VI/102ivo://CDS.VizieR/VI/102CDSLejeune T.Schaerer D.2017-06-27T06:37:44Z2003-10-05T16:36:00ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsstellar-mass-losshertzsprung-russell-diagraminfrared-photometryvisible-astronomyWide-band photometrynarrow-band-photometryThis database was created from an updated version of the empirically and semi-empirically calibrated BaSeL library of synthetic stellar spectra of Lejeune et al. (1997, Cat. <J/A+AS/125/229>, 1998, Cat. <J/A+AS/130/65>) and Westera et al. (1999, ASP Conference Series 192, 203-206) to calculate synthetic photometry in the (UBV)_J_(RI)_C_ JHKLL'M, HST-WFPC2, Geneva, and Washington systems for the entire set of non-rotating Geneva stellar evolution models covering masses from 0.4-0.8 to 120-150M_{sun}_ and metallicities Z=0.0004 (1/50Z_{sun}_) to 0.1 (5Z_{sun}_). The results are provided in a database which includes all individual stellar tracks and the corresponding isochrones covering ages from 10^3^yr to 16-20Gyr in time steps of {Delta}logt=0.05dex. The database also includes a new grid of stellar tracks of very metal-poor stars (Z=0.0004) from 0.8-150M_{sun}_ calculated with the Geneva stellar evolution code. The complete stellar grids are tabulated in the files table1.dat (summary), evol.dat (evolutionary models), and in the files ubv.dat, hst.dat, gen.dat and cmt.dat (synthetic colors in the different photometric systems). These grids are also available as mod* files in subdirectories evol, ubv, hst, gen and cmt. The isochrones for the different photometric systems are summarized in the file table2.dat; the parameters of the isochrones are tabulated in the file iso.dat, the detailed isochrones being available as files iso* in the subdirectories ubv, hst, gen and cmt.2001A&A...366..538Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/VI/102CatalogResearchIsServedByTAP VizieR generic servicerelated-tohttp://webast.ast.obs-mip.fr/stellar/ : Database of GenevaJ/A+AS/125/229 : A standard stellar library (Lejeune+ 1997)J/A+AS/130/65 : A standard stellar library. II. (Lejeune+ 1998)J/A+AS/96/269 : Grids of stellar models. I. (Schaller+, 1992)J/A+AS/98/523 : Grids of stellar models. II. (Schaerer+ 1993)J/A+AS/101/415 : Grids of stellar models III. (Charbonnel+ 1993)J/A+AS/102/339 : Grids of stellar models IV (Schaerer+, 1993)J/A+AS/103/97 : Grids of stellar models V. (Meynet+ 1994)J/A+AS/115/339 : Grids of stellar models VI. (Charbonnel+, 1996)J/A+AS/128/471 : Grids of stellar models. VII. (Mowlavi+ 1998)J/A+AS/135/405 : Grids of stellar models. VIII. (Charbonnel+ 1999)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=VI/102https://vizier.iucaa.in/viz-bin/VizieR-2?-source=VI/102http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=VI/102https://vizier.cds.unistra.fr/viz-bin/votable?-source=VI/102https://vizier.iucaa.in/viz-bin/votable?-source=VI/102http://vizieridia.saao.ac.za/viz-bin/votable?-source=VI/102GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultVI/102/table2Summary of isochrone sets included in the databaserecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintType[BEA] Type of grids (G1)meta.codecharID[ecpmol] Model type (see table1)meta.codecharZMetallicityphys.abund.ZfloatlogAgelLower value of age range (2)log(yr)time.agefloatlogAgeuUpper value of age rangelog(yr)time.agefloatDescDescriptionmeta.noteISOavailable isochrones for this modelmeta.refcharVI/102/evolStellar grids: surface parametersYHe surface abundance (mass