J/A+A/523/A64ivo://CDS.VizieR/J/A+A/523/A64doi:10.26093/cds/vizier.35230064CDSRaiter A.Schaerer D.Fosbury R.2010-11-23T09:51:17Z2010-11-19T09:41:20ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresstellar-evolutionary-modelsstellar-populationsspectroscopyultraviolet-astronomyWe have computed evolutionary synthesis models covering metallicities from PopIII to solar, a wide range of IMFs, and two star-formation histories (bursts and constant star-formation). The detailed predictions these models, including their time dependence, are given here. The predicted quantities include ionising fluxes, UV continuum properties, recombination line strengths (for Ly{alpha}, HeII and other lines), as well as several other quantities of interest. The models provided here cover a wider range of parameter space than our earlier calculations (Schaerer, 2003A&A...397..527S, Cat. VI/109).2010A&A...523A..64Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/523/A64CatalogResearchIsServedByTAP VizieR generic servicerelated-tohttp://webast.ast.obs-mip.fr/sfr/ : Models homepagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/523/A64https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/523/A64http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/523/A64https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/523/A64https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/523/A64http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/523/A64GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tap5.457270654523099e-19 5.457270654523099e-19UVdefaultJ/A+A/523/A64/type21Output related to Wolf-Rayet stars (file corresponding to output described in Schaerer & Vacca, 1998ApJ...497..618S)IMFIMF type (G1)meta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.ZcharmupUpper mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintsfhCode for star formation history (G1)meta.codecharlog(Age)Agelog(yr)time.agedoubleWNLTypeAverage WNL subtype (late WN)src.spTypefloatWCTypeAverage WC subtypesrc.spTypefloatEWHaNebular H{alpha} equivalent width (G2)0.1nmspect.line.eqWidth;em.line.HalphafloatLHaNebular H{alpha} luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HalphadoubleEWHbNebular H{beta} equivalent width (G2)0.1nmspect.line.eqWidth;em.line.HbetafloatLHbNebular H{beta} luminosity (G2)1e-07Wphys.luminosity;em.line.HbetadoubleEWHe1640Stellar He1640 equivalent width0.1nmspect.line.eqWidthfloatLHeStellar He1640 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWN4640Stellar N4640 equivalent width0.1nmspect.line.eqWidthfloatLNStellar N4640 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWC4650Stellar C4650 equivalent width0.1nmspect.line.eqWidth;em.opt.BfloatLC4650Stellar C4650 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWHe4686Stellar He4686 equivalent width0.1nmspect.line.eqWidthfloatLHe4686Stellar He4686 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWH4861Stellar H4861 equivalent width0.1nmspect.line.eqWidthfloatLH4861Stellar H4861 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWC5696Stellar C5696 equivalent width0.1nmspect.line.eqWidth;em.opt.VfloatLC5696Stellar C5996 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWC5808Stellar C5808 equivalent width0.1nmspect.line.eqWidth;em.opt.VfloatLC5808Stellar C5808 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWH6560Stellar H6560 equivalent width0.1nmspect.line.eqWidthfloatLH6560Stellar H6560 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWHe5412Stellar