Abstract
The discovery of high-energy cosmic neutrinos has raised great interest in the field of neutrino astronomy. The KM3NeT/ARCA detector is currently under construction at the bottom of the Mediterranean Sea and is measuring high-energy neutrinos. The complete detector will instrument a cubic kilometre of seawater with photomultiplier tubes that detect the Cherenkov radiation from the products of neutrino interactions. The design is focused on discovering high-energy neutrino sources which requires an excellent angular resolution. This contribution covers the reconstruction algorithms deployed in the full KM3NeT/ARCA detector and their performances. The angular resolution reaches below 0.1â—¦ for tracks and below 1â—¦ for cascades and double cascades that originate from tau neutrinos. Additionally, the neutrino selections for the full KM3NeT/ARCA diffuse and point source studies are covered.
Original language | English |
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Article number | 1074 |
Number of pages | 10 |
Journal | Proceedings of Science |
Volume | 444 |
DOIs | |
Publication status | Published - 27 Sept 2024 |
Event | International Cosmic Ray Conference - Nagoya, Japan Duration: 26 Jul 2023 → 3 Aug 2023 Conference number: 38th |
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