fraction)phys.abund.YdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial Metallicity (mass fraction)phys.abund.ZfloatiMassInitial masssolMassphys.massfloatID[celmpo] Model type (see table1.dat)meta.codecharSeqNumber of selected pointmeta.idintAgeAgeyrtime.agedoubleMassActual mass in solar massessolMassphys.massdoublelogLlog(luminosity) in solar unitslog(solLum)phys.luminosityfloatlogTefflog(effective temperature)log(K)phys.temperature.effectivefloatXH surface abundance (mass fraction)phys.abund.XdoubleC1212C surface abundance (mass fraction)phys.abunddoubleC1313C surface abundance (mass fraction)phys.abunddoubleN1414N surface abundance (mass fraction)phys.abunddoubleO1616O surface abundance (mass fraction)phys.abunddoubleO1717O surface abundance (mass fraction)phys.abunddoubleO1818O surface abundance (mass fraction)phys.abunddoubleNe2020Ne surface abundance (mass fraction)phys.abunddoubleNe2222Ne surface abundance (mass fraction)phys.abunddoubleSCTStellar core temperature for Wolf-Rayet starslog(K)phys.temperaturefloatdM/dtMass-loss ratesolMass/yrphys.mass.lossfloatVI/102/ubvStellar grids: UBV(RI)_C_JHKLL'M photometryAgeAgeyrtime.agedoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial Metallicity (mass fraction)phys.abund.ZfloatiMassInitial masssolMassphys.massfloatID[celmpo] Model type (see table1.dat)meta.codecharSeqNumber of selected pointmeta.idintMassActual mass in solar massessolMassphys.massfloatlogTefflog(effective temperature)log(K)phys.temperature.effectivefloatloggSurface gravitylog(cm.s**-2)phys.gravityfloatlogLlog(luminosity) in solar unitslog(solLum)phys.luminosityfloatVMAG? absolute V magnitudemagphys.magAbs;em.optfloatnullableU-B? U-B color indexmagphot.color;em.opt.U;em.opt.BfloatnullableB-V? B-V color indexmagphot.color;em.opt.B;em.opt.VfloatnullableV-R? V-R color indexmagphot.color;em.opt.V;em.opt.RfloatnullableV-I? V-I color indexmagphot.color;em.opt.V;em.opt.IfloatnullableV-K? V-K color indexmagphot.color;em.opt.V;em.IR.KfloatnullableR-I? R-I color indexmagphot.color;em.opt.R;em.opt.IfloatnullableI-K? I-K color indexmagphot.color;em.opt.I;em.IR.KfloatnullableJ-H? J-H color indexmagphot.color;em.IR.J;em.IR.HfloatnullableH-K? H-K color indexmagphot.color;em.IR.H;em.IR.KfloatnullableK-L? K-L color indexmagphot.color;em.IR.K;em.IR.3-4umfloatnullableJ-K? J-K color indexmagphot.color;em.IR.J;em.IR.KfloatnullableJ-L? J-L color indexmagphot.color;em.opt.R;em.opt.IfloatnullableJ-L'? J-L' color indexmagphot.color;em.opt.R;em.opt.IfloatnullableK-M? K-M color indexmagphot.color;em.IR.K;em.IR.4-8umfloatnullableSurfFull Surface Parameters for this model at the same agemeta.refcharVI/102/genStellar grids: Geneva photometrySeqNumber of selected pointmeta.idintZInitial Metallicity (mass fraction)phys.abund.ZfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintiMassInitial masssolMassphys.massfloatID[celmpo] Model type (see table1.dat)meta.codecharAgeAgeyrtime.agedoubleMassActual mass in solar massessolMassphys.massfloatlogTefflog(effective temperature)log(K)phys.temperature.effectivefloatloggSurface gravitylog(cm.s**-2)phys.gravityfloatlogLlog(luminosity) in solar unitslog(solLum)phys.luminosityfloatVMAG? absolute V magnitudemagphys.magAbs;em.optfloatnullableU-B? U-B color indexmagphot.colorfloatnullableB1-B? B1-B color indexmagphot.colorfloatnullableB2-B? B2-B color indexmagphot.colorfloatnullableV1-B? V1-B color indexmagphot.colorfloatnullableVg-B? Vg-B color indexmagphot.colorfloatnullableG-B? G-B color indexmagphot.colorfloatnullableB1-B2? B1-B2 