Ground-based transit observations of the HAT-P-18, HAT-P-19, HAT-P-27/WASP40 andWASP-21 systems

Seeliger, M.; Kitze, M.; Errmann, R.; Richter, S.; Ohlert, J.; Chen, W.; Guo, J.; Gogus, E.; Guver, T.; Aydin, B.; Mottola, S.; Hellmich, S.; Fernandez, M.; Aceituno, F.; Dimitrov, D.; Kjurkchieva, D.; Jensen, E.; Cohen, D.; Kundra, E.; Pribulla, T.; Vanko, M.; Budaj, J.; Mallonn, M.; Wu, Z.; Zhou, X.; Raetz, St.; Adam, C.; Schmidt, T.; Ide, A.; Mugrauer, M.; Marschall, L.; Hackstein, M.; Chini, R.; Haas, M.; Ak, T.; Guzel, E.; Ozdonmez, Aykut; Ginski, C.; Marka, C.; Schmidt, J.; Dincel, B.; Werner, K.; Dathe, A.; Greif, J.; Wolf, V.; Buder, S.; Pannicke, A.; Puchalski, D.; Neuhaeuser, R.

doi:10.1093/mnras/stv1187

Ground-based transit observations of the HAT-P-18, HAT-P-19, HAT-P-27/WASP40 andWASP-21 systems

Atıf İçin Kopyala

Seeliger M., Kitze M., Errmann R., Richter S., Ohlert J. M., Chen W. P., ...Daha Fazla

Monthly Notices of the Royal Astronomical Society, cilt.451, ss.4060-4072, 2015 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 451
Basım Tarihi: 2015
Doi Numarası: 10.1093/mnras/stv1187
Dergi Adı: Monthly Notices of the Royal Astronomical Society
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.4060-4072
Anahtar Kelimeler: planets and satellites: individual: HAT-P-18b, planets and satellites: individual: HAT-P-19b, planets and satellites: individual: HAT-P-27b, WASP-40b, planets and satellites: individual: WASP-21b, SPIN-ORBIT ALIGNMENT, TIMING OBSERVATIONS, EXTRASOLAR PLANETS, PHOTOMETRY, CONSTRAINTS, SEARCH, MASS
Atatürk Üniversitesi Adresli: Hayır

Özet

As part of our ongoing effort to investigate transit timing variations (TTVs) of known exoplanets, we monitored transits of the four exoplanets HAT-P-18b, HAT-P-19b, HAT-P-27b/WASP-40b and WASP-21b. All of them are suspected to show TTVs due to the known properties of their host systems based on the respective discovery papers. During the past three years 46 transit observations were carried out, mostly using telescopes of the Young Exoplanet Transit Initiative. The analyses are used to refine the systems' orbital parameters. In all cases we found no hints for significant TTVs, or changes in the system parameters inclination, fractional stellar radius and planet-to-star radius ratio. However, comparing our results with those available in the literature shows that we can confirm the already published values.