{
  "bibcode": "2013GCN.14332....1V",
  "body": "G. Vianello (Stanford), J. McEnery (NASA/GSFC), M. Ohno (Hiroshima U.),\nJ Racusin and E. Troja (CRESST) report on behalf of the Fermi-LAT team:\n\nThe Fermi Large Area Telescope (LAT) detected emission from GRB 130325A\n(GBM trigger 130325203/385879917).\n\nThis burst was detected over a 1300 s integration following the GBM \ntrigger using\nthe P7SOURCE data class. This burst seems unusual because despite being \nwithin\nthe field of view of the LAT at the time of the GBM trigger, it was not \ndetected by\nthe LAT during the prompt phase, which lasted 10 s (GCN 14329).\n\nThe best LAT on-ground location is found to be RA, DEC 122.78, -18.90 \n(J2000)\nwith an error radius of 0.25 deg (68% containment, statistical error \nonly), this\nwas 51 deg from the LAT boresight at the time of the trigger and \ntriggered an\nautonomous repoint of the spacecraft at 04:52:31.48 UT.\n\nA Swift ToO has been submitted.\n\nThe Fermi LAT point of contact for this burst is Julie McEnery \n(julie.mcenery@nasa.gov).\n\nThe Fermi LAT is a pair conversion telescope designed to cover the energy\nband from 20 MeV to greater than 300 GeV. It is the product of an \ninternational\ncollaboration between NASA and DOE in the U.S. and many scientific \ninstitutions\nacross France, Italy, Japan and Sweden.",
  "circularId": 14332,
  "createdOn": 1364350348000,
  "email": "julie.e.mcenery@nasa.gov",
  "subject": "GRB 130325A: Fermi LAT detection",
  "submitter": "Julie McEnery at NASA/GSFC  <julie.e.mcenery@nasa.gov>",
  "eventId": "GRB 130325A"
}