The Fermi Sky in a Multimessenger Context

Abstract

The Fermi Gamma-Ray Space Telescope has been launched on June 11 2008. While it has fundamentally changed our understanding of the high-energy $\gamma$-ray sky, it is even more powerful in multiwavelength and multimessenger efforts. In this work I summarize results from Fermi-LAT in the multimessenger context, pertaining to high-energy neutrinos.

Proceedings of the Neutrino Oscillation Workshop 2016, Lecce, Italy; Editors: A. Marrone, A. Mirizzi, D. Montanino; PoS(NOW2016)042

References in corpus (6)

• Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
• The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux
• IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica
• Evidence against star-forming galaxies as the dominant source of IceCube neutrinos
• Revised predictions of neutrino fluxes from Pulsar Wind Nebulae
• One-point fluctuation analysis of the high-energy neutrino sky