We have carried out Monte Carlo simulation to estimate
the sensitivity of WXM to GRBs. Here, the photon energy was limited within 3-10 keV
to reduce the blurring due to penetration. Then the position histogram in 0.5 mm bin
was simulated for the detector geometry. The GRB direction was reconstructed by
cross-correlating the simulated data with the number of templates corresponding to
various incidence angles. In the simple simulation with 2 second integrations, the
correct position was obtained for half of the events that occur within the field of
view of the WXM with peak fluxes of 4 ph/cm2/s ( erg/cm2/s
over the 3-10 keV range) and, under favorable conditions, some events down to
0.4 ph/cm2/s. Assuming the BATSE
relation, this sensitivity
results in localization of about 30 GRBs per year.
Copyright The European Southern Observatory (ESO)