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<ri:Resource created="2020-01-29T06:39:51Z" 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>Asteroseismic parameters of RGB stars</title><shortName>J/AJ/158/227</shortName><identifier>ivo://CDS.VizieR/J/AJ/158/227</identifier><altIdentifier>doi:10.26093/cds/vizier.51580227</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Grunblatt S.K.</name></creator><creator><name>Huber D.</name></creator><creator><name>Gaidos E.</name></creator><creator><name>Hon M.</name></creator><creator><name>Zinn J.C.</name></creator><creator><name>Stello D.</name></creator><date role="Updated">2021-08-11T10:36:40Z</date><date role="Created">2020-01-29T06:39:51Z</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>giant-stars</subject><subject>asteroseismology</subject><subject>stellar-radii</subject><subject>stellar-masses</subject><subject>effective-temperature</subject><subject>metallicity</subject><subject>apparent-magnitude</subject><subject>stellar-distance</subject><subject>exoplanets</subject><description>Every Sun-like star will eventually evolve into a red giant, a transition which can profoundly affect the evolution of a surrounding planetary system. The timescale of dynamical planet evolution and orbital decay has important implications for planetary habitability, as well as post-main-sequence star and planet interaction, evolution, and internal structure. Here, we investigate these effects by estimating planet occurrence around 2476 low-luminosity red giant branch (LLRGB) stars observed by the NASA K2 mission. We measure stellar masses and radii using asteroseismology, with median random uncertainties of 3.7% in mass and 2.2% in radius. We compare this planet population to the known population of planets around dwarf Sun-like stars, accounting for detection efficiency differences between the stellar populations. We find that 0.49%+/-0.28% of LLRGB stars host planets larger than Jupiter with orbital periods less than 10 days, tentatively higher than main-sequence stars hosting similar planets (0.15%+/-0.06%). Our results suggest that the effects of stellar evolution on the occurrence of close-in planets larger than Jupiter are not significant until stars have begun ascending substantially up the red giant branch (&gt;~5-6 R_{sun}_).</description><source format="bibcode">2019AJ....158..227G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/158/227</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/127">J/ApJ/767/127 : Asteroseismic solutions for 77 Kepler stars (Huber+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/2">J/ApJS/224/2 : K2 EPIC stellar properties for 138600 targets (Huber+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/107">J/AJ/154/107 : California-Kepler Survey (CKS). I. 1305 stars (Petigura+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/236/42">J/ApJS/236/42 : Asteroseismology of ~16000 Kepler red giants (Yu+, 2018)</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/158/227</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/158/227</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/158/227</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/158/227</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/158/227</mirrorURL><mirrorURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EPIC</name><description>[201089316/248295571] K2 Ecliptic Plane Input Catalog identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>numax</name><description>[50.14016/295.136787] Best-fit frequency of maximum power {nu}_max_</description><unit>uHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_numax</name><description>[0/10.74829] Uncertainty in numax</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dnu</name><description>[5.88815/20.95513] Regular frequency spacing {Delta}{nu}</description><unit>uHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Dnu</name><description>[0.0121/0.5534] Uncertainty in Dnu</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Amp</name><description>[0/59.1365] Maximum oscillation amplitude</description><unit>(10-6)</unit><ucd>src.var.amplitude;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>S/B</name><description>[-41.02358/13.99596] Asteroseismic signal-to-background ratio</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rad-AS</name><description>[3.287173/7.997912] Asteroseismic radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad-AS</name><description>[0.066606/0.368089] Uncertainty in Rad-AS</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass-AS</name><description>[0.521351/2.474164] Asteroseismic mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass-AS</name><description>[0.023016/0.160355] Uncertainty in Mass-AS</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff-iso</name><description>[3686.339893/5667.750393] Effective temperature from isoclassify</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rad-iso</name><description>[2.361485/154.402496] Radius from isoclassify</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Teff-EPIC</name><description>[3908/6222] EPIC (Cat. IV/34) recorded effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[1.567/4.971] EPIC recorded surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-2.232/0.21] EPIC recorded metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GPMag</name><description>[-4.903268/3.861973] Gaia DR2 (Cat. 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