{"paper":{"title":"Searching for Dark Matter Sub-structure with HAWC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Carrami\\~nana, A. Galv\\'an-G\\'amez, A. Iriarte, 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. Brisbois, C. de Le\\'on, C.D. Rho, C. Espinoza, C. Rivi\\`ere, D. Avila Rojas, D. Rosa-Gonz\\'alez, E. Belmont-Moreno, E. De la Fuente, E.G. P\\'erez-P\\'erez, E. Moreno, F. Hueyotl-Zahuantitla, F. Salesa Greus, G. Luis-Raya, G. Sinnis, G. Vianello, H.A. Ayala Solares, H. Fleischhack, H. Le\\'on Vargas, H. Salazar, H. Zhou, I. Martinez-Castellanos, I. Torres, J.A. Garc\\'ia-Gonz\\'alez, J.A. Goodman, J.A. Matthews, J.C. Arteaga-Vel\\'azquez, J.C. D\\'iaz-V\\'elez, J. Cotzomi, J.D. \\'Alvarez, J. Lundeen, J. Mart\\'inez-Castro, J.P. Harding, J.T. Linnemann, J. Wood, K. Engel, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, M.A. DuVernois, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Newbold, M. Rosenberg, M. Schneider, M.U. Nisa, N. Fraija, O. Martinez, P. H\\\"untemeyer, P. Miranda-Romagnoli, R. Alfaro, R. Arceo, R. Noriega-Papaqui, R.W. Springer, S. Casanova, S. Couti\\~no de Le\\'on, S. Dichiara, S.S. Marinelli, S.Y. BenZvi, T. Weisgarber, T. Yapici, W.H. Lee, Z. Ren","submitted_at":"2018-11-28T18:33:56Z","abstract_excerpt":"Simulations of dark matter show a discrepancy between the expected number of Galactic dark matter sub-halos and how many have been optically observed. Some of these unseen satellites may exist as dark dwarf galaxies: sub-halos like dwarf galaxies with no luminous counterpart. Assuming WIMP dark matter, it may be possible to detect these unseen sub-halos from gamma-ray signals originating from dark matter annihilation. The High Altitude Water Cherenkov Observatory (HAWC) is a very high energy (500 GeV to 100 TeV) gamma ray detector with a wide field-of-view and near continuous duty cycle, makin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.11732","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"}