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

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dc.creatorGorbunov, D. S.
dc.creatorRubtsov, G. I.
dc.creatorTroitsky, S. V.
dc.date2006-06-19
dc.date2007-07-05
dc.date.accessioned2026-07-07T11:42:33Z
dc.date.available2026-07-07T11:42:33Z
dc.descriptionWe 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.
dc.description27 pages, 6 figures; v2: 30 pages, journal version
dc.identifierhttps://arxiv.org/abs/astro-ph/0606442
dc.identifierhttp://arxiv.org/abs/astro-ph/0606442
dc.identifierAstropart.Phys.28:28-40,2007
dc.identifierdoi:10.1016/j.astropartphys.2007.04.003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200921
dc.subjectAstrophysics
dc.titleTowards event-by-event studies of the ultrahigh-energy cosmic-ray composition
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