Event reconstruction and neutrino selection with KM3NeT/ARCA230

Thijs Juan van Eeden; Jordan Seneca; KM3NeT collaboration; M. D. Filipović; et al.

doi:10.22323/1.444.1074

Event reconstruction and neutrino selection with KM3NeT/ARCA230

Thijs Juan van Eeden
, Jordan Seneca
, KM3NeT collaboration
, M. D. Filipović
, et al.

School of Science

National Institute for Subatomic Physics

Research output: Contribution to journal › Article › peer-review

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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
Article number	1074
Number of pages	10
Journal	Proceedings of Science
Volume	444
DOIs	https://doi.org/10.22323/1.444.1074
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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Cite this

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title = "Event reconstruction and neutrino selection with KM3NeT/ARCA230",

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 0.1{\^a}—¦ for tracks and below 1{\^a}—¦ 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.",

author = "\{van Eeden\}, \{Thijs Juan\} and Jordan Seneca and \{KM3NeT collaboration\} and Filipovi{\'c}, \{M. D.\} and \{et al.\}",

year = "2024",

month = sep,

day = "27",

doi = "10.22323/1.444.1074",

language = "English",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

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note = "International Cosmic Ray Conference, ICRC ; Conference date: 26-07-2023 Through 03-08-2023",

}

TY - JOUR

T1 - Event reconstruction and neutrino selection with KM3NeT/ARCA230

AU - van Eeden, Thijs Juan

AU - Seneca, Jordan

AU - KM3NeT collaboration,

AU - Filipović, M. D.

AU - et al.,

N1 - Conference code: 38th

PY - 2024/9/27

Y1 - 2024/9/27

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/85212302522

U2 - 10.22323/1.444.1074

DO - 10.22323/1.444.1074

M3 - Article

AN - SCOPUS:85212302522

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1074

T2 - International Cosmic Ray Conference

Y2 - 26 July 2023 through 3 August 2023

ER -

Event reconstruction and neutrino selection with KM3NeT/ARCA230

Abstract

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