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  Very metal poor stars in MW halo (Mashonkina+, 2017)
Post annotation
1.J/A+A/608/A89/table3LTE and NLTE abundances from individual lines in the sample stars (4717 rows)

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)
  Star (char) Star designation (;meta.main)
  El (char) Atom (phys.atmol.element)
  Ion (char) Ion (phys.atmol.ionStage)
  lambda 0.1nm Wavelength (em.wl)
  Eexc eV Excitation energy (phys.atmol.excitation)
  loggf  Adopted gf-value (phys.absorption.coeff)
  G6/NH rad/s/cm3van der Waals damping constant log(G6/NH) at 10000K (phys.damping;arith.zp)
  EW 0.1pm (n) Equivalent width (-1 means using spectral synthesis) (spect.line.eqWidth)
  epsLTE  LTE abundance (logeps(H)=12) (phys.abund)
  epsNLTE  (n) NLTE abundance (logeps(H)=12) (phys.abund)

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