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We present the analysis and results of 12.5 hours of high-energy gamma-rayobservations of the EGRET-detected pulsar PSR B1951+32 using the Solar TowerAtmospheric Cherenkov Effect Experiment (STACEE). STACEE is an atmosphericCherenkov detector, in Albuquerque, New Mexico, that detects cosmic gamma raysusing the shower-front-sampling technique. STACEE's sensitivity toastrophysical sources at energies around 100 GeV allows it to investigateemission from gamma-ray pulsars with expected pulsed emission cutoffs below 100GeV. We discuss the observations and analysis of STACEE's PSR 1951+32 data,accumulated during the 2005 and 2006 observing seasons.

Observations of the Pulsar PSR B1951+32 with the Solar Tower Atmospheric Cherenkov Effect Experiment