{
  "bibcode": "2003GCN..1979....1M",
  "body": "P. Martini (OCIW), P. Garnavich (Notre Dame) and K.Z. Stanek (CfA)\n\nWe imaged the optical afterglow of GRB 030328 (Peterson & Price,\nGCN 1974) with the Magellan 6.5-m Clay telescope and LDSS2\nimaging/spectrograph on March 29.181 (0.708 days after the\nburst). The R-band magnitude is estimated to be 20.8\nassuming star \"B\" (GCN 1977) is R=16.1. This is slightly\nbrighter than the extrapolation of a powerlaw with alpha=1.0\nfound by Price & Peterson (GCN 1977).\n\nThis message may be cited.",
  "circularId": 1979,
  "createdOn": 1048918594000,
  "email": "pgarnavi@miranda.phys.nd.edu",
  "subject": "GRB 030328, optical observations",
  "submitter": "Peter Garnavich at U of Notre Dame  <pgarnavi@miranda.phys.nd.edu>",
  "eventId": "GRB 030328"
}