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  Ultraviolet Spectrum of the Sun (Samain, 1995)
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1.J/A+AS/113/237/table3Observed wavelengths, laboratory values and identifications (660 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)
  SpOrd  Spectrum order (instr.order)
  SolLam 0.1nm Wavelength determination of all solar and telluric lines measurable on the spectrum (Note 1)   (em.wl)
  n_SolLam (char) See Note (Note 2)   (meta.note)
  Intens   []? Intensity of the line in an arbitrary scale from 0 to 9 (3) (Note 3)   (meta.code;spect.line.intensity)
  n_Intens (char) When '?' uncertain value (meta.note)
  Type (char) Acronyms for the type of line (Note 4)   (meta.note)
  Identif (char) Possible element responsible for the observed line (Note 5)   (phys.atmol.element)
  LabLam (char) 0.1nm Laboratory wavelength (em.wl;phys.atmol.transition)
  n_LabLam (char) [St] When 'St' the line is used or recommended as reference wavelength standard (meta.note)
  r_LabLam (char) References of the wavelength sources (Note 6)   (meta.ref)
  DLam 0.1nm []? Difference between the observed wavelength and the laboratory wavelength: dlambda=lambda(Sun or O2) - lambda(lab) (em.wl;arith.diff)

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