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<ri:Resource created="2011-02-28T09:21:00Z" 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>HAT-P-1b Ks-band secondary eclipse</title><shortName>J/A+A/528/A49</shortName><identifier>ivo://CDS.VizieR/J/A+A/528/A49</identifier><altIdentifier>doi:10.26093/cds/vizier.35280049</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>de Mooij E.J.W.</name></creator><creator><name>de Kok R.J.</name></creator><creator><name>Nefs S.V.</name></creator><creator><name>Snellen I.A.G.</name></creator><date role="Updated">2017-06-22T14:28:55Z</date><date role="Created">2011-02-28T09:21:00Z</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>infrared-photometry</subject><description>Only recently it has become possible to measure the thermal emission from hot-Jupiters at near-Infrared wavelengths using ground-based telescopes, by secondary eclipse observations. This allows the planet flux to be probed around the peak of its spectral energy distribution, which is vital for the understanding of its energy budget. The aim of the reported work is to measure the eclipse depth of the planet HAT-P-1b at 2.2micron. This planet is an interesting case, since the amount of stellar irradiation it receives falls in between that of the two best studied systems (HD209458 and HD189733), and it has been suggested to have a weak thermal inversion layer. We have used the LIRIS instrument on the William Herschel Telescope (WHT) to observe the secondary eclipse of HAT-P-1b in the Ks-band, as part of our Ground-based secondary eclipse (GROUSE) project. The observations were done in staring mode, while significantly defocusing the telescope to avoid saturation on the K=8.4 star. With an average cadence of 2.5 seconds, we collected 6520 frames during one night.</description><source format="bibcode">2011A&amp;A...528A..49D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/528/A49</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/134/1707">J/AJ/134/1707 : Six transits of exoplanet HAT-P-1b (Winn+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A84">J/A+A/523/A84 : Transit light curves of HAT-P-13b (Szabo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A85">J/A+A/527/A85 : Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A54">J/A+A/550/A54 : Ks-band observations of WASP-33b (de Mooij+, 2013)</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/A+A/528/A49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/528/A49</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/528/A49</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/528/A49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/528/A49</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/528/A49</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>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/528/A49/hatp1_ks</name><description>Ks-band time-series photometry of HAT-P-1b</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>Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>Calculated orbital phase of HAT-P-1b (1)</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Fhatp1</name><description>Flux of the target (HAT-P-1), in ADU units</description><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Fref</name><description>Flux of the reference star, in ADU units</description><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sky</name><description>Background per pixel, in ADU/pix units</description><unit>pixel**-1</unit><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TExp</name><description>Exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Airmass</name><description>Airmass</description><ucd>obs.airMass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mountPA</name><description>Position angle of the mount</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Xpos</name><description>X-position of HAT-P-1 on the detector</description><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y-position of HAT-P-1 on the detector</description><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>