{"paper":{"title":"IceCube and HAWC constraints on very-high-energy emission from the Fermi bubbles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ke Fang, Kohta Murase, Meng Su, Tim Linden","submitted_at":"2017-04-12T17:59:59Z","abstract_excerpt":"The nature of the $\\gamma$-ray emission from the \\emph{Fermi} bubbles is unknown. Both hadronic and leptonic models have been formulated to explain the peculiar $\\gamma$-ray signal observed by the Fermi-LAT between 0.1-500~GeV. If this emission continues above $\\sim$30~TeV, hadronic models of the \\emph{Fermi} bubbles would provide a significant contribution to the high-energy neutrino flux detected by the IceCube observatory. Even in models where leptonic $\\gamma$-rays produce the \\emph{Fermi} bubbles flux at GeV energies, a hadronic component may be observable at very high energies. The combi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.03869","kind":"arxiv","version":2},"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"}