The Monash University Physics Department is constructing a spectrograp
h, to be attached to a 0.46-m Cassegrainian telescope. To help future
users of the spectrograph determine the operational capabilities of th
e spectrograph a PC-based software package was created. This program a
llows the user to simulate the response of the spectrograph to various
stellar types under differing observational constraints. We have esti
mated the precision of measurements of stellar radial velocities with
the spectrograph. The estimates are reasonable but are yet to be compa
red with real data.