J/A+A/569/A21ivo://CDS.VizieR/J/A+A/569/A21doi:10.26093/cds/vizier.35690021CDSLebreton Y.Goupil M.2017-06-29T08:56:23Z2014-09-11T13:11:00ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsstellar-massesstellar-agesastronomical-modelsIn the context of space missions CoRoT, Kepler, Gaia, TESS, and PLATO, precise and accurate stellar ages, masses and radii are of paramount importance. For instance, they are crucial to constrain scenarii of planetary formation and evolution.2014A&A...569A..21Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/569/A21CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/569/A21https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/569/A21http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/569/A21https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/569/A21https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/569/A21http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/569/A21GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/569/A21/basicModel results and restitution of the observational constraints for the reference physicsLum[2.01/2.16] LuminositysolLumphys.luminosityfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel identification (G1)meta.id;stat.param;meta.modelledcharNoptNumber of optimized variations for this modelmeta.ref.urlintAge[0.8/4.5] AgeGyrtime.agefloate_AgeAge error bar (1)Gyrstat.error;time.agefloatM[1.12/1.43] Stellar masssolMassphys.massfloate_MMass error bar (1)solMassstat.errorfloatZ/X0[0.03/0.07] Initial metal to hydrogen ratiophys.abund.Zfloate_Z/X0Z/X error bar (1)stat.error;src.redshiftfloatY0Initial helium contentphys.abundfloate_Y0? Y error bar (1)stat.error;pos.cartesian.yfloatnullableal.conv[0.4/2.1] Mixing length parameter convection {alpha}_conv_stat.paramfloate_al.conv? alpha conv error bar (1)stat.errorfloatnullableal.ov[0/2] Overshooting parameter {alpha}_ov_stat.paramfloatxiPC[0/1.3] Penetrative convection parameter {xi}_PC_stat.paramfloatb[3.5/5.6]? Near surface effects correction exponent b_SE_ (2)stat.fit.paramfloatnullablea[-9.1/-0.8]? Near surface effects correction factor a_SE_ (2)stat.fit.paramfloatnullabler[1.000/1.003]? Near surface_effects correction parameter r_SE_ (2)stat.fit.paramfloatnullablechi2.cReduced chi square for classical parameters {chi}^2^_classic_stat.fit.chi2doublechi2.sReduced chi square for seismic parameters {chi}^2^_seism_stat.fit.chi2doubleTeff[5958/6228] Effective temperatureKphys.temperature.effectivefloat[Fe/H][0.19/0.39] Metallicitylog(Sun)phys.abund.Zfloatlogg[4.27/4.42] Surface gravitylog(cm.s**-2)phys.gravityfloatR[1.22/1.36] RadiussolRadphys.size.radiusfloatdnu[98/121] Mean large frequency separation <{Delta}{nu}>uHzem.freq;src.varfloatnumax[2025/2807] Frequency at maximum power {nu}_max_uHzem.freq;src.varfloatr02[0.05/0.11] Mean small frequency separation ratio <r_02_>em.freq;src.varfloatrr01/10[0.01/0.04] Mean small frequency separation ratio <rr_01/10_>em.freq;src.varfloatXc[0/0.7] Central hydrogen abundance X_c_phys.abund.XfloatdY/dZ[0/3.6] Helium to metal enrichment ratio {Delta}Y/{Delta}Zphys.abundfloatMcc[0/0.14] Convective core mass M_cc_solMassphys.massfloatRzc[0.69/0.87] Bottom of convective envelope radius R_zc_solRadphys.size.radiusfloatMpsini[1.14/1.34] Exoplanet mass M_p_sin(i), in Jupiter mass(1.898187x10+27kg)phys.massfloate_Mpsini[0.03/0.05] Mpsini error bar,(1.898187x10+27kg)stat.errorfloatJ/A+A/569/A21/optimizedModel results and restitution of the observational constraints with different optimisationse_Z/X0Z/X error bar (1)stat.error;src.