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GCN Circular 16741

Subject
Fermi TRIGGER_NUM 430583595: MASTER OT 20 hours later
Date
2014-08-25T14:10:25Z (10 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc@observ.inetcomm.ru>
N.Tyurina, V. Lipunov, E. Gorbovskoy, M.Pruzhinskaya,  V.Kornilov, D.Kuvshinov, 
P.Balanutsa,  A.Kuznetsov, V.V.Chazov,
D.Denisenko, Lomonosov Moscow State University,
Sternberg Astronomical Institute, Moscow State University

V.Yurkov, Yu.Sergienko, D.Varda, E.Sinyakov, A. Gabovich
Blagoveschensk Educational State University, Blagoveschensk


A. Tlatov, A.V. Parhomenko, D. Dormidontov, V.Sennik
Kislovodsk Solar Station of the Pulkovo Observatory

K.Ivanov, S.Yazev, N.M.Budnev, O.Gres, O.Chuvalaev, V.A.Poleshchuk
Irkutsk State University

V.Krushinski, I.Zalozhnih,  A. Popov
Ural Federal University, Kourovka

Hugo Levato and Carlos Saffe
Instituto de Ciencias Astronomicas, de la Tierra y del Espacio (ICATE)

Claudio Mallamaci, Carlos Lopez and Federico Podest
Observatorio Astronomico Felix Aguilar (OAFA)


The second epoch observation of the MASTER OT J011101.13+603337.5 (GCN 
Cirs., 16740) was obtained by
MASTER-Tunka at 2014-08-25 13:32:21 (~20 hours after first observations). 
The transient  MASTER OT  J011101.13+603337.5 slightly fell to 17.5 mag 
(unfiltered). 0.5 mag is very slow for GRB afterglow and 
CV nature of the OT is more plausible.

Follow up spectral observations  are required.


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