TITLE: GCN CIRCULAR NUMBER: 8297 SUBJECT: GRB 080928, Swift-BAT final refined analysis DATE: 08/09/29 12:41:32 GMT FROM: Scott Barthelmy at NASA/GSFC E. Fenimore (LANL), S. D. Barthelmy (GSFC), W. Baumgartner (GSFC/UMBC), J. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/UMBC), G. Sato (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+494 sec from the recent telemetry downlink, we report further analysis of BAT GRB 080928 (trigger #326115) (Sakamoto, et al., GCN Circ. 8292). The BAT ground-calculated position is RA, Dec = 95.061, -55.176 deg, which is RA(J2000) = 06h 20m 14.6s Dec(J2000) = -55d 10' 34.8" with an uncertainty of 2.3 arcmin, (radius, sys+stat, 90% containment). The partial coding was 84%. With all the data downlinked, the mask-weighted light curve shows that BAT triggered on a weak blip that occurred long before the main emission of this burst. The initial peak started at ~T-10 sec, peaked at ~T_zero, and returned to baseline around T+30 sec. Then a second, slightly larger peak, started at ~T+50 and ended at ~T+130 sec. Then the main emission started at ~T+170, with a pair of peaks at ~T+205 and ~T+215 sec. The emaission tails down to almost background at T+400 sec at which time Swift started to enter the SAA and the errors on the flux become large. T90 (15-350 keV) is 280 +- 30 sec (estimated error including systematics). The time-averaged spectrum from T+51.1 to T+381.5 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.77 +- 0.12. The fluence in the 15-150 keV band is 2.5 +- 0.2 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+202.83 sec in the 15-150 keV band is 2.1 +- 0.1 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/326115/BA/