{
  "bibcode": "2015GCN.18406....1O",
  "body": "M. Ohno (Hiroshima U.), E. Bissaldi (INFN Bari), G. Vianello (Stanford University),\nD. Kocevski (NASA/GSFC)  and F. Longo (University & INFN Trieste)\nreport on behalf of the Fermi-LAT team:\n\nAt 09:54:57.83 on October 06, 2015, Fermi-LAT detected  high-energy emission\nfrom GRB 151006A, which was also detected by Fermi-GBM (trigger 465818101;\nRoberts et al. GCN 18404)  and Swift-BAT  (Kocevski et al. GCN 18398).\n\nThe GBM location was initially inside the LAT field of view  at an angle of ~30 degrees\nto the LAT boresight.  Using the LAT Low Energy (LLE) data selection, over 400 counts above\nbackground were detected within a 30 s interval coinciding with the time of the GBM emission.\nThis data selection has insufficient spatial resolution to provide a reliable LAT localization.\nProcessing and analysis of standard data is ongoing.\n\nThe Fermi LAT point of contact for this burst is\nMasanori Ohno (ohno@hep01.hepl.hiroshima-u.ac.jp<mailto:ohno@hep01.hepl.hiroshima-u.ac.jp>).\n\nThe Fermi-LAT is a pair conversion telescope designed to cover\nthe energy band from 20 MeV to greater than 300 GeV.\nIt is the product of an international collaboration between\nNASA and DOE in the U.S. and many scientific institutions\nacross France, Italy, Japan and Sweden.",
  "circularId": 18406,
  "createdOn": 1444166013000,
  "email": "daniel.kocevski@nasa.gov",
  "subject": "GRB 151006A: Fermi-LAT detection",
  "submitter": "Daniel Kocevski at GSFC  <daniel.kocevski@nasa.gov>",
  "eventId": "GRB 151006A"
}