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<ri:Resource created="2016-01-11T12:52:34Z" 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>Terrestrial planet occurrence rates for KOI stars</title><shortName>J/ApJ/809/8</shortName><identifier>ivo://CDS.VizieR/J/ApJ/809/8</identifier><altIdentifier>doi:10.26093/cds/vizier.18090008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Burke C.J.</name></creator><creator><name>Christiansen J.L.</name></creator><creator><name>Mullally F.</name></creator><creator><name>Seader S.</name></creator><creator><name>Huber D.</name></creator><creator><name>Rowe J.F.,Coughlin J.L.</name></creator><creator><name>Thompson S.E.</name></creator><creator><name>Catanzarite J.</name></creator><creator><name>Clarke B.D.</name></creator><creator><name>Morton T.D.,Caldwell D.A.</name></creator><creator><name>Bryson S.T.</name></creator><creator><name>Haas M.R.</name></creator><creator><name>Batalha N.M.</name></creator><creator><name>Jenkins J.M.,Tenenbaum P.</name></creator><creator><name>Twicken J.D.</name></creator><creator><name>Li J.</name></creator><creator><name>Quintana E.</name></creator><creator><name>Barclay T.</name></creator><creator><name>Henze C.E.,Borucki W.J.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Still M.</name></creator><date role="Updated">2017-10-09T13:34:44Z</date><date role="Created">2016-01-11T12:52:34Z</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>multiple-stars</subject><subject>solar-system-planets</subject><description>We measure planet occurrence rates using the planet candidates discovered by the Q1-Q16 Kepler pipeline search. This study examines planet occurrence rates for the Kepler GK dwarf target sample for planet radii, 0.75&lt;=Rp&lt;=2.5R_{Earth}_, and orbital periods, 50&lt;=Porb&lt;=300days, with an emphasis on a thorough exploration and identification of the most important sources of systematic uncertainties. Integrating over this parameter space, we measure an occurrence rate of F_0_=0.77 planets per star, with an allowed range of 0.3&lt;=F0&lt;=1.9. The allowed range takes into account both statistical and systematic uncertainties, and values of F_0_ beyond the allowed range are significantly in disagreement with our analysis. We generally find higher planet occurrence rates and a steeper increase in planet occurrence rates toward small planets than previous studies of the Kepler GK dwarf sample. Through extrapolation, we find that the one year orbital period terrestrial planet occurrence rate {zeta}_1.0_=0.1, with an allowed range of 0.01&lt;={zeta}_1.0_&lt;=2, where {zeta}_1.0_ is defined as the number of planets per star within 20% of the Rp and Porb of Earth. For G dwarf hosts, the {zeta}_1.0_ parameter space is a subset of the larger {eta}_{Earth}_ parameter space, thus {zeta}_1.0_ places a lower limit on {eta}_{Earth}_ for G dwarf hosts. From our analysis, we identify the leading sources of systematics impacting Kepler occurrence rate determinations as reliability of the planet candidate sample, planet radii, pipeline completeness, and stellar parameters.</description><source format="bibcode">2015ApJ...809....8B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/809/8</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/ApJ/808/194">J/ApJ/808/194 : Performance of exoplanet search space missions (Leger+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/45">J/ApJ/807/45 : Habitable zones around M dwarfs (Dressing+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/183">J/ApJ/806/183 : Planet radii of Kepler Object of Interest (Wolfgang+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/31">J/ApJS/217/31 : Kepler planetary candidates. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>KIC</name><description>Kepler identification number of the star</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>KOI</name><description>[12.01/6251.01] Kepler Object of Interest</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Base</name><description>In Baseline sample (1:True)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ori</name><description>In Original KIC sample (1:True)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>High</name><description>In High reliability sample (1:True)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Full</name><description>In Full long period sample (1:True)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Trim</name><description>In Trimmed long period sample (1:True)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from exoplanet archive (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from exoplanet archive (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/809/8/table4</name><description>Planet distribution function (PLDF) model parameter posterior samples</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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