Enomoto, RHigashi, YYoshida, TTanimori, TBicknell, GeoffreyClay, Roger WEdwards, P GGunji, SHara, SHattori, THayashi, SHirai, Y2015-12-080004-637Xhttp://hdl.handle.net/1885/31032Kepler's supernova, discovered in 1604 October, produced a remnant that has been well studied observationally in the radio, infrared, optical, and X-ray bands, and theoretically. Some models have predicted a TeV gamma-ray flux that is detectable with current Imaging Cerenkov Atmospheric Telescopes. We report on observations carried out in 2005 April with the CANGAROO-III Telescope. No statistically significant excess was observed, and limitations on the allowed parameter range in the model are discussed.Keywords: Gamma rays: observations; Supernovae: individual (Kepler's SNR)200810.1086/5899122015-12-08