GCN Circular 10571
Subject
Master-Net observations on the Swift trigger on LS V +44 17
Date
2010-04-03T05:54:22Z (15 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc@observ.inetcomm.ru>
V.Krushinski, I.Zalozhnih, T.Kopytova, A. Popov Ural State University,
Kourovka
V.Yurkov, Yu.Sergienko, D.Varda, A.Garusina Blagoveschensk Educational State
University, Blagoveschensk
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.Zemnukhov,
M. Kornilov
Sternberg Astronomical Institute, Moscow State University
A. Tlatov, A.V. Parhomenko, D. Dormidontov
Kislovodsk Solar Station of the Pulkovo Observatory
K.Ivanov, S.Yazev, N.M.Budnev, E.Konstantinov, V.Lenok
Irkutsk State University
MASTER robotic telescope (MASTER-Net: http://observ.pereplet.ru, 2x400
mm, FOV=2x4 square degrees)
located at Ural was responted to the trigger 418109 (Swift Bat alert,
Stratt et al, GCN CIRC 10561) 19 sec after Notice time and 1820 s after
the trigger time.
MASTER took a finding chart synchronous exposure of 180 seconds with the two
filters starting 1820 seconds after the BAT trigger.
Unfortunatelly the optical star LS V+44 17 are saturated.
The message may be cited.
mailto: lipunov@sai.msu.ru