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  Atomic lines in IR spectra for ultracool dwarfs (Lyubchik+, 2004)
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1.J/A+A/416/655/table1Atomic lines found in ultracool dwarf synthetic spectrum from 1-2.5um (198 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)
  Pr  (n) Priority of the line for measurement of atomic data (Note 1)   (
  n_Ion (char) [*] Note on measurements (Note 2)   (meta.note)
  lambda 0.1nm Wavelength of the line in air (Note 3)   (em.wl;phys.atmol.transition)
  Ion (char) Element name with ionization stage (phys.atmol.element)
  UCDss  Residual flux (F(line)/F(cont.)) in "ultracool dwarf" synthetic spectrum (phot.flux;arith.ratio)
  Arss  Residual flux (F(line)/F(cont.)) in "Arcturus-like" synthetic spectrum (phot.flux;arith.ratio)
  l_ArAt (char) [~] Limit flag on ArAt (Note 4)   (meta.code.error)
  ArAt  (n) Residual line intensity from hard copy of Arcturus atlas (accuracy 0.01-0.02) (Note 6)   (spect.line.intensity)
  n_ArAt (char) [bl T] Note on ArAt (Note 5)   (meta.note)
  l_SsAt (char) [~] Limit flag on SsAt (Note 4)   (meta.code.error)
  SsAt  (n) Residual line intensity from hard copy of Sunspot umbra atlas (accuracy 0.02-0.03) (Note 5)   (spect.line.intensity)
  n_SsAt (char) [bl T] Note on SsAt (Note 5)   (meta.note)

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