GCN Circular 4485
Subject
GRB060111.2:_MASTER optical limit
Date
2006-01-11T19:15:26Z (19 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc@observ.inetcomm.ru>
V. Lipunov, V.Kornilov, D.Kuvshinov, N.Tyurina, A.Belinski, E.Gorbovskoy,
A.Krylov, G.Borisov, A.Sankovich, G.Antipov, V.Vladimirov
Sternberg Astronomical Institute, Moscow Union 'Optic'
MASTER robotic system (http://observ.pereplet.ru) responded to GRB060111.2
(GRB_TIME is 2006-01-11 04:23:06.12).
The first image was at 2006-01-11 04:25:16 UT, 130 s after the GRB
time (a half of an hour befor sunrise).
The unfiltered image is calibrated relative to USNO A2.0 (0.8 R + 0.2 B).
The robot not find OT-candidate in error box.
Our final results on OT magnitude limit are:
UT (start) Mean time After GRB time m exptime
04 25 16 04 25 31 130 s 16.0 30 sec
The first JPG-image will be available at
http://observ.pereplet.ru/images/GRB060111.2/1.jpg .
This work is supported by RFFI 04-02-16411 grant.
This message can be cited.
Mailto: lipunov@sai.msu.ru