  For some time, the Draco dwarf spheroidal galaxy has garnered interest as a
possible source for the indirect detection of dark matter. Its large
mass-to-light ratio and relative proximity to the Earth provide favorable
conditions for the production of detectable gamma rays from dark matter
self-annihilation in its core. The Solar Tower Atmospheric Cherenkov Effect
Experiment (STACEE) is an air-shower Cherenkov telescope located in
Albuquerque, NM capable of detecting gamma rays at energies above 100 GeV. We
present the results of the STACEE observations of Draco during the 2005-2006
observing season totaling 10 hours of livetime after cuts.
