  The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is an
atmospheric Cherenkov telescope (ACT) that uses a large mirror array to achieve
a relatively low energy threshold. For sources with Crab-like spectra, at high
elevations, the detector response peaks near 100 GeV. Gamma-ray burst (GRB)
observations have been a high priority for the STACEE collaboration since the
inception of the experiment. We present the results of 20 GRB follow-up
observations at times ranging from 3 minutes to 15 hours after the burst
triggers. Where redshift measurements are available, we place constraints on
the intrinsic high-energy spectra of the bursts.
