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J/MNRAS/450/397
  Spectroscopic study of RGs in the Kepler field (Takeda+, 2015)
Post annotation
img(gal)
1.J/MNRAS/450/397/tablee2Broadening velocities and abundances from 6080-6089Å fit (58 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  KIC   [1726211/12884274] KIC number (meta.id;meta.main)
  Source (char) [snc] Code indicating the source of spectrum (Note 1)   (meta.ref;pos.frame)
  Teff K [4519/5472] Effective temperature (phys.temperature.effective)
  logg [cm/s2] [2.34/3.75] Logarithmic surface gravity (phys.gravity)
  vt km/s [0.74/1.46] Microturbulent velocity (phys.veloc)
  [Fe/H]1 [Sun] [-0.72/0.37] Logarithmic Fe abundance relative to the Sun (phys.abund.Fe)
  vM km/s [3.11/4.81] Total macrobroadening (Gaussian e-folding width) (spect.line.broad)
  vip km/s [2.25/2.69] Instrumental broadening (Gaussian e-folding width) (spect.line.broad)
  vrm km/s [2.15/4.25] ip-subtracted macrobroadening [=sqrt(vM**2-vip**2)] (spect.line.broad)
  vmt km/s [1.79/2.73] Macroturbulence broadening (=4.3-0.67*log g) (spect.line.broad)

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 (i)indexed column
  vrt km/s [0.91/3.32] Rotational broadening [=sqrt(vrm**2-vmt**2)] (spect.line.broad)
  vesini km/s [1.59/4.02] Finally adopted v sini (=1.01*vrt+0.67) (phys.veloc.rotat)
  logeps(Si) [-] [7.05/7.81] Si abundance derived from 6080-6089Å fit (dex) (phys.abund)
  logeps(Ti) [-] [4.36/5.32] Ti abundance derived from 6080-6089Å fit (dex) (phys.abund)
  logeps(V) [-] [3.23/4.54] V abundance derived from 6080-6089Å fit (dex) (phys.abund)
  logeps(Fe) [-] [6.75/7.87] Fe abundance derived from 6080-6089Å fit (dex) (phys.abund.Fe)
  logeps(Co) [-] [4.22/5.38] Co abundance derived from 6080-6089Å fit (dex) (phys.abund)
  logeps(Ni) [-] [5.48/6.85] Ni abundance derived from 6080-6089Å fit (dex) (phys.abund)
  [Si/H] [-] [-0.41/0.35] Si abundance log{eps}Si(star)-log{eps}Si(Sun:7.455) (dex) (phys.abund)
  [Ti/H] [-] [-0.63/0.34] Ti abundance log{eps}Ti(star)-log{eps}Ti(Sun:4.986) (dex) (phys.abund)
  [V/H] [-] [-0.68/0.63] V abundance log{eps}V(star)-log{eps}V(Sun:3.908) (dex) (phys.abund)
  [Fe/H]2 [-] [-0.78/0.34] Fe abundance log{eps}Fe(star)-log{eps}Fe(Sun:7.534) (dex) (phys.abund.Fe)
  [Co/H] [-] [-0.58/0.58] Co abundance log{eps}Co(star)-log{eps}Co(Sun:4.798) (dex) (phys.abund)
  [Ni/H] [-] [-0.89/0.48] Ni abundance log{eps}Ni(star)-log{eps}Ni(Sun:6.367) (dex) (phys.abund)

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