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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
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