@article{fdi:010074446,
  title = {{J}oint constraints on galactic diffuse neutrino emission from the {ANTARES} and {I}ce{C}ube neutrino telescopes},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}ublin, {J}. and {A}vgitas, {T}. and {B}aret, {B}. and {B}arrios-{M}arti, {J}. and {B}asa, {S}. and {B}elhorma, {B}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. and {B}oumaaza, {J}. and {B}ourret, {S}. and {B}ouwhuis, {M}. {C}. and {B}ranzas, {H}. 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}habab, {M}. and {E}l {M}oursli, {R}. {C}. and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}oelho, {J}. {A}. {B}. and {C}oleiro, {A}. and {C}olomer, {M}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}iaz, {A}. {F}. and {D}eschamps, {A}. and {D}istefano, {C}. and {D}i {P}alma, {I}. and {D}omi, {A}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {B}ojaddaini, {I}. and {E}l {K}hayati, {N}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {E}ttahiri, {A}. and {F}assi, {F}. and {F}elis, {I}. and {F}ermani, {P}. and {F}errara, {G}. and {F}usco, {L}. and {G}ay, {P}. and {G}lotin, {H}. and {G}regoire, {T}. and {R}uiz, {R}. {G}. 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 and {I}ce{C}ube {C}ollaboration},
  editor = {},
  language = {{ENG}},
  abstract = {{T}he existence of diffuse {G}alactic neutrino production is expected from cosmic-ray interactions with {G}alactic gas and radiation fields. {T}hus, neutrinos are a unique messenger offering the opportunity to test the products of {G}alactic cosmic-ray interactions up to energies of hundreds of {T}e{V}. {H}ere we present a search for this production using ten years of {A}stronomy with a {N}eutrino {T}elescope and {A}byss environmental {RES}earch ({ANTARES}) track and shower data, as well as seven years of {I}ce{C}ube track data. {T}he data are combined into a joint likelihood test for neutrino emission according to the {KRA}(gamma) model assuming a 5 {P}e{V} per nucleon {G}alactic cosmic-ray cutoff. {N}o significant excess is found. {A}s a consequence, the limits presented in this {L}etter start constraining the model parameter space for {G}alactic cosmic-ray production and transport.},
  keywords = {cosmic rays ; diffusion ; {G}alaxy: disk ; gamma rays: diffuse background ; neutrinos},
  booktitle = {},
  journal = {{A}strophysical {J}ournal {L}etters},
  volume = {868},
  numero = {2},
  pages = {{L}20 [7 p.]},
  ISSN = {2041-8205},
  year = {2018},
  DOI = {10.3847/2041-8213/aaeecf},
  URL = {https://www.documentation.ird.fr/hor/fdi:010074446},
}