VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/A+AS/113/71
  Lines in the infrared solar spectrum (Ramsauer+, 1995)
Post annotation
  
1.J/A+AS/113/71/table1Lines judged to be relatively unblended from a visual examination between 1.00 and 1.34um (339 rows)
2.J/A+AS/113/71/table2Possible blends rejected as too weak (101 rows)
3.J/A+AS/113/71/table3Lines judged to be relatively unblended from a visual examination in the H-band(1.49-1.80um) (353 rows)
4.J/A+AS/113/71/table4Possible blends rejected as too weak in H-band (34 rows)

 
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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)SolLam 0.1nm Solar wavelength of the lines (Note 1)   (em.wl)
  (1+3)Vac cm-1 []? Vaccum wavenumber (phys.energy;phys.atmol.transition)
  (1+3)n_Vac (char) [*] See (Note 2)   (meta.note)
  (1+3)BlI1 (char) Blending index derived from Delbouille et al. (1981) (spect.index)
  (1+3)n_BlI1 (char) [ab ] See (Note 3)   (meta.note)
  (1+3)BlI2 (char) Blending index derived from Livingstone and Wallace (1991) and Wallace et al. (1993) (spect.index)
   (ALL)Ion (char) Ions and diatomic molecules identified as sources of the solar spectral line (phys.atmol.ionization)
  (1+3)n_Ion (char) [ab] See (Note 4)   (meta.note)
   (ALL)LabLam 0.1nm []? Laboratory wavelength of ions, molecules (em.wl;phys.atmol.transition)
   (ALL)n_LabLam (char) [*] See (Note 5)   (meta.note)

ALL cols
    
 (i)indexed column
  (1+3)Trans (char) Atomic or molecular transition. The notation of the terms in the identified transitions follows the National Bureau of Standards (NBS) compilations of atomic energy levels, Kurucz (1991) and Nave et al. (1994). (meta.id;phys.atmol.transition)
  (1+3)r_Trans (char) References for transition (Note 6)   (meta.ref)
  (1+3)n_Trans (char) [*!abcde] See (Note 7)   (meta.note)
   (ALL)ExcPot eV []? Excitation potential of the lower level of the transition (phys.energy;phys.atmol.excitation)
  (1+3)gcalc   []? Effective Lande factor calculated from the listed transition (phys.atmol.wOscStrength)
  (1+3)n_gcalc (char) [*a] See (Note 8)   (meta.note)
  (1+3)gemp   []? Effective Lande factor derived empirically from laboratory measurements (phys.atmol.wOscStrength)
  (1+3)n_gemp (char) [?] See (Note 9)   (meta.note)
  (1+3)ChiPi   []? Second order coefficient of the π-component of the expansion of a spectral line according to its Zeeman moments (Mathys and Stenflo 1987) (spect.line.broad.Zeeman)
  (1+3)ChiSigma   []? Second order coefficient of the σ-component of the expansion of a spectral line according to its Zeeman moments (Mathys and Stenflo 1987) (spect.line.broad.Zeeman)
  (1+3)YSigma   []? Third order coefficient of the σ-component of the expansion of a spectral line according to its Zeeman moments (Mathys and Stenflo 1987) (stat.fit.param)
  (1+3)CalcLam 0.1nm []? Calculated wavelength (em.wl)
   (ALL)log(gf)   []? Logarithm of the statistically weighted oscillator strength of the corresponding atomic line from Kurucz (1991) (phys.atmol.wOscStrength)

ALL cols
    
 (i)indexed column
   (ALL)n_log(gf) (char) [abcd] See (Note 10)   (meta.note)

ALL cols
    
 (i)indexed column
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