Search for cosmic neutrino point sources and extended sources with 6-21 lines of KM3NeT/ARCA

KM3NeT Collaboration

Search for cosmic neutrino point sources and extended sources with 6-21 lines of KM3NeT/ARCA

KM3NeT Collaboration

Physics

National Institute for Subatomic Physics
National Institute for Nuclear Physics
Université de Strasbourg
Université de Haute-Alsace
IFIC (CSIC-Universitat de València)
Aix-Marseille Université
University of Naples Federico II
Polytechnic University of Catalonia
Demokritos National Centre for Scientific Research
University of Granada
Nantes Université
Polytechnic University of Valencia
Mohammed V University in Rabat
Université de Paris
Université de Caen
Czech Technical University in Prague
Comenius University
University of Bologna
University of Campania Luigi Vanvitelli
University of Hull
North West University
Mohamed I University
University of Salerno
Institute for Space Sciences
University of Amsterdam
Netherlands Organisation for Applied Scientific Research
University of Rome La Sapienza
Cadi Ayyad University
Friedrich-Alexander University Erlangen-Nürnberg
University of the Witwatersrand
University of Catania
International Centre for Radio Astronomy Research
University of Würzburg
Western Sydney University
LPC
University of Genoa
Royal Netherlands Institute for Sea Research - NIOZ
Leiden University
National Centre for Nuclear Research
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
Ivane Javakhishvili Tbilisi State University
The University of Georgia, Tbilisi
Institut universitaire de France
IN2P3 - Institut National de Physique Nucléaire et de Physique Des Particules
Université Montpellier 2

Research output: Contribution to journal › Conference article › peer-review

5 Citations (Scopus)

Abstract

The identification of cosmic objects emitting high energy neutrinos provides new insights about the Universe and its active sources. The existence of cosmic neutrinos has been proven by the IceCube Neutrino Observatory, but the big question of which sources these neutrinos originate from remains largely unanswered. The KM3NeT detector for Astroparticle Research with Cosmics in the Abyss (ARCA), is currently being built in the Mediterranean Sea. It will have an instrumented volume of a cubic kilometre, and excel at identifying cosmic neutrino sources due to its unprecedented angular resolution (< 0.1 degree for muon neutrinos with E > 100 TeV). KM3NeT has a view of the sky complementary to IceCube, and is sensitive to neutrinos across a wide range of energies. Currently KM3NeT/ARCA is taking data with 21 detector lines. This contribution will present the results of point source and extended source searches with KM3NeT/ARCA with data from 2021 and 2022 taken with an evolving detector geometry.

Original language	English
Article number	1018
Journal	Proceedings of Science
Volume	444
Publication status	Published - 27 Sept 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: 26 Jul 2023 → 3 Aug 2023

ASJC Scopus subject areas

Multidisciplinary

Cite this

@article{b66c2ef7048b4dfc932199f6f4f91377,

title = "Search for cosmic neutrino point sources and extended sources with 6-21 lines of KM3NeT/ARCA",

abstract = "The identification of cosmic objects emitting high energy neutrinos provides new insights about the Universe and its active sources. The existence of cosmic neutrinos has been proven by the IceCube Neutrino Observatory, but the big question of which sources these neutrinos originate from remains largely unanswered. The KM3NeT detector for Astroparticle Research with Cosmics in the Abyss (ARCA), is currently being built in the Mediterranean Sea. It will have an instrumented volume of a cubic kilometre, and excel at identifying cosmic neutrino sources due to its unprecedented angular resolution (< 0.1 degree for muon neutrinos with E > 100 TeV). KM3NeT has a view of the sky complementary to IceCube, and is sensitive to neutrinos across a wide range of energies. Currently KM3NeT/ARCA is taking data with 21 detector lines. This contribution will present the results of point source and extended source searches with KM3NeT/ARCA with data from 2021 and 2022 taken with an evolving detector geometry.",

