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J/AJ/145/107
  Zr, Ba, La, and Eu abundances in 19 open clusters (Jacobson+, 2013)
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2013AJ....145..107J
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1.J/AJ/145/107/clusters(c)Cluster sample (table1), and their mean abundances (table8) (19 rows)
2.J/AJ/145/107/stars(c)Stellar atmospheric parameters and Fe abundances (table2), individual [X/Fe] rations for Zr (table4), Ba (table5), La (table6), and Eu (table7) (50 rows)
3.J/AJ/145/107/table3Line list (10 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (1+2)Cluster (char) (i) Cluster name linkRole{individual abundances } (meta.id;meta.main)
  (1)Age Gyr Cluster age (adopted from Salaris et al., 2004A&A...414..163S) (Note 1)   (time.age)
  (1)f_Age (char) [d] Cluster age from Villanova et al. 2007 (Note 1)   (meta.code)
  (1)Dist kpc Distance (pos.distance;pos.heliocentric)
  (1)Rgc kpc Galactocentric distance (R☉=8.5kpc) (pos.distance;pos.galactocentric)
  (1)Ref (char) Reference for distances (Note 2)   (meta.ref;pos.frame)
  (1)N1  Number of stars (meta.number)
  (1)N2  (n) Number of stars (from spectra obtained on Keck) (meta.number)
  (1)Tel (char) Telescope (KPNO4m, Keck, or HET) (Note 3)   (meta.id;instr.tel)
  (1)C (char) [ab] Calculation of [X/Fe] ratios (Note 4)   (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)[Fe/H] [Sun] Cluster mean [Fe/H] abundance (phys.abund.Fe;stat.mean)
  (1)s_[Fe/H] [Sun] 1σ standard deviation in [Fe/H] (stat.stdev;phys.abund.Fe)
  (1)[Zr/H] [Sun] Cluster mean [Zr/H] abundance (phys.abund)
  (1)s_[Zr/H] [Sun] 1σ standard deviation in [Zr/H] (stat.stdev;phys.abund)
  (1)[Ba/Fe] [Sun] Cluster mean [Ba/Fe] abundance (phys.abund)
  (1)s_[Ba/Fe] [Sun] 1σ standard deviation in [Ba/Fe] (stat.stdev;phys.abund)
  (1)[La/Fe] [Sun] Cluster mean [La/Fe] abundance (phys.abund)
  (1)s_[La/Fe] [Sun] 1σ standard deviation in [La/Fe] (stat.stdev;phys.abund)
  (1)[Eu/Fe] [Sun] (n) Cluster mean [Eu/Fe] abundance (phys.abund)
  (1)s_[Eu/Fe] [Sun] (n) 1σ standard deviation in [Eu/Fe] (stat.stdev;phys.abund)
  (1)N  Number of stars used to determined the mean abundances (Note 5)   (meta.number)
  (1)F+10  (n)Display the data from Friel et al. (2010, cat. J/AJ/139/1942) if any (meta.number)
  (1+2)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2)_RA deg (n)(i) Positions from SIMBAD database (right ascension part) (pos.eq.ra;meta.main)
  (1+2)_DE deg (n)(i) Positions from SIMBAD database (declination part) (pos.eq.dec;meta.main)
  (2)Star (char) Star name (in Cluster) (meta.id;meta.main)
  (2)Teff K Effective temperature (phys.temperature.effective)
  (2)logg [cm/s2] Surface gravity (phys.gravity)
  (2)vt km/s Microturbulent velocity (phys.veloc)
  (2)[FeI/H] [Sun] Metallicity from FeI lines (Note 1)   (phys.abund.Z)
  (2)s_[FeI/H] [Sun] 1σ standard deviation in [FeI/H] (stat.stdev;phys.abund)
  (2)o_[FeI/H]  Number of FeI lines (meta.number)
