Monte Carlo simulations show radio interferometry reconstructs average Gaisser-Hillas parameters of air shower profiles with enhanced separation of primary masses and hadronic models compared to fluorescence profiles.
Aabet al.(Pierre Auger), Depth of maximum of air- shower profiles at the Pierre Auger Observatory
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Minimal UHECR flux models from the Telescope Array predict cosmogenic neutrino fluxes consistent with the KM3-230213A event at the 2σ level.
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Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models
Minimal UHECR flux models from the Telescope Array predict cosmogenic neutrino fluxes consistent with the KM3-230213A event at the 2σ level.