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<ri:Resource created="2010-11-04T13:56:31Z" 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>Planetary transits of TrES-2 and TrES-3</title><shortName>J/MNRAS/408/1494</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/408/1494</identifier><altIdentifier>doi:10.26093/cds/vizier.74081494</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Colon K. D.</name></creator><creator><name>Ford E. B.</name></creator><creator><name>Lee B.</name></creator><creator><name>Mahadevan S.</name></creator><creator><name>Blake C. H.</name></creator><date role="Updated">2024-07-12T20:14:42Z</date><date role="Created">2010-11-04T13:56:31Z</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>ccd-photometry</subject><description>We present the first extrasolar planet observations from the 10.4-m Gran Telescopio Canarias (GTC). We used the Optical System for Imaging and low Resolution Integrated Spectroscopy (OSIRIS) tunable filter imager on the GTC to acquire high-precision, narrow-band photometry of the transits of the giant exoplanets, TrES-2b and TrES-3b. We obtained near-simultaneous observations in two near-infrared wavelengths (790.2 and 794.4nm). We provide normalized flux ratios for each target, where the flux ratio is defined as the target flux divided by the total combined flux from several non-variable reference stars. The flux ratios have been normalized against the baseline (out-of-transit) flux ratio for each target. We provide normalized flux ratios for each target, where the flux ratio is defined as the target flux divided by the total combined flux from several non-variable reference stars. The flux ratios have been normalized against the baseline (out-of-transit) flux ratio for each target.</description><source format="bibcode">2010MNRAS.408.1494C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/408/1494</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/AJ/136/267">J/AJ/136/267 : Six occultations of the exoplanet TrES-3 (Winn+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/500/L45">J/A+A/500/L45 : Transits of the TrES-2 exoplanet (Mislis+, 2009)</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/A+A/508/1011">J/A+A/508/1011 : Planetary transit of TrES-1 and TrES-2 (Rabus+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/510/A107">J/A+A/510/A107 : TrES-2b multi-band transit observations (Mislis+, 2010)</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/MNRAS/408/1494</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/408/1494</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/408/1494</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/408/1494</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/408/1494</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/408/1494</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"/></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/408/1494/tres2</name><description>Relative Photometry of TrES-2</description><column><name>HJD</name><description>Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><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>lambda</name><description>[790/795] Observed Wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Frel</name><description>Relative Flux Ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Frel</name><description>Uncertainty in Relative Flux Ratio</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/408/1494/tres3</name><description>Relative Photometry of TrES-3</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>lambda</name><description>[790/795] Observed Wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD</name><description>Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Frel</name><description>Relative Flux Ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Frel</name><description>Uncertainty in Relative Flux Ratio</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>