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J/A+A/556/A86
  FGK dwarf stars limb darkening coefficients (Neilson+, 2013)
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2013A&A...556A..86N
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1.J/A+A/556/A86/table14Spherical Gravity-darkening coefficients (919 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Teff K [3500/8000] Model effective temperature (phys.temperature.effective;meta.modelled)
  logg [cm/s2] [4/4.75] Model surface gravity (phys.gravity;meta.modelled)
  M Msun [0.2/1.4] Model mass (phys.mass;meta.modelled)
  Plot  Plot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebands (meta.ref.url)
model
  IT(B)  B-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(B)  B-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(B)  Gravity-darkening coefficient (phot.limbDark)
  IT(V)  V-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(V)  V-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(V)  Gravity-darkening coefficient (phot.limbDark)

ALL cols		    
 (i)indexed column
  IT(R)  R-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(R)  R-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(R)  Gravity-darkening coefficient (phot.limbDark)
  IT(I)  I-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(I)  I-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(I)  Gravity-darkening coefficient (phot.limbDark)
  IT(H)  H-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(H)  H-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(H)  Gravity-darkening coefficient (phot.limbDark)
  IT(K)  K-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(K)  K-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(K)  Gravity-darkening coefficient (phot.limbDark)
  IT(CoR)  CoRoT-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(CoR)  CoRoT-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(CoR)  CoRoT-band gravity-darkening coefficient (phot.limbDark)
  IT(Kep)  Kepler-band derivative, d(lnI)/d(lnT) (stat.fit.param)
  Ig(Kep)  Kepler-band derivative, d(lnI)/d(lng) (stat.fit.param)
  y(Kep)  Gravity-darkening coefficient (phot.limbDark)

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