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  Main-sequence star chromospheres (Houdebine+, 2010)
Post annotation
1.J/MNRAS/403/2157/table1List of the spectral lines sensitive to chromospheric activity (602 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)
  lambda0 0.1nm (n) Vacuum wavelength (em.wl)
  lambda 0.1nm (n) Gl 205 wavelength (em.wl)
  dEW 0.1pm Difference equivalent widths between Gl867A and Gl 205 (spect.line.eqWidth;arith.diff)
  Flux hW/m2 Continuum flux from Allard et al. (1997ARA&A..35..137A) (in 105erg/cm2/s) (phot.flux)
  lam.F 0.1nm Flux wavelength (em.wl)
  dFlux 10W/m2 Difference radiative losses in the lines (phot.flux)
  Ident (char) Line identification (;spect.line)
  No  (n) Order number of the corresponding spectral order (
  Rem (char) Original catalog from which we identified each line (meta.note)

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