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In the talk I present a brief overview of the largest experiments in the field -- Pierre Auger Observatory (PAO) and Telescope Array (TA) and their main results: the cosmic ray spectra in a range of energies from 10^(15.5) eV to over 10^20 EeV, the mass composition, indications of arrival anisotropy at different angular scales, and constraints on the flux of UHE photons and neutrinos. Finally, I discuss the status and perspectives of the future upgrades of the experiments.