Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022

Vasileios Tsourapis; Evangelia Drakopoulou; Christos Markou; Anna Sinopoulou; Ekaterini Tzamariudaki; KM3NeT collaboration; M. D. Filipović; et al.

doi:10.22323/1.444.1195

Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022

Vasileios Tsourapis
, Evangelia Drakopoulou
, Christos Markou
, Anna Sinopoulou
, Ekaterini Tzamariudaki
, KM3NeT collaboration
, M. D. Filipović
, et al.

School of Science

Demokritos National Centre for Scientific Research
National Technical University of Athens
National Institute for Nuclear Physics

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

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Abstract

KM3NeT is a research infrastructure hosting two neutrino detectors which are currently under construction in the Mediterranean Sea. The KM3NeT/ARCA detector focuses on the detection of high energy neutrinos (>TeV) from astrophysical sources. In this contribution, an analysis of the data obtained during 2021-2022, using machine learning techniques, is presented. The potential of KM3NeT/ARCA to detect a diffuse flux of astrophysical neutrinos at the early stages of the detector construction is reported. The results of this analysis are presented.

Original language	English
Article number	1195
Number of pages	10
Journal	Proceedings of Science
Volume	444
DOIs	https://doi.org/10.22323/1.444.1195
Publication status	Published - 27 Sept 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: 26 Jul 2023 → 3 Aug 2023

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title = "Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022",

abstract = "KM3NeT is a research infrastructure hosting two neutrino detectors which are currently under construction in the Mediterranean Sea. The KM3NeT/ARCA detector focuses on the detection of high energy neutrinos (>TeV) from astrophysical sources. In this contribution, an analysis of the data obtained during 2021-2022, using machine learning techniques, is presented. The potential of KM3NeT/ARCA to detect a diffuse flux of astrophysical neutrinos at the early stages of the detector construction is reported. The results of this analysis are presented.",

author = "Vasileios Tsourapis and Evangelia Drakopoulou and Christos Markou and Anna Sinopoulou and Ekaterini Tzamariudaki and \{KM3NeT collaboration\} and Filipovi{\'c}, \{M. D.\} and \{et al.\}",

year = "2024",

month = sep,

day = "27",

doi = "10.22323/1.444.1195",

language = "English",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

note = "38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

}

TY - JOUR

T1 - Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022

AU - Tsourapis, Vasileios

AU - Drakopoulou, Evangelia

AU - Markou, Christos

AU - Sinopoulou, Anna

AU - Tzamariudaki, Ekaterini

AU - KM3NeT collaboration,

AU - Filipović, M. D.

AU - et al.,

PY - 2024/9/27

Y1 - 2024/9/27

N2 - KM3NeT is a research infrastructure hosting two neutrino detectors which are currently under construction in the Mediterranean Sea. The KM3NeT/ARCA detector focuses on the detection of high energy neutrinos (>TeV) from astrophysical sources. In this contribution, an analysis of the data obtained during 2021-2022, using machine learning techniques, is presented. The potential of KM3NeT/ARCA to detect a diffuse flux of astrophysical neutrinos at the early stages of the detector construction is reported. The results of this analysis are presented.

AB - KM3NeT is a research infrastructure hosting two neutrino detectors which are currently under construction in the Mediterranean Sea. The KM3NeT/ARCA detector focuses on the detection of high energy neutrinos (>TeV) from astrophysical sources. In this contribution, an analysis of the data obtained during 2021-2022, using machine learning techniques, is presented. The potential of KM3NeT/ARCA to detect a diffuse flux of astrophysical neutrinos at the early stages of the detector construction is reported. The results of this analysis are presented.

UR - https://www.scopus.com/pages/publications/85200699437

U2 - 10.22323/1.444.1195

DO - 10.22323/1.444.1195

M3 - Article

AN - SCOPUS:85200699437

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1195

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022

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