{
  "bibcode": "2001GCN..1136....1T",
  "body": "G. B. Taylor (NRAO), D. A. Frail (NRAO/Caltech) and S. R. Kulkarni\n(Caltech) report on behalf of the Caltech-NRAO-CARA collaboration:\n\n\"We have continued to monitor the WFC error circle of the X-ray\ntransient 011030 (GCN 1119, 1123) with the VLA at 8.47 GHz.\nObservations were made over four epochs on Oct. 31.13,\nNov. 1.79, Nov. 4.81, and Nov 8.80 UT.  Over this period the radio source\nVLA J2044+7717 (GCN 1122) has remained constant, in agreement with the\n4.8 GHz observations by Rol et al. (GCN 1124). On 2001 Nov 8.80 UT a\nnew source was detected with high significance with a flux density of\n181 +/- 18 microJy. This new source is located near the center of the\nWFC error circle at (epoch 2000) R.A.=20:43:32.3, Dec.=+77:17:18.9,\nwith a conservative error of +/-1 arcsec in both coordinates.\n\nLittle is known about the class of such X-ray rich transients. This is\nthe first detection of a counterpart at any other wavelength to an\nX-ray rich transient. We will continue further radio observations and\nurge observations at other wavelengths.\"\n\nThis message may be cited.",
  "circularId": 1136,
  "createdOn": 1005282527000,
  "email": "gtaylor@aoc.nrao.edu",
  "subject": "The Radio Afterglow from the X-ray Rich GRB 011030",
  "submitter": "Greg Taylor at NRAO  <gtaylor@aoc.nrao.edu>",
  "eventId": "GRB 011030"
}