Search for correlations between high-energy gamma rays and neutrinos with the HAWC and ANTARES detectors

Antares Collaboration; HAWC Collaboration

Search for correlations between high-energy gamma rays and neutrinos with the HAWC and ANTARES detectors

Antares Collaboration, HAWC Collaboration

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

Abstract

ANTARES is an underwater neutrino detector in the Mediterranean Sea. Its location, reconstruction accuracy for all-flavor neutrino interactions, and low energy threshold, make it the most sensitive neutrino observatory for searches below 100 TeV over large parts of the sky. The HAWC experiment is a water Cherenkov gamma-ray detector located in Mexico. Thanks to its large field of view it is an excellent instrument to observe the very-high energy gamma-ray sky and perform high-sensitivity surveys of the Galactic Plane. The 10-year ANTARES data set and 3-year HAWC point source surveys are used to search for all-flavor neutrino emission in correlation with the highly-significant observations by HAWC in the gamma-ray sky by means of a maximum-likelihood template search. No significant observation for a correlation has been identified and upper limits on the neutrino flux from the HAWC observations have been set.

Original language	English (US)
Article number	962
Journal	Proceedings of Science
Volume	395
State	Published - Mar 18 2022
Event	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Germany Duration: Jul 12 2021 → Jul 23 2021

All Science Journal Classification (ASJC) codes

General

Cite this

@article{ac9406e2b3d54ee18cf336f293c48003,

title = "Search for correlations between high-energy gamma rays and neutrinos with the HAWC and ANTARES detectors",

abstract = "ANTARES is an underwater neutrino detector in the Mediterranean Sea. Its location, reconstruction accuracy for all-flavor neutrino interactions, and low energy threshold, make it the most sensitive neutrino observatory for searches below 100 TeV over large parts of the sky. The HAWC experiment is a water Cherenkov gamma-ray detector located in Mexico. Thanks to its large field of view it is an excellent instrument to observe the very-high energy gamma-ray sky and perform high-sensitivity surveys of the Galactic Plane. The 10-year ANTARES data set and 3-year HAWC point source surveys are used to search for all-flavor neutrino emission in correlation with the highly-significant observations by HAWC in the gamma-ray sky by means of a maximum-likelihood template search. No significant observation for a correlation has been identified and upper limits on the neutrino flux from the HAWC observations have been set.",

author = "{Antares Collaboration} and {HAWC Collaboration} and A. Albert and S. Alves and M. Andr{\'e} and M. Anghinolfi and G. Anton and M. Ardid and S. Ardid and Aubert, {J. J.} and J. Aublin and B. Baret and S. Basa and B. Belhorma and M. Bendahman and V. Bertin and S. Biagi and M. Bissinger and J. Boumaaza and M. Bouta and Bouwhuis, {M. C.} and H. Br{\^a}nza{\c s} and R. Bruijn and J. Brunner and J. Busto and B. Caiffi and A. Capone and L. Caramete and J. Carr and V. Carretero and S. Celli and M. Chabab and Chau, {T. N.} and {Cherkaoui El Moursli}, R. and T. Chiarusi and M. Circella and A. Coleiro and M. Colomer-Molla and R. Coniglione and P. Coyle and A. Creusot and D{\'i}az, {A. F.} and {de Wasseige}, G. and A. Deschamps and C. Distefano and {Di Palma}, I. and A. Domi and C. Donzaud and D. Dornic and D. Drouhin and T. Eberl and M. Mostaf{\'a}",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "English (US)",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - Search for correlations between high-energy gamma rays and neutrinos with the HAWC and ANTARES detectors

AU - Antares Collaboration

AU - HAWC Collaboration

AU - Albert, A.

AU - Alves, S.

AU - André, M.

AU - Anghinolfi, M.

AU - Anton, G.

AU - Ardid, M.

AU - Ardid, S.

AU - Aubert, J. J.

AU - Aublin, J.

AU - Baret, B.

AU - Basa, S.

AU - Belhorma, B.

AU - Bendahman, M.

AU - Bertin, V.

AU - Biagi, S.

AU - Bissinger, M.

AU - Boumaaza, J.

AU - Bouta, M.

AU - Bouwhuis, M. C.

AU - Brânzaş, H.

AU - Bruijn, R.

AU - Brunner, J.

AU - Busto, J.

AU - Caiffi, B.

AU - Capone, A.

AU - Caramete, L.

AU - Carr, J.

AU - Carretero, V.

AU - Celli, S.

AU - Chabab, M.

AU - Chau, T. N.

AU - Cherkaoui El Moursli, R.

AU - Chiarusi, T.

AU - Circella, M.

AU - Coleiro, A.

AU - Colomer-Molla, M.

AU - Coniglione, R.

AU - Coyle, P.

AU - Creusot, A.

AU - Díaz, A. F.

AU - de Wasseige, G.

AU - Deschamps, A.

AU - Distefano, C.

AU - Di Palma, I.

AU - Domi, A.

AU - Donzaud, C.

AU - Dornic, D.

AU - Drouhin, D.

AU - Eberl, T.

AU - Mostafá, M.

PY - 2022/3/18

Y1 - 2022/3/18

N2 - ANTARES is an underwater neutrino detector in the Mediterranean Sea. Its location, reconstruction accuracy for all-flavor neutrino interactions, and low energy threshold, make it the most sensitive neutrino observatory for searches below 100 TeV over large parts of the sky. The HAWC experiment is a water Cherenkov gamma-ray detector located in Mexico. Thanks to its large field of view it is an excellent instrument to observe the very-high energy gamma-ray sky and perform high-sensitivity surveys of the Galactic Plane. The 10-year ANTARES data set and 3-year HAWC point source surveys are used to search for all-flavor neutrino emission in correlation with the highly-significant observations by HAWC in the gamma-ray sky by means of a maximum-likelihood template search. No significant observation for a correlation has been identified and upper limits on the neutrino flux from the HAWC observations have been set.

AB - ANTARES is an underwater neutrino detector in the Mediterranean Sea. Its location, reconstruction accuracy for all-flavor neutrino interactions, and low energy threshold, make it the most sensitive neutrino observatory for searches below 100 TeV over large parts of the sky. The HAWC experiment is a water Cherenkov gamma-ray detector located in Mexico. Thanks to its large field of view it is an excellent instrument to observe the very-high energy gamma-ray sky and perform high-sensitivity surveys of the Galactic Plane. The 10-year ANTARES data set and 3-year HAWC point source surveys are used to search for all-flavor neutrino emission in correlation with the highly-significant observations by HAWC in the gamma-ray sky by means of a maximum-likelihood template search. No significant observation for a correlation has been identified and upper limits on the neutrino flux from the HAWC observations have been set.

UR - http://www.scopus.com/inward/record.url?scp=85145006967&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85145006967&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85145006967

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 962

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

Search for correlations between high-energy gamma rays and neutrinos with the HAWC and ANTARES detectors

Abstract

All Science Journal Classification (ASJC) codes

Other files and links

Fingerprint

Cite this