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<ri:Resource created="2021-03-25T08:24:07Z" status="active" updated="2025-09-25T20:16:39Z" 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>Search for Planets in Hot Jupiter Systems</title><shortName>J/AcA/70/181</shortName><identifier>ivo://CDS.VizieR/J/AcA/70/181</identifier><altIdentifier>doi:10.26093/cds/vizier.120700181</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Maciejewski G.</name></creator><date role="Updated">2025-09-25T20:16:39Z</date><date role="Created">2021-03-25T08:24:07Z</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>exoplanets</subject><subject>photometry</subject><description>Origins of giant planets on tight orbits, so called hot Jupiters, are a long-lasting question in the planetary formation and evolution theory. The answer seems to be hidden in architectures of those systems that remain only partially understood. Using multi-sector time-series photometry from the Transiting Exoplanet Survey Satellite, we searched for additional planets in the KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126 planetary systems using both the transit technique and transit timing method. Our homogeneous analysis has eliminated the presence of transiting companions down to the terrestrial-size regime in the KELT-23 and WASP-62 systems, and down to mini-Neptunes or Neptunes in the remaining ones. Transit timing analysis has revealed no sign of either long-term trends or periodic perturbations for all the studied hot Jupiters, including the WASP-126 b for which deviations from a Keplerian model were claimed in the literature. The loneliness of the planets of the sample speaks in favor of the high-eccentricity migration mechanism that probably brought them to their tight orbits observed nowadays. As a by-product of our study, the transit light curve parameters were redetermined with a substantial improvement of the precision for six systems. For KELT-24 b, a joint analysis allowed us to place a tighter constraint on its orbital eccentricity.</description><source format="bibcode">2020AcA....70..181M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AcA/70/181</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/153/263">J/AJ/153/263 : Transiting planetary system KELT-18 (McLeod+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/78">J/AJ/158/78 : Transiting planetary system KELT-23 (Johns+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/197">J/AJ/158/197 : Transiting planetary system KELT-24 (Rodriguez+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/224">J/AJ/157/224 : Transiting planetary system Qatar-8 (Alsubai+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/739">J/MNRAS/426/739 : Transiting planetary system WASP-62 (Hellier+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/440/1982">J/MNRAS/440/1982 : Transiting planetary system WASP-100 (Hellier+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/591/55">J/A+A/591/55 : Planetary systems WASP-119 and WASP-126 (Maxted+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/631/A76">J/A+A/631/A76 : MASCARA-3b radial and light curves (Hjorth+, 2019)</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/AcA/70/181</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AcA/70/181</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AcA/70/181</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AcA/70/181</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AcA/70/181</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AcA/70/181</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/AcA/70/181/tt</name><description>Transit mid-points</description><column><name>Ep</name><description>Epoch</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</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>All</name><description>Display all measurements for the exoplanet</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Planet</name><description>Planet name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>BJD</name><description>Mid-transit time (1)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_BJD</name><description>Positive error for BJD</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_BJD</name><description>Negative error for BJD</description><unit>d</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Datasrc</name><description>Data source (2)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column></table></schema></tableset></ri:Resource>