Neutrinos from Cosmic Accelerators including Magnetic Field and Flavor Effects

Figure 11

Regions where the sensitivity in 𝐹𝛽 exceeds 10−9 erg cm⁻² s⁻¹ [sr⁻¹] for 𝛽=𝜇 (a) and 𝛽=𝜏 (b) for several selected data samples (90% CL, 𝛼=2). The dashed regions “UHECR” indicate where 1020 eV cosmic ray protons are expected to be produced in the model. The different sources (test points) correspond to the ones in Figure 10, figure taken from [46].

(a)

(b)