  The GLAST mission to be launched in November 2007 will provide unique
information about high energy photon fluxes from gamma-ray bursts. These data
will be most useful when combined with multiwavelength observations that
provide more complete characterizations of such events. To assist this process,
we have estimated the GLAST Large Area Telescope (LAT) angular resolution for
the coordinates of ensembles of photons from GRBs as a function of burst
spectral index and fluence. This information may be useful in guiding the
development of more effective GRB optical afterglow observation programs.
