GCN Circular 16438

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

  Using the data set from T-61 to T+302 sec from the recent telemetry downlink,
we report further analysis of BAT GRB 140622A (trigger #602278) (D'Elia, et al.,
GCN Circ. 16433
Not found
 
 
).  The BAT ground-calculated position is
RA, Dec = 317.153, -14.412 deg which is

    RA(J2000)  =  21h 08m 36.7s
    Dec(J2000) = -14d 24' 44.6"

with an uncertainty of 2.5 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 57%.

The mask-weighted light curve shows a single FRED peak.  T90 (15-350 keV) is
0.13 +- 0.04 sec (estimated error including systematics).

The time-averaged spectrum from T-0.02 to T+0.13 sec is best fit (chisqr = 0.63) by
a black body spectrum with kT = 11.6 � 1.8 keV.  A simple power-law model is a
relatively poor fit (chisqr 1.13), with a photon index of 3.08 � 0.29.  A power-law
with an exponential cutoff at 44 � 8 keV nominally fits the data almost as well
(chisqr = 0.64) as the black body fit, but the power-law index below the cutoff
energy and the normalization are poorly defined.  The fluence in the 15-150 keV
band using the black body spectrum is (2.7 � 0.5) x 10^-08 erg/cm2.  The 1-sec
peak photon flux measured from T-0.45 sec in the 15-150 keV band is
0.6 � 0.2 ph/cm2/sec.  All the quoted errors are at the 90% confidence level.

 From the BAT spectrum, this event does not appear to be a short hard burst.  The
quickly fading X-ray lightcurve, however (to be reported in a later circular), does
appear consistent with a SHB, and does not appear to be similar to the lightcurves
of SGRs or other Galactic sources.

The results of the batgrbproduct analysis are available at
http://gcn.gsfc.nasa.gov/notices_s/602278/BA/