J/ApJ/860/125
  Six warm metal-poor stars iron abundances (Roederer+, 2018)
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2018ApJ...860..125R
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1.J/ApJ/860/125/table4Comparison of Fe equivalent widths and abundances from STIS -E230M (R~30000) and -E230H (R~114000) spectra (101 rows) (released 2019-11-04)
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Query by Constraints constraints help applied on Columns (Output Order: + - ) [METAcola]
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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Name (char) Star (HD84937 or HD94028) (meta.id)
  Ion (char) Species (FeI or FeII) (phys.atmol.ionStage)
  lambda 0.1nm [2297.7/3100.7] Wavelength in Angstroms (em.wl)
  ExPot eV [0/4] Excitation potential in eV (phys.atmol.excitation)
  log(gf)   [-3.1/0.5] Log of degeneracy times oscillator strength (phys.atmol.oscStrength)
  EW(E230M) 0.1pm [12.6/143] Equivalent width in milli Angstroms measured from E230M spectrum (spect.line.eqWidth)
  EW(E230H) 0.1pm [10.8/143.3] Equivalent width in milli Angstroms measured from E230H spectrum (spect.line.eqWidth)
  loge(E230M_EW) [-] [4.5/6.3] Log epsilon abundance derived from EW measured from E230M spectrum (phys.abund)
  loge(E230H_EW) [-] [4.3/6.3] Log epsilon abundance derived from EW measured from E230H spectrum (phys.abund)
  loge(E230M_s) [-] [5/6.2] Log epsilon abundance derived from synthesis of E230M spectrum (phys.abund)
  loge(E230H_s) [-] [4.9/6.3] Log epsilon abundance derived from synthesis of E230H spectrum (phys.abund)

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