VizieR

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

VizieR

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J/MNRAS/450/1900
  Chemical abundances of 257 giant stars (Adibekyan+, 2015)
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2015MNRAS.450.1900A
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/450/1900/stars(c)The stars studied: abundances of the elements derived by using the best lines, and population assignement (257 rows)
2.J/MNRAS/450/1900/table2Abundances, rms, error, and number of lines for each star and element (257 rows)
3.J/MNRAS/450/1900/ewEquivalent widths of the spectral lines used to derive abundances (30228 rows)
4.J/MNRAS/450/1900/linelistAtomic parameters for lines selected in the paper (118 rows)

Simple ConstraintList Of Constraints
 
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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)Star (char) (i) Star's identifier (meta.id;meta.main)
  (1+2)Nw  (n)Number of equivalent widths for this star (meta.number)
  (1+2)[Mg/H] [Sun] Abundance [Mg/H] (Z=12) (Note G1)   (phys.abund)
  (1+2)[Al/H] [Sun] (n) Abundance [Al/H] (Z=13) (Note G1)   (phys.abund)
  (1+2)[Si/H] [Sun] Abundance [Si/H] (Z=14) (Note G1)   (phys.abund)
  (1+2)[Ca/H] [Sun] Abundance [Ca/H] (Z=20) (Note G1)   (phys.abund)
  (1+2)[ScI/H] [Sun] Abundance [ScI/H] (Z=21.0) (Note G1)   (phys.abund)
  (1+2)[ScII/H] [Sun] Abundance [ScII/H] (Z=21.1) (Note G1)   (phys.abund)
  (1+2)[TiI/H] [Sun] Abundance [TiI/H] (Z=22.0) (Note G1)   (phys.abund)
  (1+2)[TiII/H] [Sun] Abundance [TiII/H] (Z=22.0) (Note G1)   (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2)[V/H] [Sun] Abundance [V/H] (Z=23) (Note G1)   (phys.abund)
  (1+2)[CrI/H] [Sun] Abundance [CrI/H] (Z=24.0) (Note G1)   (phys.abund)
  (1+2)[Co/H] [Sun] Abundance [Co/H] (Z=27) (Note G1)   (phys.abund)
  (1+2)[Ni/H] [Sun] Abundance [Ni/H] (Z=28) (Note G1)   (phys.abund)
  (1)Simbad (char) ask the Simbad data-base about this object (phys.abund)
  (1)Ulsr km/s (n)U velocity of the star relative to the LSR (Note 1)   (phys.veloc;pos.cartesian.x)
  (1)Vlsr km/s (n)V velocity of the star relative to the LSR (Note 1)   (phys.veloc;pos.cartesian.y)
  (1)Wlsr km/s (n)W velocity of the star relative to the LSR (Note 1)   (phys.veloc;pos.cartesian.z)
  (1)pD1  (n) [0/1] Probability of a star belonging to the thick disc according to B03 (Note 2)   (stat.fit.goodness)
  (1)ptD1  (n) [0/1] Probability of a star belonging to the thin disc according to B03 (Note 2)   (stat.fit.goodness)
  (1)pH1  (n) [0/1] Probability of a star belonging to the halo according to B03 (Note 2)   (stat.fit.goodness)
  (1)pop1 (char) probable population where the star belongs according to B03 (thin, thick or trans) (src.class)
  (1)pD2  (n) [0/1] Probability of a star belonging to the thick disc according to R03 (Note 3)   (stat.fit.goodness)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)ptD2  (n) [0/1] Probability of a star belonging to the thin disc according to R03 (Note 3)   (stat.fit.goodness)
  (1)pH2  (n) [0/1] Probability of a star belonging to the halo according to R03 (Note 3)   (stat.fit.goodness)
  (1)pop2 (char) probable population where the star belongs according to R03 (thin, thick or trans) (src.class)
  (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)[Na/H] [Sun] (n) Abundance [Na/H] (Z=11) (G1) (Note 1)   (phys.abund)
  (2)e_[Na/H] [Sun] rms uncertainty of [Na/H] (stat.error;phys.abund)
  (2)s_[Na/H] [Sun] Total error of [Na/H] (stat.error;phys.abund)
  (2)[Na/H]c [Sun] Abundance [Na/H] after correction for effective temperature trend (Note 2)   (phys.abund)
  (2)o_[Na/H]  Number of Na lines used (meta.number)
  (2)e_[Mg/H] [Sun] rms uncertainty of [Mg/H] (stat.error;phys.abund)
  (2)s_[Mg/H] [Sun] Total error of [Mg/H] (stat.error;phys.abund)
  (2)[Mg/H]c [Sun] Abundance [Mg/H] after correction for effective temperature trend (Note 2)   (phys.abund)

