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Fig. 10.

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Predicted neutrino flux from the source populations as shown in the legend (also see Fig. 5), assuming that the BHJet jet scenario explains their jet dynamics. The subplot shows the contribution of the total predicted flux to the detected Galactic neutrino diffuse emission by IceCube (IceCube Collaboration 2023). The three different colours represent the three different models used to extract the observed flux.

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