Speaker
Description
Since its first detection by the IceCube Neutrino Observatory in 2013, the diffuse flux of astrophysical neutrinos has been confirmed in several channels with increasing significance and precision. With a decade of IceCube data, we have now gained a solid picture of the astrophysical neutrino flux from the TeV up to the PeV range. Another significant milestone was the announcement of the first source of astrophysical neutrinos - the gamma-ray bright Blazar TXS 0506+056 in 2018. Although the origin of a large fraction of the astrophysical neutrino flux remains unknown, it is expected that neutrinos and gamma rays are produced in close connection at nearly the same energies. In this talk, I review the current searches that connect astrophysical neutrinos to gamma rays from different source populations. Furthermore, I will cover physical and experimental challenges, as well as the role of current and future experiments.
