J/A+A/392/1ivo://CDS.VizieR/J/A+A/392/1doi:10.26093/cds/vizier.33920001CDSSchulz J.Fritze-v.Alvensleben U.Moeller C.S.2006-12-16T15:04:57Z2006-12-16T16:03:56ZCDS support team

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

cds-question@unistra.frglobular-star-clustersopen-star-clustersstellar-evolutionary-modelsspectrophotometrytwo-color-diagramsA new set of evolutionary synthesis spectra are presented for Simple Stellar Populations (SSPs) covering ranges in metallicity from 0.02<=Z/Z_{sun}_<=2.5 and ages from 4*10^6^yr<=t<=16Gyr. They are based on the most recent isochrones from the Padova group that extend earlier models by the inclusion of the thermal pulsing AGB phase for stars in the mass range 2M_{sun}_<=m<=7M_{sun}_ in accordance with the fuel consumption theorem. We show that with respect to earlier models, inclusion of the TP-AGB phase leads to significant changes in the (V-I) and (V-K) colors of SSPs in the age range from 10^8^ to >~10^9^yr. Using model atmosphere spectra from Lejeune et al. (1997, Cat. <J/A+AS/125/229>, 1998, Cat. <J/A+AS/130/65>), we calculate the spectral evolution of single burst populations of various metallicities covering the wavelength range from 90{AA} through 160{mu}m. Isochrone spectra are convolved with filter response functions to describe the time evolution of luminosities and colors in Johnson, Thuan & Gunn, Koo, HST, Washington and Stroemgren filters. The models and their results are not only intended for use in the interpretation of star clusters but also for combination with any kind of dynamical galaxy formation and/or evolution model that contains a star formation criterion. Moreover, the evolution of these single burst single metallicity stellar populations is readily folded with any kind of star formation -- and eventually chemical enrichment -- history to describe the evolutionary spectral synthesis of composite stellar populations like galaxies of any type with continuous or discontinuous star formation. For these latter purposes we also present the time evolution of ejection rates for gas and metals for two different Initial Mass Functions (IMFs) as well as cosmological and evolutionary corrections for all the filters as a function of redshift for 0<=z<=5 and two different cosmologies.2002A&A...392....1Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/392/1CatalogResearchIsServedByTAP VizieR generic servicerelated-tohttp://www.uni-sw.gwdg.de/~galev : The Goettingen Galaxy Evolution GroupVI/102 : Geneva stellar evolution tracks and isochrones (Lejeune+ 2001)J/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/106/275 : Theoretical isochrones (Bertelli+ 1994)J/A+AS/141/371 : Low-mass stars evolutionary tracks+isochrones (Girardi+, 2000)J/A+AS/100/647 : Evolutionary Sequences II. (Bressan+ 1993)J/A+AS/104/365 : Evolutionary sequences. III. (Fagotto+ 1994)J/A+AS/105/29 : Evolutionary sequences IV. (Fagotto+ 1994)J/A+AS/105/39 : Evolutionary sequences V. (Fagotto+ 1994)J/A+AS/117/113 : Evolutionary stellar models. VI. Z=0.0001 (Girardi+, 1996)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/392/1https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/392/1http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/392/1https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/392/1https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/392/1http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/392/1GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/392/1/sajohnLuminosities and colors from the spectra in Johnson filter-system, Salpeter IMFH-KJohnson H-K color indexmagphot.color;em.IR.H;em.IR.KfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeAge of systemyrtime.agedoubleUmagJohnson U magnitudemagphot.mag;em.opt.UfloatBmagJohnson B magnitudemagphot.mag;em.opt.BfloatVmagJohnson V magnitudemagphot.mag;em.opt.VfloatRmagJohnson R magnitudemagphot.mag;em.opt.RfloatImagJohnson I magnitudemagphot.mag;em.opt.IfloatJmagJohnson J magnitudemagphot.mag;em.IR.JfloatHmagJohnson H magnitudemagphot.mag;em.IR.HfloatKmagJohnson K magnitudemagphot.mag;em.IR.KfloatLmagJohnson L magnitudemagphot.mag;em.IR.3-4umfloatU-BJohnson U-B color indexmagphot.color;em.opt.U;em.opt.BfloatB-VJohnson B-V color indexmagphot.color;em.opt.B;em.opt.VfloatU-VJohnson U-V color indexmagphot.color;em.opt.U;em.opt.VfloatV-RJohnson V-R color indexmagphot.color;em.opt.V;em.opt.RfloatR-IJohnson R-I color indexmagphot.color;em.opt.R;em.opt.IfloatV-KJohnson V-K color indexmagphot.color;em.opt.V;em.IR.KfloatI-KJohnson I-K color indexmagphot.color;em.opt.I;em.IR.KfloatB-RJohnson B-R color indexmagphot.color;em.opt.B;em.opt.RfloatB-HJohnson B-H color indexmagphot.color;em.opt.B;em.IR.HfloatJ-HJohnson J-H color indexmagphot.color;em.IR.J;em.IR.HfloatJ/A+A/392/1/scjohnLuminosities and colors from the spectra in Johnson filter-system, Scalo IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeAge of systemyrtime.agedoubleUmagJohnson U magnitudemagphot.mag;em.opt.UfloatBmagJohnson B magnitudemagphot.mag;em.opt.BfloatVmagJohnson V magnitudemagphot.mag;em.opt.VfloatRmagJohnson R magnitudemagphot.mag;em.opt.RfloatImagJohnson I magnitudemagphot.mag;em.opt.IfloatJmagJohnson J magnitudemagphot.mag;em.IR.JfloatHmagJohnson H magnitudemagphot.mag;em.IR.HfloatKmagJohnson K magnitudemagphot.mag;em.IR.KfloatLmagJohnson L magnitudemagphot.mag;em.IR.3-4umfloatU-BJohnson U-B color indexmagphot.color;em.opt.U;em.opt.BfloatB-VJohnson B-V color indexmagphot.color;em.opt.B;em.opt.VfloatU-VJohnson U-V color indexmagphot.color;em.opt.U;em.opt.VfloatV-RJohnson V-R color