J/A+A/556/A86ivo://CDS.VizieR/J/A+A/556/A86doi:10.26093/cds/vizier.35560086CDSNeilson H.R.Lester J.B.2014-02-20T14:59:48Z2013-08-01T06:19:02ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frastronomical-modelsstellar-atmosphereseclipsing-binary-starsdwarf-starsinfrared-photometryvisible-astronomyWide-band photometryLimb darkening is a fundamental ingredient for interpreting observations of planetary transits, eclipsing binaries, optical/infrared interferometry and microlensing events. However, this modeling traditionally represents limb darkening by a simple law having one or two coefficients that have been derived from plane-parallel model stellar atmospheres, which has been done by many researchers. More recently, researchers have gone beyond plane-parallel models and considered other geometries. We previously studied the limb-darkening coefficients from spherically symmetric and plane-parallel model stellar atmospheres for cool giant and supergiant stars, and in this investigation we apply the same techniques to FGK dwarf stars. We present limb-darkening coefficients, gravity-darkening coefficients and interferometric angular diameter corrections from Atlas and SAtlas model stellar atmospheres. We find that sphericity is important even for dwarf model atmospheres, leading to significant differences in the predicted coefficients.2013A&A...556A..86Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/556/A86CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/110/329 : LTE model atmospheres coeff. (Diaz-cordoves+, 1995)J/A+AS/114/247 : Limb-darkening coefficients for R I J H K (Claret+, 1995)J/A+A/363/1081 : LTE models non-linear limb-darkening law (Claret, 2000)J/A+A/401/657 : LTE models non-linear limb-darkening law. II (Claret, 2003)J/A+A/405/1095 : ATLAS9 models limb-darkening coefficients (Barban+, 2003)J/A+A/428/1001 : LTE models non-linear limb-darkening law. III (Claret, 2004)J/A+A/510/A21 : Stellar Limb-Darkening Coefficients (Sing, 2010)J/MNRAS/413/1515 : New grids of Atlas9 models (Howarth, 2011)J/A+A/546/A14 : Limb-darkening for CoRoT, Kepler, Spitzer (Claret+, 2012)J/A+A/552/A16 : Limb-darkening for CoRoT, Kepler, Spitzer. II (Claret+ 2013)J/A+A/554/A98 : Red giants limb darkening coefficients (Neilson+, 2013)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/556/A86https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/556/A86http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/556/A86https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/556/A86https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/556/A86http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/556/A86GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/A+A/556/A86/table12Planar exponential limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharg(B)B-band exponential g coefficient (G5)phot.limbDarkfloath(B)B-band exponential h coefficient (G5)phot.limbDarkfloatg(V)V-band exponential g coefficient (G5)phot.limbDarkfloath(V)V-band exponential h coefficient (G5)phot.limbDarkfloatg(R)R-band exponential g coefficient (G5)phot.limbDarkfloath(R)R-band exponential h coefficient (G5)phot.limbDarkfloatg(I)I-band exponential g coefficient (G5)phot.limbDarkfloath(I)I-band exponential h coefficient (G5)phot.limbDarkfloatg(H)H-band exponential g coefficient (G5)phot.limbDarkfloath(H)H-band exponential h coefficient (G5)phot.limbDarkfloatg(K)K-band exponential g coefficient (G5)phot.limbDarkfloath(K)K-band exponential h coefficient (G5)phot.limbDarkfloatg(CoR)CoRoT-band exponential g coefficient (G5)phot.limbDarkfloath(CoR)CoRoT-band exponential h coefficient (G5)phot.limbDarkfloatg(Kep)Kepler-band exponential g coefficient (G5)phot.limbDarkfloath(Kep)Kepler-band exponential h coefficient (G5)phot.limbDarkfloatJ/A+A/556/A86/table13Planar logarithmic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharm(B)B-band logarithmic m coefficient (G6)phot.limbDarkfloatn(B)B-band logarithmic n coefficient (G6)phot.limbDarkfloatm(V)V-band logarithmic m coefficient (G6)phot.limbDarkfloatn(V)V-band logarithmic n coefficient (G6)phot.limbDarkfloatm(R)R-band logarithmic m coefficient (G6)phot.limbDarkfloatn(R)R-band logarithmic n coefficient (G6)phot.limbDarkfloatm(I)I-band logarithmic m coefficient (G6)phot.limbDarkfloatn(I)I-band logarithmic n