Prompt and cosmogenic (muon flavor) neutrino spectra obtained for selected points in the parameter space in Fig. 11 for the Mixed Composition Dip model. Here we compare to the differential limits obtained from Aartsen et al. (2017, considering northern + southern exposure) and Aartsen et al. (2016). The different points are: A: (log₁₀(R∕km), log₁₀(L_γ∕(erg s⁻¹))) = (8.1, 50.5), B: (8.1, 49.5), C: (8.1, 51.7). Here the differential limits are defined as in Baerwald et al. (2015), such that following the differential limit curve for one decade in energy will yield one event.