Neutrino Sources from a Multi-Messenger Perspective

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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 languageEnglish
Article number01013
JournalEPJ Web of Conferences
Number of pages7
Publication statusPublished - 13 May 2019

Bibliographical note

7 pages, 3 figures, Proceedings of the 7th Roma International Conference on Astroparticle Physics

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