Image de couverture de livre

Looking For Timing Variations in the Transits of 16 Exoplanets

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Yalçınkaya, S., Esmer, E. M., Baştürk, Ö., Muhaymin, A., Kutluay, A. C., Silistre, D. İ., Akar, F., Southworth, J., Mancini, L., Davoudi, F., Karamanlı, E., Tezcan, F., Demir, E., Yılmaz, D., Güleroğlu, E., Tekin, M., Taşkın, İ., Aladağ, Y., Sertkan, E., Kurt, U. Y., Fişek, S., Kaptan, S., Aliş, S., Aksaker, N., Yelkenci, F. K., Tezcan, C. T., Kaya, A., Oğlakkaya, D., Aydın, Z. S., Yeşilyaprak, C.
Format:	Preprint
Publié:	2024
Sujets:	Earth and Planetary Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

_version_	1866913284856217600
author	Yalçınkaya, S. Esmer, E. M. Baştürk, Ö. Muhaymin, A. Kutluay, A. C. Silistre, D. İ. Akar, F. Southworth, J. Mancini, L. Davoudi, F. Karamanlı, E. Tezcan, F. Demir, E. Yılmaz, D. Güleroğlu, E. Tekin, M. Taşkın, İ. Aladağ, Y. Sertkan, E. Kurt, U. Y. Fişek, S. Kaptan, S. Aliş, S. Aksaker, N. Yelkenci, F. K. Tezcan, C. T. Kaya, A. Oğlakkaya, D. Aydın, Z. S. Yeşilyaprak, C.
author_facet	Yalçınkaya, S. Esmer, E. M. Baştürk, Ö. Muhaymin, A. Kutluay, A. C. Silistre, D. İ. Akar, F. Southworth, J. Mancini, L. Davoudi, F. Karamanlı, E. Tezcan, F. Demir, E. Yılmaz, D. Güleroğlu, E. Tekin, M. Taşkın, İ. Aladağ, Y. Sertkan, E. Kurt, U. Y. Fişek, S. Kaptan, S. Aliş, S. Aksaker, N. Yelkenci, F. K. Tezcan, C. T. Kaya, A. Oğlakkaya, D. Aydın, Z. S. Yeşilyaprak, C.
contents	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.
format	Preprint
id	arxiv_https___arxiv_org_abs_2403_17690
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Looking For Timing Variations in the Transits of 16 Exoplanets Yalçınkaya, S. Esmer, E. M. Baştürk, Ö. Muhaymin, A. Kutluay, A. C. Silistre, D. İ. Akar, F. Southworth, J. Mancini, L. Davoudi, F. Karamanlı, E. Tezcan, F. Demir, E. Yılmaz, D. Güleroğlu, E. Tekin, M. Taşkın, İ. Aladağ, Y. Sertkan, E. Kurt, U. Y. Fişek, S. Kaptan, S. Aliş, S. Aksaker, N. Yelkenci, F. K. Tezcan, C. T. Kaya, A. Oğlakkaya, D. Aydın, Z. S. Yeşilyaprak, C. Earth and Planetary Astrophysics 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.
title	Looking For Timing Variations in the Transits of 16 Exoplanets
topic	Earth and Planetary Astrophysics
url	https://arxiv.org/abs/2403.17690