  The outstanding task of gamma-ray burst astronomy is to test the hypothesis
that they are at cosmological distances. This can be done by determining the
coordinates of at least a few bursts to ~ 15'' or better. If they are in
distant galaxies, the next task is to determine from which component of the
galaxies the bursts originate; sub-arcsecond positions would answer this
question. I outline ground-based systems which can accomplish these tasks,
given BATSE/BACODINE coordinates and conservative assumptions about visible
counterparts; these systems would be a ground-based upgrade to GRO which would
accomplish the chief objectives of HETE.
