Updated Xmax measurements reveal a transition to heavier cosmic-ray mass composition above 10^18.4 eV with decreasing elemental diversity.
Abreuet al.(Pierre Auger Collaboration), The Lateral Trig- ger Probability function for the Ultra-High Energy Cosmic Ray showers detected by the Pierre Auger Observatory, Astropart
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Depth of Maximum of Air-Shower Profiles above 10^17.7 eV Measured with the Fluorescence Detector of the Pierre Auger Observatory
Updated Xmax measurements reveal a transition to heavier cosmic-ray mass composition above 10^18.4 eV with decreasing elemental diversity.