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, A.Sankovich, V.Sennik
Sternberg Astronomical Institute, Moscow State University
V.Yurkov, Yu.Sergienko, D.Varda, A.Garusina Blagoveschensk Educational
K.Ivanov, S.Yazev, N.M.Budnev, E.Konstantinov, V.Lenok, O.Gres, O.Chuvalaev
Irkutsk State University
A. Tlatov, A.V. Parkhomenko, D. Dormidontov
Kislovodsk Solar Station of the Pulkovo Observatory
V.Krushinski, I.Zalozhnih, T.Kopytova, A.Popov
Ural State University, Kourovka
MASTER Very Wide Field Cameras located at Blagoveschensk (D=50 mm, 1000
square degrees, 11 Mpx, 36" per pix) has observed FERMI error box (FERMI
trigger N295791986 ra=161.933 dec=+38.317) with 1s exposure befoure,
during and after GRB time without time gap between images. This camera is
on one mount with is more large MASTER telescope. These observation have
been received during the regular sky survey. Directly at the moment of
GRB the telescope had repointing, so sets since 3 seconds before grb to 3 sec. after grb time (2010-05-17 12:26:24 UT) is moved.
The magnitude limit of the each good image is ~ 8-m at the center of FOW,
and ~ 4-5 m on each moved image.
Our unfiltered images are calibrated relative to Tycho stars (V).
Specification of coordinates is required.
Images available here:
The message may be cited.