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Fig. 3.

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Tibet ASγ limit on high Galactic latitude γ-ray flux compared to Fermi/LAT measurements at lower energies from Neronov & Semikoz (2020) and to model predictions of neutrino (yellow lines) and γ-ray (grey lines) fluxes for the local cosmic ray source (Bouyahiaoui et al. 2020) (dashed lines), dark matter decay (Neronov et al. 2018) (solid), and 100 kpc scale halos of the Milky Way (Recchia et al. 2021) (dotted). Yellow and green areas show the astrophysical neutrino spectrum measurement in cascade (Aartsen et al. 2020) and muon (Stettner 2019) channels.

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