http://arxiv.org/abs/2304.05348
In this article, it is shown that the $C_k$ and $LCm$ variables, recently introduced as an effective way to discriminate gamma and proton-induced showers in large wide-field gamma-ray observatories, can be generalised to be used in arrays of different detectors and variable fill factors. In particular, the $C_k$ profile discrimination capabilities are evaluated for scintillator and water Cherenkov detector arrays.
R. Conceição, P. Costa, L. Gibilisco, et. al.
Wed, 12 Apr 23
23/45
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