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Kepler's supernova, discovered in October 1604, produced a remnant that hasbeen well studied observationally in the radio, infrared, optical, and X-raybands, and theoretically. Some models have predicted a TeV gamma-ray flux thatis detectable with current Imaging Cherenkov Atmospheric Telescopes. We reporton observations carried out in 2005 April with the CANGAROO-III telescope. Nostatistically significant excess was observed, and limitations on the allowedparameter range in the model are discussed.

CANGAROO-III Search for Gamma Rays from Kepler's Supernova Remnant