J/A+A/554/A98ivo://CDS.VizieR/J/A+A/554/A98doi:10.26093/cds/vizier.35540098CDSNeilson H.R.Lester J.B.2013-12-29T22:33:40Z2013-06-24T08:26:07ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmosphereslate-type-starsgiant-starsinfrared-photometryvisible-astronomybroad-band-photometryModel stellar atmospheres are fundamental tools for understanding stellar observations from interferometry, microlensing, eclipsing binaries and planetary transits. However, the calculations also include assumptions, such as the geometry of the model. We use intensity profiles computed for both plane-parallel and spherically symmetric model atmospheres to determine fitting coefficients in the BVRIHK, CoRoT and Kepler wavebands for limb darkening using several different fitting laws, for gravity-darkening and for interferometric angular diameter corrections. Comparing predicted variables for each geometry, we find that the spherically symmetric model geometry leads to different predictions for surface gravities logg<3. In particular, the most commonly used limb-darkening laws produce poor fits to the intensity profiles of spherically symmetric model atmospheres, which indicates the need for more sophisticated laws. Angular diameter corrections for spherically symmetric models range from 0.67 to 1, compared to the much smaller range from 0.95 to 1 for plane-parallel models.2013A&A...554A..98Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/554/A98CatalogResearchIsServedByTAP 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)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/554/A98https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/554/A98http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/554/A98https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/554/A98https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/554/A98http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/554/A98GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/A+A/554/A98/table2Spherical linear limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] 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/554/A98/table3Spherical quadratic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] 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)Kelper-band quadratic b coefficient (G2)phot.limbDarkfloatJ/A+A/554/A98/table4Spherical square-root limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] 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/554/A98/table5Spherical 4-parameter limb-darkening coefficientsM[0.5/20] Model masssolMassphys.mass;meta.modelledfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;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/554/A98/table6Spherical exponential limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] Model masssolMassphys.mass;meta.modelledfloatPlotPlot the of the intensity profiles for spherically-symmetric 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/554/A98/table7Spherical logarithmic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] 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/554/A98/table8Planar linear limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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/554/A98/table11Planar 4-parameter limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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.limbDarkfloatJ/A+A/554/A98/table12Planar exponential limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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/554/A98/table13Planar logarithmic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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/554/A98/table14Spherical Gravity-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] 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.paramdoublenullableIg(B)? B-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(B)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(V)? V-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(V)? V-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(V)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(R)? R-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(R)? R-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(R)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(I)? I-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(I)? I-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(I)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(H)? H-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(H)? H-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(H)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(K)? K-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(K)? K-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(K)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(CoR)? CoRoT-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(CoR)? CoRoT-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(CoR)? Gravity-darkening coefficientphot.limbDarkdoublenullableIT(Kep)? Kepler-band derivative, d(lnI)/d(lnT)stat.fit.paramdoublenullableIg(Kep)? Kepler-band derivative, d(lnI)/d(lng)stat.fit.paramdoublenullabley(Kep)? Gravity-darkening coefficientphot.limbDarkdoublenullableJ/A+A/554/A98/table16Spherical interferometric angular diameter correctionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0/20] 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/554/A98/table17Planar interferometric angular diameter corrections (M=0.0)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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[0/20] 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/554/A98/listsphList of individual intensity profiles in spherical subdirectoryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-1/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatM[0.5/20] 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/554/A98/listplaList of individual intensity profiles in planar subdirectoryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] Model surface gravitylog(cm.s**-2)phys.gravity;meta.modelledfloatFileNameName of the file in subdirectory planarmeta.id;meta.filecharJ/A+A/554/A98/table9Planar quadratic limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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/554/A98/table10Planar square-root limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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/554/A98/table15Planar Gravity-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeff[3000/8000] Model effective temperatureKphys.temperature.effective;meta.modelledintlogg[-2.25/3] 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)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)Gravity-darkening coefficientphot.limbDarkdouble