[vsnet-grb-info 9903] GRB 101020A: MASTER prompt and afterglow limit
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Sat Oct 23 00:41:44 JST 2010
TITLE: GCN CIRCULAR
NUMBER: 11361
SUBJECT: GRB 101020A: MASTER prompt and afterglow limit
DATE: 10/10/22 15:41:40 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc at observ.inetcomm.ru>
V.Krushinski, I.Zalozhnich, T.Kopytova, A. Popov
Ural State University, Kourovka
K.Ivanov, O.Chuvalaev, V.Poleschuk, E.Konstantinov, V.Lenok, O.Gres,
S.Yazev, N.M.Budnev,
Irkutsk State University
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
MASTER-Net robotic telescopes (MASTER-Net: http://observ.pereplet.ru)
located near Ekaterinburg (Kourovka) was pointed to the Swift GRB 101008A
(Saxton et al., GCN#11357) 22 s after Notice Time and 106 s after trigger time
at large zenit distance (80 degrees) (Krushinski et al., GCN Circ 11359).
We have no found any OT.
t_start-t_trig(s) mean time exp_time(s) m_lim Coadd? Filter
--------------------------------------------------------------------------
106 116 20+20 14.9 Y V
472 2836 4300 18.5 Y V
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MASTER II have 2 images per exposition time.
The message may be cited.
mailto: lipunov at sai.msu.ru
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