  At the end of the EGRET mission, only 6-8 Galactic sources had been
identified as young pulsars. Since then, several energetic pulsars have been
discovered in EGRET error boxes along the Galactic plane, as well as several
pulsar wind nebulae from which pulsations have not yet been discovered. Some of
these nebulae are associated with moderately variable EGRET sources, suggesting
that the gamma-ray emission might be coming from the nebula rather than from
the pulsar magnetosphere. There is also a population of unidentified EGRET
sources at mid-Galactic latitudes which have been proposed to be either nearby
middle-aged pulsars or millisecond pulsars. I review the current status of
observational studies of pulsars associated with EGRET sources and what they
suggest the upcoming AGILE and GLAST gamma-ray missions might observe.
