GCN Circular 1979
P. Martini (OCIW), P. Garnavich (Notre Dame) and K.Z. Stanek (CfA) We imaged the optical afterglow of GRB 030328 (Peterson & Price, GCN 1974) with the Magellan 6.5-m Clay telescope and LDSS2 imaging/spectrograph on March 29.181 (0.708 days after the burst). The R-band magnitude is estimated to be 20.8 assuming star "B" (GCN 1977) is R=16.1. This is slightly brighter than the extrapolation of a powerlaw with alpha=1.0 found by Price & Peterson (GCN 1977). This message may be cited.