GCN Circular 16893
Subject
GRB 141005A: Swift-BAT refined analysis
Date
2014-10-05T17:19:05Z (10 years ago)
From
Scott Barthelmy at NASA/GSFC <scott@lheamail.gsfc.nasa.gov>
H. A. Krimm (GSFC/USRA), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),
J. R. Cummings (GSFC/UMBC), V. D'Elia (ASDC), N. Gehrels (GSFC),
A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL),
T. Sakamoto (AGU), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (LANL)
(i.e. the Swift-BAT team):
Using the data set from T-239 to T+963 sec from the recent telemetry downlink,
we report further analysis of BAT GRB 141005A (trigger #614415)
(D'Elia, et al., GCN Circ. 16882). The BAT ground-calculated position is
RA, Dec = 291.103, 36.098 deg, which is
RA(J2000) = 19h 24m 24.7s
Dec(J2000) = +36d 05' 54.1"
with an uncertainty of 1.7 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 6%.
The mask-weighted light curve shows a single peak starting at ~T-1 sec,
peaking at ~T+2 sec, and ending at ~T+7 sec. T90 (15-350 keV) is 4.34 +- 1.08 sec
(estimated error including systematics).
The time-averaged spectrum from T+0.19 to T+5.66 sec is best fit by a simple
power-law model. The power law index of the time-averaged spectrum is
1.33 +- 0.18. The fluence in the 15-150 keV band is 1.1 +- 0.1 x 10^-6 erg/cm2.
The 1-sec peak photon flux measured from T+0.68 sec in the 15-150 keV band
is 4.2 +- 0.8 ph/cm2/sec. 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/614415/BA/