{
  "bibcode": "2013GCN.14675....1O",
  "body": "Nicola Omodei (Stanford) and Julie McEnery (GSFC) report on behalf of \nthe Fermi-LAT team:\n\nAt 13:54:37.53 UT on 18 May 2013, Fermi LAT detected high energy \nemission from GRB 130518A, which was also detected by Fermi-GBM (trigger \n390578080 /130518580, GCN 14674).\n\nThe best LAT on-ground location is found to be RA=355.809, DEC=47.641 \n(J2000) with an error radius of 0.34 deg (68% containment, statistical \nerror only).\n\nThe burst was about 43 deg from the LAT boresight at the time of the \ntrigger.\nThe data from the Fermi LAT shows emission lasting approximately 100 \nseconds with a TS of 50.\nMulti-peaked emission lasting roughly 40 seconds can be seen using the \nnon-standard LAT Low Energy (LLE) with a significance of ~15 sigma.\n\nA Swift TOO request has been submitted.\n\nThe Fermi LAT point of contact for this burst is Sara Cutini \n(sara.cutini@asdc.asi.it).\n\nThe Fermi LAT is a pair conversion telescope designed to cover the \nenergy band from 20 MeV to greater than 300 GeV. It is the product of an \ninternational collaboration between NASA and DOE in the U.S. and many \nscientific institutions across France, Italy, Japan and Sweden.",
  "circularId": 14675,
  "createdOn": 1368910952000,
  "email": "julie.e.mcenery@nasa.gov",
  "subject": "GRB 130518A: Fermi LAT detection",
  "submitter": "Julie McEnery at NASA/GSFC  <julie.e.mcenery@nasa.gov>",
  "eventId": "GRB 130518A"
}