{
  "bibcode": "2015GCN.17797....1A",
  "body": "G. E. Anderson, R. P. Fender, T. D. Staley, K. Mooley (University of Oxford),\nA. J. van der Horst (George Washington University), A. Rowlinson (CASS)\n\nWe re-observed the position of GRB 150413A (Markwardt et al., GCN 17688,\nIvanov et al., GCN 17689) at 15 GHz with the Arcminute Microkelvin Imager\n(AMI-LA) following the  possible detection of its radio counterpart reported\nin Anderson et al., GCN 17708. This observation took place on 2015 April\n15.798 to 15.964 UT, corresponding to 2.2 days post-burst, resulting in a flux\n of 0.20 +/- 0.04 mJy. A follow-up AMI observation on 2015 April 23.947 to\n24.114 UT, corresponding to 10.4 days post-burst, did not detection the radio\ncounterpart with a 3 sigma upper limit of 0.1 mJy. We therefore confirm that\nthe coincident radio source reported in Anderson et al., GCN 17708 is the\nradio counterpart to GRB 150413A.\n\nWe thank the AMI staff for scheduling these observations.",
  "circularId": 17797,
  "createdOn": 1430485708000,
  "email": "Gemma.Anderson@physics.ox.ac.uk",
  "subject": "GRB 150413A: AMI 15 GHz confirmation of radio counterpart",
  "submitter": "Gemma Anderson at U of Oxford  <Gemma.Anderson@physics.ox.ac.uk>",
  "eventId": "GRB 150413A"
}