{
  "bibcode": "2006GCN..4531....1B",
  "body": "S. Barthelmy (GSFC), L. Angelini (GSFC-JHU), L. Barbier (GSFC),\nM. Chester (PSU), J. Cummings (GSFC/NRC), E. Fenimore (LANL),\nN. Gehrels (GSFC), D. Hullinger (GSFC/UMD), H. Krimm (GSFC/USRA),\nC. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC),\nT. Sakamoto (GSFC/NRC), G. Sato (ISAS), J. Tueller (GSFC)\non behalf of the Swift-BAT team:\n\nUsing the data set from T-299 to T+303 sec from the recent telemetry downlink,\nwe report further analysis of BAT GRB 060116 (trigger #177533)\n(Compana, et al., GCN 4519).  The BAT ground-calculated position is\nRA,Dec = 84.699,-5.449 deg {5h 38m 47.8s, -5d 26' 56.0\"} (J2000) +- 1.7 arcmin,\n(radius, sys+stat, 90% containment).  The partial coding was 20%.\n \nThe lightcuve has one peak centered on T+20 sec.  There is very weak emission\nstarting as early as ~T-40 sec.  The event is over by ~T+90 sec.\nT90 (15-350 keV) is (113 +- 10) sec (estimated error including systematics).\n \nThe power law index of the time-averaged spectrum is 1.44 +- 0.18.\nThe fluence in the 15-150 keV band is (2.6 +- 0.3) x 10^-06 erg/cm2.\nThe 1-sec peak photon flux measured from T+36.08 sec in the 15-150 keV\nband is (1.1 +- 0.3) ph/cm2/sec.  All the quoted errors are at the 90%\nconfidence level.",
  "circularId": 4531,
  "createdOn": 1137467736000,
  "email": "Scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 060116:  Refined analysis of the Swift-BAT burst",
  "submitter": "Scott Barthelmy at NASA/GSFC  <Scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 060116"
}