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<ri:Resource created="2016-10-31T09:08:29Z" 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>Detection of the secondary eclipse of Qatar-1b</title><shortName>J/A+A/595/A61</shortName><identifier>ivo://CDS.VizieR/J/A+A/595/A61</identifier><altIdentifier>doi:10.26093/cds/vizier.35950061</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cruz P.</name></creator><creator><name>Barrado D.</name></creator><creator><name>Lillo-Box J.</name></creator><creator><name>Diaz M.</name></creator><creator><name>Birkby J.</name></creator><creator><name>Lopez-Morales M.,Fortney J.J.</name></creator><date role="Updated">2017-06-30T05:48:13Z</date><date role="Created">2016-10-31T09:08:29Z</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><subject>occultation</subject><description>Qatar-1b is a close-orbiting hot Jupiter (Rp~=1.18R_J_, Mp~=1.33M_J_) around a metal-rich K-dwarf, with orbital separation and period of 0.023AU and 1.42-days. We have observed the secondary eclipse of this exoplanet in the Ks band with the objective of deriving a brightness temperature for the planet and providing further constraints to the orbital configuration of the system. We obtained near-infrared photometric data from the ground by using the OMEGA2000 instrument at the 3.5m telescope at Calar Alto (Spain) in staring mode, with the telescope defocused. We have used principal component analysis (PCA) to identify correlated systematic trends in the data. A Markov chain Monte Carlo analysis was performed to model the correlated systematics and fit for the secondary eclipse of Qatar-1b using a previously developed occultation model. We adopted the prayer bead method to assess the effect of red noise on the derived parameters.</description><source format="bibcode">2016A&amp;A...595A..61C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/595/A61</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/A+A/554/A28">J/A+A/554/A28 : Qatar-1 differential light curve (Covino+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A92">J/A+A/555/A92 : Transit timing variations on Qatar-1 (von Essen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/577/A109">J/A+A/577/A109 : Transit times of Qatar-1b (Maciejewski+, 2015)</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/595/A61</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/595/A61</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/595/A61</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/595/A61</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/595/A61</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/595/A61</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/A+A/595/A61/fig3_lc</name><description>Detrended light curve with the secondary eclipse of Qatar-1b in the Ks band as a function of the orbital phase</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>Phase</name><description>Phase</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Differential normalized flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>O-C</name><description>Residuals</description><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>