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<ri:Resource created="2015-09-02T14:26:21Z" 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>Kepler planetary host stars rotation periods</title><shortName>J/ApJ/803/69</shortName><identifier>ivo://CDS.VizieR/J/ApJ/803/69</identifier><altIdentifier>doi:10.26093/cds/vizier.18030069</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Paz-Chinchon F.</name></creator><creator><name>Leao I.C.</name></creator><creator><name>Bravo J.P.</name></creator><creator><name>de Freitas D.B.,Ferreira Lopes C.E.</name></creator><creator><name>Alves S.</name></creator><creator><name>Catelan M.</name></creator><creator><name>Canto Martins B.L.,De Medeiros J.R.</name></creator><date role="Updated">2017-09-22T16:15:38Z</date><date role="Created">2015-09-02T14:26:21Z</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>stellar-masses</subject><description>We analyzed the host stars of the present sample of confirmed planets detected by Kepler and Kepler Objects of Interest to compute new photometric rotation periods and to study the behavior of their angular momentum. Lomb-Scargle periodograms and wavelet maps were computed for 3807 stars. For 540 of these stars, we were able to detect rotational modulation of the light curves at a significance level of greater than 99%. For 63 of these 540 stars, no rotation measurements were previously available in the literature. According to the published masses and evolutionary tracks of the stars in this sample, the sample is composed of M- to F-type stars (with masses of 0.48-1.53M_{sun}_) with rotation periods that span a range of 2-89 days. These periods exhibit an excellent agreement with those previously reported (for the stars for which such values are available), and the observed rotational period distribution strongly agrees with theoretical predictions. Furthermore, for the 540 sources considered here, the stellar angular momentum provides an important test of Kraft's relation based on the photometric rotation periods. Finally, this study directly contributes in a direct approach to our understanding of how angular momentum is distributed between the host star and its (detected) planetary system; the role of angular momentum exchange in such systems is an unavoidable piece of the stellar rotation puzzle.</description><source format="bibcode">2015ApJ...803...69P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/803/69</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/ApJ/801/3">J/ApJ/801/3 : Rotation periods for Q3-Q14 KOIs (Mazeh+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A34">J/A+A/572/A34 : Pulsating solar-like stars in Kepler (Garcia+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/1883">J/MNRAS/436/1883 : Properties of KOI host stars (Walkowicz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/432/1203">J/MNRAS/432/1203 : Rotation periods of M-dwarf stars (McQuillan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/428/3164">J/MNRAS/428/3164 : Spectroscopy of WASP planet host stars (Doyle+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A4">J/A+A/560/A4 : Rotation periods of active Kepler stars (Reinhold+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/L10">J/A+A/557/L10 : Rotation periods of 12000 Kepler stars (Nielsen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A63">J/A+A/555/A63 : Semi-sinusoidal variability with CoRoT (de Medeiros+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/L11">J/ApJ/775/L11 : Stellar rotation periods for KOIs (McQuillan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/L26">J/ApJ/763/L26 : SMARTS observations of eps Eridani (Metcalfe+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/485.478">J/other/Nat/485.478 : Superflares on solar-type stars (Maehara+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/30">J/ApJS/199/30 : Temperature scale for KIC stars (Pinsonneault+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A146">J/A+A/537/A146 : Stellar models with rotation (0.8&lt;M&lt;120) (Ekstrom+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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