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<ri:Resource created="2018-10-17T14:08:14Z" 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>Elemental abundances of KOIs in APOGEE. I.</title><shortName>J/AJ/155/68</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/68</identifier><altIdentifier>doi:10.26093/cds/vizier.51550068</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wilson R.F.</name></creator><creator><name>Teske J.</name></creator><creator><name>Majewski S.R.</name></creator><creator><name>Cunha K.</name></creator><creator><name>Smith V.</name></creator><creator><name>Souto D.,Bender C.</name></creator><creator><name>Mahadevan S.</name></creator><creator><name>Troup N.</name></creator><creator><name>Prieto C.A.</name></creator><creator><name>Stassun K.G.,Skrutskie M.F.</name></creator><creator><name>Almeida A.</name></creator><creator><name>Garcia-Hernandez D.A.</name></creator><creator><name>Zamora O.</name></creator><creator><name>Brinkmann J.</name></creator><date role="Updated">2018-12-13T12:57:44Z</date><date role="Created">2018-10-17T14:08:14Z</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>multiple-stars</subject><subject>effective-temperature</subject><subject>metallicity</subject><description>The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has observed ~600 transiting exoplanets and exoplanet candidates from Kepler (Kepler Objects of Interest, KOIs), most with &gt;=18 epochs. The combined multi-epoch spectra are of high signal-to-noise ratio (typically &gt;=100) and yield precise stellar parameters and chemical abundances. We first confirm the ability of the APOGEE abundance pipeline, ASPCAP, to derive reliable [Fe/H] and effective temperatures for FGK dwarf stars - the primary Kepler host stellar type - by comparing the ASPCAP-derived stellar parameters with those from independent high-resolution spectroscopic characterizations for 221 dwarf stars in the literature. With a sample of 282 close-in (P&lt;100 days) KOIs observed in the APOGEE KOI goal program, we find a correlation between orbital period and host star [Fe/H] characterized by a critical period, P_crit_=8.3_-4.1_^+0.1^ days, below which small exoplanets orbit statistically more metal-enriched host stars. This effect may trace a metallicity dependence of the protoplanetary disk inner radius at the time of planet formation or may be a result of rocky planet ingestion driven by inward planetary migration. We also consider that this may trace a metallicity dependence of the dust sublimation radius, but we find no statistically significant correlation with host T_eff_ and orbital period to support such a claim.</description><source format="bibcode">2018AJ....155...68W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/68</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/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/415/1153">J/A+A/415/1153 : [Fe/H] for 98 extra-solar planet-host stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/545/A32">J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/122">J/MNRAS/423/122 : Abundances of 93 solar-type Kepler targets</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/486.375">J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/127">J/ApJ/767/127 : Asteroseismic solutions for 77 Kepler stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A25">J/A+A/568/A25 : C and O abundances in stellar populations (Nissen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/815/5">J/ApJ/815/5 : Detailed abundances of KOI stars with planets. I.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for the 15 APOGEE chemical elements</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/187">J/AJ/152/187 : Planet occurrence and stellar metallicity for KOIs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/32">J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)</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/155/68</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/68</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/68</mirrorURL></interface></capability><capability><interface 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