Event reconstruction and neutrino selection with KM3NeT/ARCA230
- NázevTitle
- Event reconstruction and neutrino selection with KM3NeT/ARCA230Event reconstruction and neutrino selection with KM3NeT/ARCA230
- Druh výsledkuResult type
- Příspěvek ve sborníkuProceedings paper
- AutořiAuthors
- T. van Eeden, J. Seneca, S. Aiello, A. Albert, Z. Bardačová, E. Eckerová, F. Mamedov, Y. Shitov, I. Štekl
- Klíčová slovaKeywords
- KM3NeT, neutrino telescope, Event reconstruction
- KonferenceConference
- 38th International Cosmic Ray Conference (Nagoya, Japan, 2023-07-26)
- ExperimentCollaboration
- KM3NeT
- DOIDOI
- 10.22323/1.444.1074
- Časopis / citaceJournal / citation
- In: Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023), Sissa Medialab, 2024, pp. 1074 · ISSN 1824-8039
- RokYear
- 2024
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Laboratoire Souterrain de Modane - účast ČRLaboratoire Souterrain de Modane – participation of the Czech Republic; Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
- CitovánoCited by
- 6 (INSPIRE-HEP)
- Plný text (open access)Full text (open access)
- https://pos.sissa.it/444/1074/pdf
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
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 0.1◦ for tracks and below 1◦ 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.
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 0.1◦ for tracks and below 1◦ 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.