Fig. 1.
Radial kernels for the two observables under consideration. The solid black line shows the approximate redshift distribution of galaxies in the 2MRS sample using the fit found by Ando et al. (2018). The red, yellow, and blue lines show the radial kernel for the UHECR flux (Eq. (10)) for the three energy thresholds studied here (40 EeV, 63 EeV, and 100 EeV, respectively).
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