indexmagphot.color;em.opt.V;em.opt.RfloatR-IJohnson R-I color indexmagphot.color;em.opt.R;em.opt.IfloatV-KJohnson V-K color indexmagphot.color;em.opt.V;em.IR.KfloatI-KJohnson I-K color indexmagphot.color;em.opt.I;em.IR.KfloatB-RJohnson B-R color indexmagphot.color;em.opt.B;em.opt.RfloatB-HJohnson B-H color indexmagphot.color;em.opt.B;em.IR.HfloatJ-HJohnson J-H color indexmagphot.color;em.IR.J;em.IR.HfloatH-KJohnson H-K color indexmagphot.color;em.IR.H;em.IR.KfloatJ/A+A/392/1/samagLuminosities from the spectra in Koo, Thuan & Gunn, Washington and Stroemgren filter-systems, Salpeter IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeAge of systemyrtime.agedoubleukmagKoo u magnitudemagphot.magfloatjkmagKoo j magnitudemagphot.magfloatfkmagKoo f magnitudemagphot.magfloatnkmagKoo n magnitudemagphot.magfloatgmagThuan & Gunn g magnitudemagphot.mag;em.opt.RfloatrmagThuan & Gunn r magnitudemagphot.mag;em.opt.RfloatCmagWashington C magnitudemagphot.mag;em.opt.UfloatMmagWashington M magnitudemagphot.mag;em.opt.VfloatT1magWashington T1 magnitudemagphot.mag;em.opt.RfloatT2magWashington T2 magnitudemagphot.mag;em.opt.IfloatumagStroemgren u magnitudemagphot.mag;em.opt.UfloatvmagStroemgren v magnitudemagphot.mag;em.opt.BfloatbmagStroemgren b magnitudemagphot.mag;em.opt.BfloatymagStroemgren y magnitudemagphot.mag;em.opt.VfloatJ/A+A/392/1/scmagLuminosities from the spectra in Koo, Thuan & Gunn, Washington and Stroemgren filter-systems, Scalo IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeAge of systemyrtime.agedoubleukmagKoo u magnitudemagphot.magfloatjkmagKoo j magnitudemagphot.magfloatfkmagKoo f magnitudemagphot.magfloatnkmagKoo n magnitudemagphot.magfloatgmagThuan & Gunn g magnitudemagphot.mag;em.opt.RfloatrmagThuan & Gunn r magnitudemagphot.mag;em.opt.RfloatCmagWashington C magnitudemagphot.mag;em.opt.UfloatMmagWashington M magnitudemagphot.mag;em.opt.VfloatT1magWashington T1 magnitudemagphot.mag;em.opt.RfloatT2magWashington T2 magnitudemagphot.mag;em.opt.IfloatumagStroemgren u magnitudemagphot.mag;em.opt.UfloatvmagStroemgren v magnitudemagphot.mag;em.opt.BfloatbmagStroemgren b magnitudemagphot.mag;em.opt.BfloatymagStroemgren y magnitudemagphot.mag;em.opt.VfloatJ/A+A/392/1/schstLuminosities from the spectra in HST filter-system, Scalo IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeAge of systemyrtime.agedoubleF160BWHST F160BW magnitudemagphot.mag;em.UV.100-200nmdoubleF170WHST F170W magnitudemagphot.mag;em.UV.100-200nmdoubleF185WHST F185W magnitudemagphot.mag;em.UV.100-200nmdoubleF218WHST F218W magnitudemagphot.mag;em.UV.200-300nmdoubleF255WHST F255W magnitudemagphot.mag;em.UV.200-300nmdoubleF300WHST F300W = U(HDF) magnitudemagphot.mag;em.opt.UdoubleF336WHST F336W magnitudemagphot.mag;em.opt.UdoubleF380WHST F380W magnitudemagphot.mag;em.opt.UdoubleF439WHST F439W magnitudemagphot.mag;em.opt.BdoubleF450WHST F450W = B(HDF) magnitudemagphot.mag;em.opt.BdoubleF555WHST F555W = V(YSC) magnitudemagphot.mag;em.opt.VdoubleF569WHST F569W magnitudemagphot.mag;em.opt.VdoubleF606WHST F606W = V(HDF) magnitudemagphot.mag;em.opt.RdoubleF622WHST F622W magnitudemagphot.mag;em.opt.RdoubleF675WHST F675W magnitudemagphot.mag;em.opt.RdoubleF702WHST F702W magnitudemagphot.mag;em.opt.RdoubleF791WHST F791W magnitudemagphot.mag;em.opt.IdoubleF814WHST F814W = I(HDF) magnitudemagphot.mag;em.opt.IdoubleJ/A+A/392/1/saspectSpectra, with Salpeter IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity: 0.0004 0.004 0.008 0.02 0.05phys.abund.ZfloatlambdaWavelength0.1nmem.wldoubleFlux1Flux at a system age of 1.4000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux2Flux at a system age of 2.8000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux3Flux at a system age of 4.2000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux4Flux at a system age of 5.6000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux5Flux at a system age of 7.0000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux6Flux at a system age of 8.4000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux7Flux at a system age of 9.8000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux8Flux at a system age of 1.1200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux9Flux at a system age of 1.2600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux10Flux at a system age of 1.4000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux11Flux at a system age of 1.5400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux12Flux at a system age of 1.6800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux13Flux at a system age of 1.8200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux14Flux at a system age of 1.9600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux15Flux at a system age of 2.1000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux16Flux at a system age of 2.2400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux17Flux at a system age of 2.3800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux18Flux at a system age of 2.5200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux19Flux at a system age of 2.6600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux20Flux at a system age of 2.8000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux21Flux at a system age of 2.9400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux22Flux at a system age of 3.0800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux23Flux at a system age of 3.2200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux24Flux at a system age of 3.3600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux25Flux