GCN Circular 3993
Subject
GRB 050915B: Swift-BAT refined analysis
Date
2005-09-16T21:14:11Z (19 years ago)
From
David Palmer at LANL <palmer@lanl.gov>
J. Cummings (GSFC/NRC), M. Ajello (MPE), L. Barbier (GSFC),
S. Barthelmy (GSFC), E. Fenimore (LANL), R. Fink (GSFC),
N. Gehrels (GSFC), D. Hullinger (UMD), H. Krimm (GSFC/USRA),
C. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC),
T. Sakamoto (GSFC/NRC), G. Sato (ISAS), J. Tueller (GSFC),
on behalf of the Swift-BAT team:
Using the full data set from T-90 to T+300 sec from the recent
telemetry downlinks, we report further analysis of Swift-BAT
GRB 050915B (trigger #155284) (Falcone, et al., GCN 3987). The
refined BAT ground position is (RA,Dec) = 219.112, -67.412 degrees
{14h 36m 26.8, -67d 24' 43"} (J2000) +-0.7 arcmin, (radius, sys+stat,
90% containment). This is within 8 arcseconds of the XRT counterpart
(Falcone et al. GCN 3989). The partial coding was 53% including
projection effects.
The mask-weighted light curve shows a rise from T-10 seconds to a
peak at T-4, dropping off to a lumpy plateau spanning T+0 to T+25,
then steadily declining to zero at T+50. No further instances of
emission are apparent on a 1 second timescale out to T+1200 sec.
T90 (15-350 keV) is (40 +- 1) sec (estimated error including systematics).
The time-averaged spectrum is well-fit by a power law with photon
index 1.89 +- 0.06. The fluence in the 15-150 keV band is
(3.4 +- 0.1) x 10^-6 erg/cm2. The 1-sec peak photon flux measured
from T-3.1 sec in the 15-150 keV band is (2.3 +- 0.2) ph/cm2/sec.
All quoted errors are at the 90% confidence level.
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