coefficient (G6)phot.limbDarkfloatm(H)H-band logarithmic m coefficient (G6)phot.limbDarkfloatn(H)H-band logarithmic n coefficient (G6)phot.limbDarkfloatm(K)K-band logarithmic m coefficient (G6)phot.limbDarkfloatn(K)K-band logarithmic n coefficient (G6)phot.limbDarkfloatm(CoR)CoRoT-band logarithmic m coefficient (G6)phot.limbDarkfloatn(CoR)CoRoT-band logarithmic n coefficient (G6)phot.limbDarkfloatm(Kep)Kepler-band logarithmic m coefficient (G6)phot.limbDarkfloatn(Kep)Kepler-band logarithmic n coefficient (G6)phot.limbDarkfloatJ/A+A/556/A86/table14Spherical Gravity-darkening coefficientsIT(Kep)Kepler-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharIT(B)B-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(B)B-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(B)Gravity-darkening coefficientphot.limbDarkdoubleIT(V)V-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(V)V-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(V)Gravity-darkening coefficientphot.limbDarkdoubleIT(R)R-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(R)R-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(R)Gravity-darkening coefficientphot.limbDarkdoubleIT(I)I-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(I)I-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(I)Gravity-darkening coefficientphot.limbDarkdoubleIT(H)H-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(H)H-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(H)Gravity-darkening coefficientphot.limbDarkdoubleIT(K)K-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(K)K-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(K)Gravity-darkening coefficientphot.limbDarkdoubleIT(CoR)CoRoT-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(CoR)CoRoT-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(CoR)CoRoT-band gravity-darkening coefficientphot.limbDarkdoubleIg(Kep)Kepler-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(Kep)Gravity-darkening coefficientphot.limbDarkdoubleJ/A+A/556/A86/table15Planar Gravity-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharIT(B)B-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(B)B-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(B)Gravity-darkening coefficientphot.limbDarkdoubleIT(V)V-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(V)V-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(V)Gravity-darkening coefficientphot.limbDarkdoubleIT(R)R-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(R)R-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(R)Gravity-darkening coefficientphot.limbDarkdoubleIT(I)I-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(I)I-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(I)Gravity-darkening coefficientphot.limbDarkdoubleIT(H)H-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(H)H-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(H)Gravity-darkening coefficientphot.limbDarkdoubleIT(K)K-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(K)K-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(K)Gravity-darkening coefficientphot.limbDarkdoubleIT(CoR)CoRoT-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(CoR)CoRoT-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(CoR)CoRoT-band gravity-darkening coefficientphot.limbDarkdoubleIT(Kep)Kepler-band derivative, d(lnI)/d(lnT)stat.fit.paramdoubleIg(Kep)Kepler-band derivative, d(lnI)/d(lng)stat.fit.paramdoubley(Kep)Kepler-band gravity-darkening coefficientphot.limbDarkdoubleJ/A+A/556/A86/table16Spherical interferometric angular diameter correctionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharkLD(B)B-band interferometric angular diameter correctioninstr.paramfloatkLD(V)V-band interferometric angular diameter correctioninstr.paramfloatkLD(R)R-band interferometric angular diameter correctioninstr.paramfloatkLD(I)I-band interferometric angular diameter correctioninstr.paramfloatkLD(H)H-band interferometric angular diameter correctioninstr.paramfloatkLD(K)K-band interferometric angular diameter correctioninstr.paramfloatkLD(CoR)CoRoT-band interferometric angular diameter correctioninstr.paramfloatkLD(Kep)Kepler-band interferometric angular diameter correctioninstr.paramfloatJ/A+A/556/A86/table17Planar interferometric angular diameter corrections (M=0.0)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharM[0/1.4] Model