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[vsnet-grb 7] GRB000630



GRB000630

   According to recent GCN Circulars, the optical source reported by
Bartolini et al. is likely a persistent one (at R=20.3, GCN Circular 740;
also visibile at the limit of DSSS).  The radio position has yielded
no optical counterpart yet down to R=24.

Regards,
Taichi Kato

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