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<ri:Resource created="2016-02-23T15:37:49Z" 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>Transit metric for Q1-Q17 Kepler candidates</title><shortName>J/ApJ/812/46</shortName><identifier>ivo://CDS.VizieR/J/ApJ/812/46</identifier><altIdentifier>doi:10.26093/cds/vizier.18120046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Thompson S.E.</name></creator><creator><name>Mullally F.</name></creator><creator><name>Coughlin J.</name></creator><creator><name>Christiansen J.L.</name></creator><creator><name>Henze C.E.,Haas M.R.</name></creator><creator><name>Burke C.J.</name></creator><date role="Updated">2017-12-22T05:33:04Z</date><date role="Created">2016-02-23T15:37:49Z</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>solar-system-planets</subject><subject>multiple-stars</subject><description>We describe a new metric that uses machine learning to determine if a periodic signal found in a photometric time series appears to be shaped like the signature of a transiting exoplanet. This metric uses dimensionality reduction and k-nearest neighbors to determine whether a given signal is sufficiently similar to known transits in the same data set. This metric is being used by the Kepler Robovetter to determine which signals should be part of the Q1-Q17 DR24 catalog of planetary candidates. The Kepler Mission reports roughly 20000 potential transiting signals with each run of its pipeline, yet only a few thousand appear to be sufficiently transit shaped to be part of the catalog. The other signals tend to be variable stars and instrumental noise. With this metric, we are able to remove more than 90% of the non-transiting signals while retaining more than 99% of the known planet candidates. When tested with injected transits, less than 1% are lost. This metric will enable the Kepler mission and future missions looking for transiting planets to rapidly and consistently find the best planetary candidates for follow-up and cataloging.</description><source format="bibcode">2015ApJ...812...46T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/812/46</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/810/95">J/ApJ/810/95 : Kepler pipeline S/N studies. II. 2011 (Christiansen+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/809/8">J/ApJ/809/8 : Terrestrial planet occurrence rates for KOIs (Burke+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/45">J/ApJ/807/45 : Potentially habitable planets around M dwarfs (Dressing+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/31">J/ApJS/217/31 : Kepler planetary candidates. VI. 4yr Q1-Q16 (Mullally+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/18">J/ApJS/217/18 : Potential transit signals in Kepler Q1-Q17 (Seader+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/16">J/ApJS/217/16 : Kepler planetary candidates. V. 3yr Q1-Q12 (Rowe+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/19">J/ApJS/210/19 : Kepler planetary candidates. IV. 22 months (Burke+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/35">J/ApJS/207/35 : Kepler pipeline signal-to-noise studies (Christiansen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. III. (Batalha+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/24">J/ApJS/199/24 : The first three quarters of Kepler mission (Tenenbaum+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/160">J/AJ/142/160 : Kepler Mission. II. eclipsing binaries (Slawson+, 2011)</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/ApJ/736/19">J/ApJ/736/19 : Kepler planetary candidates. II. (Borucki+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/83">J/AJ/141/83 : Eclipsing binaries in Kepler first data release (Prsa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/117">J/ApJ/728/117 : Kepler planetary candidates. I. 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