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Existence of ultrahigh-energy cosmic rays is well established, but nature of these particles and ways of their production are still unknown. The limits imposed on the viable UHECR models araising from high-energy gamma-ray (Ferm-LAT) and neutrino (IceCube, ANTARES) data and importance of the future Cherenkov Telescope Array measurements for the UHECR physics will be discussed.
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Askhat Gazizov
Gran Sasso Science Institute