2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/5450The 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.4 pages, to appear in the proceedings of the conference "Radio Pulsars" held in Chania, Crete, Sept. 2002Astrophysicstext