Öztürk, OğuzErdem, Ahmet2025-02-102025-02-102021Öztürk, O., & Erdem, A. (2021). New photometric analysis of hot Jupiter: WASP-135b. New Astronomy, 82. https://doi.org/10.1016/j.newast.2020.1014541384-1076 / 1384-1092https://doi.org/10.1016/j.newast.2020.101454https://hdl.handle.net/20.500.12428/29596We 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.enginfo:eu-repo/semantics/closedAccessPlanetary systemsStars: individual: WASP-135Techniques: photometricarticle8210.1016/j.newast.2020.101454Q3WOS:0005647053000072-s2.0-85088235818Q2