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Cosmic rays in the energy range $10^{18.0}$ - $10^{18.5}$ eV are thought to have a light, probably protonic, composition.
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P. Abreu, et al. , Large scale distribution of arrival directions of cosmic rays detected above 10 18 10^{18} eV at the Pierre Auger Observatory, Astrophys. J. Suppl. 203 (2012) 34 · 2012
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R. U. Abbasi, et al. , Study of Ultra-High Energy Cosmic Ray composition using Telescope Array’s Middle Drum detector and surface array in hybrid mode, Astropart. Phys. 64 (2015) 49–62 · 2014
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P. Abreu, et al. , Constraints on the origin of cosmic rays above 10 18 10^{18} eV from large scale anisotropy searches in data of the Pierre Auger Observatory, Astrophys. J. 762 (2012) L13 · 2041
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T. Abu-Zayyad, et al. , The Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment, Astrophys. J. 768 (2013) L1 · 2041
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