author = "\{KM3NeT Collaboration\} and Rasa Muller and \{van Eeden\}, Thijs and Aart Heijboer and S. Aiello and A. Albert and \{Alves Garre\}, S. and Z. Aly and A. Ambrosone and F. Ameli and M. Andre and E. Androutsou and M. Anguita and L. Aphecetche and M. Ardid and S. Ardid and H. Atmani and J. Aublin and L. Bailly-Salins and Z. Barda{\v c}ov{\'a} and B. Baret and A. Bariego-Quintana and \{Basegmez du Pree\}, S. and Y. Becherini and M. Bendahman and F. Benfenati and M. Benhassi and Benoit, \{D. M.\} and E. Berbee and V. Bertin and S. Biagi and M. Boettcher and D. Bonanno and J. Boumaaza and M. Bouta and M. Bouwhuis and C. Bozza and Bozza, \{R. M.\} and H. Br{\^a}nza{\c s} and F. Bretaudeau and R. Bruijn and J. Brunner and R. Bruno and E. Buis and R. Buompane and J. Busto and B. Caiffi and D. Calvo and S. Campion and A. Capone and S. Razzaque",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

language = "English",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - Search for cosmic neutrino point sources and extended sources with 6-21 lines of KM3NeT/ARCA

AU - KM3NeT Collaboration

AU - Muller, Rasa

AU - van Eeden, Thijs

AU - Heijboer, Aart

AU - Aiello, S.

AU - Albert, A.

AU - Alves Garre, S.

AU - Aly, Z.

AU - Ambrosone, A.

AU - Ameli, F.

AU - Andre, M.

AU - Androutsou, E.

AU - Anguita, M.

AU - Aphecetche, L.

AU - Ardid, M.

AU - Ardid, S.

AU - Atmani, H.

AU - Aublin, J.

AU - Bailly-Salins, L.

AU - Bardačová, Z.

AU - Baret, B.

AU - Bariego-Quintana, A.

AU - Basegmez du Pree, S.

AU - Becherini, Y.

AU - Bendahman, M.

AU - Benfenati, F.

AU - Benhassi, M.

AU - Benoit, D. M.

AU - Berbee, E.

AU - Bertin, V.

AU - Biagi, S.

AU - Boettcher, M.

AU - Bonanno, D.

AU - Boumaaza, J.

AU - Bouta, M.

AU - Bouwhuis, M.

AU - Bozza, C.

AU - Bozza, R. M.

AU - Brânzaş, H.

AU - Bretaudeau, F.

AU - Bruijn, R.

AU - Brunner, J.

AU - Bruno, R.

AU - Buis, E.

AU - Buompane, R.

AU - Busto, J.

AU - Caiffi, B.

AU - Calvo, D.

AU - Campion, S.

AU - Capone, A.

AU - Razzaque, S.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - The identification of cosmic objects emitting high energy neutrinos provides new insights about the Universe and its active sources. The existence of cosmic neutrinos has been proven by the IceCube Neutrino Observatory, but the big question of which sources these neutrinos originate from remains largely unanswered. The KM3NeT detector for Astroparticle Research with Cosmics in the Abyss (ARCA), is currently being built in the Mediterranean Sea. It will have an instrumented volume of a cubic kilometre, and excel at identifying cosmic neutrino sources due to its unprecedented angular resolution (< 0.1 degree for muon neutrinos with E > 100 TeV). KM3NeT has a view of the sky complementary to IceCube, and is sensitive to neutrinos across a wide range of energies. Currently KM3NeT/ARCA is taking data with 21 detector lines. This contribution will present the results of point source and extended source searches with KM3NeT/ARCA with data from 2021 and 2022 taken with an evolving detector geometry.

AB - The identification of cosmic objects emitting high energy neutrinos provides new insights about the Universe and its active sources. The existence of cosmic neutrinos has been proven by the IceCube Neutrino Observatory, but the big question of which sources these neutrinos originate from remains largely unanswered. The KM3NeT detector for Astroparticle Research with Cosmics in the Abyss (ARCA), is currently being built in the Mediterranean Sea. It will have an instrumented volume of a cubic kilometre, and excel at identifying cosmic neutrino sources due to its unprecedented angular resolution (< 0.1 degree for muon neutrinos with E > 100 TeV). KM3NeT has a view of the sky complementary to IceCube, and is sensitive to neutrinos across a wide range of energies. Currently KM3NeT/ARCA is taking data with 21 detector lines. This contribution will present the results of point source and extended source searches with KM3NeT/ARCA with data from 2021 and 2022 taken with an evolving detector geometry.

UR - https://www.scopus.com/pages/publications/85212308387

M3 - Conference article

AN - SCOPUS:85212308387

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1018

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Search for cosmic neutrino point sources and extended sources with 6-21 lines of KM3NeT/ARCA

Abstract

ASJC Scopus subject areas

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