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<ri:Resource created="2019-11-06T07:45:08Z" 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>Kepler-13AB aperture photometry</title><shortName>J/AJ/158/113</shortName><identifier>ivo://CDS.VizieR/J/AJ/158/113</identifier><altIdentifier>doi:10.26093/cds/vizier.51580113</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Howell S.B.</name></creator><creator><name>Scott N.J.</name></creator><creator><name>Matson R.A.</name></creator><creator><name>Horch E.P.</name></creator><creator><name>Stephens A.</name></creator><date role="Updated">2019-11-06T06:50:24Z</date><date role="Created">2019-11-06T07:45:08Z</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>photometry</subject><subject>visible-astronomy</subject><subject>exoplanets</subject><description>Using the high-resolution imaging instrument, 'Alopeke, at the Gemini-N telescope, we obtained simultaneous two-channel time-series observations of the binary exoplanet host star Kepler13-AB. Our optical observations were obtained during a transit event of the exoplanet Kepler-13b and light curves were produced using both speckle interferometric and aperture photometry techniques. Both techniques confirm that the transiting object orbits the star Kepler-13A while different transit depths are seen across the optical wavelength range, being ~2 times deeper in the blue. These measurements, as well as mass determinations in the literature, are consistent with Kepler-13b being a highly irradiated gas giant with a bloated atmosphere. Our observations highlight the ability of high-resolution speckle imaging to not only assess binarity in exoplanet host stars but robustly determine which of the stars the transiting object actually orbits.</description><source format="bibcode">2019AJ....158..113H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/158/113</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/A+A/544/L12">J/A+A/544/L12 : Velocitometry transit of KOI-13 (Santerne+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/92">J/ApJ/788/92 : The hot Jupiter Kepler-13Ab planet's occultation</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/AJ/153/71">J/AJ/153/71 : Kepler follow-up observation program. I. Imaging</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/158/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/158/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/158/113</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/158/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/158/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/158/113</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/158/113/table3</name><description>Kepler-13AB aperture photometry</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Band</name><description>[562/832] Waveband</description><unit>nm</unit><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Time</name><description>[8.88/12.58]? Mean UT time</description><unit>h</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dmag</name><description>[-0.2/-0.1224]? Differential magnitude in Band</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Dmag</name><description>[0.0028/0.0065]? 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