<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2010-02-01T06:20:24Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>PopStar I: Evolutionary synthesis models</title><shortName>J/MNRAS/398/451</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/398/451</identifier><altIdentifier>doi:10.26093/cds/vizier.73980451</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Molla M.</name></creator><creator><name>Garcia-Vargas M.L.,Bressan</name></creator><creator><name>A.</name></creator><date role="Updated">2024-07-09T20:15:44Z</date><date role="Created">2010-02-01T06:20:24Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>stellar-evolutionary-models</subject><subject>line-intensities</subject><subject>photometry</subject><description>We present new evolutionary synthesis models for Simple Stellar Populations for a wide range of ages and metallicities. The models are based on the Padova isochrones. The core of the spectral library is provided by the medium resolution Lejeune et al. atmosphere models. These spectra are complemented by NLTE atmosphere models for hot stars that have an important impact in the stellar cluster's ionizing spectra: O, B and WR stellar spectra at the early ages, and spectra of post-AGB stars and planetary nebulae, at intermediate and old ages. At young ages, our models compare well with other existing models but we find that, the inclusion of the nebular continuum, not considered in several other models, reddens significantly the integrated colours of very young stellar populations. This is consistent with the results of spectral synthesis codes particularly devised for the study of starburst galaxies. At intermediate and old ages, the agreement with literature model is good and, in particular, we reproduce well the observed colours of star clusters in LMC. Given the ability to produce good integrated spectra from the far-UV to the infrared at any age, we consider that our models are particularly suited for the study of high redshift galaxies. These models are available on the web site http://www.fractal-es.com/SEDmod.htm and also through the Virtual Observatory Tools on the PopStar server.</description><source format="bibcode">2009MNRAS.398..451M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/398/451</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/398/451</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/398/451</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/398/451</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/398/451</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/398/451</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/398/451</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/398/451/PopStar1</name><description>Results of models: types of stars, energy, Ionizing photons, H{alpha} and H{beta} lines, synthetic magnitudes</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>IMF</name><description>Initial Mass Function Type (G1)</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Mlow</name><description>Low mass limit of the IMF</description><unit>solMass</unit><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mup</name><description>Upper mass limit of the IMF</description><unit>solMass</unit><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Z</name><description>Metallicity of stellar populations</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logAge</name><description>Age of each SSP in logarithmic scale</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nmas</name><description>Number of massive stars (M&gt;20M_{sun}_) (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NOB</name><description>Number of OB stars (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NWN</name><description>Number of WN-WR stars (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NWC</name><description>Number of WC-WR stars (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NRSG</name><description>Number of Red SuperGiant stars (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NSNII</name><description>Number of type II supernovae (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NPN</name><description>Number of planetary nebula (G2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ESN</name><description>Mechanical energy ejected by SNs</description><unit>1e+40J</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ewind</name><description>Mechanical energy ejected by massive star winds</description><unit>1e+40J</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Etot</name><description>Total energy injected in the star cluster</description><unit>1e+40J</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rpc</name><description>Radius of the HII region</description><unit>pc</unit><ucd>phys.size.radius;obs.field</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logQ(HeII)</name><description>logarithmic of the ionizing photons for HeII</description><unit>log(s**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logQ(OI)</name><description>logarithmic of the ionizing photons for OI</description><unit>log(s**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logQ(HeI)</name><description>logarithmic of the ionizing photons for HeI</description><unit>log(s**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logQ(H)</name><description>logarithmic of the ionizing photons for HI</description><unit>log(s**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>IHb:e</name><description>Luminosity H{beta} in emission</description><unit>solLum</unit><ucd>phys.luminosity;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IHb:a</name><description>Luminosity H{beta} in absorption</description><unit>solLum</unit><ucd>phys.luminosity;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ScHb</name><description>Luminosity of the Continuum around H{beta} (in L{sun}/{AA})</description><unit>10solLum/nm</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EWHb:e</name><description>Equivalent width of H{beta} line in emission</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EWHb:a</name><description>Equivalent width of H{beta} line in absorption</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EWHb</name><description>Total Equivalent width of H{beta} line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IHa:e</name><description>Luminosity H{alpha} in emission</description><unit>solLum</unit><ucd>phys.luminosity;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IHa:a</name><description>Luminosity H{alpha} in absorption</description><unit>solLum</unit><ucd>phys.luminosity;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ScHa</name><description>Luminosity of the Continuum around H{alpha} (in L{sun}/{AA})</description><unit>10solLum/nm</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EWHa:e</name><description>Equivalent width of H{alpha} line in emission</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EWHa:a</name><description>Equivalent width of H{alpha} line in absorption</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EWHa</name><description>Total Equivalent width of H{alpha} line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>UV1MAG</name><description>Absolute magnitude UV1 in HST system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>UV2MAG</name><description>Absolute magnitude UV2 in HST system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>UMAG</name><description>Absolute magnitude U in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B1MAG</name><description>Absolute magnitude B in the Johnson System (1)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B2MAG</name><description>Absolute magnitude B in the Johnson System (1)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VMAG</name><description>Absolute magnitude V in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RMAG</name><description>Absolute magnitude R in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>IMAG</name><description>Absolute magnitude I in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>JMAG</name><description>Absolute magnitude J in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HMAG</name><description>Absolute magnitude H in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KMAG</name><description>Absolute magnitude K in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LMAG</name><description>Absolute magnitude L in the Johnson System</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>uMAG</name><description>Absolute magnitude u in SDSS system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>gMAG</name><description>Absolute magnitude g in SDSS system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rMAG</name><description>Absolute magnitude r in SDSS system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>iMAG</name><description>Absolute magnitude i in SDSS system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zMAG</name><description>Absolute magnitude z in SDSS system</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plot</name><description>Plot the evolution for this model</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/398/451/ages</name><description>Ages for which there are a table HR</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logAge</name><description>Logarithm of the age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FileName.0001</name><description>Name of the file in subdirectory z0.0001</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>FileName.0004</name><description>Name of the file in subdirectory z0.0004</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>FileName.0040</name><description>Name of the file in subdirectory z0.0040</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>FileName.0080</name><description>Name of the file in subdirectory z0.0080</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>FileName.0200</name><description>Name of the file in subdirectory z0.0200</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>FileName.0500</name><description>Name of the file in subdirectory z0.0500</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column></table></schema></tableset></ri:Resource>