TITLE: GCN CIRCULAR NUMBER: 14011 SUBJECT: GRB 121128A, Swift-BAT refined analysis DATE: 12/11/28 14:32:00 GMT FROM: Hans Krimm at NASA-GSFC D. M. Palmer (LANL),S. D. Barthelmy (GSFC),W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (GSFC/UMBC),E. E. Fenimore (LANL),N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA),C. B. Markwardt (GSFC), S. R. Oates (UCL-MSSL), T. Sakamoto (AGU), G. Sato (ISAS), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (MSU) (i.e. the Swift-BAT team): Using the data set from T-119 to T+195 sec from the recent telemetry downlink, we report further analysis of BAT GRB 121128A (trigger #539866) (Oates, et al., GCN Circ. 14007). The BAT ground-calculated position is RA, Dec = 300.589, 54.301 deg which is RA(J2000) = 20h 02m 21.3s Dec(J2000) = +54d 18' 02.6" with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment). The partial coding was 88%. The mask-weighted light curve shows a complex, multi-peaked structure. The burst began with a faint precursor at ~T-4 sec. The main emission started at ~T+10 sec, peaked at T+22 sec and continued until just after T+40 sec, with weak emission extending out to ~T+70 sec. T90 (15-350 keV) is 23.3 +- 1.6 sec (estimated error including systematics). The time-averaged spectrum from T-0.00 to T+41.69 sec is best fit by a power law with an exponential cutoff. This fit gives a photon index 1.32 +- 0.18, and Epeak of 64.5 +- 6.8 keV (chi squared 33.43 for 56 d.o.f.). For this model the total fluence in the 15-150 keV band is 6.9 +- 0.4 x 10^-06 erg/cm2 and the 1-sec peak flux measured from T+21.68 sec in the 15-150 keV band is 12.9 +- 0.4 ph/cm2/sec. A fit to a simple power law gives a photon index of 1.86 +- 0.04 (chi squared 62.32 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/539866/BA/