GCN Circular 10486
Subject
GRB 100316A: Swift/UVOT Observations
Date
2010-03-16T04:16:17Z (15 years ago)
From
Mike Siegel at PSU/Swift MOC <siegel@astro.psu.edu>
M. H. Siegel (PSU) and W. H. Baumgartner (GSFC/UMBC) report on behalf
of the
Swift/UVOT team:
UVOT took a finding chart exposure of 150 seconds with the White filter
starting 3200 seconds after the BAT trigger. No credible afterglow
candidate
has been found in the initial data products. The 2.7'x2.7' sub-image
covers 100%
of the XRT error circle (Beardmore et al., GCN Circ. 10485). The
typical 3-sigma
upper limit has been about 19.6 mag. The 8'x8' region for the list of
sources
generated on-board covers 100% of the XRT error circle. The list of
sources is
typically complete to about 18 mag. No correction has been made for
the expected
extinction corresponding to E(B-V) of 0.03.