GCN Circular 3151
Subject
GRB050326: optical limit
Date
2005-03-27T01:33:31Z (20 years ago)
Edited On
2024-11-18T09:46:29Z (2 months ago)
From
Martin Jelinek at Inst.Astrophys.Andalucia,Granada <mates@asu.cas.cz>
Edited By
Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of Leo P. Singer at NASA/GSFC <leo.p.singer@nasa.gov>
P. Tristram (Univ. of Canterbury, New Zealand),
M. Jelinek, A. de Ugarte Postigo, J. Gorosabel, A.J.
Castro-Tirado, (IAA-CSIC, Granada, Spain), M. A. Castro Tirado (Málaga),
J. M. Castro Cerón (Univ. of Copenhagen, Denmark) and
Ph. Yock (Univ. of Auckland, New Zealand) report:
We have imaged the error box provided by Swift (trigger
112453, GCN 3147) with the 0.6m telescope (+MOA camera)
at Mt.John Observatory. A 600s second integration taken
at 16:47:45 UT (ie. 6.90 hours after burst, mean obs.
time) reveals no apparent source down to limiting mag.
20.3 in comparison with DSS. Observation was performed
with MOA broad R-band filter (similar to Ic).
[GCN OPS NOTE (28mar05): At an author's request "M. A. Castro Tirado (M?laga)"
was added to the author list.]