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THE ROLE OF STRUCTURED MAGNETIC FIELDS ON CONSTRAINING PROPERTIES OF TRANSIENT SOURCES OF ULTRA-HIGH-ENERGY COSMIC RAYS

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A lower bound on the number of cosmic ray events required to measure source catalogue correlations

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THE HIGHEST-ENERGY COSMIC RAYS CANNOT BE DOMINANTLY PROTONS FROM STEADY SOURCES

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Constraints on the AGN flares as sources of ultra-high energy cosmic rays from the Fermi-LAT observations

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