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<ri:Resource created="2009-09-20T11:13:26Z" 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>Six transits of the exoplanet XO-2b</title><shortName>J/AJ/137/4911</shortName><identifier>ivo://CDS.VizieR/J/AJ/137/4911</identifier><altIdentifier>doi:10.26093/cds/vizier.51374911</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fernandez J.M.</name></creator><creator><name>Holman M.J.</name></creator><creator><name>Winn J.N.</name></creator><creator><name>Torres G.</name></creator><creator><name>Shporer A.</name></creator><creator><name>Mazeh T.,Esquerdo G.A.</name></creator><creator><name>Everett M.E.</name></creator><date role="Updated">2009-09-20T11:20:06Z</date><date role="Created">2009-09-20T11:13:26Z</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>variable-stars</subject><subject>solar-system-planets</subject><subject>photometry</subject><description>We present photometry of six transits of the exoplanet XO-2b. By combining the light-curve analysis with theoretical isochrones to determine the stellar properties, we find the planetary radius to be 0.996^+0.031^_-0.018_R_Jup_ and the planetary mass to be 0.565+/-0.054M_Jup_. These results are consistent with those reported previously, and are also consistent with theoretical models for gas giant planets. The midtransit times are accurate to within 1 minute and are consistent with a constant period. However, the period we derive differs by 2.5{sigma } from the previously published period. More data are needed to tell whether the period is actually variable (as it would be in the presence of an additional body) or if the timing errors have been underestimated.</description><source format="bibcode">2009AJ....137.4911F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/137/4911</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/ApJ/652/1715">J/ApJ/652/1715 : Four transits of the exoplanet XO-1b (Holman+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/11">J/AJ/133/11 : Photometry of OGLE-TR 111 (Winn+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/657/1098">J/ApJ/657/1098 : Transit of TrES-1 (Winn+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/655/1103">J/ApJ/655/1103 : Five transits of the exoplanet OGLE-TR-10b (Holman+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1828">J/AJ/133/1828 : Transit light curves of HD 189733 (Winn+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/664/1185">J/ApJ/664/1185 : Three transits of the exoplanet TrES-2 (Holman+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/1707">J/AJ/134/1707 : Six transit of exoplanet HAT-P-1b (Winn+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/267">J/AJ/136/267 : Six occultations of the exoplanet TrES-3 (Winn+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/683/1076">J/ApJ/683/1076 : Transits of exoplanet XO-3b (Winn+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/693/794">J/ApJ/693/794 : Transit of exoplanet HD 17156b (Winn+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3826">J/AJ/137/3826 : Two transits of the giant planet WASP-4b (Winn+, 2009)</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/137/4911</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/137/4911</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/137/4911</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/137/4911</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/137/4911</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/137/4911</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"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/137/4911/table2</name><description>Transit light curve</description><column><name>Rflux</name><description>Relative flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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