Multi-messengers at ultra-high energies with the Pierre Auger Observatory

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Volume 3 (2020)

4open, 3 (2020) 4

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Gravitational waves and the advent of multi-messenger astronomy

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Review

Figure 6

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Upper limit to the normalization of the diffuse flux of UHE neutrino. The upper limits obtained by the Pierre Auger Observatory are compared to those obtained by IceCube and ANITA, as well as predictions from cosmogenic and astrophysical neutrino production models. Taken from [47].