TITLE: GCN CIRCULAR NUMBER: 7505 SUBJECT: GRB 080320, Swift-BAT refined analysis DATE: 08/03/22 14:06:04 GMT FROM: Scott Barthelmy at NASA/GSFC K. McLean (GSFC/UMD), S. D. Barthelmy (GSFC), J. Cummings (GSFC/UMBC), E. Fenimore (LANL), N. Gehrels (GSFC), D. Grupe (PSU), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/UMBC), G. Sato (GSFC/ISAS), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC), T. Ukwatta (GWU) (i.e. the Swift-BAT team): Using the data set from T-119 to T+183 sec from the telemetry downlinks, we report further analysis of BAT GRB 080320 (trigger #306858) (Grupe, et al., GCN Circ. 7473). The BAT ground-calculated position is RA, Dec = 177.763, 57.162 deg, which is RA(J2000) = 11h 51m 03.1s Dec(J2000) = +57d 09' 42.6" with an uncertainty of 1.8 arcmin, (radius, sys+stat, 90% containment). The partial coding was 93%. The mask-weighted light curve shows a FRED peak starting at ~T-5 sec, peaking at ~T+0, and ending at ~T+35 sec. There a possible (3 sigma) precursor peak at ~T-55 sec with a width of about 5 sec. T90 (15-350 keV) is 14 +- 2 sec (estimated error including systematics). The time-averaged spectrum from T-1.7 to T+13.8 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.70 +- 0.22. The fluence in the 15-150 keV band is 2.7 +- 0.4 x 10^-7 erg/cm2. The 1-sec peak photon flux measured from T+0.15 sec in the 15-150 keV band is 0.6 +- 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/306858/BA/