Fig. 3.
Comparison between our multi-component model and the latest IceCube analysis including 6 yr of HESE (black points) and 8 yr of TGM (yellow band) from Aartsen et al. (2017e; neutrino flux per flavor). We find good agreement above a few hundred TeV both with HESE and TGM, whereas the two points at low energies are in tension with the model. Compared to Fig. 2, here the atmospheric backgrounds have been subtracted in both the data points and the model.
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