{
  "bibcode": "2017GCN.22069....1M",
  "body": "K. P. Mooley (Hintze Fellow, Oxford), T. D. Staley, R. P. Fender \n(Oxford), G. E. Anderson (Curtin), T. Cantwell (Manchester), D. \nTitterington, S. H. Carey, J. Hickish, Y. C. Perrott, N. Razavi-Ghods, \nP. Scott (Cambridge), K. Grainge, A. Scaife (Manchester)\n\nThe AMI Large Array robotically triggered on the Swift alerts for the Be \nX-ray Binary, Swift J0243.6+6124 (e.g. Beardmore et al., GCN 22020; \nKennea et al., ATel 10809; Kouroubatzakis et al., ATel 10822; also has \nFermi alerts: Briggs et al., GCN 22047) as part of the 4pisky program, \nand several follow up observations were subsequently obtained. Our \nobservations at 15 GHz are tabulated below. Our upper limit on 11 Oct \n2017 (MJD 58037) is consistent with that reported by van den Eijnden et \nal. (ATel 10886).\n\n-----------------------\nMJD������������ Flux Density\n-----------------------\n58029.16�� <170 uJy\n58032.04�� <140 uJy\n58037.01�� <140 uJy\n58044.05�� 372+/-67 uJy (likely a detection)\n58045.00�� <300 uJy\n-----------------------\n\nWe thank the AMI staff for scheduling these observations.More \nobservations are ongoing.",
  "circularId": 22069,
  "createdOn": 1509286668000,
  "email": "kunal.mooley@physics.ox.ac.uk",
  "subject": "AMI-LA observations of the new Be X-ray binary Swift J0243.6+6124",
  "submitter": "Kunal Mooley at Oxford U  <kunal.mooley@physics.ox.ac.uk>"
}