[vsnet-grb-info 11216] GRB 111208A found in ground analysis of BAT data
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Dec 9 01:36:02 JST 2011
TITLE: GCN CIRCULAR
NUMBER: 12628
SUBJECT: GRB 111208A found in ground analysis of BAT data
DATE: 11/12/08 16:35:58 GMT
FROM: Takanori Sakamoto at NASA/GSFC <takanori at milkyway.gsfc.nasa.gov>
T. Sakamoto (GSFC/UMBC), C. Graziani (U of Chicago), J. R. Cummings (GSFC/UMBC),
S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), E. E. Fenimore (LANL),
N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), C. B. Markwardt (GSFC),
D. M. Palmer (LANL), G. Sato (ISAS), M. Stamatikos (OSU), J. Tueller (GSFC),
T. N. Ukwatta (MSU)
(i.e. the Swift-BAT team):
Automated BAT ground analysis found a burst that occurred at 08:28:11 UT
with a significance of 10.1 sigma (15-200 keV) from the failed event data
of trigger #509285. The event is temporally coincident with the Fermi GBM
345025692. The best BAT location is RA, Dec = 290.2151, +40.6686 deg, which is
RA(J2000) = 19h 20m 51.6s
Dec(J2000) = +40d 40' 07.0"
with an uncertainty of 2.2 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 10%.
The mask-weighted light curve created from the failed event data
(available from 08:28:12 to 08:28:22 UT) shows a constant positive
rate from the beginning of the data and then decaying at 08:28:20 UT.
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