Evidence for a mixed mass composition at the `ankle' in the cosmic-ray spectrum
The Pierre Auger Collaboration: A. Aab, P. Abreu, M. Aglietta, E.J., Ahn, I. Al Samarai, I.F.M. Albuquerque, I. Allekotte, P. Allison, A. Almela,, J. Alvarez Castillo, J. Alvarez-Mu\~niz, M. Ambrosio, G.A. Anastasi, L., Anchordoqui, B. Andrada, S. Andringa, C. Aramo, F. Arqueros

TL;DR
This study presents the first correlation measurement between the depth of shower maximum and water Cherenkov signals in ultra-high energy cosmic rays, revealing a mixed mass composition at the ankle energy range, challenging pure proton models.
Contribution
It introduces a robust hybrid measurement method that constrains the primary mass composition of cosmic rays with reduced systematic uncertainties.
Findings
Correlation differs from pure composition expectations.
Data favor a mixed composition with nuclei heavier than helium.
Pure proton models are disfavored by the observations.
Abstract
We report a first measurement for ultra-high energy cosmic rays of the correlation between the depth of shower maximum and the signal in the water Cherenkov stations of air-showers registered simultaneously by the fluorescence and the surface detectors of the Pierre Auger Observatory. Such a correlation measurement is a unique feature of a hybrid air-shower observatory with sensitivity to both the electromagnetic and muonic components. It allows an accurate determination of the spread of primary masses in the cosmic-ray flux. Up till now, constraints on the spread of primary masses have been dominated by systematic uncertainties. The present correlation measurement is not affected by systematics in the measurement of the depth of shower maximum or the signal in the water Cherenkov stations. The analysis relies on general characteristics of air showers and is thus robust also with…
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