at a system age of 3.5000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux26Flux at a system age of 3.6400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux27Flux at a system age of 3.7800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux28Flux at a system age of 3.9200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux29Flux at a system age of 4.0600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux30Flux at a system age of 4.2000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux31Flux at a system age of 4.3400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux32Flux at a system age of 4.4800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux33Flux at a system age of 4.6200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux34Flux at a system age of 4.7600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux35Flux at a system age of 4.9000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux36Flux at a system age of 5.0400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux37Flux at a system age of 5.1800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux38Flux at a system age of 5.3200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux39Flux at a system age of 5.4600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux40Flux at a system age of 5.6000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux41Flux at a system age of 5.7400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux42Flux at a system age of 5.8800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux43Flux at a system age of 6.0200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux44Flux at a system age of 6.1600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux45Flux at a system age of 6.3000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux46Flux at a system age of 6.4400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux47Flux at a system age of 6.5800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux48Flux at a system age of 6.7200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux49Flux at a system age of 6.8600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux50Flux at a system age of 7.0000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux51Flux at a system age of 7.1400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux52Flux at a system age of 7.2800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux53Flux at a system age of 7.4200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux54Flux at a system age of 7.5600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux55Flux at a system age of 7.7000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux56Flux at a system age of 7.8400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux57Flux at a system age of 7.9800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux58Flux at a system age of 8.1200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux59Flux at a system age of 8.2600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux60Flux at a system age of 8.4000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux61Flux at a system age of 8.5400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux62Flux at a system age of 8.6800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux63Flux at a system age of 8.8200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux64Flux at a system age of 8.9600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux65Flux at a system age of 9.1000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux66Flux at a system age of 9.2400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux67Flux at a system age of 9.3800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux68Flux at a system age of 9.5200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux69Flux at a system age of 9.6600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux70Flux at a system age of 9.8000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux71Flux at a system age of 9.9400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux72Flux at a system age of 1.0080E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux73Flux at a system age of 1.0220E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux74Flux at a system age of 1.0360E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux75Flux at a system age of 1.0500E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux76Flux at a system age of 1.0640E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux77Flux at a system age of 1.0780E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux78Flux at a system age of 1.0920E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux79Flux at a system age of 1.1060E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux80Flux at a system age of 1.1200E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux81Flux at a system age of 1.1340E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux82Flux at a system age of 1.1480E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux83Flux at a system age of 1.1620E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux84Flux at a system age of 1.1760E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux85Flux at a system age of 1.1900E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux86Flux at a system age of 1.2040E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux87Flux at a system age of 1.2180E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux88Flux at a system age of 1.2320E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux89Flux