1 Ocak 2018 Dergi makalesi Açık Erişim

Budding, E.; Puskullu, C.; Rhodes, M. D.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/28971</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>Brigham Young Univ, Provo, UT 84602 USA</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Analysis Of The Exoplanet Containing System Kepler-13</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2018</publicationYear>
  <dates>
    <date dateType="Issued">2018-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/28971</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/s10509-018-3275-4</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 close binary system analysis program WINFITTER, with its physically detailed fitting function, to an intensive study of the complex multiple system Kepler-13 using photometry data from all 13 short cadence quarters downloaded from the NASA Exoplanet Archive (NEA) (http://exoplanetarchive.ipac.caltech.edu ). The data-point error of our normalized, phase-sequenced and binned (380 points per bin: 0.00025 phase interval) flux values, at 14 ppm, allows the model's specification for the mean reference flux level of the system to a precision better than 1 ppm. Our photometrically derived values for the mass and radius of KOI13.01 are 6.8 +/- 0.6 M-J and 1.44 +/- 0.04 R-J. The star has a radius of 1.67 +/- 0.05 R-circle dot. Our modelling sets the mean of the orbital inclination i at 94.35 +/- 0.14 degrees, with the star's mean precession angle phi(p) -49.1 +/- 5.0 degrees and obliquity theta(o) 67.9 +/- 3.0 degrees, though there are known ambiguities about the sense in which such angles are measured.</description>
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