GRB 051117***A***, Swift-BAT refined analysis
 
<somebody goes first>
<add the BA alphabetically>
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 (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-300 to T+302 sec from the recent telemetry downlink,
we report further analysis of BAT GRB 051117***A*** (trigger #164268)
(NAME, et al., GCN Circ. xxxx).  The BAT ground-calculated position is
RA, Dec = 228.401, 30.864 deg which is 
   RA(J2000)  =  15h 13m 36.2s 
   Dec(J2000) = +30d 51' 51.9" 
with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment).
The partial coding was 72%.
 
[Description about the mask-weighted light curve]
T90 (15-350 keV) is 140.6 +- 13.5 sec (estimated error including systematics).
 
The time-averaged spectrum from T-29.7 to T+156.4 sec is best fit by a simple
power-law model.  The power law index of the time-averaged spectrum is
1.82 +- 0.07.  The fluence in the 15-150 keV band is 4.4 +- 0.2 x 10^-06 erg/cm2.
The 1-sec peak photon flux measured from T+2.62 sec in the 15-150 keV band
is 0.9 +- 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/164268/BA/