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Transit observations (TRESCA database) |
CzeV 340 Cas (Holý S.)
AX Cas (Holý S.)
V1107 Cas (Holý S.)
V1107 Cas (Holý S.)
CzeV 1416 Cam (Daniš S.)
CzeV 1416 Cam (Daniš S.)
NSVS 709783 Cam (Daniš S.)
NSVS 709783 Cam (Daniš S.)
NR Cam (Daniš S.)
NR Cam (Daniš S.)
KELT-1 b (M. Marini)
Qatar-1 b (S. Lopez)
TOI-1181 b (Z. Orbanić)
WASP-10 b (A. Nowak)
WASP-10 b (F. Lomoz)
WASP-10 b (F. Lomoz)
WASP-10 b (F. Lomoz)
TrES-3 b (A. Kovacs)
HAT-P-40 b (M. Raetz)
TOI 1897.01 b (F. Campos)
CCD: P. Dubovský: NOVACas2021 Cas, Z And, V 1413 Aql, NSV16874 Aur, UV Aur, : NOVACas2021 Cas, P. Dubovský: NOVACas2021 Cas, OJ287 Cnc, T CrB, TX CVn, VIZ: P. Dubovský: AR And, FN And, FO And, IW And, KV And, LX And, PQ And, QR And, RX And, Z And, Eta Aql, TT Ari, BB Aur, Eps Aur, GS Aur, NSV 16874 Aur, Psi1 Aur, SS Aur, Zeta Aur, TT Boo, Currently operating observers: Magpie observatory (FTP) STATUS: Active20:00 - 06:00 PROGRAM: V 709 Cas, main program - CV and transits of exoplanets Observatoire de la colline Tossius STATUS: Active22:00 - 05:00 PROGRAM: Exoplanet transit detection and confirmation. Each time the sky permit. Observatorio Astronómico Giordano Bruno STATUS: Active20:38 - 04:38 PROGRAM: De 20:00 a 02:30 Palidoro STATUS: Active10:47 - 18:47 PROGRAM: |
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object WASP-33 b
The parent star is a pulsating: Herrero et al., A&A 526, 10 (2011)
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Smooth brightening in the middle of the transit is real. It is clearly visible in light curves made for all comparison stars in the field. A star-spot?