He5412 equivalent width0.1nmspect.line.eqWidthfloatLHe5412Stellar He5412 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleallQuantitiesDisplay all output quantities for this model's parameters and agemeta.ref.urlcharJ/A+A/523/A64/type23Colors (filter bandpasses as in Starburst99, Leitherer et al., 1999ApJS..123....3L)IMFIMF type (G1)meta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.ZcharmupUpper mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintsfhCode for star formation history (G1)meta.codecharlog(Age)Agelog(yr)time.agedouble(130-V)(130-V) colour indexmagphot.color;em.UV;em.optfloat(210-V)(210-V) colour indexmagphot.color;em.UV;em.optfloat(U-B)(U-B) colour indexmagphot.color;em.opt.U;em.opt.Bfloat(B-V)(B-V) colour indexmagphot.color;em.opt.B;em.opt.Vfloat(V-R)(V-R) colour indexmagphot.color;em.opt.V;em.opt.Rfloat(V-I)(V-I) colour indexmagphot.color;em.opt.V;em.opt.Ifloat(V-J)(V-J) colour indexmagphot.color;em.opt.V;em.IR.Jfloat(V-H)(V-H) colour indexmagphot.color;em.opt.V;em.IR.Hfloat(V-K)(V-K) colour indexmagphot.color;em.opt.V;em.IR.Kfloat(V-L)(V-L) colour indexmagphot.color;em.opt.V;em.IR.3-4umfloatVMAGAbsolute V magnitudemagphys.magAbs;em.opt.VfloatBMAGAbsolute B magnitudemagphys.magAbs;em.opt.BfloatMbolBolometric magnitudemagphys.magAbs.bolfloatallQuantitiesDisplay all output quantities for this model's parameters and agemeta.ref.urlcharJ/A+A/523/A64/type24UV spectral informationIMFIMF type (G1)meta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.ZcharmupUpper mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintsfhCode for star formation history (G1)meta.codecharlog(Age)Agelog(yr)time.agedoubleMbolBolometric magnitudemagphys.magAbs.bolfloatlog(L15SB)Average UV luminosity at 1500{AA} (over +/-20{AA} band), in erg/s/{AA}log(1e-06W.nm**-1)phys.luminosity;em.UVfloatlog(L1500)Average UV luminosity at 1500{AA} (over +/-150{AA} band), in erg/s/{AA}log(1e-06W.nm**-1)phys.luminosity;em.UVfloatlog(L2800)Average UV luminosity at 2800{AA} (over +/-280{AA} band), in erg/s/{AA}log(1e-06W.nm**-1)phys.luminosity;em.UVfloatbeta1550UV slope 1300-1800{AA} using STELLAR + NEBULAR cont. emission (1)spect.indexfloatbeta2500UV slope 2200-2800{AA} using STELLAR + NEBULAR cont. emission (1)spect.indexfloatbeta2000UV slope 1800-2200{AA} using STELLAR + NEBULAR cont. emission (1)spect.indexfloatbeta1550*UV slope 1300-1800{AA} using pure STELLAR emission (1)spect.indexfloatbeta2500*UV slope 2200-2800{AA} using pure STELLAR emission (1)spect.indexfloatbeta2000*UV slope 1800-2200{AA} using pure STELLAR emission (1)spect.indexfloatlog(L900)Average luminosity 912- in erg/s/{AA} (2)log(1e-06W.nm**-1)phys.luminosity;em.UVfloatlog(Lybrk)Lyman-break amplitude Lybrk=912+/912-phot.flux;arith.ratiofloatlog(L1460)Average UV luminosity at 1195{AA} (over +/-85{AA} band)log(1e-06W.nm**-1)phys.luminosity;em.UVfloatbeta1460UV slope between 1195 (+/-85){AA} and 1738 (+/-127){AA}spect.indexfloatbetaGRUV slope computed using Steidel G,R filter curves (cf. Shapley et al., 2003ApJ...588...65S) (3)spect.indexfloatallQuantitiesDisplay all output quantities for this model's parameters and agemeta.ref.urlcharJ/A+A/523/A64/type25Ionising flux, UV luminosities and slopes - NEW in v2.53recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.ZcharIMFIMF type (G1)meta.codecharmupUpper mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintsfhCode for star formation history (G1)meta.codecharlog(Age)Agelog(yr)time.agedoublelog(Q0)Lyman continuum photon