{"paper":{"title":"The 2HWC HAWC Observatory Gamma Ray Catalog","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Becerril, A. Bernal, A. Carrami\\~nana, A. Gonz\\'alez Mu\\~noz, A. Hernandez-Almada, A. Iriarte, A. Jardin-Blicq, A.J. Smith, A. Lara, A.L. Longinotti, A. Sandoval, A.S. Barber, A.U. Abeysekara, A. Zepeda, B.L. Dingus, C. Alvarez, C. Brisbois, C. de Le\\'on, C.D. Rho, C.M. Hui, C. Rivi\\`ere, D. Berley, 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.G. Wisher, I. Martinez-Castellanos, I. Taboada, I. Torres, J.A. Garc\\'ia-Gonz\\'alez, J.A. Goodman, J.A. Matthews, J. Becerra Gonzalez, J. Braun, 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. Pretz, J.T. Linnemann, J. Wood, K. Engel, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, L. Villase\\~nor, M.A. DuVernois, M. Castillo, M. Gerhardt, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Newbold, M. Rosenberg, M. Schneider, M.U. Nisa, N. Bautista-Elivar, N. Fraija, O. Martinez, O. Tibolla, P. H\\\"untemeyer, P. Miranda-Romagnoli, P. Surajbali, P.W. Younk, 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. 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.N. Ukwatta, T. Weisgarber, T. Yapici, U. Cotti, V. Joshi, W.H. Lee, Z. Hampel-Arias, Z. Ren","submitted_at":"2017-02-09T21:37:39Z","abstract_excerpt":"We present the first catalog of TeV gamma-ray sources realized with the recently completed High Altitude Water Cherenkov Observatory (HAWC). It is the most sensitive wide field-of-view TeV telescope currently in operation, with a 1-year survey sensitivity of ~5-10% of the flux of the Crab Nebula. With an instantaneous field of view >1.5 sr and >90% duty cycle, it continuously surveys and monitors the sky for gamma ray energies between hundreds GeV and tens of TeV.\n  HAWC is located in Mexico at a latitude of 19 degree North and was completed in March 2015. Here, we present the 2HWC catalog, wh"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.02992","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":""},"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"}