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Transit observations (TRESCA database) |
DD CrB (Sjoerd Dufoer)
BS UMa (Sjoerd Dufoer)
NSVS 967819 (Sjoerd Dufoer)
HAT131 (Sjoerd Dufoer)
GK Boo (Sjoerd Dufoer)
LINEAR 6244503 UMa (M. Magris)
ASASSN-V J091559.38+652745.0 UMa (M. Magris)
PW UMa (M. Magris)
Ton 301 Cnc (melcer L.)
HW Vir (melcer L.)
TOI-3976 A b (G. Muler)
HAT-P-3 b (G. Nieto)
TOI-3757 b (K. and)
WASP-113 b (G. Montardit)
WASP-113 b (G. Montardit)
WASP-184 b (Y. Jongen)
WASP-113 b (G. Nieto)
HAT-P-3 b (G. Muler)
TrES-1 b (J. Gallego)
TOI-1273 b (G. Nieto)
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: BB Aur, NSV 16874 Aur, SS Aur, CR Boo, TT Boo, UZ Boo, Z Cam, AK Cnc, AT Cnc, EG Cnc, GY Cnc, OJ287 Cnc, SY Cnc, YZ Cnc, AL Com, T CrB, VW CrB, AB Dra, CP Dra, DM Dra, 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?