{"paper":{"title":"Search for very-high-energy emission from Gamma-ray Bursts using the first 18 months of data from the HAWC Gamma-ray Observatory","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. Hernandez-Almada, A. Iriarte, A. Jardin-Blicq, A.J. Smith, A.L. Longinotti, A. Sandoval, A.S. Barber, A. Zepeda, B. Hona, B.L. Dingus, C. Alvarez, C. Brisbois, C. de Le\\'on, C.D. Rho, C.M. Hui, C. Rivi\\`ere, D. Avila Rojas, D. Kieda, D. Lennarz, 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. Salesa Greus, G. Luis Raya, G. Sinnis, G. Vianello, H.A. Ayala Solares, H. Le\\'on Vargas, H. Mart\\'inez-Huerta, H. Salazar, 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.T. Linnemann, J. Wood, K. Engel, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, M.A. DuVernois, M. Castillo, M. Gerhardt, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Newbold, M. Rosenberg, M. Schneider, N. Bautista-Elivar, N. Fraija, O. Martinez, O. Tibolla, P. H\\\"untemeyer, P. Miranda-Romagnoli, P. Surajbali, P.W. Younk, R. Arceo, R. Diaz Hernandez, R.J. Lauer, R. Luna-Garc\\'ia, R. Noriega-Papaqui, R. Pelayo, R.W. Ellsworth, R.W. Springer, S. Casanova, S. Couti\\~no de Le\\'on, S. Hernandez, S. Kaufmann, S.S. Marinelli, S. Westerhoff, S.Y. BenZvi, T. Capistr\\'an, T. DeYoung, The HAWC collaboration: R. Alfaro, T.N. Ukwatta, T. Weisgarber, T. Yapici, U. Cotti, V. Joshi, W. H. Lee, Z. Hampel-Arias, Z. Ren","submitted_at":"2017-05-03T18:00:03Z","abstract_excerpt":"The High Altitude Water Cherenkov (HAWC) Gamma-ray Observatory is an extensive air shower detector operating in central Mexico, which has recently completed its first two years of full operations. If for a burst like GRB 130427A at a redshift of 0.34 and a high-energy component following a power law with index -1.66, the high-energy component is extended to higher energies with no cut-off other than from extragalactic background light attenuation, HAWC would observe gamma rays with a peak energy of $\\sim$300 GeV. This paper reports the results of HAWC observations of 64 gamma-ray bursts (GRBs)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.01551","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"}