Figure 2 - available via license: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
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The fit results of different components of a diffuse neutrino flux compared with 8 years of IceCube data for a selection of principallly throughgoing tracks.
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... larger sample of high quality track events are selected [6,7,1] which is several orders of magnitidue larger with thousands of events per year. However, a selection starting at 1 TeV becomes dominated by muon tracks from atmospheric neutrinos. A fit of the conventional atmo- spheric, prompt, and astrophysical flux for this selection of through going tracks using 8 years of IceCube data [1] can be seen in Fig 2. The resulting astrophysical fit was found to be ...
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http://deepblue.lib.umich.edu/bitstream/2027.42/173237/1/10052_2021_Article_9929.pdf