Ponente
Descripción
In recent years, the development of multi-messenger astronomy has opened a new window into understanding the most energetic phenomena of our Universe. The study of transient events by combining information from neutrinos, photons, charged particles, and gravitational waves enhances the sensitivity to identifying and characterising a wide variety of astrophysical sources.
The KM3NeT neutrino telescope is a deep-sea Cherenkov infrastructure currently taking data in the Mediterranean Sea with partial configurations. Two separate arrays are under construction: ORCA, off-shore Toulon (France), and ARCA, off-shore Sicily (Italy). This talk summarises the latest results of the searches for neutrino counterparts in coincidence with other astrophysical phenomena. These analyses have been conducted using the KM3NeT real-time platform, and cover a wide neutrino energy range from MeV to a few PeV.
