{
  "bibcode": "2008GCN..7937....1M",
  "body": "C. Markwardt (GSFC/UMD), S. D. Barthelmy (GSFC),\nW. Baumgartner (GSFC/UMBC),A. Copete (Harvard), J. Cummings (GSFC/UMBC),\nE. Fenimore (LANL), N. Gehrels (GSFC), J. Grindlay (Harvard),\nH. Krimm (GSFC/USRA),K. McLean (GSFC/UMD), D. Palmer (LANL),\nT. Sakamoto (GSFC/UMBC), G. Sato (ISAS), M. Stamatikos (GSFC/ORAU),\nJ. Tueller (GSFC), T. Ukwatta (GWU)\nOn behalf of the Swift-BAT and BATSS teams:\n\n\nUsing the event data from T-83 to T+37 seconds, we present further\nanalysis of GRB 080702B.  The best-determined position in BAT was\nRA, Dec 355.616,  -5.424 (J2000) or\n\nRA = 23h 42m 27.8s\nDec = -05d 25' 26.4\"\n\nwith an uncertainty of 3.5 arcmin (radius, sys+stat, 90% containment).\nThe partial coding was varying (the entire burst occurred during a\npreplanned Swift slew manuever), but was approximately 60% during\nthe entire burst.\n\nThe mask-weighted light curve shows a single peak with a few\nsecond rise, and slow decay.  T90 was 20 +- 3 seconds (estimated\nerror including systematics). \n\nThe time-averaged spectrum from T-2 to T+21 seconds is best fit by a\nsimple power-law model.  The power law index of the time-averaged\nspectrum is 1.44 � 0.13.  The fluence in the 15-150 keV band was\n(5.0 � 0.9) x 10^-7 ergs/cm2/s.  The 1-sec peak photon flux measured\nfrom T+4 sec in the 15-150 keV band was 0.5 +- 0.1 photons/cm2/s. \nAll the quoted errors are at the 90% confidence level.",
  "circularId": 7937,
  "createdOn": 1215115446000,
  "email": "jayc@milkyway.gsfc.nasa.gov",
  "subject": "GRB 080702B Swift-BAT refined analysis",
  "submitter": "Jay R. Cummings at NASA/GSFC/Swift  <jayc@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 080702B"
}