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<ri:Resource created="2007-01-03T15:37:33Z" 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 parameters of metal-rich solar-type stars</title><shortName>J/A+A/458/873</shortName><identifier>ivo://CDS.VizieR/J/A+A/458/873</identifier><altIdentifier>doi:10.26093/cds/vizier.34580873</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sousa S.G.</name></creator><creator><name>Santos N.C.</name></creator><creator><name>Israelian G.</name></creator><creator><name>Mayor M.</name></creator><creator><name>Monteiro M.J.P.F.G.</name></creator><date role="Updated">2017-11-10T11:16:22Z</date><date role="Created">2007-01-03T15:37:33Z</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>g-stars</subject><subject>solar-system-planets</subject><subject>chemical-abundances</subject><description>To date, metallicity is the only parameter of a star that appears to clearly correlate with the presence of planets and their properties. To check for new correlations between stars and the existence of an orbiting planet, we determine accurate stellar parameters for several metal-rich solar-type stars. 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