Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects
Figure 14
Numerical prediction (NFC) of the quasi-diffuse flux expected from the bursts used in the IC40-analysis, including the estimates for several model- or method-specific systematical uncertainties (see main text). In addition, the IC40 limit is shown, and two expectations are shown for comparison (IC59+40 from [19] and IC86 extrapolated for from IC40; see, e.g., [87]), figure taken from [44].
