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<ri:Resource created="2015-12-24T14:14:23Z" 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>Metallicities of KIC stars without planets</title><shortName>J/ApJ/808/187</shortName><identifier>ivo://CDS.VizieR/J/ApJ/808/187</identifier><altIdentifier>doi:10.26093/cds/vizier.18080187</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Buchhave L.A.</name></creator><creator><name>Latham D.W.</name></creator><date role="Updated">2017-12-07T07:27:46Z</date><date role="Created">2015-12-24T14:14:23Z</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>dwarf-stars</subject><description>Host star metallicities have been used to infer observational constraints on planet formation throughout the history of the exoplanet field. The giant planet metallicity correlation has now been widely accepted, but questions remain as to whether the metallicity correlation extends to the small terrestrial-sized planets. Here, we report metallicities for a sample of 518 stars in the Kepler field that have no detected transiting planets and compare their metallicity distribution to a sample of stars that hosts small planets (Rp&lt;1.7R_{Earth}_). Importantly, both samples have been analyzed in a homogeneous manner using the same set of tools (Stellar Parameters Classification tool). We find the average metallicity of the sample of stars without detected transiting planets to be [m/H]_SNTP,dwarf_=-0.02+/-0.02dex and the sample of stars hosting small planets to be [m/H]_STP_=-0.02+/-0.02dex. The average metallicities of the two samples are indistinguishable within the uncertainties, and the two-sample Kolmogorov-Smirnov test yields a p-value of 0.68 (0.41{sigma}), indicating a failure to reject the null hypothesis that the two samples are drawn from the same parent population. We conclude that the homogeneous analysis of the data presented here supports the hypothesis that stars hosting small planets have a metallicity similar to stars with no known transiting planets in the same area of the sky.</description><source format="bibcode">2015ApJ...808..187B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/808/187</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/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/1">J/ApJS/210/1 : Asteroseismic study of solar-type stars (Chaplin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/107">J/ApJ/771/107 : Spectroscopy of faint KOI stars (Everett+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/95">J/ApJ/767/95 : Improved parameters of smallest KIC stars (Dressing+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A36">J/A+A/551/A36 : Metallicity of M dwarfs. III. (Neves+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A109">J/A+A/549/A109 : HARPS XXXI. The M-dwarf sample (Bonfils+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/161">J/ApJ/757/161 : Spectroscopy of 56 exoplanet host stars (Torres+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/486.375">J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/112">J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A141">J/A+A/533/A141 : Stellar parameters for 582 HARPS FGK stars (Sousa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. (Fischer+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/415/1153">J/A+A/415/1153 : [Fe/H] for 98 extra-solar planet-host stars (Santos+, 2004)</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/ApJ/808/187</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/808/187</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/808/187</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/808/187</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/808/187</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/808/187</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/808/187/table1 (Metallicities of stars with no detected transiting planets)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/808/187/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/808/187/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/808/187/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>290.8884325</ra><dec>37.0893706</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>4/923 935 5/3645 3646 3647 3690 3706 3732 3733 3734 3776 3779 3780 3782 3783 3785 3786 3792 6/14573 14575 14577 14578 14579 14733 14734 14735 14738 14744 14746 14751 14752 14753 14754 14756 14757 14759 14765 14766 14767 14792 14794 14816 14818 14819 14828 14830 14915 14917 14918 14919 14921 14923 14924 14925 14926 14941 14942 14943 14945 14946 14947 14948 14950 14951 14952 14953 14955 14956 14958 14959 15041 15044 15057 15060 15061 15062 15108 15109 15110 15112 15113 15115 15124 15126 15127 15136 15137 15138 15149 15153 15155 15156 15157 15158 15172 15173 15174 15178 15200 15232</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/808/187?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/808/187/table1</name><description>Metallicities of stars with no detected transiting planets</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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