at a system age of 1.2460E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux90Flux at a system age of 1.2600E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux91Flux at a system age of 1.2740E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux92Flux at a system age of 1.2880E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux93Flux at a system age of 1.3020E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux94Flux at a system age of 1.3160E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux95Flux at a system age of 1.3300E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux96Flux at a system age of 1.3440E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux97Flux at a system age of 1.3580E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux98Flux at a system age of 1.3720E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux99Flux at a system age of 1.3860E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux100Flux at a system age of 1.4000E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleJ/A+A/392/1/scspectSpectra, with Scalo IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity: 0.0004 0.004 0.008 0.02 0.05phys.abund.ZfloatlambdaWavelength0.1nmem.wldoubleFlux1Flux at a system age of 1.4000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux2Flux at a system age of 2.8000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux3Flux at a system age of 4.2000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux4Flux at a system age of 5.6000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux5Flux at a system age of 7.0000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux6Flux at a system age of 8.4000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux7Flux at a system age of 9.8000E+08yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux8Flux at a system age of 1.1200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux9Flux at a system age of 1.2600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux10Flux at a system age of 1.4000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux11Flux at a system age of 1.5400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux12Flux at a system age of 1.6800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux13Flux at a system age of 1.8200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux14Flux at a system age of 1.9600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux15Flux at a system age of 2.1000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux16Flux at a system age of 2.2400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux17Flux at a system age of 2.3800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux18Flux at a system age of 2.5200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux19Flux at a system age of 2.6600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux20Flux at a system age of 2.8000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux21Flux at a system age of 2.9400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux22Flux at a system age of 3.0800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux23Flux at a system age of 3.2200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux24Flux at a system age of 3.3600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux25Flux at a system age of 3.5000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux26Flux at a system age of 3.6400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux27Flux at a system age of 3.7800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux28Flux at a system age of 3.9200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux29Flux at a system age of 4.0600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux30Flux at a system age of 4.2000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux31Flux at a system age of 4.3400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux32Flux at a system age of 4.4800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux33Flux at a system age of 4.6200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux34Flux at a system age of 4.7600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux35Flux at a system age of 4.9000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux36Flux at a system age of 5.0400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux37Flux at a system age of 5.1800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux38Flux at a system age of 5.3200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux39Flux at a system age of 5.4600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux40Flux at a system age of 5.6000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux41Flux at a system age of 5.7400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux42Flux at a system age of 5.8800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux43Flux at a system age of 6.0200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux44Flux at a system age of 6.1600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux45Flux at a system age of 6.3000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux46Flux at a system age of 6.4400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux47Flux at a system age of 6.5800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux48Flux at a system age of 6.7200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux49Flux at a system age of 6.8600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux50Flux at a system age of 7.0000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux51Flux