New photometric analysis of hot Jupiter: WASP-135b

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dc.authorid0000-0002-9135-9865en_US
dc.authorid0000-0001-5289-8850en_US
dc.authorscopusid57195507848en_US
dc.authorscopusid56266032500en_US
dc.authorwosid-en_US
dc.authorwosidAAA-8730-2021en_US
dc.contributor.authorÖztürk, Oğuz
dc.contributor.authorErdem, Ahmet
dc.date.accessioned2025-02-10T07:15:14Z
dc.date.available2025-02-10T07:15:14Z
dc.date.issued2021en_US
dc.departmentFakülteler, Fen Fakültesi, Fizik Bölümüen_US
dc.description.abstractWe report photometric follow-up observations of WASP-135b obtained using the 1.23-m telescope at Calar Alto Observatory and 1.00-m telescope at TÜBİTAK National Observatory during the 2017 and 2018 observational seasons. Eight new transit light curves of WASP-135b were analyzed with JKTEBOP code. The ratio of the planet radius to radius of host star, fractional radius of host star, and orbital inclination of WASP-135b were found to be 0.138 ± 0.002, 0.181 ± 0.008 and 82.44 ± 0.64 degrees, respectively. Planetary radius of WASP-135b was derived from transit parameters to be 1.075 ± 0.150 RJ. The transit ephemeris of WASP-135b was also updated using the maximum likelihood method (MLM). 165 well-known hot Jupiters (HJs) were selected from the Exoplanet Data Explorer database and the classification of these HJs together with WASP-135b, based on their equilibrium temperatures and Safronov numbers, is discussed.en_US
dc.identifier.citationÖztürk, O., & Erdem, A. (2021). New photometric analysis of hot Jupiter: WASP-135b. New Astronomy, 82. https://doi.org/10.1016/j.newast.2020.101454en_US
dc.identifier.doi10.1016/j.newast.2020.101454en_US
dc.identifier.issn1384-1076 / 1384-1092
dc.identifier.scopus2-s2.0-85088235818en_US
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1016/j.newast.2020.101454
dc.identifier.urihttps://hdl.handle.net/20.500.12428/29596
dc.identifier.volume82en_US
dc.identifier.wosWOS:000564705300007en_US
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.institutionauthorÖztürk, Oğuz
dc.institutionauthorErdem, Ahmet
dc.institutionauthorid0000-0002-9135-9865
dc.institutionauthorid0000-0001-5289-8850
dc.language.isoengen_US
dc.publisherElsevier B.V.en_US
dc.relation.ispartofNew Astronomyen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectPlanetary systemsen_US
dc.subjectStars: individual: WASP-135en_US
dc.subjectTechniques: photometricen_US
dc.titleNew photometric analysis of hot Jupiter: WASP-135ben_US
dc.typearticleen_US

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