{"paper":{"title":"Orbital Modulation of Gamma-Rays Beyond 100 TeV from LS 5039","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bernal, A. Carrami\\~nana, A. Gonzalez Mu\\~noz, A.J. Smith, A. Lara, A.L. Longinotti, Araujo, A. Rodriguez Parra, A. Sandoval, B.L. Dingus, C. de Le\\'on, C.D. Rho, C. Espinoza, D. Avila Rojas, D. Depaoli, D. Huang, D. Kieda, D. Rosa-Gonz\\'alez, D. Salazar-Gallegos, E. Belmont-Moreno, E.G. P\\'erez-P\\'erez, E. Moreno, E. Ponce, E. Varela, F. Hueyotl-Zahuantitla, G. Luis-Raya, G. Schwefer, H.A. Ayala Solares, H. Goksu, H. Le\\'on Vargas, H. Salazar, H. Wu, H. Zhou, I. Herzog, I.J. Watson, I. Torres, J.A. Garc\\'ia-Gonz\\'alez, J.A. Gonz\\'alez, J.A.Goodman, J.A. Matthews, J.A. Morales-Soto, J.C. Arteaga-Vel\\'azquez, J. Cotzomi, J. Lee, J. Mart\\'inez-Castro, J.P. Harding, J. Serna-Franco, J.T. Linnemann, K. Engel, K. Fang, K.L. Fan, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, M.A. DuVernois, M. Araya, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Najafi, M. Roth, M. Schneider, M.U. Nisa, N. Di Lalla, N. Omodei, O. Martinez, O. Tibolla, P. Bangale, P. Desiati, P. H\\\"untemeyer, P. Miranda-Romagnoli, R. Alfaro, R. Babu, R. Diaz Hernandez, R. Torres-Escobedo, R. Turner, R.W. Springer, S. Casanova, S. Couti\\~no de Le\\'on, S. Groetsch, S. Hern\\'andez-Cadena, S. Kaufmann, S. Yu, S. Yun-C\\'arcamo, T. Capistr\\'an, T. Ergin, U. Cotti, X. Wang, Y. P\\'erez, Y. Son, Z. Wang","submitted_at":"2025-03-26T19:32:26Z","abstract_excerpt":"Gamma-ray binaries are systems composed of a compact object orbiting a massive companion star. The interaction between these two objects can drive relativistic outflows, either jets or winds, in which particles can be accelerated to energies reaching hundreds of tera-electronvolts (TeV). It is however still debated where and under which physical conditions particles are accelerated in these objects and ultimately whether protons can be accelerated up to PeV energies. Among the well-known gamma-ray binaries, LS 5039 is a high-mass X-ray binary (HMXB) with an orbital period of 3.9 days that has "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.20947","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/2503.20947/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"}