{
  "bibcode": "2020GCN.27931....1O",
  "body": "M. Ohno (Hiroshima Univ.), M. Kovacevic (INFN Perugia), E. Bissaldi\n(Politecnico & INFN Bari), M. Axelsson (KTH & Stockholm Univ.) and F. Longo\n(University and INFN, Trieste) report on behalf of the Fermi-LAT\nCollaboration:\n\nOn June 13, 2020, Fermi-LAT detected high-energy emission from\nGRB 200613A, which was also detected by Fermi-GBM at T0 = 05:30:08 UT (GCN\n27926, Bissaldi et al. GCN 27930).\n\nThe GRB is detected at high energy (>100 MeV) by Fermi-LAT at a location\nof:\n\nRA, Dec = 153.03, 45.85 (degrees, J2000) with an error radius of 0.14 deg\n(90% containment, statistical error only).\n\nThis was ~29 deg from the LAT boresight when observations started, and is\n~5.9 deg from the GBM final ground position.\n\nThe photon flux above 100 MeV in the time interval 0 - 10.000 s after the\nGBM trigger is 6.6e-07 +/- 3.6e-07 ph/cm2/s.\n\nThe estimated photon index above 100 MeV is -1.73 +/- 0.36. The\nhighest-energy photon is a 7.6 GeV event which is observed ~6.2 ks after\nthe GBM trigger.\n\nA Swift ToO has been approved for this burst.\n\nThe Fermi-LAT point of contact for this burst is Masanori Ohno (\nohno@astro.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": 27931,
  "createdOn": 1592067986000,
  "email": "ohno@astro.hiroshima-u.ac.jp",
  "subject": "GRB 200613A: Fermi-LAT detection",
  "submitter": "Masanori Ohno at Hiroshima University  <ohno@astro.hiroshima-u.ac.jp>",
  "eventId": "GRB 200613A"
}