VizieR

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

VizieR

  
J/other/PARep/2.65
  Sun and HD 218209 abundance analysis (Sahin+, 2025)
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2025PAREP...2...65S
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1.J/other/PARep/2.65/table1Stellar atmospheric parameters (3 rows)
2.J/other/PARep/2.65/table2Elemental abundance ratios (33 rows)
3.J/other/PARep/2.65/tableaSpectral line list with EWs and abundances (592 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)Star (char) Target name (meta.id;meta.main)
  (1)Teff K Effective temperature (phys.temperature.effective)
  (1)e_Teff K Uncertainty in Teff (stat.error;phys.temperature.effective)
  (1)logg [cm/s2] Surface gravity (phys.gravity)
  (1)e_logg [cm/s2] Uncertainty in logg (stat.error)
  (1)[Fe/H] [-] Metallicity (phys.abund.Z)
  (1)e_[Fe/H] [-] Uncertainty in [Fe/H] (stat.error;phys.abund.Fe)
  (1)Vmic km/s Microturbulent velocity (phys.veloc)
  (1)e_Vmic km/s Uncertainty in Vmic (stat.error)
  (2+3)Species (char) Element and ionization state (e.g., Fe I, Ti II) (phys.atmol.element;phys.atmol.ionization)

ALL cols		    
 (i)indexed column
  (2)n_Species (char) [*] * for abundances calculated via the spectrum synthesis method (meta.note)
  (2)[X/Fe]* [-] (n) Abundance ratio [X/Fe] for HD 218209 (phys.abund;arith.ratio)
  (2)e_[X/Fe]* [-] (n) Uncertainty in [X/Fe] (HD 218209) (stat.error;phys.abund)
  (2)o_[X/Fe]*  (n) Number of lines used in the analysis (meta.number)
  (2+3)logepsSun [-] Logarithmic abundances calculated for the Sun (phys.abund)
  (2)e_logepsSun [-] Uncertainty in logeps(X) for the Sun (stat.error)
  (2)o_logepsSun  Number of lines used in the Solar analysis (meta.number)
  (2)logeps(X) [-] (n) Logarithmic abundances for the Sun from Sahin et al., 2023PARep...1...54S (phys.abund)
  (2)e_logeps(X) [-] (n) Uncertainty in logeps(X) for the Sun from Sahin et al., 2023PARep...1...54S (stat.error)
  (2)N  (n) Number of lines used from previous work Sahin et al., 2023PARep...1...54S (meta.number)
  (2)logeps(X)ASP09 [-] Logarithmic abundances for the Sun from Asplund et al., 2009ARA&A..47..481A (phys.abund)
  (2)e_logeps(X)ASP09 [-] Uncertainty in logeps(X)_ASP09 (stat.error)
  (2)deltaASP09 [-] Difference logarithmic abundance relative to Asplund et al., 2009ARA&A..47..481A (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)logeps(X)ASP21 [-] Logarithmic abundances for the Sun from Asplund et al., 2021A&A...653A.141A (phys.abund)
  (2)e_logeps(X)ASP21 [-] Uncertainty in logeps(X)_ASP21 (stat.error)
  (2)deltaASP21 [-] Difference logarithmic abundance relative to Asplund et al., 2021A&A...653A.141A (phys.abund)
  (3)lambda 0.1nm Wavelength of the transition (em.wl;phys.atmol.transition)
  (3)LEP eV Lower excitation potential (phys.atmol.excitation;stat.min)
  (3)loggf  Oscillator strength or transition probability (phys.atmol.oscStrength)
  (3)EW 0.1pm (n) Equivalent width in the Sun (spect.line.eqWidth)
  (3)n_EW (char) [s] s for syn (meta.note)
  (3)n_logepsSun (char) [s] s for syn (meta.note)
  (3)EW* 0.1pm (n) Equivalent width in the HD 218209 (spect.line.eqWidth)
  (3)n_EW* (char) [s] s for syn (meta.note)
  (3)logeps* [-] (n) Logarithmic abundances for HD 218209 (phys.abund)
  (3)RMT  (n) Rowland Multiplet Number (meta.id;meta.main)
  (3)Ref  Reference sources for the adopted loggf value (Note 1)   (meta.ref;pos.frame)

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