at a system age of 7.1400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux52Flux at a system age of 7.2800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux53Flux at a system age of 7.4200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux54Flux at a system age of 7.5600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux55Flux at a system age of 7.7000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux56Flux at a system age of 7.8400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux57Flux at a system age of 7.9800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux58Flux at a system age of 8.1200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux59Flux at a system age of 8.2600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux60Flux at a system age of 8.4000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux61Flux at a system age of 8.5400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux62Flux at a system age of 8.6800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux63Flux at a system age of 8.8200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux64Flux at a system age of 8.9600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux65Flux at a system age of 9.1000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux66Flux at a system age of 9.2400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux67Flux at a system age of 9.3800E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux68Flux at a system age of 9.5200E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux69Flux at a system age of 9.6600E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux70Flux at a system age of 9.8000E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux71Flux at a system age of 9.9400E+09yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux72Flux at a system age of 1.0080E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux73Flux at a system age of 1.0220E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux74Flux at a system age of 1.0360E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux75Flux at a system age of 1.0500E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux76Flux at a system age of 1.0640E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux77Flux at a system age of 1.0780E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux78Flux at a system age of 1.0920E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux79Flux at a system age of 1.1060E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux80Flux at a system age of 1.1200E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux81Flux at a system age of 1.1340E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux82Flux at a system age of 1.1480E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux83Flux at a system age of 1.1620E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux84Flux at a system age of 1.1760E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux85Flux at a system age of 1.1900E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux86Flux at a system age of 1.2040E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux87Flux at a system age of 1.2180E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux88Flux at a system age of 1.2320E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux89Flux at a system age of 1.2460E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux90Flux at a system age of 1.2600E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux91Flux at a system age of 1.2740E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux92Flux at a system age of 1.2880E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux93Flux at a system age of 1.3020E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux94Flux at a system age of 1.3160E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux95Flux at a system age of 1.3300E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux96Flux at a system age of 1.3440E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux97Flux at a system age of 1.3580E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux98Flux at a system age of 1.3720E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux99Flux at a system age of 1.3860E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleFlux100Flux at a system age of 1.4000E+10yrs10mW.m**-2.nm**-1phot.flux.densitydoubleJ/A+A/392/1/saplot1Salpeter IMF isochrone intrinsic colors, part 1SFRStar formation ratesolMass/yrphys.SFRdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (1)phys.abund.ZfloatAgeActual ageyrtime.agedoubleMassSys[1.00E+11] Total mass of systemsolMassphys.massdoubleMassStarTotal mass of stars in systemsolMassphys.massdoubleMassGasTotal mass of gas in systemsolMassphys.massdoubleYHelium abundance, Yphys.abund.YdoubleJ/A+A/392/1/scplot1Scalo IMF isochrone intrinsic colors, part 1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (1)phys.abund.ZfloatAgeActual ageyrtime.agedoubleMassSys[1.00E+11] Total mass of systemsolMassphys.massdoubleMassStarTotal mass of stars in systemsolMassphys.massdoubleMassGasTotal mass of gas in systemsolMassphys.massdoubleYHelium abundance, Yphys.abund.YdoubleSFRStar formation ratesolMass/yrphys.SFRdoubleJ/A+A/392/1/saplot2Salpeter IMF isochrone intrinsic colors, part 2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeActual ageyrtime.agedoublembolBolometric magnitudemagphot.mag.boldoubleUmagJohnson U magnitudemagphot.mag;em.opt.UdoubleBmagJohnson B magnitudemagphot.mag;em.opt.BdoubleVmagJohnson V magnitudemagphot.mag;em.opt.VdoubleRmagJohnson