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J/A+A/480/79
  Abundances of giants in five Galactic clusters (Bragaglia+, 2008)
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img(gal)
1.J/A+A/480/79/stars(c)Stars observed, and their abundances in Na, Si, Ca, TiI, TiII, CrI, CrII, Ni, Ba (table 13 of paper) (33 rows)
2.J/A+A/480/79/table14Line-by-line abundances for Mg and Al (132 rows)
3.J/A+A/480/79/ewEquivalent widths (tables 6-10 of the paper) (13002 rows)
4.J/A+A/480/79/table4WL, EP, log(gf), source of damping (209 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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+3)Cluster (char) Cluster name (meta.id.parent)
   (1+2+3)Star (char) (i) Star name in the cluster (meta.id;meta.main)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)Name (char) Original name in the paper (cluster-star) (meta.id)
  (1)SName (char) Simbad name (Note 1)   (meta.id)
  (1)SName2 (char) Second Simbad name (meta.id)
  (1)[Na/Fe]LTE [-] LTE abundance [Na/Fe] (phys.abund)
  (1)[Na/Fe]NLTE [-] NLTE abundance [Na/Fe] (phys.abund)
  (1)e_[Na/Fe]LTE [-] rms uncertainty on [Na/Fe]LTE and [Na/Fe]NLTE (stat.error;phys.abund)

ALL cols
    
 (i)indexed column
  (1)[Si/Fe] [-] Abundance [Si/Fe] (phys.abund)
  (1)e_[Si/Fe] [-] rms uncertainty on [Si/Fe] (stat.error;phys.abund)
  (1)[Ca/Fe] [-] Abundance [Ca/Fe] (phys.abund)
  (1)e_[Ca/Fe] [-] rms uncertainty on [Ca/Fe] (stat.error;phys.abund)
  (1)[TiI/Fe] [-] Abundance [Ti/Fe]I (phys.abund)
  (1)e_[TiI/Fe] [-] rms uncertainty on [TiI/Fe] (stat.error;phys.abund)
  (1)[TiII/Fe] [-] Abundance [Ti/Fe]II (phys.abund)
  (1)e_[TiII/Fe] [-] rms uncertainty on [TiII/Fe] (stat.error;phys.abund)
  (1)[CrI/Fe] [-] Abundance [Cr/Fe]I (phys.abund)
  (1)e_[CrI/Fe] [-] rms uncertainty on [CrI/Fe] (stat.error;phys.abund)
  (1)[CrII/Fe] [-] Abundance [Cr/Fe]II (phys.abund)
  (1)e_[CrII/Fe] [-] rms uncertainty on [CrII/Fe] (stat.error;phys.abund)
  (1)[Ni/Fe] [-] Abundance [Ni/Fe] (phys.abund)

ALL cols
    
 (i)indexed column
  (1)e_[Ni/Fe] [-] rms uncertainty on [Ni/Fe] (stat.error;phys.abund)
  (1)[Ba/Fe] [-] Abundance [Ba/Fe] (phys.abund)
  (1)e_[Ba/Fe] [-] rms uncertainty on [Ba/Fe] (stat.error;phys.abund)
  (2)El (char) Element (Al or Mg) (phys.atmol.element)
  (2+3+4)lambda 0.1nm Wavelength of line (em.wl;spect.line)
  (2)LogNSun [-] LogN(X) for this element in Sun (phys.abund)
  (2)LogN(X) [-] (n) LogN(X) for this element in the star (phys.abund)
  (2)[X/Fe] [-] (n) Abundance [X/Fe] for this element in the star (phys.abund)
  (3)El  Element (Note 1)   (phys.atmol.element)
  (3)EW 0.1pm Equivalent width for the star (mÅ) (spect.line.eqWidth)
  (4)Ion (char) Atom and ionization stage (phys.atmol.ionStage)
  (4)EP  Energy potential (phys.energy;phys.atmol.level)
  (4)loggf  Oscillator strength (phys.atmol.oscStrength)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)Flag   [1/4] Flag indicating source of damping (Note 1)   (meta.ref;pos.frame)

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