  We take the established relation between black hole mass, X-ray luminosity,
and radio luminosity and show that intermediate mass black holes, such as those
predicted to exist at the centers of globular clusters, will be easily
identifiable objects in deep radio observations. We show that the radio
observations will be far more senstive than any possible X-ray observations. We
also discuss the likely optical photometric and spectroscopic appearance of
such systems in the event that radio detections are made.
