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J/ApJ/931/146
  Very metal-poor stars with LAMOST & Subaru. I. (Aoki+, 2022)
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2022ApJ...931..146A
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1.J/ApJ/931/146/table5Equivalent widths of FeI lines in the primary stars of double-lined spectroscopic binaries (6 rows)

Simple ConstraintList Of Constraints
 
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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  lambda 0.1nm [4063.59/4191.5] Wavelength, FeI, Angstroms (em.wl)
  loggf [-] [-0.7/0.07] Log, statistical weight*oscillator strength (stat.weight;phys.atmol.oscStrength)
  ExPot eV [1.5/2.9] Excitation potential (phys.atmol.excitation)
  EW-J0241+0946 0.1pm (n) [46/157.6] Equivalent width, FeI, J0241+0946 (spect.line.eqWidth)
  EW-J1144+4032 0.1pm (n) [110] Equivalent width, FeI, J1144+4032 (spect.line.eqWidth)
  EW-J1216+0231 0.1pm (n) [40.8/83.8] Equivalent width, FeI, J1216+0231 (spect.line.eqWidth)
  EW-J1220+1637 0.1pm (n) [71.2] Equivalent width, FeI, J1220+1637 (spect.line.eqWidth)
  EW-J1231+1232 0.1pm (n) [65.7/110.5] Equivalent width, FeI, J1231+1232 (spect.line.eqWidth)
  EW-J1859+4506 0.1pm (n) [21.6/111.6] Equivalent width, FeI, J1859+4506 (spect.line.eqWidth)
  EW-J2121-0138 0.1pm (n) [60.9/170.6] Equivalent width, FeI, J2121-0138 (spect.line.eqWidth)

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