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<ri:Resource created="2006-01-28T12:19:49Z" 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>The planet-metallicity correlation.</title><shortName>J/ApJ/622/1102</shortName><identifier>ivo://CDS.VizieR/J/ApJ/622/1102</identifier><altIdentifier>doi:10.26093/cds/vizier.16221102</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fischer D.A.</name></creator><creator><name>Valenti J.</name></creator><date role="Updated">2017-12-15T10:55:15Z</date><date role="Created">2006-01-28T12:19:49Z</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>chemical-abundances</subject><subject>f-stars</subject><subject>solar-system-planets</subject><description>We have recently carried out spectral synthesis modeling to determine T_eff_, log(g), vsin(i), and [Fe/H] for 1040 FGK-type stars on the Keck, Lick, and Anglo-Australian Telescope planet search programs. This is the first time that a single, uniform spectroscopic analysis has been made for every star on a large Doppler planet search survey. We identify a subset of 850 stars that have Doppler observations sufficient to detect uniformly all planets with radial velocity semiamplitudes K&gt;30m/s and orbital periods shorter than 4yr.</description><source format="bibcode">2005ApJ...622.1102F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/622/1102</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/A+A/398/363">J/A+A/398/363 : Statistical properties of exoplanets II (Santos+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/415/1153">J/A+A/415/1153 : [Fe/H] for 98 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