Transit modelling of selected Kepler systems

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dc.authoridPuskullu, Caglar/0000-0001-9213-0969
dc.authoridBanks, Timothy/0000-0001-9445-4588
dc.contributor.authorHuang, Q. Y.
dc.contributor.authorBanks, T.
dc.contributor.authorBudding, E.
dc.contributor.authorPuskullu, C.
dc.contributor.authorRhodes, M. D.
dc.date.accessioned2025-01-27T20:29:33Z
dc.date.available2025-01-27T20:29:33Z
dc.date.issued2019
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThis paper employs a simple model, considering just geometry and linear or quadratic limb darkening, to fit Kepler transit data via a Markov Chain Monte Carlo (MCMC) methodology for Kepler-1b, 5b, 8b, 12b, 77b, 428b, 491b, 699b, 706b, and 730b. Additional fits were made of the systems using the more sophisticated modeller Winfitter, which gives results in general agreement with the simpler model. Analysis of data with longer integration times showed biasing of the derived parameters, as expected from the literature, leading to larger estimates for radii and reducing estimates of the system inclination.
dc.identifier.doi10.1007/s10509-019-3525-0
dc.identifier.issn0004-640X
dc.identifier.issn1572-946X
dc.identifier.issue2
dc.identifier.scopus2-s2.0-85062060579
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1007/s10509-019-3525-0
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22977
dc.identifier.volume364
dc.identifier.wosWOS:000459762300003
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
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.subjectOptimization
dc.subjectExoplanets
dc.subjectLight curve analysis
dc.titleTransit modelling of selected Kepler systems
dc.typeArticle

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