color indexmagphot.colorfloatnullableB2-V1? B2-V1 color indexmagphot.colorfloatnullableV1-G? V1-G color indexmagphot.colorfloatnullableVg-V? Vg-V color indexmagphot.colorfloatnullableSurfFull Surface Parameters for this model at the same agemeta.refcharVI/102/hstStellar grids: HST-WFPC2 photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial Metallicity (mass fraction)phys.abund.ZfloatiMassInitial masssolMassphys.massfloatID[celmpo] Model type (see table1.dat)meta.codecharSeqNumber of selected pointmeta.idintAgeAgeyrtime.agedoubleMassActual mass in solar massessolMassphys.massfloatlogTefflog(effective temperature)log(K)phys.temperature.effectivefloatloggSurface gravitylog(cm.s**-2)phys.gravityfloatlogLlog(luminosity) in solar unitslog(solLum)phys.luminosityfloatVMAG? absolute V magnitudemagphys.magAbs;em.optfloatnullableF336W-F439W? F336W-F439W color indexmagphot.color;em.opt.U;em.opt.BfloatnullableF439W-F555W? F439W-F555W color indexmagphot.color;em.opt.B;em.opt.VfloatnullableF555W-F675W? F555W-F675W color indexmagphot.color;em.opt.V;em.opt.RfloatnullableF555W-F814W? F555W-F814W color indexmagphot.color;em.opt.V;em.opt.IfloatnullableF675W-F814W? F675W-F814W color indexmagphot.color;em.opt.R;em.opt.IfloatnullableF439W-V? F439W-V color indexmagphot.color;em.opt.B;em.opt.VfloatnullableSurfFull Surface Parameters for this model at the same agemeta.refcharVI/102/cmtStellar grids: Washington CMT1T2V photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial Metallicity (mass fraction)phys.abund.ZfloatiMassInitial masssolMassphys.massfloatID[celmpo] Model type (see table1.dat)meta.codecharSeqNumber of selected pointmeta.idintAgeAgeyrtime.agedoubleMassActual mass in solar massessolMassphys.massfloatlogTefflog(effective temperature)log(K)phys.temperature.effectivefloatloggSurface gravitylog(cm.s**-2)phys.gravityfloatlogLlog(luminosity) in solar unitslog(solLum)phys.luminosityfloatVMAG? absolute V magnitudemagphys.magAbs;em.optfloatnullableC-M? C-M color indexmagphot.colorfloatnullableM-T1? M-T1 color indexmagphot.colorfloatnullableT1-T2? T1-T2 color indexmagphot.colorfloatnullableC-T1? C-T1 color indexmagphot.colorfloatnullableM-T2? M-T2 color indexmagphot.colorfloatnullableC-R? C-R color indexmagphot.color;em.opt.B;em.opt.RfloatnullableM-R? M-R color indexmagphot.color;em.opt.V;em.opt.RfloatnullableR-T2? R-T2 color indexmagphot.color;em.opt.R;em.opt.IfloatnullableV-T1? V-T1 color indexmagphot.color;em.opt.V;em.opt.RfloatnullableSurfFull Surface Parameters for this model at the same agemeta.refcharVI/102/table1Summary of stellar grids included in the databaseGridGrid numbermeta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintType[BEA] Type of grids (G1)meta.codecharID[ecpmoln] Databasemeta.codecharZMetallicity (mass fraction)phys.abund.ZfloatXH abundance (mass fraction)phys.abund.XfloatYHe abundance (mass fraction)phys.abund.YfloatMdot[1,2] Mass loss (standard or 2xstd)phys.mass.lossintMasslLower value of the mass rangesolMassphys.massfloatMassuUpper value of the mass rangesolMassphys.massfloatpaperPaper containing the data (2)meta.refcharFileName of file with model (3)meta.id;meta.filecharDescDescriptionmeta.noteVI/102/isoSummary of IsochronesID[celmpo] Model typemeta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial Metallicity (mass fraction)phys.abund.ZfloatlogAgeAge of isochronelog(yr)time.agefloatFileMain part of isochrone filenamemeta.id;meta.filecharLinkParameters from Table1 for this modelmeta.refchar