{"paper":{"title":"Constraints on the neutrino emission from the Galactic Ridge with the ANTARES telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Capone, A. Coleiro, A. Creusot, A. Deschamps, A. Enzenh\\\"ofer, A. Gleixner, A.J. Heijboer, A. Kouchner, A. Margiotta, A. Marinelli, A. Mathieu, A. Moussa, A. S\\'anchez-Losa, A. Trovato, B. Baret, B. Vallage, C. Distefano, C. Donzaud, C. Hugon, C. Lachaud, C. Mueller, C. Pellegrino, C. Perrina, C. Racca, C. Sieger, C. T\\\"onnis, C. Vall\\'ee, C.W James, D. Dornic, D. Drouhin, D. Els\\\"asser, D.F.E. Samtleben, D. Kie{\\ss}ling, D. Lef\\`evre, D. Turpin, D. Vivolo, E. Leonora, E. Nezri, E. Visser, F. Sch\\\"ussler, G. Anton, G. De Bonis, G.E. P\\u{a}v\\u{a}la\\c{s}, G. Illuminati, G. Riccobene, H. Costantini, H. Glotin, H. van Haren, I. El Bojaddaini, I. Felis, I. Kreykenbohm, J.A. Mart\\'inez-Mora, J. Barrios-Mart\\'i, J. Brunner, J. Busto, J. Carr, J.D. Zornoza, J. Hofest\\\"adt, J. H\\\"o{\\ss}l, J.-J. Aubert, J.J. Hern\\'andez-Rey, J. Schnabel, J. Wilms, J. Z\\'u\\~niga (The ANTARES Collaboration), K. Fehn, K. Geyer, K. Graf, K. Roensch, L.A. Fusco, L. Caramete, M. Andr\\'e, M. Anghinolfi, M. Ardid, M.C. Bouwhuis, M. Circella, M. de Jong, M. Kadler, M. Kreter, M. Marcelin, M. Salda\\~na, M. Sanguineti, M. Spurio, M. Taiuti, M. Tselengidou, O. Kalekin, P. Coyle, P. Gay, P. Migliozzi, P. Piattelli, P. Sapienza, R. Bormuth, R. Bruijn, R. Coniglione, R. Gracia-Ruiz, R. Lahmann, S. Adri\\'an-Mart\\'inez, S. Basa, S. Biagi, S. Celli, S. Galat\\`a, S. Gei{\\ss}els\\\"oder, S. Hallmann, S. Loucatos, S. Wagner, T. Avgitas, T. Chiarusi, T. Eberl, Th. Stolarczyk, T. Michael, T. Pradier, T. Seitz, U. Katz, V. Bertin, V. Giordano, V. Kulikovskiy, V. Popa, V. Van Elewyck, Y. Hello","submitted_at":"2016-02-09T15:41:58Z","abstract_excerpt":"Compelling evidence for the existence of astrophysical neutrinos has been reported by the IceCube collaboration. Some features of the energy and declination distributions of IceCube events hint at a North/South asymmetry of the neutrino flux. This could be due to the presence of the bulk of our Galaxy in the Southern hemisphere. The ANTARES neutrino telescope, located in the Mediterranean Sea, has been taking data since 2007. It offers the best sensitivity to muon neutrinos produced by galactic cosmic ray interactions in this region of the sky. In this letter a search for an extended neutrino "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.03036","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}