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  Main-sequence star chromospheres (Houdebine+, 2010)
Post annotation
1.J/MNRAS/403/2157/table1aTotal results for each Flux sets (32 rows)
2.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: + - )
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)dEW 0.1pm (n) Difference equivalent widths between Gl867A and Gl 205 (spect.line.eqWidth;arith.diff)
   (ALL)Flux hW/m2 Continuum flux from Allard et al. (1997ARA&A..35..137A) (in 105erg/cm2/s) (phot.flux)
   (ALL)lam.F 0.1nm (i) Flux wavelength (Å) (em.wl)
   (ALL)dFlux 10W/m2 Difference radiative losses in the lines (Note 1)   (phot.flux)
   (ALL)No  (n) Order number of the corresponding spectral order (
  (2)lambda0 0.1nm (n) Vacuum wavelength (em.wl)
  (2)lambda 0.1nm (n) Gl 205 wavelength (em.wl)
  (2)Ident (char) Line identification (;spect.line)
  (2)Rem (char) Original catalog from which we identified each line (meta.note)

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