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Tranzit exoplanety - detail> Zpět na seznam seznam pozorování |
> Předpověď minim < IO CEP (Sergey I.)
V523 Cas (Sjoerd Dufoer)
BS Vul (Sjoerd Dufoer)
RW CrB (Sergey I.)
PS Boo (Holý S.)
UV Leo (Aleh Biheza)
VW Cep (Urbaník M.)
VW Cep (Urbaník M.)
VW Cep (Urbaník M.)
VW Cep (Urbaník M.)
TrES-3 b (S. Lopez)
WASP-19 b (C. Knight)
WASP-19 b (C. Knight)
TrES-3 b (F. Scaggiante, D. Zardin, M. Fiaschi)
Kepler-13 b (A. Guerrero)
WASP-31 b (Y. Jongen)
WASP-3 b (P. Gajdoš)
HAT-P-3 b (M. Iozzi)
WASP-54 b (Y. Jongen)
Kepler-5 b (Y. Jongen)
CCD: : AH Cam, P. Dubovský: NOVACas2021 Cas, : NOVACas2021 Cas, : V 1413 Aql, NOVACas2021 Cas, NOVAHer2021 Her, NOVAVul2021 Vul, P. Dubovský: NOVACas2021 Cas, NOVAPer2020 Per, NOVAVul2021 Vul, VIZ: P. Dubovský: RX And, Z And, TT Ari, NSV 16874 Aur, SS Aur, UY Cas, V 730 Cep, AT Cnc, YZ Cnc, U Gem, V 1159 Ori, GK Per, Z And, TT Ari, Eps Aur, NSV 16874 Aur, Psi1 Aur, SS Aur, Zeta Aur, HT Cam, |
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objektu 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