@article{PAR00016179,
  title = {{T}ime-dependent search for neutrino emission from {X}-ray binaries with the {ANTARES} telescope},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nton, {G}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}vgitas, {T}. and {B}aret, {B}. and {B}arrios-{M}arti, {J}. and {B}asa, {S}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. 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}elli, {S}. and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}oleiro, {A}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}i {P}alma, {I}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {B}ojaddaini, {I}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {F}elis, {I}. 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}lotin, {H}. and {G}racia-{R}uiz, {R}. and {G}raf, {K}. and {H}allmann, {S}. and van {H}aren, {H}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and et al. and {A}ntares {C}ollaboration},
  editor = {},
  language = {{ENG}},
  abstract = {{ANTARES} is currently the largest neutrino telescope operating in the {N}orthern {H}emisphere, aiming at the detection of high-energy neutrinos from astrophysical sources. {N}eutrino telescopes constantly monitor at least one complete hemisphere of the sky, and are thus well-suited to detect neutrinos produced in transient astrophysical sources. {A} time-dependent search has been applied to a list of 33 {X}-ray binaries undergoing high flaring activities in satellite data ({RXTE}/{ASM}, {MAXI} and {S}wift/{BAT}) and during hardness transition states in the 2008-2012 period. {T}he background originating from interactions of charged cosmic rays in the {E}arth's atmosphere is drastically reduced by requiring a directional and temporal coincidence with astrophysical phenomena. {T}he results of this search are presented together with comparisons between the neutrino flux upper limits and the neutrino flux predictions from astrophysical models. {T}he neutrino flux upper limits resulting from this search limit the jet parameter space for some astrophysical models.},
  keywords = {neutrino astronomy ; {X}-ray binaries ; {X}-ray telescopes},
  booktitle = {},
  journal = {{J}ournal of {C}osmology and {A}stroparticle {P}hysics},
  numero = {4},
  pages = {art. 019},
  ISSN = {1475-7516},
  year = {2017},
  DOI = {10.1088/1475-7516/2017/04/019},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00016179},
}