GCN Circular 1994
M. Uemura (Kyoto U.), H. Yamaoka (Kyushu U.), R. Ishioka, and T. Kato (Kyoto U.) report on behalf of VSNET-GRB collaboration: The precise position for the optical afterglow candidate of GRB 030329 (GCN 1985, 1986, 1987, 1689) was derived from Kyoto images (GCN 1689) as (with mean error of measurements of nine images): R.A.= 10h44m50s.030 +/- 0s.005, Decl. = +21d31'18".15 +/- 0".07. On the DSS 2 B, R, and I images, there is no distinct source down to the limiting magnitudes, which indicates the parent galaxy is more than 8-9 mag dimmer of the OT at 76 minutes after explosion. This message may be cited.