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VERIFICATION OF THE KEPLER INPUT CATALOG FROM ASTEROSEISMOLOGY OF SOLAR-TYPE STARS

Identifieur interne : 006576 ( Main/Exploration ); précédent : 006575; suivant : 006577

VERIFICATION OF THE KEPLER INPUT CATALOG FROM ASTEROSEISMOLOGY OF SOLAR-TYPE STARS

Auteurs : G. A. Verner [Royaume-Uni] ; W. J. Chaplin [Royaume-Uni] ; S. Basu [États-Unis] ; T. M. Brown [États-Unis] ; S. Hekker [Royaume-Uni, Pays-Bas] ; D. Huber [Australie] ; C. Karoff [Danemark] ; S. Mathur [États-Unis] ; T. S. Metcalfe [États-Unis] ; B. Mosser [France] ; P.-O. Quirion [Canada] ; T. Appourchaux [France] ; T. R. Bedding [Australie] ; H. Bruntt [Danemark] ; T. L. Campante [Portugal] ; Y. Elsworth [Royaume-Uni] ; R. A. Garcia [France] ; R. Handberg [Danemark] ; C. Regulo [Espagne] ; I. W. Roxburgh [Royaume-Uni] ; D. Stello [Australie] ; J. Christensen-Dalsgaard [Danemark] ; R. L. Gilliland [États-Unis] ; S. D. Kawaler [États-Unis] ; H. Kjeldsen [Danemark] ; C. Allen [États-Unis] ; B. D. Clarke [États-Unis] ; F. R. Girouard [États-Unis]

Source :

RBID : Pascal:11-0466207

Descripteurs français

English descriptors

Abstract

We calculate precise stellar radii and surface gravities from the asteroseismic analysis of over 500 solar-type pulsating stars observed by the Kepler space telescope. These physical stellar properties are compared with those given in the Kepler Input Catalog (KIC), determined from ground-based multi-color photometry. For the stars in our sample, we find general agreement but we detect an average overestimation bias of 0.23 dex in the KIC determination of log(g) for stars with log(g)KIC > 4.0 dex, and a resultant underestimation bias of up to 50% in the KIC radii estimates for stars with RKIC < 2 R◦.. Part of the difference may arise from selection bias in the asteroseismic sample; nevertheless, this result implies there may be fewer stars characterized in the KIC with R ˜ 1 R◦. than is suggested by the physical properties in the KIC. Furthermore, if the radius estimates are taken from the KIC for these affected stars and then used to calculate the size of transiting planets, a similar underestimation bias may be applied to the planetary radii.


