Constraints on the origin of ultra-high-energy cosmic rays from cosmogenic neutrinos and photons

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Fig. 13

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Same as in Fig. 11, we now take a source at 20 Mpc with a luminosity 20 times lower than in Fig. 12. Pure proton and pure iron cases are considered as well as maximum energies of Z × 10^20.5 eV and Z × 10¹⁹ eV.

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Open with DEXTER

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