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), Techniques for measuring aerosol attenuation using the Central Laser Facility at the Pierre Auger Observatory, JINST8, P04009 (2013)
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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.