flux (Q_0_=Q_H_)log(s**-1)phot.flux.density;spect.continuumfloatlog(Q0/L1500)Ionising photon flux per 1500{AA} luminosity (in erg/{AA})log(1e-06W.nm**-1)phys.luminosityfloatMbolBolometric magnitudemagphys.magAbs.bolfloatlog(L15SB)Average UV luminosity at 1500{AA} (over +/-20{AA} band), in erg/s/{AA}log(1e-06W.nm**-1)phys.luminosity;em.UVfloatlog(L1500)Average UV luminosity at 1500{AA} (over +/-150{AA} band), in erg/s/{AA}log(1e-06W.nm**-1)phys.luminosity;em.UVfloatlog(L2800)Average UV luminosity at 2800{AA} (over +/-280{AA} band), in erg/s/{AA}log(1e-06W.nm**-1)phys.luminosity;em.UVfloatbeta1550UV slope 1300-1800{AA} using STELLAR + NEBULAR continuum emission (1)spect.indexfloatbeta2500UV slope 2200-2800{AA} using STELLAR + NEBULAR continuum emission (1)spect.indexfloatbeta2000UV slope 1800-2200{AA} using STELLAR + NEBULAR continuum emission (1)spect.indexfloatbeta1550*UV slope 1300-1800{AA} using pure STELLAR emission (1)spect.indexfloatbeta2500*UV slope 2200-2800{AA} using pure STELLAR emission (1)spect.indexfloatbeta2000*UV slope 1800-2200{AA} using pure STELLAR emission (1)spect.indexfloatlog(L900)Average luminosity 912- (2)log(1e-06W.nm**-1)phys.luminosity;em.UVfloatlog(Lybrk)Lyman-break amplitude Lyb=912+/912- (2)phot.flux;arith.ratiofloatneb/1500Contribution of the nebular continuum to the total continuum at 1500{AA} (3)stat.paramfloatneb/2800Contribution of the nebular continuum to the total continuum at 2800{AA} (4)stat.paramfloatallQuantitiesDisplay all output quantities for this model's parameters and agemeta.ref.urlcharJ/A+A/523/A64/type22Nebular recombination lines and Ly{alpha} absorptionrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.ZcharIMFIMF type (G1)meta.codecharmupUpper mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintsfhCode for star formation history (G1)meta.codecharlog(Age)Agelog(yr)time.agedoublelog(Q0)Lyman continuum photon flux (Q_0_=Q_H_)log(s**-1)phot.flux.density;spect.continuumfloatlog(Q1)He0 ionising photon flux (Q_1_=Q_He_)log(s**-1)phot.fluxfloatlog(Q2)He+ ionising photon flux (Q_0_=Q_He+_)log(s**-1)phot.fluxfloatLHbH{beta} luminosity (G2)1e-07Wphys.luminosity;em.line.HbetadoubleEWHLyaLyman{alpha} equivalent width (G2)0.1nmspect.line.eqWidthdoubleIHLyaLyman{alpha} intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHaH{alpha} equivalent width (G2)0.1nmspect.line.eqWidth;em.line.HalphadoubleIHaH{alpha} intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHbH{beta} equivalent width (G2)0.1nmspect.line.eqWidth;em.line.HbetadoubleIHb[1.00E+00] H{beta} intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHeIHeI 4471 equivalent width (CAUTION: Saturation effect !) (G2)0.1nmspect.line.eqWidthfloatIHeIHeI 4471 intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHeII1640HeII1640 equivalent width (G2)0.1nmspect.line.eqWidthfloatIHeII1640HeII1640 intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHeII4686HeII4686 equivalent width (G2)0.1nmspect.line.eqWidthfloatIHeII4686HeII4686 intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHeII3203HeII3203 equivalent width (G2)0.1nmspect.line.eqWidthfloatIHeII3203HeII3203 intensity relative to H{beta} (G2)phys.luminosity;em.line.HbetadoubleEWHeII4541HeII4541 equivalent width (G2)0.1nmspect.line.eqWidthfloatIHeII4541HeII4541 intensity relative to H{beta}phys.luminosity;em.line.HbetadoubleLyaAbsLy{alpha} absorption equivalent width (1)0.1nmspect.line.eqWidthfloatILyaAbsLy{alpha} absorption intensity relative to