number)
  loge(CrII) [-] (n) [2.1/4.73] Log epsilon mean abundance of CrII (phys.abund;stat.mean)
  [CrII/Fe] [-] (n) [-0.39/0.58] CrII abundance relative to FeI (phys.abund;arith.ratio)
  e_[CrII/Fe] [-] (n) [0.15/0.65] Total uncertainty in [CrII/Fe] (stat.error;phys.abund;arith.ratio)
  nNiI  (n) [1/18] Number of NiI LTE lines used (meta.number)
  loge(NiI) [-] (n) [2.03/5.24] Log epsilon mean abundance of NiI (phys.abund;stat.mean)
  [NiI/Fe] [-] (n) [-0.34/0.49] NiI abundance relative to FeI (phys.abund;arith.ratio)
  e_[NiI/Fe] [-] (n) [0.06/0.41] Total uncertainty in [NiI/Fe] (stat.error;phys.abund;arith.ratio)
  nZnI  (n) [1/3] Number of ZnI LTE lines used (meta.number)
  loge(ZnI) [-] (n) [1.28/3.81] Log epsilon mean abundance of ZnI (phys.abund;stat.mean)
  [ZnI/Fe] [-] (n) [-0.55/1.04] ZnI abundance relative to FeI (phys.abund;arith.ratio)
  e_[ZnI/Fe] [-] (n) [0.1/0.54] Total uncertainty in [ZnI/Fe] (stat.error;phys.abund;arith.ratio)

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