GCN Circular 7582
Subject
GRB 080409: Swift-BAT refined analysis
Date
2008-04-10T13:14:20Z (17 years ago)
From
Jay R. Cummings at NASA/GSFC/Swift <jayc@milkyway.gsfc.nasa.gov>
D. Palmer (LANL), S. D. Barthelmy (GSFC), W. Baumgartner (GSFC/UMBC) ,
J. Cummings (GSFC/UMBC), E. Fenimore (LANL), N. Gehrels (GSFC),
S. T. Holland (CRESST/USRA/GSFC), H. Krimm (GSFC/USRA),
C. Markwardt (GSFC/UMD), K. McLean (GSFC/UMD), A. Parsons (GSFC),
T. Sakamoto (GSFC/UMBC), G. Sato (GSFC/ISAS), M. Stamatikos (GSFC/ORAU),
J. Tueller (GSFC), T. Ukwatta (GWU)
(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 080409 (trigger #308812)
(Holland, et al., GCN Circ. 7573). The BAT ground-calculated position
is RA, Dec = 84.304, 5.078 deg which is
RA(J2000) = 05h 37m 12.9s
Dec(J2000) = +05d 04' 39.9"
with an uncertainty of 2.0 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 46%.
The mask-weighted light curve shows 3 well-separated peaks, at T-13,
T+0, and T+10 sec, that are about 1, 2, and, 2 sec wide respectively.
The first is much smaller than the others, the second at T+0 is the
largest. T90 (15-350 keV) is 20.2 +- 8.0 sec (estimated error including
systematics).
The time-averaged spectrum from T-13.1 to T+10.4 sec is best fit by a
simple power-law model. The power law index of the time-averaged
spectrum is 2.10 +- 0.20. The fluence in the 15-150 keV band is
6.1 +- 0.7 x 10^-07 erg/cm2. The 1-sec peak photon flux measured from
T+0.00 sec in the 15-150 keV band is 3.7 +- 0.3 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/308812/BA/