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| Name：Victorludge | 17, Oct, 2023 10:22:51 | |
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the upper limit is 2 x 10(^ 10) cm(^ 2) s(^ 1) above a cosmic ray threshold of 500 GeV. Chapter five introduces a new method for the parameterisation of Cerenkov images of extensive air showers recorded by atmospheric Cerenkov telescopes. It explains why it is of particular interest and relevant to | |
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