J/A+A/567/A3ivo://CDS.VizieR/J/A+A/567/A3doi:10.26093/cds/vizier.35670003CDSClaret A.Dragomir D.Matthews J.M.2017-07-12T15:33:22Z2014-07-04T09:26:32ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresinfrared-photometryvisible-astronomysloan-photometrymedium-band-photometryWide-band photometryWe present new calculations of limb and gravity-darkening coefficients to be used as input in many fields of stellar physics such as synthetic light curves of double-lined eclipsing binaries and planetary transits, studies of stellar diameters or line profiles in rotating stars. We compute the limb-darkening coefficients specifically for the photometric system of the satellite MOST (Microvariability and Oscillations in STars). All computations were performed by adopting the least-square method, but for completeness we also performed calculations for the linear and bi-parametric approaches by adopting the flux conservation method. The passband gravity-darkening coefficients y({lambda}) were computed by adopting a more general differential equation, which also takes the effects of convection into account. We used two stellar atmosphere models: ATLAS (plane-parallel) and PHOENIX (spherical and quasi-spherical). We adopted six laws to describe the specific intensity distribution: linear, quadratic, square root, logarithmic, exponential, and a more general one with four terms. The covered ranges of T_eff_, log g, metallicities, and microturbulent velocities are [1500-50000K, 0-5.5,-5.0-1.0, 0-8km/s], respectively.2014A&A...567A...3Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/567/A3CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/110/329 : LTE model atmospheres coeff. (Diaz-cordoves+, 1995)J/A+AS/114/247 : Limb-darkening coeff. for RIJHK (Claret+, 1995)J/A+A/335/647 : Limb-darkening coefficients for ubvyUBVRIJHK (Claret 1998)J/A+A/363/1081 : LTE models non-linear limb-darkening law. I. (Claret, 2000)J/A+A/401/657 : LTE models non-linear limb-darkening law. II. (Claret, 2003)J/A+A/428/1001 : LTE models non-linear limb-darkening law. III. (Claret, 2005)J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 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/567/A3https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/567/A3http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/567/A3https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/567/A3https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/567/A3http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/567/A3GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfraredOpticaldefaultJ/A+A/567/A3/table23y gravity-darkening coefficient (GDCs) ATLAS models, all metallicities, {xi}=2,0,1,4,8 km/s for MOSTrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogZ[-5/1] Metallicity (log[M/H])log(Sun)phys.abund.Zfloatxi[2/8] microturbulent velocity {xi}km/sphys.velocfloatlogg[0/5] Surface gravitylog(cm.s**-2)phys.gravityfloatlogTe[3.5/4.7] log Effective temperaturelog(K)phys.temperature.effectivefloatyGravity-darkening coefficient (MOST)phot.limbDarkfloatJ/A+A/567/A3/solarCombined table from original tablesuLlinear LDC (MOST LSM) (G1)phot.limbDarkfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogg[2.5/5.5] Surface gravitylog(cm.s**-2)phys.gravityfloatTeff[1500/10000] Effective temperatureKphys.temperature.effectivefloatlogZ[0] Metallicity (log[M/H])log(Sun)phys.abund.ZfloatL/HP[2] Mixing-length parameterstat.paramfloatuFlinear LDC (MOST FCM) (G1)phot.limbDarkfloataLa quadratic LDC (MOST LSM) (G1)phot.limbDarkfloatbLb quadratic LDC (MOST LSM) (G1)phot.limbDarkfloataFa quadratic LDC (MOST FCM) (G1)phot.limbDarkfloatbFb quadratic LDC (MOST FCM) (G1)phot.limbDarkfloatcLc root-square LDC (MOST LSM) (G1)phot.limbDarkfloatdLd root-square LDC (MOST LSM) (G1)phot.limbDarkfloatcFc root-square LDC (MOST FCM) (G1)phot.limbDarkfloatdFd root-square LDC (MOST FCM) (G1)phot.limbDarkfloateLe logarithmic LDC (MOST LSM) (G1)phot.limbDarkfloatfLf logarithmic LDC (MOST LSM) (G1)phot.limbDarkfloateFe logarithmic LDC (MOST FCM) (G1)phot.limbDarkfloatfFf logarithmic LDC (MOST FCM) (G1)phot.limbDarkfloatgg exponential LDC in PHOENIX quasi-spherical model (MOST LSM) (G1)phot.limbDarkfloathh exponential LDC in PHOENIX quasi-spherical model (MOST LSM) (G1)phot.limbDarkfloata1a1 LDC in PHOENIX quasi-spherical model (G1)phot.limbDarkdoublea2a2 LDC in PHOENIX quasi-spherical model (G1)phot.limbDarkdoublea3a3 LDC in PHOENIX quasi-spherical model (G1)phot.limbDarkdoublea4a4 LDC in PHOENIX quasi-spherical model (G1)phot.limbDarkdoublegSg exponential LDC in PHOENIX spherical model (MOST LSM) (G1)phot.limbDarkfloathSh exponential LDC in PHOENIX spherical model (MOST LSM) (G1)phot.limbDarkfloata1Sa1 LDC in PHOENIX spherical model (G1)phot.limbDarkdoublea2Sa2 LDC in PHOENIX spherical model (G1)phot.limbDarkdoublea3Sa3 LDC in PHOENIX spherical model (G1)phot.limbDarkdoublea4Sa4 LDC in PHOENIX spherical model (G1)phot.limbDarkdoubleJ/A+A/567/A3/atlasCombined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogg[0/5] Surface gravitylog(cm.s**-2)phys.gravityfloatTeff[3500/50000] Effective temperatureKphys.temperature.effectivefloatlogZ[-5/1] Metallicity (log[M/H])log(Sun)phys.abund.Zfloatxi[0/8] Microturbulent velocity {xi}km/sphys.velocfloatuLlinear LDC (MOST, LSM) (G1)phot.limbDarkfloatuFlinear LDC (MOST, FSM) (G1)phot.limbDarkfloataLa quadratic LDC (MOST LSM) (G1)phot.limbDarkfloatbLb quadratic LDC (MOST LSM) (G1)phot.limbDarkfloataFa quadratic LDC (MOST FCM) (G1)phot.limbDarkfloatbFb quadratic LDC (MOST FCM) (G1)phot.limbDarkfloatcLc root-square LDC (MOST LSM) (G1)phot.limbDarkfloatdLd root-square LDC (MOST LSM) (G1)phot.limbDarkfloatcFc root-square LDC (MOST FCM) (G1)phot.limbDarkfloatdFd root-square LDC (MOST FCM) (G1)phot.limbDarkfloateLe logarithmic LDC (MOST LSM) (G1)phot.limbDarkfloatfLf logarithmic LDC (MOST LSM) (G1)phot.limbDarkfloateFe logarithmic LDC (MOST FCM) (G1)phot.limbDarkfloatfFf logarithmic LDC (MOST FCM) (G1)phot.limbDarkfloata1a1 LDC (MOST LSM) (G1)phot.limbDarkfloata2a2 LDC (MOST LSM) (G1)phot.limbDarkfloata3a3 LDC (MOST LSM) (G1)phot.limbDarkfloata4a4 LDC (MOST LSM) (G1)phot.limbDarkfloat