{"paper":{"title":"GAMMA-400 gamma-ray observatory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A.A. Kaplun, A.A. Leonov, A.A. Moiseev, A.A. Taraskin, A.I. Arkhangelskiy, A.L. Menshenin, A.M. Galper, A. Rappoldi, A. Tiberio, A. Vacchi, A.V. Bakaldin, B.I. Hnatyk, C. De Donato, D. Gascon, E.A. Bogomolov, E. Berti, E. Mocchiutti, E.M. Tyurin, E. Vannuccini, F. Longo, F. Ryde, G. Bigongiari, G. Castellini, G.I. Vasilyev, G.L. Dedenko, I.V. Arkhangelskaja, I.V. Moskalenko, J.E. Ward, J. Larsson, J.M. Paredes, L. Bergstrom, L. Bonechi, M. Boezio, M. Bongi, M.D. Kheymits, M.F. Runtso, M. Martinez, M. Pearce, M.S. Gorbunov, M. Tavani, M.V. Ulanov, N. Finetti, N. Mori, N.P. Topchiev, N. Zampa, O. Adriani, O.D. Dalkarov, O.V. Serdin, P. Cumani, P. Maestro, P. Papini, P. Picozza, P.S. Marrocchesi, P. Spillantini, P.W. Cattaneo, P.Yu. Naumov, R.L. Aptekar, R. Sparvoli, S. Bottai, S.G. Bobkov, S.I. Suchkov, S. Ricciarini, V.A. Dogiel, V.A. Kaplin, V.A. Loginov, V. Bonvicini, V.E. Korepanov, V.G. Zverev, V.N. Zirakashvili, V.V. Kadilin, V.V. Mikhailov, Yu.I. Stozhkov, Yu.T. Yurkin, Yu.V. Gusakov","submitted_at":"2015-07-22T16:38:31Z","abstract_excerpt":"The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electrons + positrons. Precision investigations of gamma-ray emission from Galactic Center, Crab, Vela, Cygnus, Geminga, and other regions will be performed, as well as diffuse gamma-ray emission, along with measurements of high-energy electron + positron and nuclei fluxes. Furthermore, it will study gamma-ray bursts and gamma-ray emission from the Sun during periods of solar activity. The energy range of GAMMA-400 is expect"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.06246","kind":"arxiv","version":3},"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"}