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Transit observations (TRESCA database)Derived system geometry
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HW Vir (L. Šmelcer)
HW Vir (L. Šmelcer)
HW Vir (L. Šmelcer)
HW Vir (L. Šmelcer)
HW Vir (L. Šmelcer)
HW Vir (L. Šmelcer)
XY Boo (L. Šmelcer)
XY Boo (L. Šmelcer)
XY Boo (L. Šmelcer)
V502 Oph (M. Mašek)
WASP-25 b (P. Evans)
HAT-P-3 b (S. Poddanı)
WASP-3 b (F. Martinelli)
WASP-2 b (A. Oksanen)
Kepler-15 b (F. Lomoz)
WASP-2 b (A. Oksanen)
WASP-3 b (A. Marchini)
Kepler-15 b (F. Lomoz)
WASP-3 b (A. Marchini)
WASP-3 b (R. Naves)
CCD: M. Lehkı: , , , , , , , P. Dubovskı: , , , VIZ: P. Dubovskı: , , , , , , , , , , , , , , , , , , , , Currently operating observers: Liptovská Štiavnica, Slovakia STATUS: Is active 22:00 - 04:00 PROGRAM: V2637 Oph OAC, ORBA, EABA y OAEGG STATUS: Is active 16:01 - 00:01 PROGRAM: B.R.N.O TRESCA Sternenstaub Observatorium STATUS: Is active 08:26 - 16:26 PROGRAM: Exoplanet Observing |
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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?