{
  "bibcode": "2013GCN.15016....1S",
  "body": "M. Stamatikos (OSU), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),\nJ. R. Cummings (GSFC/UMBC),E. E. Fenimore (LANL), N. Gehrels (GSFC),\nH. A. Krimm (GSFC/USRA), A. Y. Lien (NASA/GSFC/ORAU), C. B. Markwardt (GSFC),\nF. E. Marshall (NASA/GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU),\nG. Sato (ISAS), J. Tueller (GSFC), T. N. Ukwatta (MSU)\n(i.e. the Swift-BAT team):\n  \nUsing the data set from T-239 to T+963 sec from the recent telemetry downlink,\nwe report further analysis of BAT GRB 130719A (trigger #562625) (Marshall,\net al., GCN Circ. 15012).  The BAT ground-calculated position is\nRA, Dec = 89.038, -11.591 deg which is\n    RA(J2000)  =  05h 56m 09.2s\n    Dec(J2000) = -11d 35' 29.0\"\nwith an uncertainty of 1.9 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 50%.\n  \nThe mask-weighted light curve shows a single weak approximately FRED peak.\nT90 (15-350 keV) is 177.7 +- 20.5 sec (estimated error including systematics).\n  \nThe time-averaged spectrum from T+6.2 to T+205.2 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.63 +- 0.17.  The fluence in the 15-150 keV band is 2.3 +- 0.2 x 10^-06 erg/cm2.\nThe 1-sec peak photon flux measured from T+82.68 sec in the 15-150 keV band\nis 0.6 +- 0.2 ph/cm2/sec.  All the quoted errors are at the 90% confidence\nlevel.\n  \nThe results of the batgrbproduct analysis are available at\nhttp://gcn.gsfc.nasa.gov/notices_s/562625/BA/",
  "circularId": 15016,
  "createdOn": 1374492278000,
  "email": "james.r.cummings@nasa.gov",
  "subject": "GRB 130719A, Swift-BAT refined analysis",
  "submitter": "Jay R. Cummings at NASA/GSFC/Swift  <james.r.cummings@nasa.gov>",
  "eventId": "GRB 130719A"
}