1 Ocak 2018 Dergi makalesi Açık Erişim

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

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{
  "@context": "https://schema.org/", 
  "@id": 28971, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "name": "Budding, E."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Univ Canakkale, TR-17020 Canakkale, Turkey", 
      "name": "Puskullu, C."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Brigham Young Univ, Provo, UT 84602 USA", 
      "name": "Rhodes, M. D."
    }
  ], 
  "datePublished": "2018-01-01", 
  "description": "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.", 
  "headline": "Analysis of the exoplanet containing system Kepler-13", 
  "identifier": 28971, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Analysis of the exoplanet containing system Kepler-13", 
  "url": "https://aperta.ulakbim.gov.tr/record/28971"
}