arXiv · 2403.17690
Looking For Timing Variations in the Transits of 16 Exoplanets
Abstract
We update the ephemerides of 16 transiting exoplanets using our ground-based observations, new TESS data, and previously published observations including those of amateur astronomers. All these light curves were modeled by making use of a set of quantitative criteria with the EXOFAST code to obtain mid-transit times. We searched for statistically significant secular and/or periodic trends in the mid-transit times. We found that the timing data are well modeled by a linear ephemeris for all systems except for XO-2 b, for which we detect an orbital decay with the rate of -12.95 $\pm$ 1.85 ms/yr that can be confirmed with future observations. We also detect a hint of potential periodic variations in the TTV data of HAT-P-13 b which also requires confirmation with further precise observations.
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S. Yalçınkaya, E. M. Esmer, Ö. Baştürk, A. Muhaymin, A. C. Kutluay, D. İ. Silistre, F. Akar, J. Southworth, L. Mancini, F. Davoudi, E. Karamanlı, F. Tezcan, E. Demir, D. Yılmaz, E. Güleroğlu, M. Tekin, İ. Taşkın, Y. Aladağ, E. Sertkan, U. Y. Kurt, S. Fişek, S. Kaptan, S. Aliş, N. Aksaker, F. K. Yelkenci, C. T. Tezcan, A. Kaya, D. Oğlakkaya, Z. S. Aydın, C. Yeşilyaprak. 2024-03-26. Looking For Timing Variations in the Transits of 16 Exoplanets. https://doi.org/10.1093/mnras/stae854
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