Results of the follow-up of ANTARES neutrino alerts

ANTARES Collaboration; MASTER Collaboration; M.W.A. collaboration; Swift collaboration; TAROT collaboration

doi:10.1088/1475-7516/2024/09/042

Results of the follow-up of ANTARES neutrino alerts

ANTARES Collaboration
, MASTER Collaboration
, M.W.A. collaboration
, Swift collaboration
, TAROT collaboration

Université de Strasbourg
Université de Haute Alsace
University of Valencia
Universidad Politecnica de Catalunia
Universitat Politècnica de València
Aix-Marseille Université
Astroparticule and Cosmol APC
LAM
Centre National de l'Energie des Sciences Techniques Nucleaires
Faculté des Sciences Rabat
INFN Sezione di Bologna
University of Bologna
INFN Sezione di Catania
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
Université Mohamed Premier
Science Park 105
Institute of Space Sciences
University of Amsterdam
Sezione di Genova
Sezione di Roma
Dipartimento di Fisica
Université Cadi Ayyad
INFN Sezione di Bari
International Centre for Radio Astronomy Research
University of Granada
Université Paris-Saclay
University of Salerno
Clermont-Auvergne University
Université du Sud Toulon-Var
University of Genoa
Royal Netherlands Institute for Sea Research
Observatoire de la Côte d'Azur
Universiteit Leiden
University of Würzburg
USTV
INFN Sezione di Napoli
University of Naples Federico II
Institut Universitaire de France
Moscow State University
South African Astronomical Observatory
Southern African Large Telescope
University of Cape Town
University of the Free State
Irkutz State University
Universidad Nacional de San Juan
Observatorio Astronomico Felix Aguilar(OAFA)
Instituto de Astrofisica de Canarias
University of California, Berkeley
SETI Institute
University of Wisconsin-Milwaukee
Swinburne University of Technology
ARC Centre of Excellence for Gravitational Wave Discovery
Commonwealth Scientific and Industrial Research Organization
Curtin University
University of Leicester
Pennsylvania State University
NASA Goddard Space Flight Center
University of Maryland, College Park
Université Côte d’Azur
IRAP/CNRS
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
Ruhr-University Bochum
Universidad Católica del Norte
Observatoire de Sauverny
Dpartement d'Astronomie Université de Geǹve

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

5 Citations (Scopus)

Résumé

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES collaboration since 2009. This program, named TAToO, has triggered robotic optical telescopes (MASTER, TAROT, ROTSE and the SVOM ground based telescopes) immediately after the detection of any relevant neutrino candidate and scheduled several observations in the weeks following the detection. A subset of ANTARES events with highest probabilities of being of cosmic origin has also been followed by the Swift and the INTEGRAL satellites, the Murchison Widefield Array radio telescope and the H.E.S.S. high-energy gamma-ray telescope. The results of twelve years of observations are reported. In September 2015, ANTARES issued a neutrino alert and during the follow-up, a potential transient counterpart was identified by Swift and MASTER. A multi-wavelength follow-up campaign has allowed to identify the nature of this source and has proven its fortuitous association with the neutrino. No other optical and X-ray counterpart has been significantly associated with an ANTARES candidate neutrino signal. Constraints on transient neutrino emission have been set. The return of experience is particularly important for the design of the alert system of KM3NeT, the next generation neutrino telescope in the Mediterranean Sea.

langue originale	Anglais
Numéro d'article	042
journal	Journal of Cosmology and Astroparticle Physics
Volume	2024
Numéro de publication	9
Les DOIs	https://doi.org/10.1088/1475-7516/2024/09/042
état	Publié - 1 sept. 2024
Modification externe	Oui

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10.1088/1475-7516/2024/09/042

Contient cette citation

@article{4ac1ee8891f0473eae09c24463cf73f3,

title = "Results of the follow-up of ANTARES neutrino alerts",

abstract = "High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES collaboration since 2009. This program, named TAToO, has triggered robotic optical telescopes (MASTER, TAROT, ROTSE and the SVOM ground based telescopes) immediately after the detection of any relevant neutrino candidate and scheduled several observations in the weeks following the detection. A subset of ANTARES events with highest probabilities of being of cosmic origin has also been followed by the Swift and the INTEGRAL satellites, the Murchison Widefield Array radio telescope and the H.E.S.S. high-energy gamma-ray telescope. The results of twelve years of observations are reported. In September 2015, ANTARES issued a neutrino alert and during the follow-up, a potential transient counterpart was identified by Swift and MASTER. A multi-wavelength follow-up campaign has allowed to identify the nature of this source and has proven its fortuitous association with the neutrino. No other optical and X-ray counterpart has been significantly associated with an ANTARES candidate neutrino signal. Constraints on transient neutrino emission have been set. The return of experience is particularly important for the design of the alert system of KM3NeT, the next generation neutrino telescope in the Mediterranean Sea.",

keywords = "X-ray telescopes, gamma ray experiments, neutrino astronomy, neutrino experiments",

