{
  "bibcode": "2014GCN.16001....1Y",
  "body": "G. Younes (USRA/MSFC) and V. Connaughton (UAH) report on behalf of the Fermi GBM Team:\n\n\"At 02:12:46.11 UT on 19 March 2014, the Fermi Gamma-Ray Burst Monitor\nTriggered and located GRB 140320A (trigger 416974369/140320092), which\nwas  also detected by Swift (Cannizzo et al. 2014, GCN 16000).\n\nThe double peaked structure seen with BAT, with ~150 s separation, and\nreported by Cannizzo et al. is also visible with FERMI/GBM, however, a\nlocation analysis with GBM shows that the two peaks are unrelated. The\nfirst peak (trigger peak) is most likely due to a short/hard GRB located at\nRA~284.6 DEC~-5.0 deg, consistent with the BAT location. The second peak,\n150 s after the trigger, is much softer and locates at RA~265.0 DEC~-28.0,\nthe location of the bursting pulsar GRO J1744-28, which is currently active.\n\nHence, we encourage multi-wavelength follow-up observations of this candidate short/hard GRB.�",
  "circularId": 16001,
  "createdOn": 1395291301000,
  "email": "younes.ge@gmail.com",
  "subject": "GRB 140320A: Fermi GBM observations suggest a short GRB",
  "submitter": "George A. Younes at USRA/NASA/MSFC  <younes.ge@gmail.com>",
  "eventId": "GRB 140320A"
}