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VHE observations of unidentified EGRET sources

Observations of unidentified EGRET sources were made with the Whipple 10m imaging atmospheric Cerenkov telescope between Fall 1999 and Spring 2001. During this period, a high resolution 490 pixel camera with 4° 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.