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Constraints on atmospheric charmed-meson production from IceCube

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Figure

Figure 1. Measurements andpredictions for the absolute
Figure 3. Left: Best-fit prompt normalization in ERS units for each scan pointtwo-dimensional contours forprompt normalization in ERS units; Right: Prompt atmospheric muon neutrino flux predictions from selectedperturbative QCD calculations (dashed lines) in

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