{"paper":{"title":"Search for extreme energy cosmic ray candidates in the TUS orbital experiment data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"A.A. Botvinko, A.A. Grinyuk, A.E. Puchkov, A.N. Senkovsky, A.V. Shirokov, A.V. Tkachenko, B.A. Khrenov, E. Ponce, G.K. Garipov, H. Salazar, I.H. Park, I.V. Yashin, J. Lee, L.G. Tkachev, M.A. Kaznacheeva, M.I. Panasyuk, M. Kim, M.V. Lavrova, M.Yu. Zotov, N.N. Kalmykov, N.P. Chirskaya, O.A. Saprykin, O. Martinez, P.A. Klimov, S.A. Sharakin, S. Jeong, S.V. Biktemerova, V.E. Eremeev, V.L. Petrov, V.M. Grebenyuk","submitted_at":"2017-06-16T17:53:24Z","abstract_excerpt":"TUS (Track Ultraviolet Setup) is the first space experiment aimed to check the possibility of registering extreme energy cosmic rays (EECRs) at E>50 EeV by measuring the fluorescence signal of extensive air showers in the atmosphere. The detector operates as a part of the scientific payload of the Lomonosov satellite for more than a year. We describe an algorithm of searching for EECR events in the TUS data and briefly discuss a number of candidates selected by formal criteria."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.05369","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"}