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

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

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)e_[V/H] [Sun] rms uncertainty of [V/H] (stat.error;phys.abund)
  (2)s_[V/H] [Sun] Total error of [V/H] (stat.error;phys.abund)
  (2)[V/H]c [Sun] Abundance [V/H] after correction for effective temperature trend (Note 2)   (phys.abund)
  (2)o_[V/H]  Number of VI lines used (meta.number)
  (2)e_[CrI/H] [Sun] rms uncertainty of [CrI/H] (stat.error;phys.abund)
  (2)s_[CrI/H] [Sun] Total error of [CrI/H] (stat.error;phys.abund)
  (2)[CrI/H]c [Sun] Abundance [CrI/H] after correction for effective temperature trend (Note 2)   (phys.abund)
  (2)o_[CrI/H]  Number of CrI lines used (meta.number)
  (2)[CrII/H] [Sun] (n) Abundance [CrII/H] (Z=24.1) (G1) (Note 1)   (phys.abund)
  (2)e_[CrII/H] [Sun] (n) rms uncertainty of [CrII/H] (stat.error;phys.abund)
  (2)s_[CrII/H] [Sun] (n) Total error of [CrII/H] (stat.error;phys.abund)
  (2)[CrII/H]c [Sun] (n) Abundance [CrII/H] after correction for effective temperature trend (Note 2)   (phys.abund)
  (2)o_[CrII/H]  (n) Number of CrII lines used (meta.number)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)[Mn/H] [Sun] Abundance [Mn/H] (Z=25) (G1) (Note 1)   (phys.abund)
  (2)e_[Mn/H] [Sun] rms uncertainty of [Mn/H] (stat.error;phys.abund)
  (2)s_[Mn/H] [Sun] Total error of [Mn/H] (stat.error;phys.abund)
  (2)o_[Mn/H]  Number of MnI lines used (meta.number)
  (2)e_[Co/H] [Sun] rms uncertainty of [Co/H] (stat.error;phys.abund)
  (2)s_[Co/H] [Sun] Total error of [Co/H] (stat.error;phys.abund)
  (2)[Co/H]c [Sun] Abundance [Co/H] after correction for effective temperature trend (Note 2)   (phys.abund)
  (2)o_[Co/H]  Number of CoI lines used (meta.number)
  (2)e_[Ni/H] [Sun] rms uncertainty of [Ni/H] (stat.error;phys.abund)
  (2)s_[Ni/H] [Sun] Total error of [Ni/H] (stat.error;phys.abund)
  (2)[Ni/H]c [Sun] Abundance [Ni/H] after correction for effective temperature trend (Note 2)   (phys.abund)
  (2)o_[Ni/H]  Number of NiI lines used (meta.number)
  (3+4)lambda 0.1nm Central wavelength (em.wl.central)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)EW 0.1pm Equivalent width of the line (spect.line.eqWidth)
  (4)El (char) Element and ionization state (phys.atmol.element;phys.atmol.ionization)
  (4)EP eV Excitation potential (phys.atmol.excitation)
  (4)loggf [-] Oscilator strength (phys.atmol.collStrength)
  (4)Dab [-] [-3.9/10.8] Difference in abundances between dwarfs and giants relative to σ (Note 1)   (phys.abund)

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