@article{PAR00010820,
  title = {{S}earch for a correlation between {ANTARES} neutrinos and {P}ierre {A}uger {O}bservatory {UHECR}s arrival directions},
  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}eemster, {L}. {J}. 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}oniglione, {R}. 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}raf, {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}ossl, {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}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}anchez-{L}osa, {A}. 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 {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, {D}. and {Z}uniga, {J}.},
  editor = {},
  language = {{ENG}},
  abstract = {{A} multimessenger analysis optimized for a correlation of arrival directions of ultra-high energy cosmic rays ({UHECR}s) and neutrinos is presented and applied to 2190 neutrino candidate events detected in 2007-2008 by the {ANTARES} telescope and 69 {UHECR}s observed by the {P}ierre {A}uger {O}bservatory between 2004 {J}anuary 1 and 2009 {D}ecember 31. {N}o significant correlation is observed. {A}ssuming an equal neutrino flux ({E}-2 energy spectrum) from all {UHECR} directions, a 90% {CL} upper limit on the neutrino flux of 5.0 x 10(-8) {G}e{V} cm(-2) s(-1) per source is derived.},
  keywords = {astroparticle physics ; cosmic rays ; neutrinos},
  booktitle = {},
  journal = {{A}strophysical {J}ournal},
  volume = {774},
  numero = {1},
  pages = {19 [7 ]},
  ISSN = {0004-637{X}},
  year = {2013},
  DOI = {10.1088/0004-637x/774/1/19},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00010820},
}