Results of the follow-up of ANTARES neutrino alerts

Albert A, Alves S, André M, Ardid M, Ardid S, Aubert JJ, Aublin J, Baret B, Basa S, Becherini Y, Belhorma B, Bendahman M, Benfenati F, Bertin V, Biagi S, Bissinger M, Boumaaza J, Bouta M, Bouwhuis MC, Brǎnzaş H, Bruijn R, Brunner J, Busto J, Caiffi B, Calvo D, Campion S, Capone A, Caramete L, Carenini F, Carr J, Carretero V, Celli S, Cerisy L, Chabab M, El Moursli RC, Chiarusi T, Circella M, Coelho JA, Coleiro A, Coniglione R, Coyle P, Creusot A, Cruz AS, Díaz AF, De Martino B, Distefano C, Di Palma I, Donzaud C, Dornic D, Drouhin D, Eberl T, van Eeden T, van Eijk D, El Hedri S, El Khayati N, Enzenhöfer A, Fermani P, Ferrara G, Filippini F, Fusco L, Gagliardini S, García J, Oliver CG, Gay P, Geißelbrecht N, Glotin H, Gozzini R, Gracia Ruiz R, Graf K, Guidi C, Haegel L, Hallmann S, van Haren H, Heijboer AJ, Hello Y, Hennig L, Hernańdez-Rey JJ, Hößl J, Hofestädt J, Huang F, Illuminati G, James CW, Jisse-Jung B, de Jong M, de Jong P, Kadler M, Kalekin O, Katz U, Kouchner A, Kreykenbohm I, Kulikovskiy V, Lahmann R, Lamoureux M, Lazo A, Lefèvre D, Leonora E, Levi G, Le Stum S, Loucatos S, Maderer L, Manczak J, Marcelin M, Margiotta A, Marinelli A, Martínez-Mora JA, Migliozzi P, Moussa A, Muller R, Navas S, Nezri E, Fearraigh BO, Oukacha E, Pǎun A, Pǎvǎlan GE, Peña-Martínez S, Perrin-Terrin M, Piattelli P, Popa V, Pradier T, Randazzo N, Real D, Riccobene G, Romanov A, Sánchez-Losa A, Saina A, Greus FS, Samtleben DF, Sanguineti M, Sapienza P, Schnabel J, Schumann J, Schüssler F, Seneca J, Spurio M, Stolarczyk T, Taiuti M, Tayalati Y, Tingay SJ, Vallage B, Vannoye G, Van Elewyck V, Viola S, Vivolo D, Wilms J, Zavatarelli S, Zegarelli A, Zornoza JD, Zúñiga J, Lipunov V, Antipov G, Balanutsa P, Buckley D, Budnev N, Chasovnikov A, Cheryasov D, Francile C, Gabovich A, Gorbovskoy E, Gorbunov I, Gress O, Kornilov V, Kuznetsov A, Iyudin A, Podesta R, Podesta F, Lopez RR, Senik V, Sierra-Rucart M, Svertilov S, Tiurina N, Vlasenko D, Yashin I, Zhirkov K, Croft S, Kaplan DL, Anderson GE, Williams A, Dobie D, Bannister KW, Hancock PJ, Evans PA, Kennea JA, Osborne JP, Cenko SB, Antier S, Atteia JL, Boër M, Klotz A, Chaty S, Hodapp K, Savchenko V (2024)


Publication Language: English

Publication Type: Journal article

Publication year: 2024

Journal

Book Volume: 2024

Article Number: 042

Journal Issue: 9

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

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.

Authors with CRIS profile

Involved external institutions

National Institute for Nuclear Physics / Istituto Nazionale di Fisica Nucleare (INFN) IT Italy (IT) Mohammed V University (UMVA) / جامعة محمد الخامس‎ MA Morocco (MA) Université Paris Cité FR France (FR) Institut national de physique nucléaire et de physique des particules (IN2P3) FR France (FR) Laboratoire d'Astrophysique de Marseille (LAM) FR France (FR) Julius-Maximilians-Universität Würzburg DE Germany (DE) FOM Foundation NL Netherlands (NL) Mohammed First University / Université Mohammed Premier / جامعة محمد الأول MA Morocco (MA) Polytechnic University of Catalonia / Universitat Politècnica de Catalunya · BarcelonaTech (UPC) / Universidad Politécnica de Cataluña ES Spain (ES) University of València / Universitat de València ES Spain (ES) Polytechnic University of Valencia / Universidad Politécnica de Valencia ES Spain (ES) National Institute for Laser, Plasma & Radiation Physics (INFLPR) RO Romania (RO) Lomonosov Moscow State University / Московский государственный университет имени М.В.Ломоносова RU Russian Federation (RU) International Centre for Radio Astronomy Research AU Australia (AU) Mediterranean Institute of Oceanography (MIO) / Institut méditerranéen d'océanologie FR France (FR) National University of San Juan / Universidad Nacional de San Juan AR Argentina (AR) University of Wisconsin-Milwaukee US United States (USA) (US) Commonwealth Scientific and Industrial Research Organisation (CSIRO) AU Australia (AU) University of Leicester GB United Kingdom (GB) Institut de Recherche en Astrophysique et Planétologie (IRAP) FR France (FR) University of Côte d'Azur / Université Côte d'Azur FR France (FR) École Polytechnique Fédérale de Lausanne (EPFL) CH Switzerland (CH) Pennsylvania State University (Penn State) US United States (USA) (US) Université de Strasbourg (UDS) FR France (FR) South African Astronomical Observatory (SAAO) ZA South Africa (ZA) Royal Netherlands Institute for Sea Research (NIOZ) NL Netherlands (NL) Institute of Research into the Fundamental Laws of the Universe / Institut de recherche sur les lois fondamentales de l'univers (IRFU) FR France (FR) University of Toulon / Université de Toulon (UTLN) FR France (FR) Cadi Ayyad University / جامعة القاضي عياض‎ MA Morocco (MA) Swinburne University of Technology AU Australia (AU) Irkutsk State University / Иркутский государственный университет RU Russian Federation (RU) Instituto de Astrofísica de Canarias (IAC) ES Spain (ES) UMR Géoazur - Campus Azur du CNRS FR France (FR) University of California, Berkeley (UC Berkeley) US United States (USA) (US) Università degli Studi di Salerno IT Italy (IT) Universidad de Granada ES Spain (ES) National Aeronautics and Space Administration (NASA) US United States (USA) (US) Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences PL Poland (PL) The National Center for Nuclear Energy, Sciences and Techniques (CNESTEN) MA Morocco (MA) Université Paris-Saclay FR France (FR)

How to cite

APA:

Albert, A., Alves, S., André, M., Ardid, M., Ardid, S., Aubert, J.J.,... Savchenko, V. (2024). Results of the follow-up of ANTARES neutrino alerts. Journal of Cosmology and Astroparticle Physics, 2024(9). https://doi.org/10.1088/1475-7516/2024/09/042

MLA:

Albert, A., et al. "Results of the follow-up of ANTARES neutrino alerts." Journal of Cosmology and Astroparticle Physics 2024.9 (2024).

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