GCN Circular 29612
Subject
GRB 210306B: Swift-BAT refined analysis
Date
2021-03-07T13:14:21Z (3 years ago)
From
Takanori Sakamoto at AGU <tsakamoto@phys.aoyama.ac.jp>
A. Y. Lien (GSFC/UMBC), S. D. Barthelmy (GSFC), J. R. Cummings (CPI),
A. D'Ai (INAF-IASFPA), H. A. Krimm (NSF), S. Laha (GSFC/UMBC),
C. B. Markwardt (GSFC), 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 downlink,
we report further analysis of BAT GRB 210306B (trigger #1036024)
(D'Ai, et al., GCN Circ. 29601). The BAT ground-calculated position is
RA, Dec = 331.813, 10.152 deg which is
RA(J2000) = 22h 07m 15.1s
Dec(J2000) = +10d 09' 06.8"
with an uncertainty of 1.9 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 21%.
The BAT light curve showed a multi-peaked structure that starts at T-2 s and
ends at ~T+25 s. T90 (15-350 keV) is 24.32 +- 2.45 sec (estimated error
including systematics).
The time-averaged spectrum from T-2.42 to T+24.63 sec is best fit by a simple
power-law model. The power law index of the time-averaged spectrum is
1.38 +- 0.20. The fluence in the 15-150 keV band is 1.7 +- 0.2 x 10^-6 erg/cm2.
The 1-sec peak photon flux measured from T+1.04 sec in the 15-150 keV band
is 2.4 +- 0.5 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/1036024/BA/