Towards event-by-event studies of the ultrahigh-energy cosmic-ray composition

Astronomy and Astrophysics – Astrophysics

Scientific paper

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27 pages, 6 figures; v2: 30 pages, journal version

Scientific paper

10.1016/j.astropartphys.2007.04.

We suggest a method which improves the precision of studies of the primary composition of ultra-high-energy cosmic rays. Two principal ingredients of the method are (1) comparison of the observed and simulated parameters for individual showers, without averaging over arrival directions and (2) event-by-event selection of simulated showers by the physical observables and not by the reconstructed primary parameters. A detailed description of the algorithm is presented and illustrated by several examples.

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