H{beta} (1)phys.absorption.gal;arith.ratiodoubleLyaAbscLy{alpha} absorption computed EXCLUDING nebular continuum equivalent width (1)0.1nmspect.line.eqWidth;spect.continuum;meta.modelledfloatFcontLyaContinuum flux (stellar+nebular) at Ly{alpha} (in erg/s/{AA} units) (1)10000W.m**-1phot.flux;em.UVdoubleLyaAbs2Ly{alpha} absorption equivalent width (2)0.1nmspect.line.eqWidthfloatILyaAbs2Ly{alpha} absorption intensity relative to H{beta} (2)phys.absorption.gal;arith.ratiodoubleLyaAbsc2Ly{alpha} absorption computed EXCLUDING nebular continuum equivalent width (2)0.1nmspect.line.eqWidth;spect.continuum;meta.modelledfloatFcontLya2Continuum flux (stellar+nebular) at Ly{alpha} (in erg/s/{AA} units) (2)10000W.m**-1phot.flux;em.UVdoubleE(Q)Average energy per photon in Lyman-continuumeVstat.paramfloatallQuantitiesDisplay all output quantities for this model's parameters and agemeta.ref.urlcharJ/A+A/523/A64/type20Main output (file corresponding to output described in Schaerer & Vacca, 1998ApJ...497..618S) plus additional quantities (last four columns)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.ZcharIMFIMF type (G1)meta.codecharmupUpper mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)solMassphys.massintsfhCode for star formation history (G1)meta.codecharlog(Age)Agelog(yr)time.agedoubleMbolBolometric magnitudemagphys.magAbs.bolfloatlog(Q0)Lyman continuum photon flux (Q_0=Q_H)log(s**-1)phot.flux.density;spect.continuumfloatlog(Q1)He0 ionising photon flux (Q_1=Q_He)log(s**-1)phot.fluxfloatlog(Q2)He+ ionising photon flux (Q_0=Q_He+)log(s**-1)phot.fluxfloatNOstarNumber of O starsmeta.numberdoubleWR/(WR+O)Ratio of WR to WR+O starsstat.paramdoubleWR/ORatio of WR to O starsstat.paramdoubleWNL/(WR+O)Ratio of WNL (late WN) to WR+O starsstat.paramdoubleWNE/(WR+O)Ratio of WNE (early WN) to WR+O starsstat.paramdoubleWC/(WR+O)Ratio of WC to WR+O stars WC/(WR+O)stat.paramdoubleEWHbNebular H{beta} equivalent width (G2)0.1nmspect.line.eqWidth;em.line.HbetadoubleLHbNebular H{beta} luminosity (G2)1e-07Wphys.luminosity;em.line.HbetadoubleEWHeINebular HeI 4471 equivalent width (CAUTION: Saturation effect !) (G2)0.1nmspect.line.eqWidthdoubleLHeINebular HeI 4471 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWHeIINebular HeII 4686 equivalent width (G2)0.1nmspect.line.eqWidthdoubleLHeIINebular HeII 4686 luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWWRWR bump (CIII/IV 4650 + HeII 4686) equivalent width0.1nmspect.line.eqWidthdoubleLWRWR bump (CIII/IV 4650 + HeII 4686) luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleEWCICI V-WR equivalent width0.1nmspect.line.eqWidthdoubleLCICI V-WR luminosity (in H{beta} unit) (G2)phys.luminosity;em.line.HbetadoubleBalmerBalmer jump, defined as -2.5*log(F(3640{AA})/F(3650{AA})magphot.magfloatlog(QH2)Ionising photon flux in Lyman-Werner band (Q_H2_=Q_LW_)log(s**-1)phot.fluxfloatE(Q)Average energy per photon in Lyman-continuumeVstat.paramfloatE(QHe+)Average energy per photon with E>54eVeVstat.paramfloatallQuantitiesDisplay all output quantities for this model's parameters and agemeta.ref.urlcharJ/A+A/523/A64/initial*List of available setsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZCode for metallicity Z (G1)phys.abund.Zcharttt[ge0] Tracks (G1)meta.codecharIMFIMF type (G1)meta.codecharmupUpper mass cut-off of IMF in M_{sun}_ (G1)phys.massintlowLower mass cut-off of IMF in M_{sun}_ (G1)phys.massintsfhCode for star formation history (G1)meta.codecharmodelDisplay all the data for this set of parametersmeta.ref.urlchar