{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:LLYC2K2PSIRCO6BTYVMXDE6Q3W","short_pith_number":"pith:LLYC2K2P","schema_version":"1.0","canonical_sha256":"5af02d2b4f9222277833c5597193d0dd9debf1e71d39897cd9c193af079e9f25","source":{"kind":"arxiv","id":"1411.5273","version":2},"attestation_state":"computed","paper":{"title":"A Monte Carlo Bayesian Search for the Plausible Source of the Telescope Array Hotspot","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alexander Kusenko, Bin-Bin Zhang, Hao-Ning He, Rui-zhi Yang, Shigehiro Nagataki, Yi-Zhong Fan","submitted_at":"2014-11-19T16:10:10Z","abstract_excerpt":"The Telescope Array (TA) collaboration has reported a hotspot of 19 ultrahigh-energy cosmic rays (UHECRs). Using a universal model with one source and energy-dependent magnetic deflections, we show that the distribution of the TA hotspot events is consistent with a single source hypothesis, although multiple sources cannot be ruled out. The chance probability of this distribution arising from a homogeneous distribution is $0.2\\%$. We describe a Monte Carlo Bayesian (MCB) inference approach, which can be used to derive parameters of the magnetic fields as well as the source coordinates, and we "},"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":"1411.5273","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-19T16:10:10Z","cross_cats_sorted":[],"title_canon_sha256":"955e324164afc808c9fea3c7db37cf62676fd2708b9a405df1cc4b98b8112074","abstract_canon_sha256":"b8fb5327f8f19b98dbbf028eb2601f724800ae88244ec89267b59358797d1a7c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:12.143509Z","signature_b64":"RsKz9PiLVahBe5QfpTzvtbSNguYz5U3j1r2f/rlc/revkTWtk3nCGYuv7LB8mFhLsowdcCcMqIwoOlmHns5jBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5af02d2b4f9222277833c5597193d0dd9debf1e71d39897cd9c193af079e9f25","last_reissued_at":"2026-05-18T01:20:12.142973Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:12.142973Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Monte Carlo Bayesian Search for the Plausible Source of the Telescope Array Hotspot","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alexander Kusenko, Bin-Bin Zhang, Hao-Ning He, Rui-zhi Yang, Shigehiro Nagataki, Yi-Zhong Fan","submitted_at":"2014-11-19T16:10:10Z","abstract_excerpt":"The Telescope Array (TA) collaboration has reported a hotspot of 19 ultrahigh-energy cosmic rays (UHECRs). Using a universal model with one source and energy-dependent magnetic deflections, we show that the distribution of the TA hotspot events is consistent with a single source hypothesis, although multiple sources cannot be ruled out. The chance probability of this distribution arising from a homogeneous distribution is $0.2\\%$. We describe a Monte Carlo Bayesian (MCB) inference approach, which can be used to derive parameters of the magnetic fields as well as the source coordinates, and we "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.5273","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1411.5273","created_at":"2026-05-18T01:20:12.143047+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.5273v2","created_at":"2026-05-18T01:20:12.143047+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.5273","created_at":"2026-05-18T01:20:12.143047+00:00"},{"alias_kind":"pith_short_12","alias_value":"LLYC2K2PSIRC","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_16","alias_value":"LLYC2K2PSIRCO6BT","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_8","alias_value":"LLYC2K2P","created_at":"2026-05-18T12:28:38.356838+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W","json":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W.json","graph_json":"https://pith.science/api/pith-number/LLYC2K2PSIRCO6BTYVMXDE6Q3W/graph.json","events_json":"https://pith.science/api/pith-number/LLYC2K2PSIRCO6BTYVMXDE6Q3W/events.json","paper":"https://pith.science/paper/LLYC2K2P"},"agent_actions":{"view_html":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W","download_json":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W.json","view_paper":"https://pith.science/paper/LLYC2K2P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.5273&json=true","fetch_graph":"https://pith.science/api/pith-number/LLYC2K2PSIRCO6BTYVMXDE6Q3W/graph.json","fetch_events":"https://pith.science/api/pith-number/LLYC2K2PSIRCO6BTYVMXDE6Q3W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W/action/storage_attestation","attest_author":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W/action/author_attestation","sign_citation":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W/action/citation_signature","submit_replication":"https://pith.science/pith/LLYC2K2PSIRCO6BTYVMXDE6Q3W/action/replication_record"}},"created_at":"2026-05-18T01:20:12.143047+00:00","updated_at":"2026-05-18T01:20:12.143047+00:00"}