Abstract
The detection of astrophysical neutrinos by the IceCube Collaboration (Aartsen et al., 2013) triggered numerous efforts to identify their origins. These observations add up to hundreds of ultra high-energy cosmic rays (UHECR) observed over the last decades, whose distribution -in both cases- are mainly isotropic and suggests extragalactic origin. In this context, High Synchrotron Peak (HS…