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Transit observations (TRESCA database) |
PS Boo (Holý S.)
PS Boo (Holý S.)
PS Boo (Holý S.)
PS Boo (Holý S.)
DY CVn (Massimo Banfi, Liceo Iris Versari)
WISE J141530.7+592234 UMa (Tylar M.)
GJ 3236 Cas (melcer L.)
GJ 3236 Cas (melcer L.)
GU Boo (melcer L.)
GU Boo (melcer L.)
TOI-1273 b (M. Tylar)
TOI-1273 b (F. Walter)
HAT-P-36 b (R. Roy)
WASP-39 b (F. Lomoz)
Qatar-10 b (M. Alava)
TOI-1194 b (M. Salisbury)
CoRoT-11 b (G. Calapai)
XO-1 b (R. Roy)
WASP-85 A b (B. Wenzel)
HAT-P-55 b (E. Lorenz)
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: WY And, Z And, Eta Aql, TT Boo, UZ Boo, HT Cam, SY Cam, Z Cam, BX Cas, KS Cas, NOVACas2021 Cas, NSV 332 Cas, ST Cas, UY Cas, V 365 Cas, VY Cas, Delta Cep, TZ Cep, V 730 Cep, AT Cnc, Currently operating observers: Magpie observatory (FTP) STATUS: Active20:00 - 06:00 PROGRAM: V 709 Cas, main program - CV and transits of exoplanets Observatorio Astronómico Giordano Bruno STATUS: Active20:38 - 04:38 PROGRAM: De 20:00 a 02:30 Osservatorio Astronomico Citta di Seveso STATUS: Active12:30 - 10:45 PROGRAM: 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?