VizieR

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

  
J/A+A/661/A103
  High-precision chemical abundances of Sequoia (Matsuno+, 2022)
ReadMe+ftp
2022A&A...661A.103M
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Post annotation 		img(gal)
1.J/A+A/661/A103/lineLine list (3173 rows)

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)
  Object (char) Object name used in this study (meta.id;meta.main)
  species (char) Name of the species (phys.atmol.element)
  lambda 0.1nm Wavelength (em.wl)
  chi eV Excitation potential (phys.atmol.excitation)
  loggf  loggf value (phys.atmol.oscStrength)
  EW 0.1pm Equivalent width (mÅ) (spect.line.eqWidth)
  e_EW 0.1pm Uncertainty in equivalent width (mÅ) (stat.error;spect.line.eqWidth)
  A  Abundance from this line (phys.abund)
  eAteff  Uncertainty in abundance due to effective temperature (stat.error)
  eAlogg  Uncertainty in abundance due to surface gravity (stat.error)
  eAvt  Uncertainty in abundance due to microturbulent velocity (stat.error)
  eA[Fe/H]  Uncertainty in abundance due to metallicity (stat.error)
  eAEW (char) Uncertainty in abundance due to equivalent widths of this star and the reference star (stat.error)
  sX  Uncertainty floor (stat.error)
  Weight  Weight used to obtain the best estimate for the abundance of the species (phys.atmol.weight;meta.modelled)

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