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
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2verdicts
UNVERDICTED 2representative citing papers
Minimal UHECR flux models from the Telescope Array predict cosmogenic neutrino fluxes consistent with the KM3-230213A event at the 2σ level.
citing papers explorer
-
Average universal shower profile reconstruction using radio interferometry
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.
-
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.