@article{fdi:010068139,
  title = {{C}onstraints on the neutrino emission from the {G}alactic {R}idge with the {ANTARES} telescope},
  author = {{A}drian-{M}artinez, {S}. and {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}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}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}ehn, {K}. 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.,},
  editor = {},
  language = {{ENG}},
  abstract = {{A} highly significant excess of high-energy astrophysical neutrinos has been reported by the {I}ce{C}ube {C}ollaboration. {S}ome features of the energy and declination distributions of {I}ce{C}ube events hint at a {N}orth/{S}outh asymmetry of the neutrino flux. {T}his could be due to the presence of the bulk of our {G}alaxy in the {S}outhern hemisphere. {T}he {ANTARES} neutrino telescope, located in the {M}editerranean {S}ea, has been taking data since 2007. {I}t offers the best sensitivity to muon neutrinos produced by galactic cosmic ray interactions in this region of the sky. {I}n this letter a search for an extended neutrino flux from the {G}alactic {R}idge region is presented. {D}ifferent models of neutrino production by cosmic ray propagation are tested. {N}o excess of events is observed and upper limits for different neutrino flux spectral indices {G}amma are set. {F}or {G}amma = 2.4 the 90% confidence level flux upper limit at 100 {T}e{V} for one neutrino flavour corresponds to phi(1f)(0) (100{T}e{V}) = 2.0 . 10(-17) {G}e{V}-1 cm(-2) s(-1) sr(-1). {U}nder this assumption, at most two events of the {I}ce{C}ube cosmic candidates can originate from the {G}alactic {R}idge. {A} simple power-law extrapolation of the {F}ermi-{LAT} flux to account for {I}ce{C}ube {H}igh {E}nergy {S}tarting {E}vents is excluded at 90% confidence level.},
  keywords = {{N}eutrino telescope ; {D}iffuse muon neutrino flux ; {ANTARES} ; {MEDITERRANEE}},
  booktitle = {},
  journal = {{P}hysics {L}etters {B}},
  volume = {760},
  numero = {},
  pages = {143--148},
  ISSN = {0370-2693},
  year = {2016},
  DOI = {10.1016/j.physletb.2016.06.051},
  URL = {https://www.documentation.ird.fr/hor/fdi:010068139},
}