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<ri:Resource created="2020-06-11T08:47:12Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Planets around main sequence stars in GALEX UV</title><shortName>J/AJ/159/194</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/194</identifier><altIdentifier>doi:10.26093/cds/vizier.51590194</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Viswanath G.</name></creator><creator><name>Narang M.</name></creator><creator><name>Manoj P.</name></creator><creator><name>Mathew B.</name></creator><creator><name>Kartha S.S.</name></creator><date role="Updated">2020-09-01T09:58:11Z</date><date role="Created">2020-06-11T08:47:12Z</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>exoplanets</subject><subject>ultraviolet-astronomy</subject><subject>stellar-masses</subject><subject>effective-temperature</subject><description>Most (~82%) of the over 4000 confirmed exoplanets known today orbit very close to their host stars, within 0.5au. Planets at such small orbital distances can result in significant interactions with their host stars, which can induce increased activity levels in them. In this work, we have searched for statistical evidence for star-planet interactions in the ultraviolet (UV) using the largest sample of 1355 Galaxy Evolution Explorer (GALEX) detected host stars with confirmed exoplanets and making use of the improved host-star parameters from Gaia DR2. From our analysis, we do not find any significant correlation between the UV activity of the host stars and their planetary properties. We further compared the UV properties of planet host stars to that of chromospherically active stars from the RAdial Velocity Experiment (RAVE) survey. Our results indicate that the enhancement in chromospheric activity of host stars due to star-planet interactions may not be significant enough to reflect in their near and far V broadband flux.</description><source format="bibcode">2020AJ....159..194V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/194</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/III/279">III/279 : RAVE 5th data release (Kunder+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised cat. of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A82">J/A+A/540/A82 : CaIIHK emission stars with close-in planets (Krejcova+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/154">J/ApJ/746/154 : Improved kinematic parallaxes Sco-Cen members (Pecaut+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A119">J/A+A/552/A119 : Planet-star and moon-planet interaction (Saur+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/766/9">J/ApJ/766/9 : GALEX observations of exoplanet host stars (Shkolnik, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/9">J/ApJS/211/9 : Variability in UV line emission of F-M stars (Loyd+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/163">J/ApJ/799/163 : Chandra observations of solar analogs (Miller+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/6">J/ApJS/218/6 : The Spitzer Interacting Galaxies Survey (Brassington+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/17">J/ApJ/834/17 : Mass &amp; radius of planets, moons, low mass stars (Chen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/61">J/ApJ/835/61 : Chromospherically active stars in RAVE. II. (Zerjal+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/89">J/AJ/155/89 : California-Kepler Survey (CKS). IV. Planets (Petigura+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/109">J/AJ/158/109 : Occurrence rates of planets orbiting FGK stars (Hsu+, 2019)</relatedResource><relatedResource>http://exoplanetarchive.ipac.caltech.edu/ : NASA exoplanet archives</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/AJ/159/194</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/159/194</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/159/194</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/159/194</accessURL><mirrorURL title="VizieR at IUCAA: 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