VizieR

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

VizieR

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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+A/545/A32
  Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)
Post annotation
img(gal)
1.J/A+A/545/A32/table45(c)Abundances, rms, number of lines for each star, and assignements to a Galactic population (1111 rows)
2.J/A+A/545/A32/ewEquivalent widths of the spectral lines used to derive abundances (179638 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)
   (ALL)Star (char) (i) Star's identifier (meta.id;meta.main)
  (1)Teff K Effective Temperature (Note 1)   (phys.temperature.effective)
  (1)logg [cm/s2] Surface gravity (Note 1)   (phys.gravity)
  (1)[Fe/H]  Iron abundance [Fe/H] (Note 1)   (phys.abund.Fe)
  (1)Vtur km/s Turbulence speed (Note 1)   (phys.abund)
  (1)[Na/H] [Sun] (n) Abundance [Na/H] (Z=11) (Note 2)   (phys.abund)
  (1)e_[Na/H] [Sun] (n) rms uncertainty of [Na/H] (stat.error;phys.abund)
  (1)o_[Na/H]  (n) Number of Na lines used (meta.number)
  (1)[Na/H]c [Sun] (n) Abundance [Na/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[Mg/H] [Sun] Abundance [Mg/H] (Z=12) (Note 2)   (phys.abund)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)e_[Mg/H] [Sun] rms uncertainty of [Mg/H] (stat.error;phys.abund)
  (1)o_[Mg/H]  Number of MgI lines used (meta.number)
  (1)[Al/H] [Sun] (n) Abundance [Al/H] (Z=13) (Note 2)   (phys.abund)
  (1)e_[Al/H] [Sun] (n) rms uncertainty of [Al/H] (stat.error;phys.abund)
  (1)o_[Al/H]  (n) Number of AlI lines used (meta.number)
  (1)[Al/H]c [Sun] (n) Abundance [Al/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[Si/H] [Sun] Abundance [Si/H] (Z=14) (Note 2)   (phys.abund)
  (1)e_[Si/H] [Sun] rms uncertainty of [Si/H] (stat.error;phys.abund)
  (1)o_[Si/H]  Number of SiI lines used (meta.number)
  (1)[Ca/H] [Sun] Abundance [Ca/H] (Z=20) (Note 2)   (phys.abund)
  (1)e_[Ca/H] [Sun] rms uncertainty of [Ca/H] (stat.error;phys.abund)
  (1)o_[Ca/H]  Number of CaI lines used (meta.number)
  (1)[ScI/H] [Sun] (n) Abundance [ScI/H] (Z=21.0) (Note 2)   (phys.abund)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)e_[ScI/H] [Sun] (n) rms uncertainty of [ScI/H] (stat.error;phys.abund)
  (1)o_[ScI/H]  (n) Number of ScI lines used (meta.number)
  (1)[ScI/H]c [Sun] (n) Abundance [ScI/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[ScII/H] [Sun] Abundance [ScII/H] (Z=21.1) (Note 2)   (phys.abund)
  (1)e_[ScII/H] [Sun] rms uncertainty of [ScII/H] (stat.error;phys.abund)
  (1)o_[ScII/H]  Number of ScII lines used (meta.number)
  (1)[TiI/H] [Sun] Abundance [TiI/H] (Z=22.0) (Note 2)   (phys.abund)
  (1)e_[TiI/H] [Sun] rms uncertainty of [TiI/H] (stat.error;phys.abund)
  (1)o_[TiI/H]  Number of TiI lines used (meta.number)
  (1)[TiI/H]c [Sun] Abundance [TiI/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[TiII/H] [Sun] Abundance [TiII/H] (Z=22.1) (Note 2)   (phys.abund)
  (1)e_[TiII/H] [Sun] rms uncertainty of [TiII/H] (stat.error;phys.abund)
  (1)o_[TiII/H]  Number of TiII lines used (meta.number)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)[V/H] [Sun] (n) Abundance [V/H] (Z=23) (Note 2)   (phys.abund)
  (1)e_[V/H] [Sun] (n) rms uncertainty of [V/H] (stat.error;phys.abund)
  (1)o_[V/H]  (n) Number of VI lines used (meta.number)
  (1)[V/H]c [Sun] (n) Abundance [V/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[CrI/H] [Sun] Abundance [CrI/H] (Z=24.0) (Note 2)   (phys.abund)
  (1)e_[CrI/H] [Sun] rms uncertainty of [CrI/H] (stat.error;phys.abund)
  (1)o_[CrI/H]  Number of CrI lines used (meta.number)
  (1)[CrII/H] [Sun] Abundance [CrII/H] (Z=24.1) (Note 2)   (phys.abund)
  (1)e_[CrII/H] [Sun] rms uncertainty of [CrII/H] (stat.error;phys.abund)
  (1)o_[CrII/H]  Number of CrII lines used (meta.number)
  (1)[CrII/H]c [Sun] Abundance [CrII/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[Mn/H] [Sun] Abundance [Mn/H] (Z=25) (Note 2)   (phys.abund)
  (1)e_[Mn/H] [Sun] rms uncertainty of [Mn/H] (stat.error;phys.abund)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)o_[Mn/H]  Number of MnI lines used (meta.number)
  (1)[Co/H] [Sun] (n) Abundance [Co/H] (Z=27) (Note 2)   (phys.abund)
  (1)e_[Co/H] [Sun] (n) rms uncertainty of [Co/H] (stat.error;phys.abund)
  (1)o_[Co/H]  (n) Number of CoI lines used (meta.number)
  (1)[Co/H]c [Sun] (n) Abundance [Co/H] after correction for effective temperature trend (Note 3)   (phys.abund)
  (1)[Ni/H] [Sun] Abundance [Ni/H] (Z=28) (Note 2)   (phys.abund)
  (1)e_[Ni/H] [Sun] rms uncertainty of [Ni/H] (stat.error;phys.abund)
  (1)o_[Ni/H]  Number of NiI lines used (meta.number)
  (1)Ulsr km/s U velocity of the star relative to the LSR (Note 4)   (phys.veloc;pos.cartesian.x)
  (1)Vlsr km/s V velocity of the star relative to the LSR (Note 4)   (phys.veloc;pos.cartesian.y)
  (1)Wlsr km/s W velocity of the star relative to the LSR (Note 4)   (phys.veloc;pos.cartesian.z)
  (1)pDB  Probability of a star belonging to the thick disc according to B03 (Note 5)   (stat.fit.goodness)
  (1)pTDB  Probability of a star belonging to the thin disc according to B03 (Note 5)   (stat.fit.goodness)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)pHB  Probability of a star belonging to the halo according to B03 (Note 5)   (stat.fit.goodness)
  (1)popB (char) probable population where the star belongs according to B03 (halo, thin, thick, trans) (Note 5)   (meta.id)
  (1)pDR  Probability of a star belonging to the thick disc according to R03 (Note 6)   (stat.fit.goodness)
  (1)pTDR  Probability of a star belonging to the thin disc according to R03 (Note 6)   (stat.fit.goodness)
  (1)pHR  Probability of a star belonging to the halo according to R03 (Note 6)   (stat.fit.goodness)
  (1)popR (char) probable population where the star belongs according to R03 (halo, thin, thick, trans) (Note 6)   (meta.id)
  (1)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)
  (1)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (1)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (2)lambda 0.1nm Central wavelength (Å) (em.wl.central)
  (2)EW 0.1pm Equivalent width of the line (mÅ) (spect.line.eqWidth)

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