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.
Original language | English |
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Article number | 01013 |
Journal | EPJ Web of Conferences |
Volume | 209 |
Number of pages | 7 |
DOIs | |
Publication status | Published - 13 May 2019 |