{
  "bibcode": "2006GCN..5403....1B",
  "body": "L. Barbier (GSFC),  S. Barthelmy (GSFC), J. Cummings (GSFC/ORAU),\nE. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (BYU-Idaho),\nM. Koss (GSFC/UMD), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD),\nD. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/ORAU),\nG. Sato (GSFC/JSPS/USRA), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC),\non behalf of the Swift-BAT team:\n\nUsing the data set from T-240 to T+963 sec from the recent telemetry\ndownlink, we report further analysis of BAT GRB 060805\n(trigger #222683)  (Ziaeepour, et al., GCN Circ. 5398).  The BAT\nground-calculated position is (RA,Dec) = 220.925, 12.576 deg\n{14h 43m 41.9s, 12d 34' 35.0\"} (J2000) +- 2.7 arcmin,\n(radius, sys+stat, 90% containment).  The partial coding was 96%.\n\nThe currently available event data record has several gaps, most significantly\nfrom T+14.3 to T+19.5 sec. Based on the available data, the mask weighted light\ncurve shows a single peak with a roughly square profile and a duration\nof ~6 sec.  Emission was only seen below 100 keV, which is consistent with the\nvery soft spectrum found. T90 (15-350 keV) is 5.4 +- 0.5 sec (estimated error\nincluding systematics).\n\nThe time-averaged spectrum from T-1.6 to T+4.7 is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n2.23 +- 0.42. The fluence in the 15-150 keV band is 7.4 +- 2.0 x 10^-8 erg/cm2.\nThe 1-sec peak photon flux measured from T+0.71 sec in the 15-150 keV\nband is 0.3 +- 0.1 ph/cm2/sec.  All the quoted errors are at the 90%\nconfidence level.",
  "circularId": 5403,
  "createdOn": 1154795288000,
  "email": "krimm@milkyway.gsfc.nasa.gov",
  "subject": "GRB 060805: Swift-BAT Refined Analysis",
  "submitter": "Hans Krimm at NASA-GSFC  <krimm@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 060805"
}