{
  "bibcode": "2006GCN..5256....1B",
  "body": "S. Barthelmy (GSFC), L. Barbier (GSFC), J. Cummings (GSFC/UMD),\nE. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (BYU-Idaho),\nH. Krimm (GSFC/USRA), M. Koss (GSFC/UMD),\nC. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC),\nT. Sakamoto (GSFC/ORAU), G. Sato (GSFC/ISAS),\nM. Stamatikos (GSFC/ORAU), J. Tueller (GSFC), on behalf of the Swift-BAT team:\n\nUsing the data set from T-120 s to T+180 sec from the recent telemetry\ndownlink, we report further analysis of BAT GRB 060614 (trigger #214805)\n(Parsons et al 2006, GCN 5252). The BAT ground-calculated position is\n(RA,Dec) = 320.88, -53.035  { 21h 23m 31.8s , -53d 02' 04.4\" }\n[deg; J2000]+-1.0 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 16%.\n\nThe BAT mask-weighted light curve shows an unusual multi-peaked burst\nstructure that begins with an initial bright, ~ 6 second wide peak\nfollowed by a set of 5 fainter and somewhat softer peaks that increase\nin intensity. After about T+45s, the light curve shows a smooth slope\ndown to the baseline level for a total duration of T90 (15-350 keV) =\n102 +/- 5 sec.\n\nThe power law index of the time-averaged spectrum is 2.13 +- 0.04. The\nfluence in the 15-150 keV band is 2.17+- 0.04 x 10^-5 erg/cm2.  The\n1-sec peak photon flux measured from T - 1.3 sec in the 15-150 keV band\nis 11.6 +- 0.7 ph/cm2/sec.  All the quoted errors are at the 90%\nconfidence level.",
  "circularId": 5256,
  "createdOn": 1150315849000,
  "email": "krimm@milkyway.gsfc.nasa.gov",
  "subject": "GRB 060614: Swift-BAT refined analysis",
  "submitter": "Hans Krimm at NASA-GSFC  <krimm@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 060614"
}