GCN Circular 16553

C. B. Markwardt (GSFC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),
J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), L. M. Z. Hagen (PSU),
H. A. Krimm (GSFC/USRA), A. Y. Lien (NASA/UMBC), D. M. Palmer (LANL),
T. Sakamoto (AGU), M. Stamatikos (OSU), J. Tueller (GSFC),
T. N. Ukwatta (MSU) (i.e. the Swift-BAT team):

Using the data set from T-239 to T+626 sec from the recent telemetry downlink,
we report further analysis of BAT GRB 140709A (trigger #603810)
(Hagen, et al., GCN Circ. 16546
Not found
 
 
).  The BAT ground-calculated position is
RA, Dec = 304.666, 51.222 deg which is
    RA(J2000)  =  20h 18m 39.9s
    Dec(J2000) = +51d 13' 17.8"
with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 61%.

The mask-weighted light curve shows a complex structure.  Burst activity begins
at T-50 sec, with a gradual rise to a peak at T+0 sec, punctuated by several
subsidiary peaks.  Then there is a return to near background by T+8 sec,
followed by a second main peak at T+15 sec.  There are additional smaller and
softer peaks centered at T+55 and T+75 sec. T90 (15-350 keV) is 98.6 +- 7.7 sec
(estimated error including systematics).

The time-averaged spectrum from T-46.1 to T+93.4 sec is best fit by a power law
with an exponential cutoff.  This fit gives a photon index 1.23 +- 0.27,
and Epeak of 78.0 +- 20.4 keV (chi squared 57.80 for 56 d.o.f.).  For this
model the total fluence in the 15-150 keV band is 5.2 +- 0.2 x 10^-6 erg/cm2
and the 1-sec peak flux measured from T+15.48 sec in the 15-150 keV band is
3.1 +- 0.3 ph/cm2/sec.  A fit to a simple power law gives a photon index
of 1.74 +- 0.06 (chi squared 69.09 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/603810/BA/