Above 5 EeV, cosmic rays are extragalactic atomic nuclei whose average mass rises with energy, with arrival directions clustering toward nearby galaxies, but their sources are still unknown.
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What do we know about cosmic rays with energies above 5 EeV?
Above 5 EeV, cosmic rays are extragalactic atomic nuclei whose average mass rises with energy, with arrival directions clustering toward nearby galaxies, but their sources are still unknown.