{
  "bibcode": "2016GCN.19892....1M",
  "body": "K. P. Mooley, T. D. Staley, R. P. Fender (Oxford), G. E. Anderson \n(Curtin), T. Cantwell (Manchester), C. Rumsey, D. Titterington, S. H. \nCarey, J. Hickish, Y. C. Perrott, N. Razavi-Ghods, P. Scott (Cambridge), \nK. Grainge, A. Scaife (Manchester)\n\nWe observed the Fermi/LAT GRB 160816A (Racusin et al., GCN 19802) with \nthe AMI Large Array at 15 GHz on 2016 Aug 18.02, Aug 19.06, and Sep \n03.02 (UT) as part of the 4pisky program. We detect a possible radio \nafterglow (consistent with the XRT location; Kennea et al., GCN 19806) \nin the second epoch with a peak flux density of 129+/-32 uJy, and 3sigma \nupper limits of 111 uJy and 168 uJy in the first and third epochs \nrespectively.\n\nWe thank the AMI staff for scheduling these observations. The AMI-GRB \ndatabase is a log of all GRB follow up observations with the AMI, and is \navailable at http://4pisky.org/ami-grb/.",
  "circularId": 19892,
  "createdOn": 1473106911000,
  "email": "kunal.mooley@physics.ox.ac.uk",
  "subject": "GRB 160816A: Possible radio afterglow detection at 15 GHz with AMI",
  "submitter": "Kunal Mooley at Oxford U  <kunal.mooley@physics.ox.ac.uk>",
  "eventId": "GRB 160816A"
}