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OBSERVERS LOGTransit observations (TRESCA database)
BX Tri (Šmelcer L.)
BX Tri (Šmelcer L.)
BX Tri (Šmelcer L.)
BX Tri (Šmelcer L.)
CSS J022048.7+332751 Tri (Šmelcer L.)
CSS J022048.7+332751 Tri (Šmelcer L.)
CSS J022048.7+332751 Tri (Šmelcer L.)
BX Tri (Šmelcer L.)
BX Tri (Šmelcer L.)
BX Tri (Šmelcer L.)
WASP-76 b (A. Kovacs, E. Pakštienė)
WASP-93 b (M. Morales)
HAT-P-17 b (j. plazas)
TOI-2154 b (V. Školník)
WASP-43 b (C. Hakes)
TOI 1168.01 b (F. Lomoz)
WASP-59 b (E. Lorenz)
TOI-4010 c (F. Campos)
WASP-10 b (r. naves)
TOI 1168.01 b (F. Lomoz)
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: AR And, FN And, FO And, IW And, KV And, LX And, PQ And, QR And, RX And, Z And, Eta Aql, TT Ari, BB Aur, Eps Aur, GS Aur, NSV 16874 Aur, Psi1 Aur, SS Aur, Zeta Aur, TT Boo,
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: AR And, FN And, FO And, IW And, KV And, LX And, PQ And, QR And, RX And, Z And, Eta Aql, TT Ari, BB Aur, Eps Aur, GS Aur, NSV 16874 Aur, Psi1 Aur, SS Aur, Zeta Aur, TT Boo,
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
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