{
  "bibcode": "2006GCN..5091....1B",
  "body": "L. Barbier (GSFC), S. Barthelmy (GSFC), J. Cummings (GSFC/ORAU), \nH. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL),\nT. Sakamoto (GSFC/ORAU), J. Tueller (GSFC)\non behalf of the Swift-BAT team:\n\nNow having recieved the full downlinked data that fills in the gaps\n(Tueller et al, GCN 5090), we report the updated refined analysis\non Swift-BAT GRB 060507 (trigger 208870).\n\nThe lightcurve description in GCN 5090 does not change, nor does T90.\n \nThe time-averaged spectrum from T-10.2 to T+192.4 is best fit by \na simple power-law model.  The power law index of the time-averaged\nspectrum is 1.83 +- 0.09.  The fluence in the 15-150 keV band is\n4.5 +- 0.2 x 10^-6 erg/cm2.  The 1-sec peak photon flux measured\nfrom T+1.24 sec in the 15-150 keV band is 1.3 +- 0.2 ph/cm2/sec.\nAll the quoted errors are at the 90% confidence level.",
  "circularId": 5091,
  "createdOn": 1147123087000,
  "email": "Scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 060507:  Final Refined analysis of the Swift-BAT burst",
  "submitter": "Scott Barthelmy at NASA/GSFC  <Scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 060507"
}