R magnitudemagphot.mag;em.opt.RdoubleImagJohnson I magnitudemagphot.mag;em.opt.IdoubleJmagJohnson J magnitudemagphot.mag;em.IR.JdoubleHmagJohnson H magnitudemagphot.mag;em.IR.HdoubleKmagJohnson K magnitudemagphot.mag;em.IR.KdoubleJ/A+A/392/1/scplot2Scalo IMF isochrone intrinsic colors, part 2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeActual ageyrtime.agedoublembolBolometric magnitudemagphot.mag.boldoubleUmagJohnson U magnitudemagphot.mag;em.opt.UdoubleBmagJohnson B magnitudemagphot.mag;em.opt.BdoubleVmagJohnson V magnitudemagphot.mag;em.opt.VdoubleRmagJohnson R magnitudemagphot.mag;em.opt.RdoubleImagJohnson I magnitudemagphot.mag;em.opt.IdoubleJmagJohnson J magnitudemagphot.mag;em.IR.JdoubleHmagJohnson H magnitudemagphot.mag;em.IR.HdoubleKmagJohnson K magnitudemagphot.mag;em.IR.KdoubleJ/A+A/392/1/saplot3Salpeter IMF isochrone intrinsic colors, part 3recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeActual ageyrtime.agedoubleU-BJohnson color index U-Bmagphot.color;em.opt.U;em.opt.BdoubleB-VJohnson color index B-Vmagphot.color;em.opt.B;em.opt.VdoubleV-RJohnson color index V-Rmagphot.color;em.opt.V;em.opt.RdoubleR-IJohnson color index R-Imagphot.color;em.opt.R;em.opt.IdoubleI-JJohnson color index I-Jmagphot.color;em.IR;em.IRdoubleJ-HJohnson color index J-Hmagphot.color;em.IR.J;em.IR.HdoubleH-KJohnson color index H-Kmagphot.color;em.IR.H;em.IR.KdoubleU-VJohnson color index U-Vmagphot.color;em.opt.U;em.opt.VdoubleV-KJohnson color index V-Kmagphot.color;em.opt.V;em.IR.KdoubleJ/A+A/392/1/scplot3Scalo IMF isochrone intrinsic colors, part 3U-BJohnson color index U-Bmagphot.color;em.opt.U;em.opt.BdoubleB-VJohnson color index B-Vmagphot.color;em.opt.B;em.opt.VdoubleV-RJohnson color index V-Rmagphot.color;em.opt.V;em.opt.RdoubleR-IJohnson color index R-Imagphot.color;em.opt.R;em.opt.IdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeActual ageyrtime.agedoubleI-JJohnson color index I-Jmagphot.color;em.IR;em.IRdoubleJ-HJohnson color index J-Hmagphot.color;em.IR.J;em.IR.HdoubleH-KJohnson color index H-Kmagphot.color;em.IR.H;em.IR.KdoubleU-VJohnson color index U-Vmagphot.color;em.opt.U;em.opt.VdoubleV-KJohnson color index V-Kmagphot.color;em.opt.V;em.IR.KdoubleJ/A+A/392/1/saplot4Salpeter IMF isochrone intrinsic colors, part 4recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeActual ageyrtime.agedoubleLbolbolometric luminositysolLumphys.luminositydoubleLUmagluminosity in UsolLumphys.luminosity;em.optdoubleLBmagluminosity in BsolLumphys.luminosity;em.optdoubleLVmagluminosity in VsolLumphys.luminosity;em.optdoubleLRmagluminosity in RsolLumphys.luminositydoubleLImagluminosity in IsolLumphys.luminosity;em.IRdoubleLJmagluminosity in JsolLumphys.luminosity;em.IRdoubleLHmagluminosity in HsolLumphys.luminosity;em.IRdoubleLKmagluminosity in ksolLumphys.luminosity;em.IRdoubleJ/A+A/392/1/scplot4Scalo IMF isochrone intrinsic colors, part 4recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeActual ageyrtime.agedoubleLbolbolometric luminositysolLumphys.luminositydoubleLUmagluminosity in UsolLumphys.luminosity;em.optdoubleLBmagluminosity in BsolLumphys.luminosity;em.optdoubleLVmagluminosity in VsolLumphys.luminosity;em.optdoubleLRmagluminosity in RsolLumphys.luminositydoubleLImagluminosity in IsolLumphys.luminosity;em.IRdoubleLJmagluminosity in JsolLumphys.luminosity;em.IRdoubleLHmagluminosity in HsolLumphys.luminosity;em.IRdoubleLKmagluminosity in ksolLumphys.luminosity;em.IRdoubleJ/A+A/392/1/scecoeffCoefficients of e-correction in luminosity, Scalo IMFH0Hubble constant value (65 or 75)stat.paramintckve- or k-correction for Koo farith.factordoublecF450We- or k-correction HST F450W <==> B(HDF)arith.factordoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatzRedshiftsrc.redshiftdoublecue- or k-correction for Johnson Uarith.factordoublecbe- or k-correction for Johnson Barith.factordoublecve- or k-correction for Johnson Varith.factordoublecre- or k-correction for Johnson Rmeta.code;phot.colordoublecie- or k-correction for Johnson Iarith.factordoublecje- or k-correction for Johnson Jarith.factordoubleche- or k-correction for Johnson Harith.factordoublecke- or k-correction for Johnson Karith.factordoubleckue- or k-correction for Koo uarith.factordoubleckbe- or k-correction for Koo jarith.factordoubleckre- or k-correction for Koo narith.factordoublecgie- or k-correction for Thuan & gunn garith.factordoublecgje- or k-correction for Thuan & gunn rarith.factordoublecF160BWe- or k-correction HST F160BWarith.factordoublecF170We- or k-correction HST F170Warith.factordoublecF185We- or k-correction HST F185Warith.factordoublecF218We- or k-correction HST F218Warith.factordoublecF255We- or k-correction HST F255Warith.factordoublecF300We- or k-correction HST F300W <==> U(HDF)arith.factordoublecF336We or k-correction HST F336Warith.factordoublecF380We- or k-correction HST F380Warith.factordoublecF439We- or k-correction HST F439Warith.factordoublecF555W? e- or k-correction HST F555W <==> V(YSC)arith.factordoublenullablecF569W? e- or k-correction HST F569Warith.factordoublenullablecF606W? e- or k-correction HST F606W <==> V(HDF)arith.factordoublenullablecF622W? e- or k-correction HST F622Warith.factordoublenullablecF675W? e- or k-correction HST F675Warith.factordoublenullablecF702W? e- or k-correction HST F702Warith.factordoublenullablecF791W? e- or k-correction HST F791Warith.factordoublenullablecF814W? e- or k-correction HST F814W <==> I(HDF)arith.factordoublenullableJ/A+A/392/1/saecoeffCoefficients of e-correction in luminosity, Salpeter IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatH0Hubble