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<ri:Resource created="2021-12-08T08:34:17Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Searching for Small Circumbinary Planets. I. STANLEY</title><shortName>J/AJ/162/84</shortName><identifier>ivo://CDS.VizieR/J/AJ/162/84</identifier><altIdentifier>doi:10.26093/cds/vizier.51620084</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Martin D.V.</name></creator><creator><name>Fabrycky D.C.</name></creator><date role="Updated">2022-03-16T11:40:27Z</date><date role="Created">2021-12-08T08:34:17Z</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>exoplanets</subject><subject>multiple-stars</subject><subject>eclipsing-binary-stars</subject><description>No circumbinary planets have been discovered smaller than 3R{Earth}, yet planets of this small size comprise over 75% of the discoveries around single stars. The observations do not prove the nonexistence of small circumbinary planets; rather, they are much harder to find than around single stars because their transit timing variations are much larger than the transit durations. We present Stanley, an automated algorithm to find small circumbinary planets. It employs custom methods to detrend eclipsing binary light curves and stack shallow transits of variable duration and interval using N-body integrations. Applied to the Kepler circumbinaries, we recover all known planets, including the three planets of Kepler-47, and constrain the absence of additional planets of similar or smaller size. We also show that we could have detected &lt;3R{Earth} planets in half of the known systems. Our work will ultimately be applied to a broad sample of eclipsing binaries to (hopefully) produce new discoveries and derive a circumbinary size distribution that can be compared to that for single stars.</description><source format="bibcode">2021AJ....162...84M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/162/84</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/83">J/AJ/141/83 : Kepler Mission. I. Eclipsing binaries in DR1 (Prsa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/337.1511">J/other/Sci/337.1511 : Kepler-47 transits (Orosz+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/761/123">J/ApJ/761/123 : KELT-1 photometry and spectroscopy follow-up (Siverd+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/481.475">J/other/Nat/481.475 : Rvel of Kepler-34b &amp; Kepler-35b (Welsh+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/127">J/ApJ/768/127 : Q1-11 Kepler light curve of KIC 4862625 (Schwamb+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/561/A138">J/A+A/561/A138 : Transiting planets Matlab/Octave source code (Ofir+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/45">J/ApJ/807/45 : Habitable planets orbiting M dwarfs (Dressing+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/68">J/AJ/151/68 : Kepler Mission. VII. Eclipsing binaries in DR3 (Kirk+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/109">J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/602/A117">J/A+A/602/A117 : Periods of 2290 CoRoT binaries (Klagyivik+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/216">J/AJ/154/216 : Rvel of 41 Kepler eclipsing binaries (Matson+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/78">J/AJ/156/78 : 44 validated planets from K2 Campaign 10 (Livingston+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/174">J/AJ/157/174 : Transiting planets in Kepler-47 circumb. system (Orosz+, 2019)</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/AJ/162/84</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/162/84</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/162/84</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/162/84</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/162/84</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/162/84</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/AJ/162/84/fig5</name><description>*Common false positive times</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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