J/A+AS/114/247ivo://CDS.VizieR/J/A+AS/114/247CDSClaret A.Diaz-Cordoves J.Gimenez A.1999-02-27T11:10:49Z1999-02-27T12:10:41ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresinfrared-photometryWe have computed limb-darkening coefficients for five commonly used near infrared photometric bands, namely R, I, J, H, and K, using the stellar atmosphere models by Kurucz (1993). Since the behaviour of the specific intensities is very dependent on the range of effective temperatures considered, we have adopted three analytical approximations to the limb darkening: linear, quadratic and square root. The least-squares method has been adopted for the fit of the limb-darkening coefficients to the model atmospheres.1995A&AS..114..247Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/114/247CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/114/247https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/114/247http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/114/247https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/114/247https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/114/247http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/114/247GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/A+AS/114/247/table1Linear (u) limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintloggSurface gravitylog(cm.s**-2)phys.gravityfloatTeffEffective temperatureKphys.temperature.effectiveintu(R)Linear Limb-darkening coefficient (Filter R)phot.limbDarkfloatu(I)Linear Limb-darkening coefficient (Filter I)phot.limbDarkfloatu(J)Linear Limb-darkening coefficient (Filter J)phot.limbDarkfloatu(H)Linear Limb-darkening coefficient (Filter H)phot.limbDarkfloatu(K)Linear Limb-darkening coefficient (Filter K)phot.limbDarkfloatJ/A+AS/114/247/table2Quadratic (a, b) limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintloggSurface gravitylog(cm.s**-2)phys.gravityfloatTeffEffective temperatureKphys.temperature.effectiveinta(R)Quadratic Limb-darkening coeff. (a) (Filter R)phot.limbDarkfloatb(R)Quadratic Limb-darkening coeff. (b) (Filter R)phot.limbDarkfloata(I)Quadratic Limb-darkening coeff. (a) (Filter I)phot.limbDarkfloatb(I)Quadratic Limb-darkening coeff. (b) (Filter I)phot.limbDarkfloata(J)Quadratic Limb-darkening coeff. (a) (Filter J)phot.limbDarkfloatb(J)Quadratic Limb-darkening coeff. (b) (Filter J)phot.limbDarkfloata(H)Quadratic Limb-darkening coeff. (a) (Filter H)phot.limbDarkfloatb(H)Quadratic Limb-darkening coeff. (b) (Filter H)phot.limbDarkfloata(K)Quadratic Limb-darkening coeff. (a) (Filter K)phot.limbDarkfloatb(K)Quadratic Limb-darkening coeff. (b) (Filter K)phot.limbDarkfloatJ/A+AS/114/247/table3Square root (c, d) limb-darkening coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintloggSurface gravitylog(cm.s**-2)phys.gravityfloatTeffEffective temperatureKphys.temperature.effectiveintc(R)Square root Limb-darkening coeff. (c) (Filter R)phot.limbDarkfloatd(R)Square root Limb-darkening coeff. (d) (Filter R)phot.limbDarkfloatc(I)Square root Limb-darkening coeff. (c) (Filter I)phot.limbDarkfloatd(I)Square root Limb-darkening coeff. (d) (Filter I)phot.limbDarkfloatc(J)Square root Limb-darkening coeff. (c) (Filter J)phot.limbDarkfloatd(J)Square root Limb-darkening coeff. (d) (Filter J)phot.limbDarkfloatc(H)Square root Limb-darkening coeff. (c) (Filter H)phot.limbDarkfloatd(H)Square root Limb-darkening coeff. (d) (Filter H)phot.limbDarkfloatc(K)Square root Limb-darkening coeff. (c) (Filter K)phot.limbDarkfloatd(K)Square root Limb-darkening coeff. (d) (Filter K)phot.limbDarkfloat