New photometric analysis of hot Jupiter: WASP-135b |
| |
| Institution: | 1. Astrophysics Research Centre and Observatory, Çanakkale Onsekiz Mart University, Terzioğlu Kampüsü, Çanakkale TR-17020, Turkey;2. Department of Physics, Faculty of Arts and Sciences, Çanakkale Onsekiz Mart University, Terzioğlu Kampüsü, Canakkale TR-17020, Turkey;1. Astronomy & Meteorology Department, Faculty of Science, Al-Azhar University, Nasr City, Cairo, 11488, Egypt;2. Astronomy, Space Science & Meteorology Department, Faculty of Science, Cairo University, Giza, 12613, Egypt;1. Department of Physics and Astronomy, Shumen University, Shumen 9700, Bulgaria;2. Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Mexico;1. The International Occultation Timing Association Middle East section, Iran;2. Adana Organised Industrial Zones Vocational School of Technical Science, University of Çukurova, 01410, Adana, Turkey;3. Space Science and Solar Energy Research and Application Center (UZAYMER), University of Çukurova, 01330, Adana, Turkey;1. Department of Mathematics, Zakir Husain Delhi College, University of Delhi, Delhi 110002, India;2. Department of Mathematics, College of Natural and Computational Science, Mizan-Tepi University, Tepi Campus, Ethiopia;1. Department of Physics and Astronomy, Shumen University, Shumen, Bulgaria;2. IRIDA Observatory, Rozhen NAO, Bulgaria;3. Institute of Astronomy and NAO, Bulgarian Academy of Sciences, Sofia, Bulgaria |
| |
| Abstract: | We 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. |
| |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
