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<ri:Resource created="2008-12-21T07:37:08Z" 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>Transiting extrasolar planet HD 209458b</title><shortName>J/ApJ/649/1043</shortName><identifier>ivo://CDS.VizieR/J/ApJ/649/1043</identifier><altIdentifier>doi:10.26093/cds/vizier.16491043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Richardson L.J.</name></creator><creator><name>Harrington J.</name></creator><creator><name>Seager S.</name></creator><creator><name>Deming D.</name></creator><date role="Updated">2017-06-12T08:24:49Z</date><date role="Created">2008-12-21T07:37:08Z</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>solar-system-planets</subject><subject>photometry</subject><description>We have measured the infrared transit of the extrasolar planet HD 209458b using the Spitzer Space Telescope. We observed two primary eclipse events (one partial and one complete transit) using the 24um array of the Multiband Imaging Photometer for Spitzer (MIPS). We analyzed a total of 2392 individual images (10s integrations) of the planetary system, recorded before, during, and after transit. We performed optimal photometry on the images and used the local zodiacal light as a short-term flux reference. At this long wavelength, the transit curve has a simple boxlike shape, allowing robust solutions for the stellar and planetary radii independent of stellar limb darkening, which is negligible at 24um. We derive a stellar radius of R*=(1.06+/-0.07)R_{sun}_, a planetary radius of Rp=(1.26+/-0.08)R_J_, and a stellar mass of 1.17M_{sun}_. Within the errors, our results agree with the measurements at visible wavelengths. The 24um radius of the planet therefore does not differ significantly compared to the visible result. We point out the potential for deriving extrasolar transiting planet radii to high accuracy using transit photometry at slightly shorter IR wavelengths where greater photometric precision is possible.</description><source format="bibcode">2006ApJ...649.1043R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/649/1043</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/649/1043</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/649/1043</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/649/1043</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/649/1043</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/649/1043</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/649/1043</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/649/1043/table1</name><description>Calibrated, unbinned 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>HJD</name><description>Time at start of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>Orbital phase</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Int</name><description>Relative intensity</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Int</name><description>rms uncertainty on Int</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>