{"paper":{"title":"Extended Measurement of the Cosmic-Ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Moiseev, A.M. Messineo, A. Shiomi, A. Sulaj, A.V. Penacchioni, A. Yoshida, B.F. Rauch, C. Checchia, C. Kato, E. Berti, E. Vannuccini, F. Palma, F. Stolzi, G.A. de Nolfo, G. Bigongiari, G. Castellini, G. Collazuol, H. Fuke, H.M. Motz, H. Murakami, H.S. Krawczynski, H. Tomida, I. Takahashi, J.E. Suh, J.F. Krizmanic, J.F. Ormes, J.H. Buckley, J. Kataoka, J. Nishimura, J.P. Wefel, J.W. Mitchell, K. Asano, K. Ebisawa, K. Hibino, K. Ioka, K. Kasahara, K. Kohri, K. Mori, K. Munakata, K. Sakai, K. Yamaoka, K. Yoshida, L. Pacini, M. Bongi, M.G. Bagliesi, M. Hareyama, M.H. Israel, M. Ichimura, M.L. Cherry, M. Mori, M. Sasaki, M. Takayanagi, M. Takita, N. Cannady, N. Hasebe, N. Kawanaka, N. Mori, N. Tateyama, O. Adriani, P. Brogi, P. Maestro, P. Papini, P.S. Marrocchesi, P. Spillantini, R. Kataoka, R. Sparvoli, S. Bonechi, S.B. Ricciarini, S. Miyake, S. Nakahira, S. Okuno, S. Ozawa, S. Torii, S. Ueno, S. Yanagita, T.G. Guzik, T. Hams, T. Lomtadze, T. Sakamoto, T. Tamura, T. Terasawa, V. Di Felice, W. Ishizaki, W.R. Binns, Y. Akaike, Y. Asaoka, Y. Katayose, Y. Kawakubo, Y. Shimizu, Y. Tsunesada, Y. Uchihori","submitted_at":"2018-06-25T23:53:57Z","abstract_excerpt":"Extended results on the cosmic-ray electron + positron spectrum from 11 GeV to 4.8 TeV are presented based on observations with the Calorimetric Electron Telescope (CALET) on the International Space Station utilizing the data up to November 2017. The analysis uses the full detector acceptance at high energies, approximately doubling the statistics compared to the previous result. CALET is an all-calorimetric instrument with a total thickness of 30 $X_0$ at normal incidence and fine imaging capability, designed to achieve large proton rejection and excellent energy resolution well into the TeV "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.09728","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"}