  The majority of Galactic high-energy gamma-ray sources continue to elude
identification. Currently, we have a handful of firm pulsar identifications,
one of which is radio quiet, and a few marginal detections, including one
millisecond pulsar. Recently, both blind searches of EGRET error boxes and
targeted searches of X-ray counterpart candidates have had some success in
finding new pulsars. I review these results, and discuss our current program of
searching mid-Galactic latitude EGRET error boxes using the Parkes multi-beam
system.
