GCN Circular 19592
Subject
GRB 160625A: Swift-BAT refined analysis
Date
2016-06-26T17:23:45Z (8 years ago)
From
Scott Barthelmy at NASA/GSFC <scott@lheamail.gsfc.nasa.gov>
S. D. Barthelmy (GSFC), J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC),
H. A. Krimm (GSFC/USRA), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC),
A. Maselli (INAF-IASFPA), D. M. Palmer (LANL), T. Sakamoto (AGU),
M. Stamatikos (OSU), T. N. Ukwatta (LANL)
(i.e. the Swift-BAT team):
Using the data set from T-240 to T+962 sec from the recent telemetry downlinks,
we report further analysis of BAT GRB 160625A (trigger #701503)
(Maselli, et al., GCN Circ. 19577). The BAT ground-calculated position is
RA, Dec = 176.939, -65.142 deg, which is
RA(J2000) = 11h 47m 45.3s
Dec(J2000) = -65d 08' 30.9"
with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 57%.
The mask-weighted light curve shows at least 7 peaks, the first starting
at ~T-35 sec, the brightest peak at ~T+36 sec, and the last peak ending at ~T+70 sec.
The peak mentioned in GCN Circ 19577 at T+170 sec is due to GRB 160625B (as suggested
by Kann, Circ 19579) and confirmed by our analysis.
T90 (15-350 keV) is 53.9 +- 3.1 sec (estimated error including systematics).
The time-averaged spectrum from T-15.04 to T+47.41 sec is best fit by a simple
power-law model. The power law index of the time-averaged spectrum is
2.08 +- 0.07. The fluence in the 15-150 keV band is 3.3 +- 0.1 x 10^-6 erg/cm2.
The 1-sec peak photon flux measured from T+35.07 sec in the 15-150 keV band
is 3.0 +- 0.2 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/701503/BA/