http://arxiv.org/abs/2105.06414
In this letter, we present an update of a method for analysing arrival directions of ultra-high-energy cosmic rays (UHECRs) above the Greisen–Zatsepin–Kuz’min cut-off with a deep convolutional neural network developed originally in Kalashev, Pshirkov, Zotov (2020). Namely, we introduce energy as another variable employed in the analysis. This allows us to take into account the intrinsic uncertainties in energy of primary cosmic rays present in any experiment, which were not taken into account in the previous study, without any loss of quality of the classifier. We present the architecture of the new neural network, results of its application to mock maps of UHECR arrival directions and outline possible directions of a further improvement of the method.
O. Kalashev, M. Pshirkov and M. Zotov
Fri, 14 May 21
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Comments: 7 pages, 1 figure. arXiv admin note: substantial text overlap with arXiv:1912.00625