constant value (65 or 75)stat.paramintzRedshiftsrc.redshiftdoublecue- or k-correction for Johnson Uarith.factordoublecbe- or k-correction for Johnson Barith.factordoublecve- or k-correction for Johnson Varith.factordoublecre- or k-correction for Johnson Rmeta.code;phot.colordoublecie- or k-correction for Johnson Iarith.factordoublecje- or k-correction for Johnson Jarith.factordoubleche- or k-correction for Johnson Harith.factordoublecke- or k-correction for Johnson Karith.factordoubleckue- or k-correction for Koo uarith.factordoubleckbe- or k-correction for Koo jarith.factordoubleckve- or k-correction for Koo farith.factordoubleckre- or k-correction for Koo narith.factordoublecgie- or k-correction for Thuan & gunn garith.factordoublecgje- or k-correction for Thuan & gunn rarith.factordoublecF160BWe- or k-correction HST F160BWarith.factordoublecF170We- or k-correction HST F170Warith.factordoublecF185We- or k-correction HST F185Warith.factordoublecF218We- or k-correction HST F218Warith.factordoublecF255We- or k-correction HST F255Warith.factordoublecF300We- or k-correction HST F300W <==> U(HDF)arith.factordoublecF336We or k-correction HST F336Warith.factordoublecF380We- or k-correction HST F380Warith.factordoublecF439We- or k-correction HST F439Warith.factordoublecF450We- or k-correction HST F450W <==> B(HDF)arith.factordoublecF555W? e- or k-correction HST F555W <==> V(YSC)arith.factordoublenullablecF569W? e- or k-correction HST F569Warith.factordoublenullablecF606W? e- or k-correction HST F606W <==> V(HDF)arith.factordoublenullablecF622W? e- or k-correction HST F622Warith.factordoublenullablecF675W? e- or k-correction HST F675Warith.factordoublenullablecF702W? e- or k-correction HST F702Warith.factordoublenullablecF791W? e- or k-correction HST F791Warith.factordoublenullablecF814W? e- or k-correction HST F814W <==> I(HDF)arith.factordoublenullableJ/A+A/392/1/sckcoeffCoefficients of k-correction in luminosity, Scalo IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatH0Hubble constant value (65 or 75)stat.paramintzRedshiftsrc.redshiftdoublecue- or k-correction for Johnson Uarith.factordoublecbe- or k-correction for Johnson Barith.factordoublecve- or k-correction for Johnson Varith.factordoublecre- or k-correction for Johnson Rmeta.code;phot.colordoublecie- or k-correction for Johnson Iarith.factordoublecje- or k-correction for Johnson Jarith.factordoubleche- or k-correction for Johnson Harith.factordoublecke- or k-correction for Johnson Karith.factordoubleckue- or k-correction for Koo uarith.factordoubleckbe- or k-correction for Koo jarith.factordoubleckve- or k-correction for Koo farith.factordoubleckre- or k-correction for Koo narith.factordoublecgie- or k-correction for Thuan & gunn garith.factordoublecgje- or k-correction for Thuan & gunn rarith.factordoublecF160BWe- or k-correction HST F160BWarith.factordoublecF170We- or k-correction HST F170Warith.factordoublecF185We- or k-correction HST F185Warith.factordoublecF218We- or k-correction HST F218Warith.factordoublecF255We- or k-correction HST F255Warith.factordoublecF300We- or k-correction HST F300W <==> U(HDF)arith.factordoublecF336We or k-correction HST F336Warith.factordoublecF380We- or k-correction HST F380Warith.factordoublecF439We- or k-correction HST F439Warith.factordoublecF450We- or k-correction HST F450W <==> B(HDF)arith.factordoublecF555W? e- or k-correction HST F555W <==> V(YSC)arith.factordoublenullablecF569W? e- or k-correction HST F569Warith.factordoublenullablecF606W? e- or k-correction HST F606W <==> V(HDF)arith.factordoublenullablecF622W? e- or k-correction HST F622Warith.factordoublenullablecF675W? e- or k-correction HST F675Warith.factordoublenullablecF702W? e- or k-correction HST F702Warith.factordoublenullablecF791W? e- or k-correction HST F791Warith.factordoublenullablecF814W? e- or k-correction HST F814W <==> I(HDF)arith.factordoublenullableJ/A+A/392/1/sakcoeffCoefficients of k-correction in luminosity, Salpeter IMFzRedshiftsrc.redshiftdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatH0Hubble constant value (65 or 75)stat.paramintcue- or k-correction for Johnson Uarith.factordoublecbe- or k-correction for Johnson Barith.factordoublecve- or k-correction for Johnson Varith.factordoublecre- or k-correction for Johnson Rmeta.code;phot.colordoublecie- or k-correction for Johnson Iarith.factordoublecje- or k-correction for Johnson Jarith.factordoubleche- or k-correction for Johnson Harith.factordoublecke- or k-correction for Johnson Karith.factordoubleckue- or k-correction for Koo uarith.factordoubleckbe- or k-correction for Koo jarith.factordoubleckve- or k-correction for Koo farith.factordoubleckre- or k-correction for Koo narith.factordoublecgie- or k-correction for Thuan & gunn garith.factordoublecgje- or k-correction for Thuan & gunn rarith.factordoublecF160BWe- or k-correction HST F160BWarith.factordoublecF170We- or k-correction HST F170Warith.factordoublecF185We- or k-correction HST F185Warith.factordoublecF218We- or k-correction HST F218Warith.factordoublecF255We- or k-correction HST F255Warith.factordoublecF300We- or k-correction HST F300W <==> U(HDF)arith.factordoublecF336We or k-correction HST F336Warith.factordoublecF380We- or k-correction HST F380Warith.factordoublecF439We- or k-correction HST F439Warith.factordoublecF450We- or k-correction HST F450W <==> B(HDF)arith.factordoublecF555W? e- or k-correction HST F555W <==> V(YSC)arith.factordoublenullablecF569W? e- or k-correction HST F569Warith.factordoublenullablecF606W? e- or k-correction HST F606W <==> V(HDF)arith.factordoublenullablecF622W? e- or