@article{fdi:010057286,
  title = {{S}earch for neutrino emission from gamma-ray flaring blazars with the {ANTARES} telescope},
  author = {{A}drian-{M}artinez, {S}. and {A}l {S}amarai, {I}. and {A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}nton, {G}. and {A}nvar, {S}. and {A}rdid, {M}. and {A}straatmadja, {T}. and {A}ubert, {J}. {J}. and {B}aret, {B}. and {B}asa, {S}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}igongiari, {C}. and {B}ogazzi, {C}. and {B}ou-{C}abo, {M}. and {B}ouhou, {B}. and {B}ouwhuis, {M}. {C}. and {B}runner, {J}. and {B}usto, {J}. and {C}amarena, {F}. and {C}apone, {A}. and {C}arloganu, {C}. and {C}arminati, {G}. and {C}arr, {J}. and {C}ecchini, {S}. and {C}harif, {Z}. and {C}harvis, {P}hilippe and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}ore, {L}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {C}urtil, {C}. and {D}e {B}onis, {G}. and {D}ecowski, {M}. {P}. and {D}ekeyser, {I}. and {D}eschamps, {A}. and {D}istefano, {C}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}orosti, {Q}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}manuele, {U}. and {E}nzenhofer, {A}. and {E}rnenwein, {J}. {P}. and {E}scoffier, {S}. and {F}ehn, {K}. and {F}ermani, {P}. and {F}erri, {M}. and {F}erry, {S}. and {F}laminio, {V}. and {F}olger, {F}. and {F}ritsch, {U}. and {F}uda, {J}. {L}. and {G}alata, {S}. and {G}ay, {P}. and {G}eyer, {K}. and {G}iacomelli, {G}. and {G}iordano, {V}. and {G}omez-{G}onzalez, {J}. {P}. and {G}raft, {K}. and {G}uillard, {G}. and {H}alladjian, {G}. and {H}allewell, {G}. and van {H}aren, {H}. and {H}artman, {J}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and {H}ernandez-{R}ey, {J}. {J}. and {H}erold, {B}. and {H}oessl, {J}. and {H}su, {C}. {C}. and de {J}ong, {M}. and {K}adler, {M}. and {K}alekin, {O}. and {K}appes, {A}. and {K}atz, {U}. and {K}avatsyuk, {O}. and {K}ooijman, {P}. and {K}opper, {C}. and {K}ouchner, {A}. and {K}reykenbohm, {I}. and {K}ulikovskiy, {V}. and {L}ahmann, {R}. and {L}ambard, {G}. and {L}arosa, {G}. and {L}attuada, {D}. and {L}efevre, {D}. and {L}im, {G}. and {L}o {P}resti, {D}. and {L}oehner, {H}. and {L}oucatos, {S}. and {L}ouis, {F}. and {M}angano, {S}. and {M}arcelin, {M}. and {M}argiotta, {A}. and {M}artinez-{M}ora, {J}. {A}. and {M}eli, {A}. and {M}ontaruli, {T}. and {M}organti, {N}. and {M}oscoso, {L}. and {M}otz, {H}. and {N}eff, {M}. and {N}ezri, {E}. and {P}alioselitis, {D}. and {P}avalas, {G}. {E}. and {P}ayet, {K}. and {P}ayre, {P}. and {P}etrovic, {J}. and {P}iattelli, {P}. and {P}icot-{C}lemente, {N}. and {P}opa, {V}. and {P}radier, {T}. and {P}resani, {E}. and {R}acca, {C}. and {R}eed, {C}. and {R}iccobene, {G}. and {R}ichardt, {C}. and {R}ichter, {R}. and {R}iviere, {C}. and {R}obert, {A}. and {R}oensch, {K}. and {R}ostovtsev, {A}. and {R}uiz-{R}ivas, {J}. and {R}ujoiu, {M}. and {R}usso, {G}. {V}. and {S}alesa, {F}. and {S}amtleben, {D}. {F}. {E}. and {S}apienza, {P}. and {S}chock, {F}. and {S}chuller, {J}. {P}. and {S}chussler, {F}. and {S}eitz, {T}. and {S}hanidze, {R}. and {S}imeone, {F}. and {S}pies, {A}. and {S}purio, {M}. and {S}teijger, {J}. {J}. {M}. and {S}tolarczyk, {T}. and {S}anchez-{L}osa, {A}. and {T}aiuti, {M}. and {T}amburini, {C}. and {T}oscano, {S}. and {V}allage, {B}. and {V}allee, {C}. and {V}an {E}lewyck, {V}. and {V}annoni, {G}. and {V}ecchi, {M}. and {V}ernin, {P}. and {V}isser, {E}. and {W}agner, {S}. and {W}ijnker, {G}. and {W}ilms, {J}. and de {W}olf, {E}. and {Y}epes, {H}. and {Z}aborov, {D}. and {Z}ornoza, {J}. {D}. and {Z}uniga, {J}.},
  editor = {},
  language = {{ENG}},
  abstract = {{T}he {ANTARES} telescope is well-suited to detect neutrinos produced in astrophysical transient sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. {R}adio-loud active galactic nuclei with jets pointing almost directly towards the observer, the so-called blazars, are particularly attractive potential neutrino point sources. {T}he all-sky monitor {LAT} on board the {F}ermi satellite probes the variability of any given gamma-ray bright blazar in the sky on time scales of hours to months. {A}ssuming hadronic models, a strong correlation between the gamma-ray and the neutrino fluxes is expected. {S}electing a narrow time window on the assumed neutrino production period can significantly reduce the background. {A}n unbinned method based on the minimization of a likelihood ratio was applied to a subsample of data collected in 2008 (61 days live time). {B}y searching for neutrinos during the high state periods of the {AGN} light curve, the sensitivity to these sources was improved by about a factor of two with respect to a standard time-integrated point source search. {F}irst results on the search for neutrinos associated with ten bright and variable {F}ermi sources are presented.},
  keywords = {{ANTARES} ; {N}eutrino astronomy ; {F}ermi {LAT} transient sources ; {T}ime-dependent search ; {B}lazars},
  booktitle = {},
  journal = {{A}stroparticle {P}hysics},
  volume = {36},
  numero = {1},
  pages = {204--210},
  ISSN = {0927-6505},
  year = {2012},
  DOI = {10.1016/j.astropartphys.2012.06.001},
  URL = {https://www.documentation.ird.fr/hor/fdi:010057286},
}