{
  "bibcode": "2015GCN.17997....1M",
  "body": "K. P. Mooley, G. E. Anderson, R. P. Fender, T. D. Staley (University of \nOxford),\nA. J. van der Horst (George Washington University), A. Rowlinson (CASS)\n\nWe observed the position of GRB 150626B (McCauley et al., GCN 17966,\nGoad et al., GCN 17968) at 16 GHz with the Arcminute Microkelvin Imager\n(AMI-LA) at 2015 June 26.85, June 27.58, and July 03.56 UT, corresponding\nto 0.01 days, 0.73 days and 6.71 days post-burst respectively. The GRB\nflux densities at these three epochs were <0.19 mJy (3 sigma upper limit),\n0.17+/-0.05 mJy (marginal detection), and 0.29+/-0.06 mJy (confirmed \ndetection)\nrespectively.\n\nFurther AMI monitoring is ongoing. We thank the AMI scheduling team for\ncarrying out these observations.",
  "circularId": 17997,
  "createdOn": 1436278347000,
  "email": "kunal.mooley@physics.ox.ac.uk",
  "subject": "GRB 150626B: AMI 16 GHz detection of the radio counterpart",
  "submitter": "Kunal Mooley at Oxford U  <kunal.mooley@physics.ox.ac.uk>",
  "eventId": "GRB 150626B"
}