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