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<ri:Resource created="2012-01-12T09:22:58Z" status="active" updated="2026-05-19T14:25:37Z" 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>HAT-P-12 light curve</title><shortName>J/ApJ/706/785</shortName><identifier>ivo://CDS.VizieR/J/ApJ/706/785</identifier><altIdentifier>doi:10.26093/cds/vizier.17060785</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hartman J.D.</name></creator><creator><name>Bakos G.A.</name></creator><creator><name>Torres G.</name></creator><creator><name>Kovacs G.</name></creator><creator><name>Noyes R.W.</name></creator><creator><name>Pal A.,Latham D.W.</name></creator><creator><name>Sipocz B.</name></creator><creator><name>Fischer D.A.</name></creator><creator><name>Johnson J.A.</name></creator><creator><name>Marcy G.W.,Butler R.P.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Esquerdo G.A.</name></creator><creator><name>Sasselov D.D.</name></creator><creator><name>Kovacs G.,Stefanik R.P.</name></creator><creator><name>Fernandez J.M.</name></creator><creator><name>Lazar J.</name></creator><creator><name>Papp I.</name></creator><creator><name>Sari P.</name></creator><date role="Updated">2026-05-19T14:25:37Z</date><date role="Created">2012-01-12T09:22:58Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>multiple-stars</subject><subject>solar-system-planets</subject><description>We report on the discovery of HAT-P-12b, a transiting extrasolar planet orbiting the moderately bright V~12.8 K4 dwarf GSC 03033-00706, with a period P=3.2130598+/-0.0000021d, transit epoch T_c_=2454419.19556+/-0.00020 (BJD), and transit duration 0.0974+/-0.0006d. The host star has a mass of 0.73+/-0.02M_{sun}_, radius of 0.70^+0.02^_-0.01_R_{sun}_, effective temperature 4650+/-60K, and metallicity [Fe/H]=-0.29+/-0.05. We find a slight correlation between the observed spectral line bisector spans and the radial velocity, so we consider, and rule out, various blend configurations including a blend with a background eclipsing binary, and hierarchical triple systems where the eclipsing body is a star or a planet. We conclude that a model consisting of a single star with a transiting planet best fits the observations, and show that a likely explanation for the apparent correlation is contamination from scattered moonlight. Based on this model, the planetary companion has a mass of 0.211+/-0.012M_J_ and radius of 0.959^+0.029^_-0.021_R_J_ yielding a mean density of 0.295+/-0.025g/cm^3^. Comparing these observations with recent theoretical models, we find that HAT-P-12b is consistent with a ~1-4.5Gyr, mildly irradiated, H/He-dominated planet with a core mass M_C_&lt;~10M_{earth}_.</description><source format="bibcode">2009ApJ...706..785H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/706/785</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/706/785</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/706/785</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/706/785</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/706/785</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/706/785</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/706/785</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><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/706/785/table2</name><description>Photometry follow-up of HAT-P-12</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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