Marcos Santander
Published 2016-06-30Version 1
The recent discoveries of high-energy astrophysical neutrinos and gravitational waves have opened new windows of exploration to the Universe. Combining neutrino observations with measurements of electromagnetic radiation and cosmic rays promises to unveil the sources responsible for the neutrino emission and to help solve long-standing problems in astrophysics such as the origin of cosmic rays. Neutrino observations may also help localize gravitational-wave sources, and enable the study of their astrophysical progenitors. In this work we review the current status and future plans for multi-messenger searches of neutrino sources.
Comments: To appear in "Neutrino Astronomy- Current status, future prospects", Eds. T. Gaisser & A. Karle (World Scientific)
Limits on Neutrino Emission from Gamma-Ray Bursts with the 40 String IceCube Detector
The neutrino emission from thermal processes in very massive stars in the local universe
Multi-messenger astronomy with INTEGRAL
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