{"paper":{"title":"Limits on the Diffuse Gamma-Ray Background above 10 TeV with HAWC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Carrami\\~nana, A. Iriarte, A.J. Smith, A. Lara, A.L. Longinotti, A. Nayerhoda, A. Peisker, A. Sandoval, B.L. Dingus, C. Alvarez, C. Brisbois, C. de Le\\'on, C.D. Rho, C. Espinoza, D. Avila Rojas, D. Garcia, D. Huang, D. Kieda, D. Rosa-Gonz\\'alez, E. Belmont-Moreno, E. De la Fuente, E.G. P\\'erez-P\\'erez, E. Moreno, E. Ruiz-Velasco, E. Willox, F. Garfias, F. Hueyotl-Zahuantitla, F. Salesa Greus, F. Ure\\~na-Mena, G. Luis-Raya, H.A. Ayala Solares, HAWC Collaboration: A. Albert, H. Le\\'on Vargas, H. Salazar, H. Zhou, I. Torres, J.A. Garc\\'ia-Gonz\\'alez, J.A. Goodman, J.A. Matthews, J.A. Morales-Soto, J.C. Arteaga-Vel\\'azquez, J.C. D\\'iaz-V\\'elez, J. Cotzomi, J.D. \\'Alvarez, J. Hinton, J. Mart\\'inez-Castro, J.P. Harding, J. Serna-Franco, J.T. Linnemann, K. Engel, K.L. Fan, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, L. Villase\\~nor, M.A. DuVernois, M. Durocher, M. Fern\\'andez Alonso, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Newbold, M. Schneider, M.U. Nisa, N. Fraija, N. Omodei, O. Chaparro-Amaro, O. Martinez, O. Tibolla, P. H\\\"untemeyer, P. Miranda-Romagnoli, R. Alfaro, R. Babu, R. Diaz Hernandez, R. Noriega-Papaqui, R. Torres-Escobedo, R. Turner, R.W. Springer, S. Casanova, S. Couti\\~no de Le\\'on, S. Hernandez, S. Kaufmann, T. Capistr\\'an, U. Cotti, V. Joshi, W.H. Lee, X. Wang, Y. P\\'erez Araujo, Y. Son","submitted_at":"2022-09-16T18:00:04Z","abstract_excerpt":"The high-energy Diffuse Gamma-Ray Background (DGRB) is expected to be produced by unresolved isotropically distributed astrophysical objects, potentially including dark matter annihilation or decay emissions in galactic or extragalactic structures. The DGRB has only been observed below 1 TeV; above this energy, upper limits have been reported. Observations or stringent limits on the DGRB above this energy could have significant multi-messenger implications, such as constraining the origin of TeV-PeV astrophysical neutrinos detected by IceCube. The High Altitude Water Cherenkov (HAWC) Observato"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.08106","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.08106/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"}