{
  "bibcode": "1998GCN...121....1F",
  "body": "D. A. Frail, National Radio Astronomy Observatory and S. R. Kulkarni,\nCalifornia Institute of Technology report: \n\nThe recent renewed activity from SGR1900+14 (GCN #94) and the\nnewly-discovered SGR1627-41 (GCN #107) prompted VLA radio observations\nat 8.46 GHz on 1998 June 25. For SGR1900+14 we observed a field\ncentered on the proposed X-ray/infrared counterpart (Hurley et\nal. ApJ, 463, L13, 1996, Vrba et al. ApJ, 468, 225, 1996). For\nSGR1627-41 we observed the 95 arcsec diameter supernova remnant CTB33\n(IAU Circ. 6948), most recently studied by Sarma, Goss, Green & Frail\n(ApJ, 483, 335, 1997).  The synthesized beam was approximately 1\narcsec. The interferometer is insensitive to extended structure on\nangular scales larger than 20 arcsec.\n\nNo point sources were visible above 200 microJy and 345 microJy\n(4-sigma) for the SGR1900+14 and SGR1627-41, respectively.\n\nThis report can be cited.",
  "circularId": 121,
  "createdOn": 899313046000,
  "email": "dfrail@nrao.edu",
  "subject": "Radio observations of SGRs",
  "submitter": "Dale A Frail at NRAO  <dfrail@nrao.edu>"
}