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OBSERVERS LOGTransit observations (TRESCA database)
CSS_J002044.1+432237 (Antonino Brosio)
V0700 Cyg (Ehrenberger R.)
V0700 Cyg (Ehrenberger R.)
V0700 Cyg (Ehrenberger R.)
ASASSN-V J193048.83+463522.7 Cyg (Ehrenberger R.)
ASASSN-V J193048.83+463522.7 Cyg (Ehrenberger R.)
ASASSN-V J193048.83+463522.7 Cyg (Ehrenberger R.)
V1815 Cyg (Bragagnolo U.)
NSVS 1217423 Dra (Bragagnolo U.)
LZ Dra (Bragagnolo U.)
TrES-3 b (N. Thomas)
WASP-10 b (E. Lorenz)
TrES-3 b (N. Thomas)
TrES-1 b (N. Thomas)
WASP-29 b (Y. Jongen)
HATS-43 b (Y. Jongen)
WASP-145A b (Y. Jongen)
WASP-12 b (Y. Jongen)
WASP-61 b (Y. Jongen)
WASP-78 b (Y. Jongen)
CCD:
P. Dubovský: NOVACas2021 Cas, Z And, V 1413 Aql, NSV16874 Aur, UV Aur,
: NOVACas2021 Cas,
P. Dubovský: NOVACas2021 Cas, OJ287 Cnc, T CrB, TX CVn,
VIZ:
P. Dubovský: QR And, RX And, WY And, Z And, TT Ari, NOVACas2021 Cas, UY Cas, BF Cyg, CH Cyg, CI Cyg, EM Cyg, SS Cyg, V 1742 Cyg, V 1805 Cyg, V 1981 Cyg, V 2037 Cyg, V 441 Cyg, V 482 Cyg, V 840 Cyg, KP Lyr,
P. Dubovský: NOVACas2021 Cas, Z And, V 1413 Aql, NSV16874 Aur, UV Aur,
: NOVACas2021 Cas,
P. Dubovský: NOVACas2021 Cas, OJ287 Cnc, T CrB, TX CVn,
VIZ:
P. Dubovský: QR And, RX And, WY And, Z And, TT Ari, NOVACas2021 Cas, UY Cas, BF Cyg, CH Cyg, CI Cyg, EM Cyg, SS Cyg, V 1742 Cyg, V 1805 Cyg, V 1981 Cyg, V 2037 Cyg, V 441 Cyg, V 482 Cyg, V 840 Cyg, KP Lyr,
Currently operating observers:
Observers on-line chat
Magpie observatory (FTP)
(Martin Bartošík)
STATUS: Active20:00 - 06:00
PROGRAM: V 709 Cas, main program - CV and transits of exoplanets
Observatoire de la colline Tossius
(guillaume biesse)
STATUS: Active22:00 - 05:00
PROGRAM: Exoplanet transit detection and confirmation. Each time the sky permit.
Observatorio Astronómico Giordano Bruno
(Fco- Manuel Santos Álamo)
STATUS: Active20:38 - 04:38
PROGRAM: De 20:00 a 02:30
Osservatorio Astronomico Citta di Seveso
(Pietro Aceti)
STATUS: Active12:30 - 10:45
PROGRAM:
Palidoro
(Giuseppe Conzo)
STATUS: Active10:47 - 18:47
PROGRAM:
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Comment
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