author = "\{ANTARES Collaboration\} and \{MASTER Collaboration\} and \{M.W.A. collaboration\} and \{Swift collaboration\} and \{TAROT collaboration\} and A. Albert and S. Alves and M. Andr{\'e} and M. Ardid and S. Ardid and Aubert, \{J. J.\} and J. Aublin and B. Baret and S. Basa and Y. Becherini and B. Belhorma and M. Bendahman and F. Benfenati and V. Bertin and S. Biagi and M. Bissinger and J. Boumaaza and M. Bouta and Bouwhuis, \{M. C.\} and H. Brǎnza{\c s} and R. Bruijn and J. Brunner and J. Busto and B. Caiffi and D. Calvo and S. Campion and A. Capone and L. Caramete and F. Carenini and J. Carr and V. Carretero and S. Celli and L. Cerisy and M. Chabab and \{El Moursli\}, \{R. Cherkaoui\} and T. Chiarusi and M. Circella and Coelho, \{J. A.B.\} and A. Coleiro and R. Coniglione and P. Coyle and A. Creusot and Cruz, \{A. S.M.\} and D{\'i}az, \{A. F.\} and \{De Martino\}, B. and C. Distefano and \{Di Palma\}, I. and C. Donzaud and D. Dornic and S. Chaty",

note = "Publisher Copyright: {\textcopyright} 2024 IOP Publishing Ltd and Sissa Medialab.",

year = "2024",

month = sep,

day = "1",

doi = "10.1088/1475-7516/2024/09/042",

language = "English",

volume = "2024",

journal = "Journal of Cosmology and Astroparticle Physics",

issn = "1475-7516",

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TY - JOUR

T1 - Results of the follow-up of ANTARES neutrino alerts

AU - ANTARES Collaboration

AU - MASTER Collaboration

AU - M.W.A. collaboration

AU - Swift collaboration

AU - TAROT collaboration

AU - Albert, A.

AU - Alves, S.

AU - André, M.

AU - Ardid, M.

AU - Ardid, S.

AU - Aubert, J. J.

AU - Aublin, J.

AU - Baret, B.

AU - Basa, S.

AU - Becherini, Y.

AU - Belhorma, B.

AU - Bendahman, M.

AU - Benfenati, F.

AU - Bertin, V.

AU - Biagi, S.

AU - Bissinger, M.

AU - Boumaaza, J.

AU - Bouta, M.

AU - Bouwhuis, M. C.

AU - Brǎnzaş, H.

AU - Bruijn, R.

AU - Brunner, J.

AU - Busto, J.

AU - Caiffi, B.

AU - Calvo, D.

AU - Campion, S.

AU - Capone, A.

AU - Caramete, L.

AU - Carenini, F.

AU - Carr, J.

AU - Carretero, V.

AU - Celli, S.

AU - Cerisy, L.

AU - Chabab, M.

AU - El Moursli, R. Cherkaoui

AU - Chiarusi, T.

AU - Circella, M.

AU - Coelho, J. A.B.

AU - Coleiro, A.

AU - Coniglione, R.

AU - Coyle, P.

AU - Creusot, A.

AU - Cruz, A. S.M.

AU - Díaz, A. F.

AU - De Martino, B.

AU - Distefano, C.

AU - Di Palma, I.

AU - Donzaud, C.

AU - Dornic, D.

AU - Chaty, S.

PY - 2024/9/1

Y1 - 2024/9/1

N2 - High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES collaboration since 2009. This program, named TAToO, has triggered robotic optical telescopes (MASTER, TAROT, ROTSE and the SVOM ground based telescopes) immediately after the detection of any relevant neutrino candidate and scheduled several observations in the weeks following the detection. A subset of ANTARES events with highest probabilities of being of cosmic origin has also been followed by the Swift and the INTEGRAL satellites, the Murchison Widefield Array radio telescope and the H.E.S.S. high-energy gamma-ray telescope. The results of twelve years of observations are reported. In September 2015, ANTARES issued a neutrino alert and during the follow-up, a potential transient counterpart was identified by Swift and MASTER. A multi-wavelength follow-up campaign has allowed to identify the nature of this source and has proven its fortuitous association with the neutrino. No other optical and X-ray counterpart has been significantly associated with an ANTARES candidate neutrino signal. Constraints on transient neutrino emission have been set. The return of experience is particularly important for the design of the alert system of KM3NeT, the next generation neutrino telescope in the Mediterranean Sea.

AB - High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino alerts has been operating within the ANTARES collaboration since 2009. This program, named TAToO, has triggered robotic optical telescopes (MASTER, TAROT, ROTSE and the SVOM ground based telescopes) immediately after the detection of any relevant neutrino candidate and scheduled several observations in the weeks following the detection. A subset of ANTARES events with highest probabilities of being of cosmic origin has also been followed by the Swift and the INTEGRAL satellites, the Murchison Widefield Array radio telescope and the H.E.S.S. high-energy gamma-ray telescope. The results of twelve years of observations are reported. In September 2015, ANTARES issued a neutrino alert and during the follow-up, a potential transient counterpart was identified by Swift and MASTER. A multi-wavelength follow-up campaign has allowed to identify the nature of this source and has proven its fortuitous association with the neutrino. No other optical and X-ray counterpart has been significantly associated with an ANTARES candidate neutrino signal. Constraints on transient neutrino emission have been set. The return of experience is particularly important for the design of the alert system of KM3NeT, the next generation neutrino telescope in the Mediterranean Sea.

KW - X-ray telescopes

KW - gamma ray experiments

KW - neutrino astronomy

KW - neutrino experiments

U2 - 10.1088/1475-7516/2024/09/042

DO - 10.1088/1475-7516/2024/09/042

M3 - Article

AN - SCOPUS:85205472449

SN - 1475-7516

VL - 2024

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

IS - 9

M1 - 042

ER -

Results of the follow-up of ANTARES neutrino alerts

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