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  Warm molecular hydrogen in SINGS galaxy sample (Roussel+, 2007)
Post annotation
1.J/ApJ/669/959/table4Derived temperatures, column densities and high temperature ortho to para ratio (OPRhighT) (153 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)
  Name (char) Galaxy name (Note 1)   (;meta.main)
  f_Name (char) [abc] Flag on name (Note 2)   (phys.mass;arith.ratio)
  l_T1 (char) Limit flag on T1 (meta.code.error)
  T1 K Lower temperature component (phys.temperature)
  l_f1 (char) Limit flag on f1 (meta.code.error)
  f1  Discrete component mass fraction at T1 (phys.mass;arith.ratio)
  l_T2 (char) Limit flag on T2 (meta.code.error)
  T2 K Upper temperature component (phys.temperature)
  l_f2 (char) Limit flag on f2 (meta.code.error)
  f2  Discrete component mass fraction at T2 (phys.mass;arith.ratio)
  OPR  (n) Ortho to para ratio in the high-temperature limit (phys.atmol.branchingRatio)
  e_OPR  (n) Uncertainty in OPR (stat.error)
  Ntot 10+20/cm2Total H2 column density for T>T1 (phys.columnDensity)
  RNtot  (n) Ratio of the total H2 column densities, Ntot(OPR=3)/Ntot(OPR<3) (phys.columnDensity)

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