@article{PAR00014172,
  title = {{S}earch for muon-neutrino emission from {G}e{V} and {T}e{V} gamma-ray flaring blazars using five years of data of the {ANTARES} telescope},
  author = {{A}drian-{M}artinez, {S}. and {A}lbert, {A}. and {A}ndre, {M}. and {A}nton, {G}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {B}aret, {B}. and {B}arrios-{M}arti, {J}. and {B}asa, {S}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}ogazzi, {C}. and {B}ormuth, {R}. and {B}ou-{C}abo, {M}. and {B}ouwhuis, {M}. {C}. 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}hiarusi, {T}. and {C}ircella, {M}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}ekeyser, {I}. and {D}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {D}umas, {A}. and {E}berl, {T}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {F}ehn, {K}. and {F}elis, {I}. and {F}ermani, {P}. and {F}olger, {F}. and {F}usco, {L}. {A}. and {G}alata, {S}. and {G}ay, {P}. and {G}eisselsoder, {S}. and {G}eyer, {K}. and {G}iordano, {V}. and {G}leixner, {A}. and {G}racia-{R}uiz, {R}. and {G}raf, {K}. and van {H}aren, {H}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and et al.},
  editor = {},
  language = {{ENG}},
  abstract = {{T}he {ANTARES} telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. {T}he background due to atmospheric particles can be drastically reduced, and the point-source sensitivity improved, by selecting a narrow time window around possible neutrino production periods. {B}lazars, being radio-loud active galactic nuclei with their jets pointing almost directly towards the observer, are particularly attractive potential neutrino point sources, since they are among the most likely sources of the very high-energy cosmic rays. {N}eutrinos and gamma rays may be produced in hadronic interactions with the surrounding medium. {M}oreover, blazars generally show high time variability in their light curves at different wavelengths and on various time scales. {T}his paper presents a time-dependent analysis applied to a selection of flaring gamma-ray blazars observed by the {FERMI}/{LAT} experiment and by {T}e{V} {C}herenkov telescopes using five years of {ANTARES} data taken from 2008 to 2012. {T}he results are compatible with fluctuations of the background. {U}pper limits on the neutrino fluence have been produced and compared to the measured gamma-ray spectral energy distribution.},
  keywords = {{X}-ray binaries ; neutrino astronomy},
  booktitle = {},
  journal = {{J}ournal of {C}osmology and {A}stroparticle {P}hysics},
  numero = {12},
  pages = {014},
  ISSN = {1475-7516},
  year = {2015},
  DOI = {10.1088/1475-7516/2015/12/014},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00014172},
}