Photometric Study of Hot Jupiters: WASP-10 b and HAT-P-36 b

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dc.authoridPuskullu, Caglar/0000-0001-9213-0969
dc.contributor.authorPuskullu, C.
dc.contributor.authorSoydugan, Faruk
dc.contributor.authorErdem, A.
dc.contributor.authorBudding, E.
dc.contributor.authorSoydugan, Esin
dc.contributor.authorTuysuz, M.
dc.contributor.authorRhodes, M.
dc.date.accessioned2025-01-27T20:41:42Z
dc.date.available2025-01-27T20:41:42Z
dc.date.issued2015
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionConference on Living Together: Planets, Host Stars and Binaries -- SEP 08-12, 2014 -- Litomysl, CZECH REPUBLIC
dc.description.abstractThis work presents preliminary results of WINFITTER analyses of photometric observations of two hot Jupiters, WASP-10 b and HAT-P-36 b. According to these results, HAT-P-36 b has mean radius of R-p = 1.40 +/- 0.25 R-Jup, and transit parameter b = 0.44 +/- 0.09. WASP-10b shows some additional variations, and we therefore preferred to model its transit light curve with and without probable spot variations.
dc.description.sponsorshipSci Org Comm
dc.identifier.endpage357
dc.identifier.isbn978-1-58381-877-0
dc.identifier.isbn978-1-58381-876-3
dc.identifier.startpage356
dc.identifier.urihttps://hdl.handle.net/20.500.12428/24214
dc.identifier.volume496
dc.identifier.wosWOS:000369467900083
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofLiving Together: Planets, Host Stars, and Binaries
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectLight Curves
dc.subjectPlanets
dc.titlePhotometric Study of Hot Jupiters: WASP-10 b and HAT-P-36 b
dc.typeConference Object

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