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  Deep NIR spectrum of the Orion Bar PDR (Kaplan+, 2017)
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1.J/ApJ/838/152/table1H2 lines observed in the Orion Bar (link to Fig.1) (87 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)
  lambda um [1.5/2.5] H2 line vacuum wavelength (Note 1)   (em.wl;spect.line)
  Dellam 10-6um [-21.5/9.7] Difference between lambda and observed centroid (Note 2)   (
  Line (char) H2 line rovibrational identifier (Note 3)   (;spect.line)
  logFi/Fr [-] [-1.7/1.3] Log normalized line flux (Note 4)   (phot.flux;arith.ratio)
  E_logFi/Fr [-] [0/0.1] Upper uncertainty in logFi/Fr (stat.error;stat.max)
  e_logFi/Fr [-] [0/0.2] Lower uncertainty in logFi/Fr (stat.error;phys.abund)
  S/N   [4/1032] Signal-to-Noise (Note 5)   (stat.snr)
  vu   [1/10] Transition upper vibrational state (phys.mol;phys.atmol.transition)
  Ju   [0/13] Transition upper rotational state (phys.mol.qn)
  Eu/k K [6149/45317] Energy of upper state (Note 6)   (
  logAul [s-1] [-8/-5.5] Log rovibrational radiative transition probability (Note 7)   (phys.atmol.transProb)
  lnR [-] [-5.2/4] Natural log column density (Note 8)   (phys.columnDensity)
  E_lnR [-] [0.001/0.3] Upper uncertainty in lnR (stat.error;stat.max)
  e_lnR [-] [0.001/0.3] Lower uncertainty in lnR (stat.error)
  Nu/Nm   [0.3/2] Ratio observed column density (Note 9)   (

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