{
  "bibcode": "2012GCN.13474....1B",
  "body": "C. Bathurst (U. South Florida), D. A. Frail (NRAO) and S. B. Cenko (UC\nBerkeley) report on behalf of a larger collaboration:\n\nWe have observed the field of the potential X-ray afterglow (GCN 13400,\n13394) of the Fermi GBM (GCN 13377) and LAT (GCN 13379) GRB 120624B with\nthe VLA. In observations taken on 2012 July 10.00 UT, at center\nfrequencies of 5 GHz and 14 GHz, we find an unresolved radio source\ncoincident with the position of the claimed X-ray afterglow (GCN 13400).\nThe radio source is detected at 5-6 sigma significance and it has a\nrising spectrum consistent with the extrapolation of the 3mm PdBI\ndetection (GCN 14321). Further 5 GHz observations were also made on June\n26, June 29 and July 11. The 5 GHz flux density of the radio source shows\nno evidence for variability through these 4 epochs.\n\nFurther observations are planned.",
  "circularId": 13474,
  "createdOn": 1342324218000,
  "email": "cenko@srl.caltech.edu",
  "subject": "GRB 120624B: VLA Observations",
  "submitter": "S. Bradley Cenko at Caltech  <cenko@srl.caltech.edu>",
  "eventId": "GRB 120624B"
}