The Antares Neutrino Telescope and Multi-Messenger Astronomy
Thierry Pradier (on behalf of the Antares Collaboration)
TL;DR
The Antares neutrino telescope aims to detect high-energy astrophysical neutrinos and enhance multi-messenger astronomy by correlating neutrino data with photons, cosmic rays, and gravitational waves.
Contribution
This paper presents Antares' latest results and introduces multi-messenger programs to improve detection and correlation capabilities.
Findings
Antares has achieved new upper limits on neutrino fluxes.
Development of multi-messenger correlation strategies.
Enhanced sensitivity to astrophysical neutrino sources.
Abstract
Antares is currently the largest neutrino telescope operating in the Northern Hemisphere, aiming at the detection of high-energy neutrinos from astrophysical sources. Such observations would provide important clues about the processes at work in those sources, and possibly help solve the puzzle of ultra-high energy cosmic rays. In this context, Antares is developing several programs to improve its capabilities of revealing possible spatial and/or temporal correlations of neutrinos with other cosmic messengers: photons, cosmic rays and gravitational waves. The neutrino telescope and its most recent results are presented, together with these multi-messenger programs.
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