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Budding, E.; Puskullu, C.; Rhodes, M. D.; Demircan, O.; Erdem, A.
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<identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/57773</identifier>
<creators>
<creator>
<creatorName>Budding, E.</creatorName>
<givenName>E.</givenName>
<familyName>Budding</familyName>
</creator>
<creator>
<creatorName>Puskullu, C.</creatorName>
<givenName>C.</givenName>
<familyName>Puskullu</familyName>
<affiliation>Univ Canakkale, TR-17020 Canakkale, Turkey</affiliation>
</creator>
<creator>
<creatorName>Rhodes, M. D.</creatorName>
<givenName>M. D.</givenName>
<familyName>Rhodes</familyName>
<affiliation>BYU, Provo, UT USA</affiliation>
</creator>
<creator>
<creatorName>Demircan, O.</creatorName>
<givenName>O.</givenName>
<familyName>Demircan</familyName>
<affiliation>Univ Canakkale, TR-17020 Canakkale, Turkey</affiliation>
</creator>
<creator>
<creatorName>Erdem, A.</creatorName>
<givenName>A.</givenName>
<familyName>Erdem</familyName>
<affiliation>Univ Canakkale, TR-17020 Canakkale, Turkey</affiliation>
</creator>
</creators>
<titles>
<title>Analysis Of The Exoplanet Containing System Kepler-91</title>
</titles>
<publisher>Aperta</publisher>
<publicationYear>2016</publicationYear>
<dates>
<date dateType="Issued">2016-01-01</date>
</dates>
<resourceType resourceTypeGeneral="Text">Journal article</resourceType>
<alternateIdentifiers>
<alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/57773</alternateIdentifier>
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<relatedIdentifiers>
<relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/s10509-015-2564-4</relatedIdentifier>
</relatedIdentifiers>
<rightsList>
<rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
<rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
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<descriptions>
<description descriptionType="Abstract">We have applied the graphical user interfaced close binary system analysis program WINFITTER to an intensive study of Kepler-91 using all the available photometry from the NASA Exoplanet Archive (NEA) at the Caltech website: http://exoplanetarchive.ipac.caltech.edu. Our fitting function for the tidal distortion derives from the relevant Radau equation and includes terms up to the fifth power of the fractional radius. This results in a systematic improvement in the mass ratio estimation over that of Lillo-Box et al. (Astron. Astrophys. 562:A109, 2014a) and our derived value for the mass ratio is in close agreement with that inferred from recent high-resolution spectroscopic data.</description>
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