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OBSERVERS LOGTransit observations (TRESCA database)
BE Dra (Ehrenberger R.)
XY LMi (Bragagnolo U.)
HL Aur (Bragagnolo U.)
GSC 04021-01132 (Bragagnolo U.)
V1011 Cas (Bragagnolo U.)
BX tri (Lomoz F.)
BX Tri (Lomoz F.)
BX Tri (Lomoz F.)
AE LMi (Bragagnolo U.)
V0460 Cam (Bragagnolo U.)
Qatar-5 b (Y. Jongen)
KELT-1 b (M. Raetz)
HAT-P-25 b (E. Girardin)
Kepler-15 b (Y. Jongen)
TrES-2 b (M. Bretton)
HAT-P-19 b (Y. Jongen)
Qatar-1 b (Y. Jongen)
WASP-2 b (B. Wenzel)
WASP-2 b (B. Wenzel)
WASP-93 b (l. rousselot)
CCD:
P. Dubovský: V 392 Per, Vend47 Sge, GK Per, V 392 Per, Vend47 Sge, V 392 Per, GK Per, V 392 Per, Vend47 Sge, BF Cyg,
VIZ:
P. Dubovský: WY And, Z And, SY Cam, BX Cas, KS Cas, NSV 332 Cas, NSV 650 Cas, ST Cas, TU Cas, UY Cas, V 365 Cas, V 465 Cas, V 764 Cas, VY Cas, TZ Cep, R CrB, T CrB, AG Dra, V 818 Her, V 939 Her,
P. Dubovský: V 392 Per, Vend47 Sge, GK Per, V 392 Per, Vend47 Sge, V 392 Per, GK Per, V 392 Per, Vend47 Sge, BF Cyg,
VIZ:
P. Dubovský: WY And, Z And, SY Cam, BX Cas, KS Cas, NSV 332 Cas, NSV 650 Cas, ST Cas, TU Cas, UY Cas, V 365 Cas, V 465 Cas, V 764 Cas, VY Cas, TZ Cep, R CrB, T CrB, AG Dra, V 818 Her, V 939 Her,
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object HAT-P-36 b
I discovered that the star TYC 3020-2195-1, usually adopted as reference for HAT-P-36, is a variable with amplitude 0.015 magn. and a period of 1h (probably a delta Scuti): www of the light curves of the transit of HAT-P-36b present in ETD were obtained using that star. Giuseppe Marino.
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This observation is in error and can be removed. Correct data is re-imported. Petri Kehusmaa