  The CELESTE experiment will be an Atmospheric Cherenkov detector designed to
bridge the gap in energy sensitivity between current satellite and ground-based
gamma-ray telescopes, 20 to 300 GeV. We present test results made at the former
solar power plant, Themis, in the French Pyrenees. The tests confirm the
viability of using a central tower heliostat array for Cherenkov wavefront
sampling.
