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<ri:Resource created="2011-11-06T18:04:47Z" 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>Stellar population trends in S0 galaxies</title><shortName>J/MNRAS/412/423</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/412/423</identifier><altIdentifier>doi:10.26093/cds/vizier.74120423</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chamberlain L.C.P.</name></creator><creator><name>Courteau S.</name></creator><creator><name>McDonald M.</name></creator><creator><name>Rose J.A.</name></creator><date role="Updated">2024-07-13T20:15:01Z</date><date role="Created">2011-11-06T18:04:47Z</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>galaxies</subject><subject>photometry</subject><subject>galaxy-classification-systems</subject><subject>chemical-abundances</subject><description>We present stellar population age and metallicity trends for a sample of 59 S0 galaxies based on optical Sloan Digital Sky Survey (SDSS) and near-infrared (NIR) J and H photometry. When combined with optical g and r passband imaging data from the SDSS archive and stellar population models, we obtain radial age and metallicity trends out to at least five effective radii for most of the galaxies in our sample. 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