Photometric Analysis of the Exoplanet Containing System Kepler-491

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dc.authoridSoydugan, Faruk/0000-0002-5141-7645
dc.authoridPuskullu, Caglar/0000-0001-9213-0969
dc.contributor.authorPuskullu, Caglar
dc.contributor.authorSoydugan, Faruk
dc.date.accessioned2025-01-27T21:07:13Z
dc.date.available2025-01-27T21:07:13Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description32nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEY
dc.description.abstractIn this study, we present solutions of the transit light curves of the recently discovered planet Kepler-491h observed by Kepler space-telescope within a span of four years. In order to obtain stellar, planetary and orbital properties, WINFITTER code was applied to light curve data available at the NASA Exoplanet Archive (NEA). We also searched for significant signals at the transit timing variation (TIV).
dc.description.sponsorshipTurkish Phys Soc
dc.identifier.doi10.1063/1.4976454
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85016044513
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976454
dc.identifier.urihttps://hdl.handle.net/20.500.12428/27932
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100110
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofProceedings of The Turkish Physical Society 32nd International Physics Congress (Tps32)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titlePhotometric Analysis of the Exoplanet Containing System Kepler-491
dc.typeConference Object

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