{
  "bibcode": "2014GCN.16048....1V",
  "body": "G. Vianello (Stanford U.), D. Kocevski (NASA/Goddard), and J. Racusin (NASA/Goddard) report on behalf of the Fermi-LAT team:\n\nAt 04:19:54.47 UT on March 30, 2014, Fermi-LAT detected high-energy emission from GRB 140330A, which was also detected by Fermi-GBM (trigger 417845997).\n\nThe best LAT on-ground location is found to be\n\nRA, Dec 325.59, -64.30 (J2000)\n\nwith an error radius of 0.2 deg (90% containment, statistical error only). This was within 15 deg from the LAT boresight at the time of the trigger.  More than 10 photons above 100 MeV and 2 photons above 1 GeV are observed within 6000 seconds after the GBM trigger. The highest-energy photon is a 4.5 GeV event, which is observed 252 seconds after the GBM trigger.\n\nA Swift ToO has been requested and accepted for this burst.\n\nThe Fermi-LAT point of contact for this burst is Daniel Kocevski (daniel.kocevski@<mailto:xxxx@xxx.xxx>nasa.gov<http://nasa.gov>).\n\nThe Fermi-LAT is a pair conversion telescope designed to cover the energy band from 20 MeV to greater than 300 GeV. It is the product of an international collaboration between NASA and DOE in the U.S. and many scientific institutions across France, Italy, Japan and Sweden.",
  "circularId": 16048,
  "createdOn": 1396238734000,
  "email": "daniel.kocevski@nasa.gov",
  "subject": "GRB 140330A: Fermi-LAT Detection",
  "submitter": "Daniel Kocevski at GSFC  <daniel.kocevski@nasa.gov>",
  "eventId": "GRB 140330A"
}