Author:
Albert A.,Alves S.,André M.,Ardid M.,Ardid S.,Aubert J.-J.,Aublin J.,Baret B.,Basa S.,Belhorma B.,Bendahman M.,Benfenati F.,Bertin V.,Biagi S.,Bissinger M.,Boumaaza J.,Bouta M.,Bouwhuis M.C.,Brânzaş H.,Bruijn R.,Brunner J.,Busto J.,Caiffi B.,Calvo D.,Campion S.,Capone A.,Caramete L.,Carr J.,Carretero V.,Celli S.,Chabab M.,Chau T.N.,Cherkaoui El Moursli R.,Chiarusi T.,Circella M.,Coelho J.A.B.,Coleiro A.,Coniglione R.,Coyle P.,Creusot A.,Díaz A.F.,De Martino B.,Distefano C.,Di Palma I.,Domi A.,Donzaud C.,Dornic D.,Drouhin D.,Eberl T.,van Eeden T.,van Eijk D.,El Khayati N.,Enzenhöfer A.,Fasano M.,Fermani P.,Ferrara G.,Filippini F.,Fusco L.,Gagliardini S.,García J.,Gay P.,Geißelbrecht N.,Glotin H.,Gozzini R.,Gracia Ruiz R.,Graf K.,Guidi C.,Haegel L.,Hallmann S.,van Haren H.,Heijboer A.J.,Hello Y.,Hernández-Rey J.J.,Hößl J.,Hofestädt J.,Huang F.,Illuminati G.,James C.W.,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.,Lefèvre D.,Leonora E.,Levi G.,Le Stum S.,Lopez-Coto D.,Loucatos S.,Maderer L.,Manczak J.,Marcelin M.,Margiotta A.,Marinelli A.,Martínez-Mora J.A.,Melis K.,Migliozzi P.,Moussa A.,Muller R.,Nauta L.,Navas S.,Nezri E.,Fearraigh B.Ó,Păun A.,Păvălaş G.E.,Pellegrino C.,Perrin-Terrin M.,Pestel V.,Piattelli P.,Pieterse C.,Poirè C.,Popa V.,Pradier T.,Randazzo N.,Real D.,Reck S.,Riccobene G.,Romanov A.,Saina A.,Sánchez-Losa A.,Salesa Greus F.,Samtleben D.F.E.,Sanguineti M.,Sapienza P.,Schnabel J.,Schumann J.,Schüssler F.,Seneca J.,Spurio M.,Stolarczyk Th.,Taiuti M.,Tayalati Y.,Tingay S.J.,Vallage B.,Van Elewyck V.,Versari F.,Viola S.,Vivolo D.,Wilms J.,Zavatarelli S.,Zegarelli A.,Zornoza J.D.,Zúñiga J.
Abstract
Abstract
By constantly monitoring a very large portion of the sky, neutrino telescopes are well-designed to detect neutrinos emitted by transient astrophysical events. Real-time searches with the ANTARES telescope have been performed to look for neutrino candidates coincident with gamma-ray bursts detected by the Swift and Fermi satellites, high-energy neutrino events registered by IceCube, transient events from blazars monitored by HAWC, photon-neutrino coincidences by AMON notices and gravitational wave candidates observed by LIGO/Virgo. By requiring temporal coincidence, this approach increases the sensitivity and the significance of a potential discovery. This paper summarises the results of the follow-up performed of the ANTARES telescope between January 2014 and February 2022, which corresponds to the end of the data-taking period.