{"paper":{"title":"Cosmic ray Nickel nuclei spectrum by the NUCLEON experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"1 (2), 14-b Metrolohichna Str., 2), (2) oint Institute for Nuclear Research, (3) Skobeltsyn Institute of Nuclear Physics, 4), (4) Bogolyubov Institute for Theoretical Physics, 6, A.Kurganov (3), A. Panov (3), A. Tkachenko (2, A.Turundaevskiy (3), A. Voronin (3) ((1) \"DUBNA\" University, D. Karmanov (3), D. Podorozhny (3), Dubna, GSP-1, I. Kovalev (3), I. Kudryashov (3), Joliot-Curie, Kiev, Leninskie gory, L. Tkachev (1, Moscow, Moscow region, Moscow State University, O. Vasiliev (3), Russia, Ukraine), Universitetskaya str., V. Grebenyuk (1","submitted_at":"2018-09-19T16:25:00Z","abstract_excerpt":"The NUCLEON experiment is designed to measure chemical composition of cosmic rays with charges from Z=1 to 30 in an energy region from 5*10^11 to 10^15 eV. In this article the data analysis algorithm and spectra of Ni and Fe nuclei, measured in the NUCLEON experiment, are presented."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.07285","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":""},"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"}