Regions of Excessive Flux of PeV Cosmic Rays
M. Yu. Zotov, G. V. Kulikov

TL;DR
This paper identifies regions with unusually high flux of PeV cosmic rays using data from two arrays, analyzes their significance, and explores potential astrophysical sources.
Contribution
It presents a comparative analysis of regions of excessive cosmic ray flux in two datasets and investigates their possible astrophysical origins.
Findings
Multiple regions of excessive flux identified
Probabilities of regions' appearance estimated
Potential correlation with astrophysical sources discussed
Abstract
An analysis of arrival directions of extensive air showers generated by cosmic rays in the PeV energy range and registered with the EAS MSU and EAS-1000 Prototype arrays reveals a considerable number of regions of excessive flux of cosmic rays. We present results of comparative analysis of regions found in the two data sets, estimate probabilities of their appearance, and discuss correlation of their locations with coordinates of possible astrophysical sources of PeV cosmic rays.
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