After 19 years of data, the combined Auger spectrum confirms the instep feature in the ultra-high-energy cosmic-ray flux at 5.5-sigma significance.
Schmidt (Pierre Auger), inthese proceedings
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Measurement of the cosmic-ray energy spectrum above 2.5 EeV using 19 years of operation of the Pierre Auger Observatory
After 19 years of data, the combined Auger spectrum confirms the instep feature in the ultra-high-energy cosmic-ray flux at 5.5-sigma significance.