arXiv · 1911.08331
Transit Timing Variations of Five Transiting Planets
Abstract
Transiting planets provide a unique opportunity to search for unseen additional bodies gravitationally bound to a system. It is possible to detect the motion of the center-of-mass of the observed transiting planet-host star duo due to the gravitational tugs of the unseen bodies from the Roemer delay. In order to achieve the goal, determination of the mid-times of the transits of the planets in high precision and accuracy and correct them for the orbital motion of the Earth is a primary condition. We present transit timing variations and update the ephemeris information of 5 transiting planets; HAT-P-23b, WASP-103b, GJ-1214b, WASP-69b, and KELT-3b within this contribution, based on all the quality transit light curves from amateur and professional observers, converted to Dynamic Barycentric Julian Days (BJD-TDB).
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Ozgur Basturk, Ekrem M. Esmer, Seyma Torun, Selcuk Yalcinkaya, Fadel El Helweh, Ertugrul Karamanli, Mehmet Oncu, H. Ozgur Albayrak, Afra F. M. Akram, Muammer G. Kahraman, Shaad Sufi, Muhammed Uzumcu, Fatemeh Davoudi. 2019-11-18. Transit Timing Variations of Five Transiting Planets. https://doi.org/10.1063/1.5135417
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