TITLE: GCN CIRCULAR NUMBER: 13851 SUBJECT: Swift-BAT refined analysis of the SGR 1806-20 outburst (trigger 535747) DATE: 12/10/11 20:59:24 GMT FROM: Scott Barthelmy at NASA/GSFC S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (GSFC/UMBC), E. E. Fenimore (LANL), N. Gehrels (GSFC), S. T. Holland (STScI), H. A. Krimm (GSFC/USRA), C. B. Markwardt (GSFC), D. M. Palmer (LANL), 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-239 to T+807 sec from recent telemetry downlinks, we report further analysis of BAT trigger (#535747) from SGR1806-20 (Barthelmy, et al., GCN Circ. 13844). The BAT ground-calculated position is RA, Dec = 272.172, -20.448 deg, which is RA(J2000) = 18h 08m 41.2s Dec(J2000) = -20d 26' 52.3" with an uncertainty of 2.4 arcmin, (radius, sys+stat, 90% containment). The partial coding was 98%. The mask-weighted light curve shows a single FRED-like pulse starting at ~T-0.05 sec, peaking at ~T+0.1 sec, with a long low-level tail out to T+0.5 or T+1.0 sec. T90 (15-350 keV) is 0.67 +- 0.16 sec (estimated error including systematics). There is no evidence of additional outbursts in the post 800 sec of the lightcurve at the 0.13 ph/cm2/sec upper limit. The time-averaged spectrum from T-0.05 to T+0.68 sec fit by a simple power-law model shows the power law index of 2.38 +- 0.42 (chi squared 69.8 for 57 d.o.f.). The fluence in the 15-150 keV band is 3.3 +- 0.8 x 10^-8 erg/cm2. The 1-sec peak photon flux measured from T-0.18 sec in the 15-150 keV band is 0.6 +- 0.1 ph/cm2/sec. A single blackbody fit to the time-averaged spectrum shows the blackbody temperature of 8.1 +- 2.1 keV (chi squared 71.9 for 59 d.o.f.). A thermal bremsstrahlung model fit shows the temperature of 38.3 +- 21.6 keV (chi squared 68.1 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/535747/BA/