masssolMassphys.mass;meta.modelledfloatkLD(B)B-band interferometric angular diameter correctioninstr.paramfloatkLD(V)V-band interferometric angular diameter correctioninstr.paramfloatkLD(R)R-band interferometric angular diameter correctioninstr.paramfloatkLD(I)I-band interferometric angular diameter correctioninstr.paramfloatkLD(H)H-band interferometric angular diameter correctioninstr.paramfloatkLD(K)K-band interferometric angular diameter correctioninstr.paramfloatkLD(CoR)CoRoT-band interferometric angular diameter correctioninstr.paramfloatkLD(Kep)Kepler-band interferometric angular diameter correctioninstr.paramfloatJ/A+A/556/A86/listsphList of individual intensity profiles in spherical subdirectoryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharFileNameName of the file in subdirectory sphericmeta.id;meta.filecharJ/A+A/556/A86/listplaList of individual intensity profiles in planar subdirectoryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatFileNameName of the file in subdirectory planarmeta.id;meta.filecharJ/A+A/556/A86/table2Spherical linear LDCsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharu(B)B-band linear u coefficient (G1)phot.limbDarkfloatu(V)V-band linear u coefficient (G1)phot.limbDarkfloatu(R)R-band linear u coefficient (G1)phot.limbDarkfloatu(I)I-band linear u coefficient (G1)phot.limbDarkfloatu(H)H-band linear u coefficient (G1)phot.limbDarkfloatu(K)K-band linear u coefficient (G1)phot.limbDarkfloatu(CoR)CoRoT-band linear u coefficient (G1)phot.limbDarkfloatu(Kep)Kepler-band linear u coefficient (G1)phot.limbDarkfloatJ/A+A/556/A86/table3Spherical quadratic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlchara(B)B-band quadratic a coefficient (G2)phot.limbDarkfloatb(B)B-band quadratic b coefficient (G2)phot.limbDarkfloata(V)V-band quadratic a coefficient (G2)phot.limbDarkfloatb(V)V-band quadratic b coefficient (G2)phot.limbDarkfloata(R)R-band quadratic a coefficient (G2)phot.limbDarkfloatb(R)R-band quadratic b coefficient (G2)phot.limbDarkfloata(I)I-band quadratic a coefficient (G2)phot.limbDarkfloatb(I)I-band quadratic b coefficient (G2)phot.limbDarkfloata(H)H-band quadratic a coefficient (G2)phot.limbDarkfloatb(H)H-band quadratic b coefficient (G2)phot.limbDarkfloata(K)K-band quadratic a coefficient (G2)phot.limbDarkfloatb(K)K-band quadratic b coefficient (G2)phot.limbDarkfloata(CoR)CoRoT-band quadratic a coefficient (G2)phot.limbDarkfloatb(CoR)CoRoT-band quadratic b coefficient (G2)phot.limbDarkfloata(Kep)Kepler-band quadratic a coefficient (G2)phot.limbDarkfloatb(Kep)Kepler-band quadratic b coefficient (G2)phot.limbDarkfloatJ/A+A/556/A86/table4Spherical square-root limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharc(B)B-band square-root c coefficient (G3)phot.limbDarkfloatd(B)B-band square-root d coefficient (G3)phot.limbDarkfloatc(V)V-band square-root c coefficient (G3)phot.limbDarkfloatd(V)V-band square-root d coefficient (G3)phot.limbDarkfloatc(R)R-band square-root c coefficient (G3)phot.limbDarkfloatd(R)R-band square-root d coefficient (G3)phot.limbDarkfloatc(I)I-band square-root c coefficient (G3)phot.limbDarkfloatd(I)I-band square-root d coefficient (G3)phot.limbDarkfloatc(H)H-band square-root c coefficient (G3)phot.limbDarkfloatd(H)H-band square-root d coefficient (G3)phot.limbDarkfloatc(K)K-band square-root c coefficient (G3)phot.limbDarkfloatd(K)K-band square-root d coefficient (G3)phot.limbDarkfloatc(CoR)CoRoT-band square-root c coefficient (G3)phot.limbDarkfloatd(CoR)CoRoT-band square-root d coefficient (G3)phot.limbDarkfloatc(Kep)Kepler-band square-root c coefficient (G3)phot.limbDarkdoubled(Kep)Kepler-band square-root d coefficient (G3)phot.limbDarkdoubleJ/A+A/556/A86/table5Spherical 4-parameter limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharf1(B)B-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(B)B-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(B)B-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(B)B-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(V)V-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(V)V-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(V)V-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(V)V-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(R)R-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(R)R-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(R)R-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(R)R-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(I)I-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(I)I-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(I)I-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(I)I-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(H)H-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(H)H-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(H)H-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(H)H-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(K)K-band four-parameter f_1_ coefficient (G4)phot.limbDarkdoublef2(K)K-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(K)K-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(K)K-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(CoR)CoRoT-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(CoR)CoRoT-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(CoR)CoRoT-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(CoR)CoRoT-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoublef1(Kep)Kepler-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(Kep)Kepler-band four-parameter f_2_ coefficient (G4)phot.limbDarkdoublef3(Kep)Kepler-band four-parameter f_3_ coefficient (G4)phot.limbDarkdoublef4(Kep)Kepler-band four-parameter f_4_ coefficient (G4)phot.limbDarkdoubleJ/A+A/556/A86/table6Spherical exponential limb-darkening coefficientsg(B)B-band exponential g coefficient (G5)phot.limbDarkfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharh(B)B-band exponential h coefficient (G5)phot.limbDarkfloatg(V)V-band exponential g coefficient (G5)phot.limbDarkfloath(V)V-band exponential h coefficient (G5)phot.limbDarkfloatg(R)R-band exponential g coefficient (G5)phot.limbDarkfloath(R)R-band exponential h coefficient (G5)phot.limbDarkfloatg(I)I-band exponential g coefficient (G5)phot.limbDarkfloath(I)I-band exponential h coefficient (G5)phot.limbDarkfloatg(H)H-band exponential g coefficient (G5)phot.limbDarkfloath(H)H-band exponential h coefficient (G5)phot.limbDarkfloatg(K)K-band exponential g coefficient (G5)phot.limbDarkfloath(K)K-band exponential h coefficient (G5)phot.limbDarkfloatg(CoR)CoRoT-band exponential g coefficient (G5)phot.limbDarkfloath(CoR)CoRoT-band exponential h coefficient (G5)phot.limbDarkfloatg(Kep)Kepler-band exponential g coefficient (G5)phot.limbDarkfloath(Kep)Kepler-band exponential h coefficient (G5)phot.limbDarkfloatJ/A+A/556/A86/table7Spherical logarithmic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.2/1.4] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharm(B)B-band logarithmic m coefficient (G6)phot.limbDarkfloatn(B)B-band logarithmic n coefficient (G6)phot.limbDarkfloatm(V)V-band logarithmic m coefficient (G6)phot.limbDarkfloatn(V)V-band logarithmic n coefficient (G6)phot.limbDarkfloatm(R)R-band logarithmic m coefficient (G6)phot.limbDarkfloatn(R)R-band logarithmic n coefficient (G6)phot.limbDarkfloatm(I)I-band logarithmic m coefficient (G6)phot.limbDarkfloatn(I)I-band logarithmic n coefficient (G6)phot.limbDarkfloatm(H)H-band logarithmic m coefficient (G6)phot.limbDarkfloatn(H)H-band logarithmic n coefficient (G6)phot.limbDarkfloatm(K)K-band logarithmic m coefficient (G6)phot.limbDarkfloatn(K)K-band logarithmic n coefficient (G6)phot.limbDarkfloatm(CoR)CoRoT-band logarithmic m coefficient (G6)phot.limbDarkfloatn(CoR)CoRoT-band logarithmic n coefficient (G6)phot.limbDarkfloatm(Kep)Kepler-band logarithmic m coefficient (G6)phot.limbDarkfloatn(Kep)Kepler-band logarithmic n coefficient (G6)phot.limbDarkfloatJ/A+A/556/A86/table8Planar linear limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharu(B)B-band linear u coefficient (G1)phot.limbDarkfloatu(V)V-band linear u coefficient (G1)phot.limbDarkfloatu(R)R-band linear u coefficient (G1)phot.limbDarkfloatu(I)I-band linear u coefficient (G1)phot.limbDarkfloatu(H)H-band linear u coefficient (G1)phot.limbDarkfloatu(K)K-band linear u coefficient (G1)phot.limbDarkfloatu(CoR)CoRoT-band linear u coefficient (G1)phot.limbDarkfloatu(Kep)Kepler-band linear u coefficient (G1)phot.limbDarkfloatJ/A+A/556/A86/table9Planar quadratic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlchara(B)B-band