TITLE: GCN CIRCULAR NUMBER: 8783 SUBJECT: GRB 090107: Swift-BAT refined analysis DATE: 09/01/07 13:51:47 GMT FROM: Scott Barthelmy at NASA/GSFC G. Sato (ISAS), 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/UMD), D. M. Palmer (LANL), T. Sakamoto (GSFC/UMBC), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC), T. N. Ukwatta (GWU) (i.e. the Swift-BAT team): Using the data set from T-240 to T+962 sec from recent telemetry downlinks, we report further analysis of BAT GRB 090107 (trigger #339295) (Ukwatta, et al., GCN Circ. 8782). The BAT ground-calculated position is RA, Dec = 302.409, 4.744 deg, which is RA(J2000) = 20h 09m 38.2s Dec(J2000) = +04d 44' 37.9" with an uncertainty of 2.4 arcmin, (radius, sys+stat, 90% containment). The partial coding was 74%. The mask-weighted light curve shows two peaks. The first is about 1.2 sec wide and peaks at ~T+0.9 sec. The second is about 6 sec wide and peaks at ~T+11 sec. Because of the Sun observing constraint and because of a regular pre-planned target slew, the BAT has no data on this event past T+260 sec, until the next orbit. T90 (15-350 keV) is 12.2 +- 0.7 sec (estimated error including systematics). The time-averaged spectrum from T+0.2 to T+12.9 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.69 +- 0.27. The fluence in the 15-150 keV band is 2.3 +- 0.5 x 10^-7 erg/cm2. The 1-sec peak photon flux measured from T+0.30 sec in the 15-150 keV band is 1.1 +- 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/339295/BA/