TITLE: GCN CIRCULAR NUMBER: 13002 SUBJECT: GRB 120302A, Swift-BAT refined analysis DATE: 12/03/02 21:11:23 GMT FROM: Takanori Sakamoto at NASA/GSFC T. Sakamoto (GSFC/UMBC), C. Graziani (U of Chicago), J. R. Cummings (GSFC/UMBC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), E. E. Fenimore (LANL), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), C. B. Markwardt (GSFC), D. M. Palmer (LANL), G. Sato (ISAS), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (MSU) (i.e. the Swift-BAT team): Using the event data from T-220 to T+30 sec (T is the trigger time of the ground code which is 01:55:30.8 UT), we report further analysis of GRB 120302A (Sakamoto, et al., GCN Circ. 13000). The mask-weighted light curve created from the event data shows at least two peaks, the first starting and also peaking at ~T sec. The second starts at ~T+10 sec, peaks at ~T+13 sec, and ends at ~T+20 sec. Although there might be another weak episode starting at ~T+20 sec, it is hard to say conclusively because the event data ends at T+30 sec. From the BAT raw light curve, the duration of the event is 35-40 sec long. The spectrum extracted from T to T+30 sec is best fit by a simple power-law model. The power law index of the spectrum is 1.4 +- 0.3 (90% confidence). The fluence measured in this interval is 6.6 +- 1.3 x 10^-7 erg/cm2 (15-150 keV) and 1-sec peak flux measured from T sec in the 15-150 keV band is 0.6 +- 0.3 ph/cm2/s. All the quoted erros are at the 90% confidence level. Swift ToO has been approved and the observation is on-going.