Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects
Figure 8
Limits for selected muon neutrino spectra (including flavor mixing) from [34] for different declination bands for the time-integrated point source search in IC40 (90% CL) [13]. The thick lines show the limits for an flux (in the dominant energy range), and the thick curves the differential limits, figure taken from [46]. The different spectra correspond to the test points in Figure 10 (same numbers used).