quadratic a coefficient (G2)phot.limbDarkfloatb(B)B-band quadratic b coefficient (G2)phot.limbDarkfloata(V)V-band quadratic a coefficient (G2)phot.limbDarkfloatb(V)V-band quadratic b coefficient (G2)phot.limbDarkfloata(R)R-band quadratic a coefficient (G2)phot.limbDarkfloatb(R)R-band quadratic b coefficient (G2)phot.limbDarkfloata(I)I-band quadratic a coefficient (G2)phot.limbDarkfloatb(I)I-band quadratic b coefficient (G2)phot.limbDarkfloata(H)H-band quadratic a coefficient (G2)phot.limbDarkfloatb(H)H-band quadratic b coefficient (G2)phot.limbDarkfloata(K)K-band quadratic a coefficient (G2)phot.limbDarkfloatb(K)K-band quadratic b coefficient (G2)phot.limbDarkfloata(CoR)CoRoT-band quadratic a coefficient (G2)phot.limbDarkfloatb(CoR)CoRoT-band quadratic b coefficient (G2)phot.limbDarkfloata(Kep)Kepler-band quadratic a coefficient (G2)phot.limbDarkfloatb(Kep)Kepler-band quadratic b coefficient (G2)phot.limbDarkfloatJ/A+A/556/A86/table10Planar square-root limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharc(B)B-band square-root c coefficient (G3)phot.limbDarkfloatd(B)B-band square-root d coefficient (G3)phot.limbDarkfloatc(V)V-band square-root c coefficient (G3)phot.limbDarkfloatd(V)V-band square-root d coefficient (G3)phot.limbDarkfloatc(R)R-band square-root c coefficient (G3)phot.limbDarkfloatd(R)R-band square-root d coefficient (G3)phot.limbDarkfloatc(I)I-band square-root c coefficient (G3)phot.limbDarkfloatd(I)I-band square-root d coefficient (G3)phot.limbDarkfloatc(H)H-band square-root c coefficient (G3)phot.limbDarkfloatd(H)H-band square-root d coefficient (G3)phot.limbDarkfloatc(K)K-band square-root c coefficient (G3)phot.limbDarkfloatd(K)K-band square-root d coefficient (G3)phot.limbDarkfloatc(CoR)CoRoT-band square-root c coefficient (G3)phot.limbDarkfloatd(CoR)CoRoT-band square-root d coefficient (G3)phot.limbDarkfloatc(Kep)Kepler-band square-root c coefficient (G3)phot.limbDarkfloatd(Kep)Kepler-band square-root d coefficient (G3)phot.limbDarkfloatJ/A+A/556/A86/table11Planar 4-parameter limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3500/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[4/4.75] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatPlotPlot the of the intensity profiles for plane-parallel stellar atmosphere in Johnson-Cousins BVRIHK, CoRoT and Kepler wavebandsmeta.ref.urlcharf1(B)B-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(B)B-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(B)B-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(B)B-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(V)V-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(V)V-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(V)V-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(V)V-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(R)K-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(R)K-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(R)K-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(R)K-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(I)I-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(I)I-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(I)I-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(I)I-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(H)H-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(H)H-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(H)H-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(H)H-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(K)K-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(K)K-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(K)K-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(k)K-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(CoR)CoRoT-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(CoR)CoRoT-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(CoR)CoRoT-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(CoR)CoRoT-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloatf1(Kep)Kepler-band four-parameter f_1_ coefficient (G4)phot.limbDarkfloatf2(Kep)Kepler-band four-parameter f_2_ coefficient (G4)phot.limbDarkfloatf3(Kep)Kepler-band four-parameter f_3_ coefficient (G4)phot.limbDarkfloatf4(Kep)Kepler-band four-parameter f_4_ coefficient (G4)phot.limbDarkfloat