VizieR

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

VizieR

  
J/MNRAS/441/3127
  FeI oscillator strengths for Gaia-ESO (Ruffoni+, 2014)
Post annotation
  
1.J/MNRAS/441/3127/table3Experimental branching fractions, transition probabilities, and log(gf)s for the FeI levels listed in table 2 of the paper (167 rows)
2.J/MNRAS/441/3127/table4Lines measured in previous studies, or predicted to have a BF greater than 1%, that were omitted from the BF measurements shown in table 3 (32 rows)
3.J/MNRAS/441/3127/table5Lines from table 3 selected for solar analysis (36 rows)

 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
  (1+2)State (char) [A-L] State (Note G1)   ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (1+2)Level (char) Lower Level ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (1+2)Note (char) [*] Wavenumber from our spectra (Note G2)   ((unassigned);(unassigned);(unassigned);phys.veloc.orbital)
   (ALL)lam.Air 0.1nm (i) [2722/13261] Transition air wavelength (Å) ((unassigned);(unassigned);(unassigned);meta.bib.author;(unassigned))
  (1+2)sigma cm-1 [7539/36727] Transition wavenumber {sigma} ((unassigned);(unassigned);(unassigned);instr.spect)
  (1)S (char) S indicates lines selected for solar analysis (table5) ((unassigned);phys.veloc.orbital;arith.diff;pos.geocentric)
  (1)BF  (n) [0/1] Branching fraction (Note 1)   ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (1)e_BF % (n) Precentage uncertainty in branching fraction ((unassigned);phys.veloc.orbital;arith.diff;time.age;meta.main)
  (1)Aul 10-6s-1 (n) Transition probability ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (1+3)loggf [-] (n) Oscillator strength measured in this work ((unassigned);(unassigned);(unassigned);(unassigned))

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+3)e_loggf [-] (n) Uncertainty in oscillator strength ((unassigned);phys.veloc.orbital;arith.diff;time.age;phys.fluence)
   (ALL)loggf0 [-] (n) Best previously published oscillator strength ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.dispersion;(unassigned);src.orbital.inclination)
   (ALL)e_loggf0 [-] (n) Uncertainty in loggf0 (Note G3)   ((unassigned);(unassigned);(unassigned);time.age;meta.main)
   (ALL)q_loggf0 (char) [DE+ ] Uncertainty flag on loggf0 (Note G3)   ((unassigned);pos.wcs.naxis;arith.grad;pos.cartesian)
   (ALL)r_loggf0 (char) Reference to source of loggf0 (Note G4)   ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.dispersion;€?**ucdid=0**?)
  (1)GES (char) 'Yes' if the line is a GES target (Gaia-ESO public Spectroscopic survey) ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.orbital)
  (2)l_BFp (char) [<] Contains '<' if BFp is less than 0.001 ((unassigned);phys.veloc.orbital;arith.diff;pos.galactic.lon)
  (2)BFp   [0/1] Predicted branching fraction ((unassigned);(unassigned);(unassigned);(unassigned))
  (2)Reason (char) Reason for omission of the line ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.orbital)
  (2)Blend (char) List of blended lines when Reason='Blended' (Note 1)   ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.orbital)
  (3)chi eV Lower level transition energy {chi} ((unassigned);(unassigned);(unassigned);(unassigned);(unassigned))
  (3)VdW  Van der Waals damping parameter (Note 1)   ((unassigned);(unassigned);(unassigned);time.obs.end;meta.main)
  (3)eps [-] Solar iron abundance, log{epsilon}(Fe), obtained for this line using loggf ((unassigned);(unassigned);(unassigned);phys.reflectance)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)eps0 [-] Solar iron abundance, log{epsilon}(Fe), obtained for this line using loggf0 ((unassigned);(unassigned);(unassigned);phys.reflectance)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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