{"paper":{"title":"Observation of Anisotropy of TeV Cosmic Rays with Two Years of HAWC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Becerril, A. Bernal, A. Carrami\\~nana, A. Gonz\\'alez Mu\\~noz, A. Iriarte, A. Jardin-Blicq, A.J. Smith, A. Lara, A.L. Longinotti, A. Nayerhoda, A. Sandoval, A.U. Abeysekara, A. Zepeda, B. Hona, B.L. Dingus, C. Alvarez, C. de Le\\'on, C.D. Rho, C.M. Hui, C. Rivi\\`ere, D. Avila Rojas, D. L\\'opez-C\\'amara, D. Rosa-Gonz\\'alez, D.W. Fiorino, E. Belmont-Moreno, E. De la Fuente, E.G. P\\'erez-P\\'erez, E. Moreno, E. Ruiz-Velasco, F. Garfias, F. Hueyotl-Zahuantitla, F. Salesa Greus, F. Werner, G. Luis-Raya, G. Sinnis, G. Vianello, H.A. Ayala Solares, H. Le\\'on Vargas, H. Mart\\'inez-Huerta, H. Schoorlemmer, H. Zhou, I. Martinez-Castellanos, I. Taboada, I. Torres, J.A. Garc\\'ia-Gonz\\'alez, J.A. Goodman, J.A. Matthews, J. Braun, J.C. Arteaga-Vel\\'azquez, J.C. D\\'iaz-V\\'elez, J. Cotzomi, J.D. Alvarez, J. Mart\\'inez-Castro, J.P. Harding, J. Pretz, J. Wood, K. Engel, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, L. Villase\\~nor, M.A. DuVernois, M. Castillo, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Newbold, M. Rosenberg, M. Schneider, M. Seglar Arroyo, M.U. Nisa, N. Fraija, O. Martinez, O. Tibolla, P. H\\\"untemeyer, P. Miranda-Romagnoli, P. Surajbali, R. Alfaro, R. Arceo, R. Diaz Hernandez, R.J. Lauer, R. L\\'opez-Coto, R. Luna-Garc\\'ia, R. Noriega-Papaqui, R. Pelayo, R.W. Springer, S. Casanova, S. Dichiara, S. Hernandez, S. Kaufmann, S.S. Marinelli, S. Westerhoff, S.Y. BenZvi, T. Capistr\\'an, T. Weisgarber, T. Yapici, U. Cotti, V. Joshi, W.H. Lee, Z. Hampel-Arias, Z. Ren","submitted_at":"2018-05-04T16:43:50Z","abstract_excerpt":"After two years of operation, the High-Altitude Water Cherenkov (HAWC) Observatory has analyzed the TeV cosmic-ray sky over an energy range between $2.0$ and $72.8$ TeV. The HAWC detector is a ground-based air-shower array located at high altitude in the state of Puebla, Mexico. Using 300 light-tight water tanks, it collects the Cherenkov light from the particles of extensive air showers from primary gamma rays and cosmic rays. This detection method allows for uninterrupted observation of the entire overhead sky (2~sr instantaneous, 8.5~sr integrated) in the energy range from a few TeV to hund"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.01847","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"}