GCN Circular 13807
Subject
GRB 120923A: Swift-BAT refined analysis
Date
2012-09-23T13:37:37Z (12 years ago)
From
Scott Barthelmy at NASA/GSFC <scott@lheamail.gsfc.nasa.gov>
C. B. Markwardt (GSFC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),
J. R. Cummings (GSFC/UMBC), E. E. Fenimore (LANL), N. Gehrels (GSFC),
H. A. Krimm (GSFC/USRA), D. M. Palmer (LANL), T. Sakamoto (GSFC/UMBC),
G. Sato (ISAS), M. Stamatikos (OSU), J. Tueller (GSFC),
T. N. Ukwatta (MSU), V. N. Yershov (UCL-MSSL)
(i.e. the Swift-BAT team):
Using the data set from T-61 to T+242 sec from recent telemetry downlinks,
we report further analysis of BAT GRB 120923A (trigger #534402)
(Yershov, et al., GCN Circ. 13796). The BAT ground-calculated position is
RA, Dec = 303.781, 6.255 deg, which is
RA(J2000) = 20h 15m 07.3s
Dec(J2000) = +06d 15' 16.8"
with an uncertainty of 2.1 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 79%.
The mask-weighted light curve shows the burst starting at ~T-5 sec, peaking
at ~T+25 sec, and ending at ~T+30 sec. T90 (15-350 keV) is 27.2 +- 3.0 sec
(estimated error including systematics).
The time-averaged spectrum from T-2.93 to T+26.64 sec is best fit by a power law
with an exponential cutoff. This fit gives a photon index -0.29 +- 1.66,
and Epeak of 44.4 +- 10.6 keV (chi squared 43.83 for 56 d.o.f.). For this
model the total fluence in the 15-150 keV band is 3.2 +- 0.8 x 10^-7 erg/cm2
and the 1-sec peak flux measured from T+24.67 sec in the 15-150 keV band is
0.6 +- 0.1 ph/cm2/sec. A fit to a simple power law gives a photon index
of 1.80 +- 0.23 (chi squared 51.10 for 57 d.o.f.). All the quoted errors
are at the 90% confidence level.
The results of the batgrbproduct analysis are available at
http://gcn.gsfc.nasa.gov/notices_s/534402/BA/