Looking for timing variations in the transits of 16 exoplanets

Esmer, E.; Baştürk, Özgür; Muhaymin, Abdul; Kutluay, Ahmet; Silistre, D.; Akar, F.; Southworth, John; Mancini, Luigi; Davoudi, F.; Karamanlı, E.; Tezcan, Fatma; Demir, E.; Yılmaz, D.; Güleroğlu, E.; Tekin, M.; Taşkın, İ.; Aladağ, Y.; Sertkan, E.; Kurt, U.; Fişek, Süleyman; Kaptan, Seda; Aksaker, Nazım; Tezcan, Cihan; Kaya, A.; Oğlakkaya, D.; Aydın, Z.; Yeşilyaprak, Cahit

doi:10.1093/mnras/stae854

Looking for timing variations in the transits of 16 exoplanets

Esmer E. M., Baştürk Ö., Muhaymin A., Kutluay A. C., Silistre D. İ., Akar F., ...Daha Fazla

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.0, sa.0, 2024 (SCI-Expanded, Scopus)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 0 Sayı: 0
Basım Tarihi: 2024
Doi Numarası: 10.1093/mnras/stae854
Dergi Adı: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, Aerospace Database, Applied Science & Technology Source, Communication Abstracts, Compendex, INSPEC, Metadex, zbMATH, DIALNET, Civil Engineering Abstracts
Atatürk Üniversitesi Adresli: Evet

Özet

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 ± 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.