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<ri:Resource created="2012-10-22T12:52:29Z" 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>Transits of OGLE-TR-132b</title><shortName>J/ApJ/728/125</shortName><identifier>ivo://CDS.VizieR/J/ApJ/728/125</identifier><altIdentifier>doi:10.26093/cds/vizier.17280125</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Adams E.R.</name></creator><creator><name>Lopez-Morales M.</name></creator><creator><name>Elliot J.L.</name></creator><creator><name>Seager S.</name></creator><creator><name>Osip D.J.</name></creator><date role="Updated">2017-06-28T06:57:56Z</date><date role="Created">2012-10-22T12:52:29Z</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><subject>photometry</subject><description>We report the results of the first transit timing variation analysis of the very hot Jupiter OGLE-TR-132b, using 10 transits collected over a seven-year period. Our analysis combines three previously published transit light curves with seven new transits, which were observed between 2008 February and 2009 May with the new MagIC-e2V instrument on the Magellan Telescopes in Chile. We provide a revised planetary radius of R_p_=1.23+/-0.07R_J_, which is slightly larger, but consistent within the errors, than that given by previously published results. Analysis of the planet-to-star radius ratio, orbital separation, inclination, and transit duration reveals no apparent variation in any of those parameters during the time span observed. We also find no sign of transit timing variations larger than -108+/-49s, with most residuals very close to zero. This allows us to place an upper limit of 5-10M_{earth}_ for a coplanar, low-eccentricity perturber in either the 2:1 or 3:2 mean-motion resonance with OGLE-TR-132b. We similarly find that the data are entirely consistent with a constant orbital period and there is no evidence for orbital decay within the limits of precision of our data.</description><source format="bibcode">2011ApJ...728..125A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/728/125</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/II/278">II/278 : Transits observed in OGLE 2001-2003 (Udalski+, 2002-2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/1336">J/ApJ/716/1336 : Stability analysis of single-planet (Kopparapu+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/L9">J/ApJ/692/L9 : Tidal evolution of transiting extrasolar planets (Levrard+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/466/743">J/A+A/466/743 : Transiting planet OGLE-TR-132b (Gillon+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/475/359">J/A+A/475/359 : Predicting radio fluxes of extrasolar planets (Griessmeier+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/458/997">J/A+A/458/997 : Abundances for 6 transiting planet host stars (Santos+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/424/L31">J/A+A/424/L31 : Transiting exoplanet OGLE-TR-132b (Moutou+, 2004)</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/ApJ/728/125</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/728/125</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/728/125</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/728/125</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/728/125</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/728/125</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/ApJ/728/125/table3</name><description>Flux values for seven transits of OGLE-TR-132b</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>JD</name><description>Mid-exposure Julian Date; UTC</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BJD</name><description>Mid-exposure Baryocentric Julian Date; TDB corrected</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Normalized stellar flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>The RMS error in NFlux</description><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>