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<title xml:lang="en" level="a">VERIFICATION OF THE KEPLER INPUT CATALOG FROM ASTEROSEISMOLOGY OF SOLAR-TYPE STARS</title>
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<s1>Department of Astronomy, Yale University, P.O. Box 208101</s1>
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<s1>Department of Physics and Astronomy, Aarhus University</s1>
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<s1>Centro de Astroffsica, Universidade do Porto, Rua das Estrelas</s1>
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<s1>Departamento de Astrofisica, Universidad de La Laguna</s1>
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<country>Espagne</country>
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<s1>Instituto de Astrofísica de Canarias</s1>
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<s1>Department of Physics and Astronomy, Iowa State University</s1>
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</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Orbital Sciences Corporation/NASA Ames Research Center</wicri:noRegion>
</affiliation>
</author>
</analytic>
<series>
<title level="j" type="main">The Astrophysical journal</title>
<title level="j" type="abbreviated">Astrophys. j.</title>
<idno type="ISSN">0004-637X</idno>
<imprint>
<date when="2011">2011</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">The Astrophysical journal</title>
<title level="j" type="abbreviated">Astrophys. j.</title>
<idno type="ISSN">0004-637X</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Astronomical catalogues</term>
<term>Astroseismology</term>
<term>Be stars</term>
<term>Color</term>
<term>G stars</term>
<term>Photometry</term>
<term>Physical properties</term>
<term>Planets</term>
<term>Solar type star</term>
<term>Surface gravity</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Catalogue astronomique</term>
<term>Astéroséismologie</term>
<term>Etoile type solaire</term>
<term>Gravité surface</term>
<term>Propriété physique</term>
<term>Couleur</term>
<term>Photométrie</term>
<term>Etoile G</term>
<term>Etoile Be</term>
<term>Planète</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We calculate precise stellar radii and surface gravities from the asteroseismic analysis of over 500 solar-type pulsating stars observed by the Kepler space telescope. These physical stellar properties are compared with those given in the Kepler Input Catalog (KIC), determined from ground-based multi-color photometry. For the stars in our sample, we find general agreement but we detect an average overestimation bias of 0.23 dex in the KIC determination of log(g) for stars with log(g)
<sub>KIC</sub>
> 4.0 dex, and a resultant underestimation bias of up to 50% in the KIC radii estimates for stars with R
<sub>KIC</sub>
< 2 R
<sub>◦.</sub>
. Part of the difference may arise from selection bias in the asteroseismic sample; nevertheless, this result implies there may be fewer stars characterized in the KIC with R ˜ 1 R
<sub>◦.</sub>
than is suggested by the physical properties in the KIC. Furthermore, if the radius estimates are taken from the KIC for these affected stars and then used to calculate the size of transiting planets, a similar underestimation bias may be applied to the planetary radii.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>Australie</li>
<li>Canada</li>
<li>Danemark</li>
<li>Espagne</li>
<li>France</li>
<li>Pays-Bas</li>
<li>Portugal</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region>
<li>Angleterre</li>
<li>Grand Londres</li>
<li>Hollande-Septentrionale</li>
<li>Iowa</li>
<li>Midlands de l'Ouest</li>
<li>Nouvelle-Galles du Sud</li>
<li>Île-de-France</li>
</region>
<settlement>
<li>Ames (Iowa)</li>
<li>Amsterdam</li>
<li>Birmingham</li>
<li>Londres</li>
<li>Paris</li>
<li>Sydney</li>
</settlement>
<orgName>
<li>Université Pierre-et-Marie-Curie</li>
<li>Université d'Amsterdam</li>
<li>Université d'État de l'Iowa</li>
<li>Université de Birmingham</li>
<li>Université de Londres</li>
<li>Université de Sydney</li>
</orgName>
</list>
<tree>
<country name="Royaume-Uni">
<region name="Angleterre">
<name sortKey="Verner, G A" sort="Verner, G A" uniqKey="Verner G" first="G. A." last="Verner">G. A. Verner</name>
</region>
<name sortKey="Chaplin, W J" sort="Chaplin, W J" uniqKey="Chaplin W" first="W. J." last="Chaplin">W. J. Chaplin</name>
<name sortKey="Elsworth, Y" sort="Elsworth, Y" uniqKey="Elsworth Y" first="Y." last="Elsworth">Y. Elsworth</name>
<name sortKey="Hekker, S" sort="Hekker, S" uniqKey="Hekker S" first="S." last="Hekker">S. Hekker</name>
<name sortKey="Roxburgh, I W" sort="Roxburgh, I W" uniqKey="Roxburgh I" first="I. W." last="Roxburgh">I. W. Roxburgh</name>
<name sortKey="Verner, G A" sort="Verner, G A" uniqKey="Verner G" first="G. A." last="Verner">G. A. Verner</name>
</country>
<country name="États-Unis">
<noRegion>
<name sortKey="Basu, S" sort="Basu, S" uniqKey="Basu S" first="S." last="Basu">S. Basu</name>
</noRegion>
<name sortKey="Allen, C" sort="Allen, C" uniqKey="Allen C" first="C." last="Allen">C. Allen</name>
<name sortKey="Brown, T M" sort="Brown, T M" uniqKey="Brown T" first="T. M." last="Brown">T. M. Brown</name>
<name sortKey="Clarke, B D" sort="Clarke, B D" uniqKey="Clarke B" first="B. D." last="Clarke">B. D. Clarke</name>
<name sortKey="Gilliland, R L" sort="Gilliland, R L" uniqKey="Gilliland R" first="R. L." last="Gilliland">R. L. Gilliland</name>
<name sortKey="Girouard, F R" sort="Girouard, F R" uniqKey="Girouard F" first="F. R." last="Girouard">F. R. Girouard</name>
<name sortKey="Kawaler, S D" sort="Kawaler, S D" uniqKey="Kawaler S" first="S. D." last="Kawaler">S. D. Kawaler</name>
<name sortKey="Mathur, S" sort="Mathur, S" uniqKey="Mathur S" first="S." last="Mathur">S. Mathur</name>
<name sortKey="Metcalfe, T S" sort="Metcalfe, T S" uniqKey="Metcalfe T" first="T. S." last="Metcalfe">T. S. Metcalfe</name>
</country>
<country name="Pays-Bas">
<region name="Hollande-Septentrionale">
<name sortKey="Hekker, S" sort="Hekker, S" uniqKey="Hekker S" first="S." last="Hekker">S. Hekker</name>
</region>
</country>
<country name="Australie">
<region name="Nouvelle-Galles du Sud">
<name sortKey="Huber, D" sort="Huber, D" uniqKey="Huber D" first="D." last="Huber">D. Huber</name>
</region>
<name sortKey="Bedding, T R" sort="Bedding, T R" uniqKey="Bedding T" first="T. R." last="Bedding">T. R. Bedding</name>
<name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name>
</country>
<country name="Danemark">
<noRegion>
<name sortKey="Karoff, C" sort="Karoff, C" uniqKey="Karoff C" first="C." last="Karoff">C. Karoff</name>
</noRegion>
<name sortKey="Bruntt, H" sort="Bruntt, H" uniqKey="Bruntt H" first="H." last="Bruntt">H. Bruntt</name>
<name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name>
<name sortKey="Handberg, R" sort="Handberg, R" uniqKey="Handberg R" first="R." last="Handberg">R. Handberg</name>
<name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name>
</country>
<country name="France">
<region name="Île-de-France">
<name sortKey="Mosser, B" sort="Mosser, B" uniqKey="Mosser B" first="B." last="Mosser">B. Mosser</name>
</region>
<name sortKey="Appourchaux, T" sort="Appourchaux, T" uniqKey="Appourchaux T" first="T." last="Appourchaux">T. Appourchaux</name>
<name sortKey="Garcia, R A" sort="Garcia, R A" uniqKey="Garcia R" first="R. A." last="Garcia">R. A. Garcia</name>
</country>
<country name="Canada">
<noRegion>
<name sortKey="Quirion, P O" sort="Quirion, P O" uniqKey="Quirion P" first="P.-O." last="Quirion">P.-O. Quirion</name>
</noRegion>
</country>
<country name="Portugal">
<noRegion>
<name sortKey="Campante, T L" sort="Campante, T L" uniqKey="Campante T" first="T. L." last="Campante">T. L. Campante</name>
</noRegion>
</country>
<country name="Espagne">
<noRegion>
<name sortKey="Regulo, C" sort="Regulo, C" uniqKey="Regulo C" first="C." last="Regulo">C. Regulo</name>
</noRegion>
<name sortKey="Regulo, C" sort="Regulo, C" uniqKey="Regulo C" first="C." last="Regulo">C. Regulo</name>
</country>
</tree>
</affiliations>
</record>

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