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel identification (G1)meta.id;stat.param;meta.modelledcharAge[0.8/4.5] AgeGyrtime.agefloate_AgeAge error bar (1)Gyrstat.error;time.agefloatM[1.12/1.43] Stellar masssolMassphys.massfloate_MMass error bar (1)solMassstat.errorfloatZ/X0[0.03/0.07] Initial metal to hydrogen ratiophys.abund.ZfloatY0Initial helium contentphys.abundfloate_Y0? Y error bar (1)stat.error;pos.cartesian.yfloatnullableal.conv[0.4/2.1] Mixing length parameter convection {alpha}_conv_stat.paramfloate_al.conv? alpha conv error bar (1)stat.errorfloatnullableal.ov[0/2] Overshooting parameter {alpha}_ov_stat.paramfloatxiPC[0/1.3] Penetrative convection parameter {xi}_PC_stat.paramfloatb[3.5/5.6]? Near surface effects correction exponent b_SE_ (2)stat.fit.paramfloatnullablea[-9.1/-0.8]? Near surface effects correction factor a_SE_ (2)stat.fit.paramfloatnullabler[1.000/1.003]? Near surface_effects correction parameter r_SE_ (2)stat.fit.paramfloatnullablechi2.cReduced chi square for classical parameters {chi}^2^_classic_stat.fit.chi2doublechi2.sReduced chi square for seismic parameters {chi}^2^_seism_stat.fit.chi2doubleTeff[5958/6228] Effective temperatureKphys.temperature.effectivefloatLum[2.01/2.16] LuminositysolLumphys.luminosityfloat[Fe/H][0.19/0.39] Metallicitylog(Sun)phys.abund.Zfloatlogg[4.27/4.42] Surface gravitylog(cm.s**-2)phys.gravityfloatR[1.22/1.36] RadiussolRadphys.size.radiusfloatdnu[98/121] Mean large frequency separation <{Delta}{nu}>uHzem.freq;src.varfloatnumax[2025/2807] Frequency at maximum power {nu}_max_uHzem.freq;src.varfloatr02[0.05/0.11] Mean small frequency separation ratio <r_02_>em.freq;src.varfloatrr01/10[0.01/0.04] Mean small frequency separation ratio <rr_01/10_>em.freq;src.varfloatXc[0/0.7] Central hydrogen abundance X_c_phys.abund.XfloatdY/dZ[0/3.6] Helium to metal enrichment ratio {Delta}Y/{Delta}Zphys.abundfloatMcc[0/0.14] Convective core mass M_cc_solMassphys.massfloatRzc[0.69/0.87] Bottom of convective envelope radius R_zc_solRadphys.size.radiusfloatMpsini[1.14/1.34] Exoplanet mass M_p_sin(i), in Jupiter mass(1.898187x10+27kg)phys.massfloate_Mpsini[0.03/0.05] Mpsini error bar,(1.898187x10+27kg)stat.errorfloatJ/A+A/569/A21/optionsModel results and restitution of the observational constraints with different input physicsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel identification (G1)meta.id;stat.param;meta.modelledcharAge[0.8/4.5] AgeGyrtime.agefloate_AgeAge error bar (1)Gyrstat.error;time.agefloatM[1.12/1.43] Stellar masssolMassphys.massfloate_MMass error bar (1)solMassstat.errorfloatZ/X0[0.03/0.07] Initial metal to hydrogen ratiophys.abund.Zfloate_Z/X0Z/X error bar (1)stat.error;src.redshiftfloatY0Initial helium contentphys.abundfloate_Y0? Y error bar (1)stat.error;pos.cartesian.yfloatnullableal.conv[0.4/2.1] Mixing length parameter convection {alpha}_conv_stat.paramfloate_al.conv? alpha conv error bar (1)stat.errorfloatnullableal.ov[0/2] Overshooting parameter {alpha}_ov_stat.paramfloatxiPC[0/1.3] Penetrative convection parameter {xi}_PC_stat.paramfloatb[3.5/5.6]? Near surface effects correction exponent b_SE_ (2)stat.fit.paramfloatnullablea[-9.1/-0.8]? Near surface effects correction factor a_SE_ (2)stat.fit.paramfloatnullabler[1.000/1.003]? Near surface_effects correction parameter r_SE_ (2)stat.fit.paramfloatnullablechi2.cReduced chi square for classical parameters {chi}^2^_classic_stat.fit.chi2doublechi2.sReduced chi square for seismic parameters {chi}^2^_seism_stat.fit.chi2doubleTeff[5958/6228] Effective temperatureKphys.temperature.effectivefloatLum[2.01/2.16] LuminositysolLumphys.luminosityfloat[Fe/H][0.19/0.39] Metallicitylog(Sun)phys.abund.Zfloatlogg[4.27/4.42] Surface gravitylog(cm.s**-2)phys.gravityfloatR[1.22/1.36] RadiussolRadphys.size.radiusfloatdnu[98/121] Mean large frequency separation <{Delta}{nu}>uHzem.freq;src.varfloatnumax[2025/2807] Frequency at maximum power {nu}_max_uHzem.freq;src.varfloatr02[0.05/0.11] Mean small frequency separation ratio <r_02_>em.freq;src.varfloatrr01/10[0.01/0.04] Mean small frequency separation ratio <rr_01/10_>em.freq;src.varfloatXc[0/0.7] Central hydrogen abundance X_c_phys.abund.XfloatdY/dZ[0/3.6] Helium to metal enrichment ratio {Delta}Y/{Delta}Zphys.abundfloatMcc[0/0.14] Convective core mass M_cc_solMassphys.massfloatRzc[0.69/0.87] Bottom of convective envelope radius R_zc_solRadphys.size.radiusfloatMpsini[1.14/1.34] Exoplanet mass M_p_sin(i), in Jupiter mass(1.898187x10+27kg)phys.massfloate_Mpsini[0.03/0.05] Mpsini error bar,(1.898187x10+27kg)stat.errorfloat