{"paper":{"title":"Probing the Galactic neutrino flux at neutrino energies above 200 TeV with the Baikal Gigaton Volume Detector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Doroshenko, A. A. Kulikov, A. D. Avrorin, A. E. Sirenko, A. G. Solovjev, A. N. Dyachok, A. P. Koshechkin, A. P. Stromakov, A. R. Gafarov, A. S. Chepurnov, A. S. Nikolaev, A. V. Avrorin, A. V. Korobchenko, A. V. Plavin, A. V. Skurikhin, B. A. Shaybonov, B. B. Ulzutuev, D. N. Zaborov, D. P. Petukhov, D. V. Naumov, D. V. Semikoz, D. Y. Zvezdov (Baikal-GVD Collaboration), E. A. Bondarev, E. Eckerov\\'a, E. N. Pliskovsky, E. V. Khramov, E. V. Ryabov, E. V. Shirokov, F. \\v{S}imkovic, G. B. Safronov, G. V. Domogatsky, I. A. Belolaptikov, I. A. Perevalova, I. V. Borina, I. V. Kharuk, I. \\v{S}tekl, K. G. Kebkal, K. V. Golubkov, K. V. Konischev, M. I. Kleimenov, M. I. Rozanov, M. M. Kolbin, M. N. Sorokovikov, M. V. Kruglov, N. M. Budnev, N. S. Gorshkov, O. V. Suvorova, R. Dvornick\\'y, R. R. Mirgazov, S. I. Zavyalov, S. O. Koligaev, S. V. Troitsky, T. I. Gress, T. V. Elzhov, V. A. Allakhverdyan, V. A. Chadymov, V. A. Kozhin, V. A. Tabolenko, V. F. Kulepov, V. I. Tretjak, V. K. Kebkal, V. M. Aynutdinov, V. N. Fomin, V. Y. Dik, V. Y. Shishkin, Y. E. Lemeshev, Y. V. Yablokova, Y. Y. Kovalev, Z. Barda\\v{c}ov\\'a, Zh.-A. M. Dzhilkibaev","submitted_at":"2024-11-08T14:52:42Z","abstract_excerpt":"Recent observations of the Galactic component of the high-energy neutrino flux, together with the detection of the diffuse Galactic gamma-ray emission up to sub-PeV energies, open new possibilities to study the acceleration and propagation of cosmic rays in the Milky Way. At the same time, both large non-astrophysical backgrounds at TeV energies and scarcity of neutrino events in the sub-PeV band currently limit these analyses. Here we use the sample of cascade events with estimated neutrino energies above 200 TeV, detected by the partially deployed Baikal Gigaton Volume Detector (GVD) in six "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.05608","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.05608/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}