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  Abundances of HD221170 (Yushchenko+, 2005)
Post annotation
1.J/A+A/430/255/table1Iron lines in the spectrum of HD 221170 (251 rows)
2.J/A+A/430/255/table2Lines of other elements in the spectrum of HD 221170 (617 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)lambda 0.1nm Wavelength (em.wl)
  (1)Ion (char) Ion (phys.atmol.ionStage)
  (1)EW 0.1pm Equivalent width (spect.line.eqWidth)
   (ALL)loggf [-] Oscillator strength (phys.atmol.oscStrength)
   (ALL)Elow eV Energy of lower level (;phys.atmol.level)
  (1)logN  Abundance, in logN(H)=12 scale (phys.abund)
  (2)Ion  Ion number (e.g. 26.00 = Fe I) (;meta.main)
  (2)n_loggf (char) [ab] Note on loggf (Note 1)   (meta.note)
  (2)l_Abun (char) Limit flag on DlogN (meta.code.error)
  (2)Abun [Sun] Abundance of ion (relative to Sun, log scale) (phys.abund)

ALL cols
 (i)indexed column
  (2)l_logN (char) Limit flag on logN (meta.code.error)
  (2)logN [-] HD 221170 abundance (in logN(H)=12 scale) (Note 2)   (phys.abund)
  (2)logNS [-] (n) Sun abundance (in logN(H)=12 scale) (phys.abund)
  (2)Blend  (n) HD 221170 level of blending (1=clean line) (meta.note)
  (2)BlendS  (n) Sun level of blending (1=clean line) (meta.note)
  (2)Depth  (n) HD 221170 depth in synthetic spectra (Note 2)   (phot.flux.density;arith.ratio)
  (2)DepthS  (n) Sun depth in synthetic spectra (phot.flux.density;arith.ratio)
  (2)dAbG [Sun] (n) Abundance change with logg (+0.2) (stat.error)
  (2)dAbT [Sun] (n) Abundance change with Teff (+100K) (stat.error)

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