{
  "bibcode": "2014GCN.17022....1V",
  "body": "G.Vianello (Stanford U.), D. Kocevski (NASA/GSFC),\nV. Connaughton (UAH), M. Arimoto (Tokyo Tech), S. Guiriec (NASA/GSFC)\n\nAt 12:51:39.26 on November 2, 2014, Fermi-LAT detected faint high-energy\nemission from the short GRB 141102A, which was also detected by Fermi-GBM\n(Zhang et al., GCN 17021) and Swift/BAT (Cummings et al., GCN 17020)\nand initiated an autonomous repoint of the spacecraft.  The high-energy emission\nwas detected during the ~300 s interval following the GBM trigger.\n\nThe best LAT on-ground location is found to be\n\n(RA, Dec.) = 208.6, -47.7 deg\n\nwith an error radius of 0.6 deg (90% containment, statistical error\nonly), which is compatible\nwith the position measured by Swift/BAT (Cummings et al., GCN 17020).\n\nFurther follow up is encouraged.\n\nThe Fermi-LAT point of contact for this burst is\nMakoto Arimoto (arimoto@hp.phys.titech.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": 17022,
  "createdOn": 1414989277000,
  "email": "giacomov@slac.stanford.edu",
  "subject": "GRB 141102A: Fermi-LAT detection",
  "submitter": "Giacomo Vianello at SLAC  <giacomov@slac.stanford.edu>",
  "eventId": "GRB 141102A"
}