  (2)[FeII/H] [Sun] Metallicity from FeII lines (Note 1)   (phys.abund.Z)
  (2)s_[FeII/H] [Sun] 1σ standard deviation in [FeII/H] (stat.stdev;phys.abund)
  (2)o_[FeII/H]  Number of FeII lines (meta.number)
  (2)[Zr/Fe]1 [Sun] Abundance from the ZrIλ6127 lines (Note 7)   (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)[Zr/Fe]2 [Sun] (n) Abundance from ZrIλ6134 lines (Note 7)   (phys.abund)
  (2)[Zr/Fe]3 [Sun] Abundance from the ZrIλ6143 lines (Note 7)   (phys.abund)
  (2)<[Zr/Fe]> [Sun] Mean star [Zr/Fe] abundance (phys.abund)
  (2)s_<[Zr/Fe]> [Sun] 1σ standard deviation in <[Zr/Fe]> (stat.stdev;phys.abund)
  (2)[Ba/Fe]1 [Sun] Abundance from the BaIIλ5853 lines (Note 8)   (phys.abund)
  (2)[Ba/Fe]2 [Sun] Abundance from the BaIIλ6141 lines (Note 8)   (phys.abund)
  (2)[Ba/Fe]3 [Sun] Abundance from the BaIIλ6496 lines (Note 8)   (phys.abund)
  (2)<[Ba/Fe]> [Sun] Mean star [Ba/Fe] abundance (Note 9)   (phys.abund)
  (2)s_<[Ba/Fe]> [Sun] 1σ standard deviation in <[Ba/Fe]> (Note 9)   (stat.stdev;phys.abund)
  (2)[La/Fe]1 [Sun] (n) Abundance from LaIIλ6262 lines (Note 10)   (phys.abund)
  (2)e_[La/Fe]1 [Sun] (n) Uncertainty in [La/Fe]1 (Note 11)   (stat.error;phys.abund)
  (2)[La/Fe]2 [Sun] (n) Abundance from LaIIλ6390 lines (Note 10)   (phys.abund)
  (2)e_[La/Fe]2 [Sun] (n) Uncertainty in [La/Fe]2 (Note 11)   (stat.error;phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)<[La/Fe]> [Sun] (n) Mean star [La/Fe] abundance (phys.abund)
  (2)s_<[La/Fe]> [Sun] (n) 1σ standard deviation in <[La/Fe]> (stat.stdev;phys.abund)
  (2)[Eu/Fe]1 [Sun] (n) Abundance from EuIIλ6437 lines (Note 12)   (phys.abund)
  (2)e_[Eu/Fe]1 [Sun] (n) Uncertainty in [Eu/Fe]1 (Note 13)   (stat.error;phys.abund)
  (2)[Eu/Fe]2 [Sun] (n) Abundance from EuIIλ6645 lines (Note 12)   (phys.abund)
  (2)e_[Eu/Fe]2 [Sun] (n) Uncertainty in [Eu/Fe]2 (Note 13)   (stat.error;phys.abund)
  (2)<[Eu/Fe]> [Sun] (n) Mean star [Eu/Fe] abundance (phys.abund)
  (2)s_<[Eu/Fe]> [Sun] (n) 1σ standard deviation in <[Eu/Fe]> (stat.stdev;phys.abund)
  (2)OCat  (n)Cross-match with Yong et al. (2012, cat. J/AJ/144/95), Jacobson et al. (2009, cat. J/AJ/137/4753), and Friel et al. (2010, cat. J/AJ/139/1942) within 1.5" (meta.ref.url)
  (3)El (char) Element/Ion (Zr I, Ba II, La II, or Eu II) (meta.note)
  (3)lambda 0.1nm Wavelength (Å) (em.wl)
  (3)EP eV Excitation potential (phys.atmol.excitation)
  (3)loggf [-] Log of the oscillator strength (phys.atmol.oscStrength)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)f_loggf (char) [e] Origin of loggf (Note 2)   (meta.code)
  (3)Abund1 [-] Element Solar abundance (logε(Fe)) (Note 3)   (phys.abund)
  (3)Abund2 [-] Element Solar abundance (logε(Fe)) (Note 4)   (phys.abund)
  (3)Abund3 [-] Element Arcturus abundance (logε(X)) (Note 5)   (phys.abund)
  (3)f_Abund3 (char) [f] This abundance is forced to match that for the EuII 6645 feature; details in Section 3.2.4 (meta.code)
  (3)[X/Fe] [Sun] Arcturus [X/Fe] ratio (Note 6)   (phys.abund)

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