@article{PAR00022431,
  title = {{ANTARES} upper limits on the multi-{T}e{V} neutrino emission from the {GRB}s detected by {IACT}s},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}nton, {G}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}ublin, {J}. and {B}aret, {B}. and {B}asa, {S}. and {B}elhorma, {B}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}issinger, {M}. and {B}oumaaza, {J}. and {B}outa, {M}. and {B}ouwhuis, {M}. {C}. and {B}ranzas, {H}. and {B}ruijn, {R}. and {B}runner, {J}. and {B}usto, {J}. and {C}apone, {A}. and {C}aramete, {L}. and {C}arr, {J}. and {C}arretero, {V}. and {C}elli, {S}. and {C}habab, {M}. and {C}hau, {T}. {N}. and {E}l {M}oursli, {R}. {C}. and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}oleiro, {A}. and {C}olamer-{M}olla, {M}. and {C}oniglione, {R}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}iaz, {A}. {F}. and de {W}asseige, {G}. and {D}eschamps, {A}. and {D}istefano, {C}. and {D}i {P}alma, {I}. and {D}omi, {A}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {K}hayati, {N}. and {E}nzenhofer, {A}. and {E}ttahiri, {A}. and {F}ermani, {P}. and {F}errara, {G}. and {F}ilippini, {F}. and {F}usco, {L}. and {G}arcia, {R}. and {G}ay, {P}. and {G}lotin, {H}. and {G}ozzini, {R}. and {G}raf, {K}. and {G}uidi, {C}. and {H}allmann, {S}. and van {H}aren, {H}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and et al. and {ANTARES} {C}ollaboration},
  editor = {},
  language = {{ENG}},
  abstract = {{T}he first gamma-ray burst detections by {I}maging {A}tmospheric {C}herenkov {T}elescopes have been recently announced: {GRB} 190114{C}, detected by {MAGIC}, {GRB} 180720{B} and {GRB} 190829{A}, observed by {H}.{E}.{S}.{S}. {A} dedicated search for neutrinos in space and time coincidence with the gamma-ray emission observed by {IACT}s has been performed using {ANTARES} data. {T}he search covers both the prompt and afterglow phases, yielding no neutrinos in coincidence with the three {GRB}s studied. {U}pper limits on the energetics of the neutrino emission are inferred. {T}he resulting upper limits are several orders of magnitude above the observed gamma-ray emission, and they do not allow to constrain the available models.},
  keywords = {neutrino astronomy ; ultra high energy photons and neutrinos ; particle ; acceleration ; gamma ray bursts theory},
  booktitle = {},
  journal = {{J}ournal of {C}osmology and {A}stroparticle {P}hysics},
  numero = {3},
  pages = {092 [16 ]},
  ISSN = {1475-7516},
  year = {2021},
  DOI = {10.1088/1475-7516/2021/03/092},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00022431},
}