{
  "bibcode": "2000GCN...857....1T",
  "body": "G. B. Taylor (NRAO) reports on behalf of a larger collaboration:\n\n\"We imaged the IPN error box of GRB001018 (GCN #853) with the VLA at\n8.46 GHz, starting on Oct. 19.88 UT.  A second observation was\nobtained starting on Oct. 20.76 UT.  One unresolved radio source (size\n< 0.25 arcsec) is detected within the IPN error box at (J2000) R.A.=\n13 14 12.385, Dec. =11 48 57.90 with an error of approximately 50 mas\nin each coordinate.  The VLA flux density at 8.46 GHz was 258 +/- 65\nmicroJy on Oct 19.88, and 405 +/- 50 microJy on Oct 20.76.  No source\nis detected in the NRAO VLA Sky Survey (NVSS; Condon et al. 1998, AJ,\n115, 1693) above their flux limit of 1 mJy at 1.4 GHz.  Based on its\ncompact and possibly variable nature we suggest that the source VLA\nJ1314+1148 could be the radio afterglow from G001018.  Further\nobservations with the VLA are planned.\"\n\nThis message may be cited.",
  "circularId": 857,
  "createdOn": 972108197000,
  "email": "gtaylor@aoc.nrao.edu",
  "subject": "GRB 001018, Possible Radio Afterglow",
  "submitter": "Greg Taylor at NRAO  <gtaylor@aoc.nrao.edu>",
  "eventId": "GRB 001018"
}