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Recently, the IceCube Collaboration reported a ${\\sim}{3}\\sigma$ neutrino signal from the direction of a nearby Seyfert galaxy NGC 4151. However, two gamma-ray loud BL Lac objects, 4FGL 1210.3+3928 and 4FGL J1211.6+3901, lie close to NGC 4151, at angular distances of 0.08$^\\circ$ and 0.43$^\\circ$, respectively. We investigate the potential contribution of these two blazars to the observed neutrino signal from the direction of NGC 415"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2411.09332","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-11-14T10:28:39Z","cross_cats_sorted":[],"title_canon_sha256":"7f0a0aa92aa8f199cf0033af0a93af9cffa7dc8454acf535b28833e6461ef2e3","abstract_canon_sha256":"018e81e43b73a42e8056b4a01681e6ef911268c9c31251f7b9461f5b8a192223"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:21:05.642990Z","signature_b64":"skX7coRySi6eNz4cKv0z60fN1AUlO1hbTp50oxjE0VZzuJAPddJRKks4+8XQB6xlLe0VQElKr/76hBx7GzYfDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b17de7eff683ce5a0187e78ad95dc90e369e8e1edcea5299b5cf20122c09a6b","last_reissued_at":"2026-07-05T10:21:05.642474Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:21:05.642474Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the possible contributions of two nearby blazars to the NGC 4151 neutrino hotspot","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Anastasiia Omeliukh, Samuel Barnier, Yoshiyuki Inoue","submitted_at":"2024-11-14T10:28:39Z","abstract_excerpt":"The origin of the high-energy astrophysical neutrinos discovered by IceCube remains unclear, with both blazars and Seyfert galaxies emerging as potential sources. 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