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arXiv · 0805.1091

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

R. Enomoto·Y. Higashi·T. Yoshida·T. Tanimori
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Abstract

Kepler's supernova, discovered in October 1604, 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 Cherenkov 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.

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R. Enomoto, Y. Higashi, T. Yoshida, T. Tanimori. 2008-05-08. CANGAROO-III Search for Gamma Rays from Kepler's Supernova Remnant. https://doi.org/10.1086/589912

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