  EGRET can now study six pulsars since the recent detection of PSR B1951+32.
Careful analysis of the three brightest pulsars shows that gamma rays are
emitted through essentially the entire rotation. This calls into question the
previous interpretation of the Crab's low-level emission as due entirely to its
nebula. The pulse light curves have either well-separated double peaks or very
broad peaks which might be resolved into multiple components. The spectra are
consistent with power laws over a large portion of the EGRET energy range, and
many show a dropoff at a few GeV.
