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KomentářeTranzit exoplanety - detail
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SW Lac (Gerald Persha)
V1018 Cyg (Walter F., Šebek F., Jakimčík V.)
ER Vul (Urbaník M.)
ER Vul (Urbaník M.)
ER Vul (Urbaník M.)
ER Vul (Urbaník M.)
V0505 Per (Urbaník M.)
V0505 Per (Urbaník M.)
V0505 Per (Urbaník M.)
DM Per (Urbaník M.)
Qatar-4 b (A. Tomatis)
Qatar-4 b (A. Tomatis)
HAT-P-50 b (P. Guerra)
WASP-43 b (Y. Jongen)
Qatar-4 b (Y. Jongen)
HAT-P-53 b (M. Nikolay)
WASP-43 b (M. Talafha)
WASP-114 b (A. Wunsche)
WASP-52 b (A. Wünsche)
Qatar-4 b (S. Gudmundsson)
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: 3C66A And, AR And, FN And, FO And, IW And, KV And, LL And, LS And, LX And, PQ And, QR And, RX And, V 402 And, V 455 And, Z And, BB Aur, NSV 16874 Aur, UY Cas, V 730 Cep, EM Cyg,
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: 3C66A And, AR And, FN And, FO And, IW And, KV And, LL And, LS And, LX And, PQ And, QR And, RX And, V 402 And, V 455 And, Z And, BB Aur, NSV 16874 Aur, UY Cas, V 730 Cep, EM Cyg,
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Komentář
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