Author:
Albert A.,André M.,Anghinolfi M.,Anton G.,Ardid M.,Aubert J.-J.,Aublin J.,Baret B.,Basa S.,Belhorma B.,Bertin V.,Biagi S.,Bissinger M.,Boumaaza J.,Bouta M.,Bouwhuis M.C.,Brânzaş H.,Bruijn R.,Brunner J.,Busto J.,Capone A.,Caramete L.,Carr J.,Carretero V.,Celli S.,Chabab M.,Chau T.N.,Cherkaoui El Moursli R.,Chiarusi T.,Circella M.,Coleiro A.,Colomer-Molla M.,Coniglione R.,Coyle P.,Creusot A.,Díaz A.F.,de Wasseige G.,Deschamps A.,Distefano C.,Di Palma I.,Domi A.,Donzaud C.,Dornic D.,Drouhin D.,Eberl T.,El Khayati N.,Enzenhöfer A.,Ettahiri A.,Fermani P.,Ferrara G.,Filippini F.,Fusco L.,García R.,Gay P.,Glotin H.,Gozzini R.,Graf K.,Guidi C.,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.,Jongen M.,Kadler M.,Kalekin O.,Katz U.,Khan-Chowdhury N.R.,Kouchner A.,Kreykenbohm I.,Kulikovskiy V.,Lahmann R.,Le Breton R.,Lefèvre D.,Leonora E.,Levi G.,Lincetto M.,Lopez-Coto D.,Loucatos S.,Maderer L.,Manczak J.,Marcelin M.,Margiotta A.,Marinelli A.,Martínez-Mora J.A.,Mazzou S.,Melis K.,Migliozzi P.,Moser M.,Moussa A.,Muller R.,Nauta L.,Navas S.,Nezri E.,Nuñez-Castiñeyra A.,O'Fearraigh B.,Organokov M.,Păvălaş G.E.,Pellegrino C.,Perrin-Terrin M.,Piattelli P.,Pieterse C.,Poirè C.,Popa V.,Pradier T.,Randazzo N.,Reck S.,Riccobene G.,Sánchez-Losa A.,Samtleben D.F.E.,Sanguineti M.,Sapienza P.,Schnabel J.,Schüssler F.,Spurio M.,Stolarczyk Th.,Taiuti M.,Tayalati Y.,Thakore T.,Tingay S.J.,Vallage B.,Van Elewyck V.,Versari F.,Viola S.,Vivolo D.,Wilms J.,Zegarelli A.,Zornoza J.D.,Zúñiga J.
Abstract
Abstract
The first gamma-ray burst detections by Imaging Atmospheric
Cherenkov Telescopes have been recently announced: GRB 190114C,
detected by MAGIC, GRB 180720B and GRB 190829A, observed by
H.E.S.S. A dedicated search for neutrinos in space and time
coincidence with the gamma-ray emission observed by IACTs has been
performed using ANTARES data. The search covers both the prompt and
afterglow phases, yielding no neutrinos in coincidence with the
three GRBs studied. Upper limits on the energetics of the neutrino
emission are inferred. The resulting upper limits are several orders
of magnitude above the observed gamma-ray emission, and they do not
allow to constrain the available models.