{
  "bibcode": "2014GCN.16725....1A",
  "body": "G. E. Anderson, T. D. Staley, R. P. Fender (University of Oxford),\nM. M. Kasliwal (Carnegie), A. Horesh (Caltech)\nWe observed the position of iPTF14eag (Singer et al., GCN 16668),\nwhich is the optical afterglow of the Fermi GBM detected GRB 140808A\n(Zhang, GCN 16669), at 15 GHz with the Arcminute Microkelvin Imager\n(AMI-LA). The observations started on 2014 August 18.61 to 18.78 UT,\ncorresponding to 10.6 days post-burst. We have detected the radio\ncounterpart (Corsi et al., GCN 16694) with a preliminary flux of\n0.30 +/- 0.06 mJy.\n\nAn earlier observation conducted on 2014 August 12.61 to 12.78 UT,\ncorresponding to 4.6 days post-burst, yielded a marginal 3.8 sigma\ndetection of 0.15 +/- 0.04 mJy.\n\nFurther AMI monitoring is planned. We thank the AMI staff for scheduling\nthese observations.\n\nThese observations were made as part of the 4 PI SKY project.",
  "circularId": 16725,
  "createdOn": 1408526160000,
  "email": "gemma.anderson@astro.ox.ac.uk",
  "subject": "GRB 140808A/iPTF14eag: AMI 15 GHz detection",
  "submitter": "Gemma Anderson at U of Oxford  <gemma.anderson@astro.ox.ac.uk>",
  "eventId": "GRB 140808A"
}