[vsnet-grb-info 5799] GRB 080319B: TORTORA synchronous observation
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Thu Mar 20 02:39:18 JST 2008
TITLE: GCN CIRCULAR
NUMBER: 7452
SUBJECT: GRB 080319B: TORTORA synchronous observation
DATE: 08/03/19 17:33:14 GMT
FROM: Sergey Karpov at SAO RAS <karpov at sao.ru>
S. Karpov, G. Beskin, S. Bondar, C. Bartolini, G. Greco, A. Guarnieri,
D. Nanni, A. Piccioni, F. Terra, E. Molinari, G. Chincarini, F.M. Zerbi,
S. Covino, V. Testa, G. Tosti, F. Vitali, L.A. Antonelli, P. Conconi, G.
Cutispoto, G. Malaspina, L. Nicastro, E. Palazzi, E. Meurs, P. Goldoni
report on behalf of the TORTOREM team:
TORTORA wide-field optical camera (12 cm diameter, 20x25 deg FOV, TV-CCD,
unfiltered) mounted on REM robotic 60-cm telescope located at La Silla
(Chile) observed the field of GRB 080319B (GCN 7427, Racusin et al.)
before, during and after the gamma-emission with 0.13 s time resolution.
We observe optical emission at the position given by Swift XRT:
1. We did not detect any transient brighter than 8.5m (unfiltered,
near B) at T-100 - T+16 s
2. We detect rapidly rising OT (~5 second rise front) and observe it
between T+16 and T+30, the peak brightness has been around 5 m
3. Between T+30 and T+36 the observations have been paused due to
repointing of REM telescope
4. Since T+36 we continuously observe the transient until it faded below
the detection limit (~8.5m) at T+90 s
The detailed analysis is in progress.
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