Neutrino Sources from a Multi-Messenger Perspective
arXiv:1811.07633 · doi:10.1051/epjconf/201920901013
Abstract
The field of high-energy neutrino astronomy is undergoing a rapid evolution. After the discovery of a diffuse flux of astrophysical TeV-PeV neutrinos in 2013, the IceCube observatory has recently found first compelling evidence for neutrino emission from blazars. In this brief review, I will summarize the status of these neutrino observations and highlight the strong role of multi-messenger astronomy for their interpretation.
7 pages, 3 figures, Proceedings of the 7th Roma International Conference on Astroparticle Physics