GRB 100829.9
GCN Circular 11157
Subject
GRB 100829.9: MASTER Optical Limits
Date
2010-08-31T06:29:13Z (15 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc@observ.inetcomm.ru>
E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina,
D.Kuvshinov, P.Balanutsa, V.V.Chazov, P.V.Kortunov, A.Kuznetsov,
D.Zimnukhov, M. Kornilov
Sternberg Astronomical Institute, Moscow State University
A. Tlatov, A.V. Parhomenko, D. Dormidontov, V.Sennik
Kislovodsk Solar Station of the Pulkovo Observatory
V.Yurkov, Yu.Sergienko, D.Varda, I.Kudelina
Blagoveschensk Educational State University, Blagoveschensk
V.Krushinski, I.Zalozhnich, T.Kopytova, A. Popov
Ural State University, Kourovka
K.Ivanov, S.Yazev, N.M.Budnev, E.Konstantinov, V.Lenok, O.Gres,
O.Chuvalaev, V.Poleschuk
Irkutsk State University
MASTER robotic telescopes (MASTER-Net: http://observ.pereplet.ru, 6
Very Wide Field cameras and 2 Wide Field Telescopes ) located near
Kislovodsk was pointed to the FERMI GRB 100829.9 (FERMI Trigger N
304808530 ) 30 sec after Notice time and 44 s after trigger time
We have 12 polarization images from two tube with exposition from 10 to 60
seconds, before objects set below horizont.
start UT end UT t_exp(s) mlim t_start-tGRB(s) Coadd?
Filter
--------------------------------------------------------------------------
21:02:55 21:03:05 10 14.0 44.0 N
21:02:55 21:08:03 200 15.7 44.0 Y
The message may be cited.
mailto: lipunov@sai.msu.ru