{
  "bibcode": "1999GCN...337....1F",
  "body": "D. A. Frail (NRAO), S. R. Kulkarni (Caltech), C. H. Young\n(MSU, NRAO) and G. B. Taylor (NRAO) report:\n\n\"We have analyzed additional VLA observations of the fast X-ray\ntransient detected by BeppoSAX (GCN 333) taken at 1.4, 4.8 and 8.5 GHz\nbeginning on May 20.93 UT. The positional accuracy of the radio source\nreported in GCN 334 has improved to (equinox 2000) R.A.=08 36 1.1\n(+/-0.1s), decl.=+51 17 6.5 (+/-1\") and it is now coincident with the\ncenter of the optical galaxy reported by Bloom et al. (GCN 335). There\nwas no evidence of any variability between the two VLA observations.\nIt now appears that this is an inverted spectrum radio source, present\nalso at a weak level (3-sigma) in the VLA FIRST survey at 1.4 GHz.\n\nThis message is citeable.\"",
  "circularId": 337,
  "createdOn": 927262612000,
  "email": "dfrail@nrao.edu",
  "subject": "radio observations of X-ray/GRB transient field",
  "submitter": "Dale A. Frail at NRAO  <dfrail@nrao.edu>"
}