| Autor: |
Baştürk, Ö., Esmer, E. M., Torun, Ş., Yalçınkaya, S., El Helweh, F., Karamanlı, E., Öncü, M., Albayrak, H. Ö., Akram, F. A. M., Kahraman, M. G., Sufi, S., Üzümcü, M., Davoudi, F. |
| Předmět: |
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| Zdroj: |
AIP Conference Proceedings; 2019, Vol. 2178 Issue 1, p030019-1-030019-4, 4p |
| Abstrakt: |
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, WASP1-103b, 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). [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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