  Observations of unidentified EGRET sources were made with the Whipple 10m
imaging atmospheric Cherenkov telescope between Fall 1999 and Spring 2001.
During this period, a high resolution 490 pixel camera with 4 degree field of
view was present on the telescope. Characterization of the off-axis response of
this instrument was done using observations of the Crab Nebula. No significant
emission was detected from the eight unidentified EGRET sources observed and
upper limits are presented as a function of position.
