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A flux of extra-terrestrial neutrinos at energies $\gg10^{15}$ eV has the potential to serve as a cosmological probe of the high-energy universe as well as tests of fundamental particle interactions.
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2017
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Ivanov, D., et al., “Report of the Telescope Array – Pierre Auger Observatory Working Group on Energy Spectrum”, 35th ICRC 2017, Busan, South Korea, Proceedings of Science, PoS(ICRC2017)498, (2017)
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de Souza, V., at al., “Testing the agreement between the Xmax distributions measured by the Pierre Auger and Telescope Array Observatories”, 35th ICRC 2017, Busan, South Korea, Proceedings of Science, PoS(ICRC2017)522, (2017)
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The Pierre Auger Collaboration, “Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory”, Jour. of Cosmo. and Astropart. Phys., 04 038, (2017)
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Zhang, B. T., Murase, K., Oikonomou, F., Li, Z., “High-energy cosmic ray nuclei from tidal disruption events: Origin, survival, and implications”, Phys. Rev. D, 96, 063007, (2017)
2017
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Wittkowski, D., for the Pierre Auger Collaboration, “Reconstructed properties of the sources of UHECR and their dependence on the extragalactic magnetic field”, 36th ICRC 2017, Busan, South Korea, Proceedings of Science, PoS(ICRC2017)563, (2017)
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2017
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Kimura, S. S., Murase, K., Zhang, B. T., “Ultrahigh-energy cosmic-ray nuclei from black hole jets: Recycling galactic cosmic rays through shear acceleration”, Phys. Rev. D, 97, 023026, (2018)
2018
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