VizieR

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

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J/A+AS/113/71
  Lines in the infrared solar spectrum (Ramsauer+, 1995)
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1.J/A+AS/113/71/table4Possible blends rejected as too weak in H-band (34 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)
  SolLam 0.1nm Solar wavelength of the lines (em.wl)
  Ion (char) Ions and diatomic molecules identified as sources of the solar spectral line (phys.atmol.ionization)
  LabLam 0.1nm Laboratory wavelength of ions and molecules (em.wl;phys.atmol.transition)
  n_LabLam (char) [*] See Note (5) in Table 1 and 3 (meta.note)
  ExcPot eV Excitation potential of the lower level of the transition (phys.energy;phys.atmol.excitation)
  log(gf)  Logarithm of the statistically weighted oscillator strength of the corresponding atomic line from Kurucz (1991) (phys.atmol.wOscStrength)
  n_log(gf) (char) [b] See Note (10) in Table 1 and 3 (meta.note)

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