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Fig. 10


Redshift distribution for sources inside (top) and outside (bottom) of the error radius R50 of the IceCube HESE neutrino events with energies in excess of 100 TeV. There is no apparent peak in the distribution for the subsample in coincidence with the R50 radii of > 100 TeV IceCube HESE neutrino events, but a KS test yields a p-value of 0.11 that both samples were drawn from the same underlying distribution.

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