An investigation into exoplanet transits and uncertainties

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dc.authoridBanks, Timothy/0000-0001-9445-4588
dc.contributor.authorJi, Y.
dc.contributor.authorBanks, T.
dc.contributor.authorBudding, E.
dc.contributor.authorRhodes, M. D.
dc.date.accessioned2025-01-27T21:00:02Z
dc.date.available2025-01-27T21:00:02Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractA simple transit model is described along with tests of this model against published results for 4 exoplanet systems (Kepler-1, 2, 8, and 77). Data from the Kepler mission are used. The Markov Chain Monte Carlo (MCMC) method is applied to obtain realistic error estimates. Optimisation of limb darkening coefficients is subject to data quality. It is more likely for MCMC to derive an empirical limb darkening coefficient for light curves with S/N (signal to noise) above 15. Finally, the model is applied to Kepler data for 4 Kepler candidate systems (KOI 760.01, 767.01, 802.01, and 824.01) with previously unpublished results. Error estimates for these systems are obtained via the MCMC method.
dc.identifier.doi10.1007/s10509-017-3096-x
dc.identifier.issn0004-640X
dc.identifier.issn1572-946X
dc.identifier.issue6
dc.identifier.urihttps://doi.org/10.1007/s10509-017-3096-x
dc.identifier.urihttps://hdl.handle.net/20.500.12428/26918
dc.identifier.volume362
dc.identifier.wosWOS:000404219200007
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofAstrophysics and Space Science
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectOptimisation
dc.subjectExoplanets
dc.subjectLight curve analysis
dc.titleAn investigation into exoplanet transits and uncertainties
dc.typeArticle

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