k-correction HST F622Warith.factordoublenullablecF675W? e- or k-correction HST F675Warith.factordoublenullablecF702W? e- or k-correction HST F702Warith.factordoublenullablecF791W? e- or k-correction HST F791Warith.factordoublenullablecF814W? e- or k-correction HST F814W <==> I(HDF)arith.factordoublenullableJ/A+A/392/1/sckattCoefficients of k-correction with attenuation in luminosity, Scalo IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatH0Hubble constant value (65 or 75)stat.paramintzRedshiftsrc.redshiftdoublecue- or k-correction for Johnson Uarith.factordoublecbe- or k-correction for Johnson Barith.factordoublecve- or k-correction for Johnson Varith.factordoublecre- or k-correction for Johnson Rmeta.code;phot.colordoublecie- or k-correction for Johnson Iarith.factordoublecje- or k-correction for Johnson Jarith.factordoubleche- or k-correction for Johnson Harith.factordoublecke- or k-correction for Johnson Karith.factordoubleckue- or k-correction for Koo uarith.factordoubleckbe- or k-correction for Koo jarith.factordoubleckve- or k-correction for Koo farith.factordoubleckre- or k-correction for Koo narith.factordoublecgie- or k-correction for Thuan & gunn garith.factordoublecgje- or k-correction for Thuan & gunn rarith.factordoublecF160BWe- or k-correction HST F160BWarith.factordoublecF170We- or k-correction HST F170Warith.factordoublecF185We- or k-correction HST F185Warith.factordoublecF218We- or k-correction HST F218Warith.factordoublecF255We- or k-correction HST F255Warith.factordoublecF300We- or k-correction HST F300W <==> U(HDF)arith.factordoublecF336We or k-correction HST F336Warith.factordoublecF380We- or k-correction HST F380Warith.factordoublecF439We- or k-correction HST F439Warith.factordoublecF450We- or k-correction HST F450W <==> B(HDF)arith.factordoublecF555W? e- or k-correction HST F555W <==> V(YSC)arith.factordoublenullablecF569W? e- or k-correction HST F569Warith.factordoublenullablecF606W? e- or k-correction HST F606W <==> V(HDF)arith.factordoublenullablecF622W? e- or k-correction HST F622Warith.factordoublenullablecF675W? e- or k-correction HST F675Warith.factordoublenullablecF702W? e- or k-correction HST F702Warith.factordoublenullablecF791W? e- or k-correction HST F791Warith.factordoublenullablecF814W? e- or k-correction HST F814W <==> I(HDF)arith.factordoublenullableJ/A+A/392/1/sakattCoefficients of k-correction with attenuation in luminosity, Salpeter IMFzRedshiftsrc.redshiftdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatH0Hubble constant value (65 or 75)stat.paramintcue- or k-correction for Johnson Uarith.factordoublecbe- or k-correction for Johnson Barith.factordoublecve- or k-correction for Johnson Varith.factordoublecre- or k-correction for Johnson Rmeta.code;phot.colordoublecie- or k-correction for Johnson Iarith.factordoublecje- or k-correction for Johnson Jarith.factordoubleche- or k-correction for Johnson Harith.factordoublecke- or k-correction for Johnson Karith.factordoubleckue- or k-correction for Koo uarith.factordoubleckbe- or k-correction for Koo jarith.factordoubleckve- or k-correction for Koo farith.factordoubleckre- or k-correction for Koo narith.factordoublecgie- or k-correction for Thuan & gunn garith.factordoublecgje- or k-correction for Thuan & gunn rarith.factordoublecF160BWe- or k-correction HST F160BWarith.factordoublecF170We- or k-correction HST F170Warith.factordoublecF185We- or k-correction HST F185Warith.factordoublecF218We- or k-correction HST F218Warith.factordoublecF255We- or k-correction HST F255Warith.factordoublecF300We- or k-correction HST F300W <==> U(HDF)arith.factordoublecF336We or k-correction HST F336Warith.factordoublecF380We- or k-correction HST F380Warith.factordoublecF439We- or k-correction HST F439Warith.factordoublecF450We- or k-correction HST F450W <==> B(HDF)arith.factordoublecF555W? e- or k-correction HST F555W <==> V(YSC)arith.factordoublenullablecF569W? e- or k-correction HST F569Warith.factordoublenullablecF606W? e- or k-correction HST F606W <==> V(HDF)arith.factordoublenullablecF622W? e- or k-correction HST F622Warith.factordoublenullablecF675W? e- or k-correction HST F675Warith.factordoublenullablecF702W? e- or k-correction HST F702Warith.factordoublenullablecF791W? e- or k-correction HST F791Warith.factordoublenullablecF814W? e- or k-correction HST F814W <==> I(HDF)arith.factordoublenullableJ/A+A/392/1/sahstLuminosities from the spectra in HST filter-system, Salpeter IMFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity (0.0004 0.004 0.008 0.02 0.05)phys.abund.ZfloatAgeAge of systemyrtime.agedoubleF160BWHST F160BW magnitudemagphot.mag;em.UV.100-200nmdoubleF170WHST F170W magnitudemagphot.mag;em.UV.100-200nmdoubleF185WHST F185W magnitudemagphot.mag;em.UV.100-200nmdoubleF218WHST F218W magnitudemagphot.mag;em.UV.200-300nmdoubleF255WHST F255W magnitudemagphot.mag;em.UV.200-300nmdoubleF300WHST F300W = U(HDF) magnitudemagphot.mag;em.opt.UdoubleF336WHST F336W magnitudemagphot.mag;em.opt.UdoubleF380WHST F380W magnitudemagphot.mag;em.opt.UdoubleF439WHST F439W magnitudemagphot.mag;em.opt.BdoubleF450WHST F450W = B(HDF) magnitudemagphot.mag;em.opt.BdoubleF555WHST F555W = V(YSC) magnitudemagphot.mag;em.opt.VdoubleF569WHST F569W magnitudemagphot.mag;em.opt.VdoubleF606WHST F606W = V(HDF) magnitudemagphot.mag;em.opt.RdoubleF622WHST F622W magnitudemagphot.mag;em.opt.RdoubleF675WHST F675W magnitudemagphot.mag;em.opt.RdoubleF702WHST F702W magnitudemagphot.mag;em.opt.RdoubleF791WHST F791W magnitudemagphot.mag;em.opt.IdoubleF814WHST F814W = I(HDF) magnitudemagphot.mag;em.opt.Idouble