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Tranzit exoplanety - detail> Zpět na seznam seznam pozorování |
> Předpověď minim < RT LMi (Ehrenberger R.)
RT LMi (Ehrenberger R.)
RT LMi (Ehrenberger R.)
ASASSN-V J140432.65+391802.7 (Ehrenberger R.)
GN CVn (Ehrenberger R.)
ASAS J073603-5710.2 Car (Mašek M.)
ASAS J072612-5655.5 Car (Mašek M.)
ASAS J072612-5655.5 Car (Mašek M.)
LINEAR 7055103 Hya (Mašek M.)
LINEAR 7055103 Hya (Mašek M.)
WASP-92 b (V. Hentunen)
XO-6 b (S. Gudmundsson)
WASP-15 b (Y. Jongen)
WASP-41 b (Y. Jongen)
HATS-25 b (Y. Jongen)
WASP-41 b (A. Wünsche)
TOI 1516.01 b (V. Hentunen)
HAT-P-44 b (S. Gudmundsson)
TOI 1455.01 b (V. Hentunen)
HAT-P-3 b (A. Wünsche)
CCD: P. Dubovský: NOVACas2021 Cas, YY Her, NOVAPer2020 Per, NOVACas2021 Cas, YY Her, NOVAPer2020 Per, NOVACas2021 Cas, YY Her, NOVAPer2020 Per, NOVACas2021 Cas, VIZ: P. Dubovský: TT Boo, UZ Boo, HT Cam, Z Cam, R CrB, T CrB, VW CrB, CP Dra, DO Dra, AH Her, HZ Her, V 592 Her, V 660 Her, V 844 Her, YY Her, LX Ser, NY Ser, QZ Ser, BZ UMa, CH UMa, |
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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