{
  "bibcode": "2005GCN..4074....1C",
  "body": "P. B. Cameron (Caltech) reports on behalf of the Caltech-NRAO-Carnegie\ncollaboration:\n\n\"We observed the field of GRB 051008 (GCN 4069) with the Very Large Array \nat 8.5 GHz beginning October 8.86 UT (~4 hours after the burst). No radio \nsource is detected within the XRT error circle (GCN 4073) with a 2-sigma \nupper limit of 80 uJy.\n\nWe find one source above the 4-sigma level in the BAT error circle at\n\nRA(J2000) 13:31:22.92  +/-  0.07\nDEC      +42:04:31.7   +/-  0.3\n\nwith a flux density of 175 +/- 40 uJy. However, the probability of finding \na source of this brightness in a region with 3-arcmin radius is ~54% \n(Fomalont et al., 2002, ApJ, 123, 2402).\n\nThe National Radio Astronomy Observatory is a facility of the National\nScience Foundation operated under cooperative agreement by Associated\nUniversities, Inc.\"",
  "circularId": 4074,
  "createdOn": 1128812442000,
  "email": "pbc@astro.caltech.edu",
  "subject": "GRB051008: Radio Observation",
  "submitter": "Patrick B. Cameron at Caltech  <pbc@astro.caltech.edu>",
  "eventId": "GRB 051008"
}