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<ri:Resource created="2008-03-09T21:51:22Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>alpha-enhanced integrated Lick/IDS spectral indices</title><shortName>J/ApJS/160/176</shortName><identifier>ivo://CDS.VizieR/J/ApJS/160/176</identifier><altIdentifier>doi:10.26093/cds/vizier.21600176</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lee H.-C.</name></creator><creator><name>Worthey G.</name></creator><date role="Updated">2017-10-16T14:58:30Z</date><date role="Created">2008-03-09T21:51:22Z</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>globular-star-clusters</subject><subject>spectroscopy</subject><description>All 25 Lick/IDS spectral indices have been computed for the integrated light of simple stellar populations over broad ranges of age and metallicity and with effects from horizontal-branch stars fully implemented. Our models employ {alpha}-enhanced isochrones at the sub-solar metallicity regime, but solar-scaled ones at solar and super-solar metallicity. We have also employed the updated response functions of Houdashelt et al. (2002AAS...201.1405H) at the solar and super-solar metallicity regime, so that we could assess the light-element enhancement phenomena seen from metal-rich early-type galaxies.</description><source format="bibcode">2005ApJS..160..176L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/160/176</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/111/377">J/ApJS/111/377 : H{gamma} + H{delta} absorption features (Worthey+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/94/687">J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/116/1">J/ApJS/116/1 : Old Stellar Populations. VI. 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