{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:HGNZD4UDK3DYQ3QLEH7AHVEV23","short_pith_number":"pith:HGNZD4UD","schema_version":"1.0","canonical_sha256":"399b91f28356c7886e0b21fe03d495d6f589f67cae21c8a5f2b38cbd35378c62","source":{"kind":"arxiv","id":"2009.08914","version":3},"attestation_state":"computed","paper":{"title":"Directional association of TeV to PeV astrophysical neutrinos with radio blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A.V. Plavin (ASC Lebedev, Mipt), MIPT, Mpifr), S.V. Troitsky (INR), Y.A. Kovalev (ASC Lebedev), Y.Y. Kovalev (ASC Lebedev","submitted_at":"2020-09-18T16:21:10Z","abstract_excerpt":"Recently we have shown that high-energy neutrinos above 200 TeV detected by IceCube are produced within several parsecs in the central regions of radio-bright blazars, that is active galactic nuclei with jets pointing towards us. To independently test this result and extend the analysis to a wider energy range, we use public data for all neutrino energies from seven years of IceCube observations. The IceCube point-source likelihood map is analyzed against the positions of blazars from a statistically complete sample selected by their compact radio flux density. The latter analysis delivers a 3"},"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":"2009.08914","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-09-18T16:21:10Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9c313dafc6ba3275617abdd3e09dc7b38d19007175f1fe5d9786de85dd52d768","abstract_canon_sha256":"8707ed9aa94e9fdebcb314960923eaeb0473a57e8b3965626122b34e4e5177b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:16:37.702652Z","signature_b64":"Aefv6Mp14YjlyQmIvmLBJl3UpHwMR1eK6STkNN32EvLvoqk1YCqfW1UsoX6fV2y4qZN/Osk6waKvW1VMOycAAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"399b91f28356c7886e0b21fe03d495d6f589f67cae21c8a5f2b38cbd35378c62","last_reissued_at":"2026-07-05T02:16:37.702217Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:16:37.702217Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Directional association of TeV to PeV astrophysical neutrinos with radio blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A.V. Plavin (ASC Lebedev, Mipt), MIPT, Mpifr), S.V. Troitsky (INR), Y.A. Kovalev (ASC Lebedev), Y.Y. Kovalev (ASC Lebedev","submitted_at":"2020-09-18T16:21:10Z","abstract_excerpt":"Recently we have shown that high-energy neutrinos above 200 TeV detected by IceCube are produced within several parsecs in the central regions of radio-bright blazars, that is active galactic nuclei with jets pointing towards us. To independently test this result and extend the analysis to a wider energy range, we use public data for all neutrino energies from seven years of IceCube observations. The IceCube point-source likelihood map is analyzed against the positions of blazars from a statistically complete sample selected by their compact radio flux density. The latter analysis delivers a 3"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.08914","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2009.08914/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2009.08914","created_at":"2026-07-05T02:16:37.702277+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.08914v3","created_at":"2026-07-05T02:16:37.702277+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.08914","created_at":"2026-07-05T02:16:37.702277+00:00"},{"alias_kind":"pith_short_12","alias_value":"HGNZD4UDK3DY","created_at":"2026-07-05T02:16:37.702277+00:00"},{"alias_kind":"pith_short_16","alias_value":"HGNZD4UDK3DYQ3QL","created_at":"2026-07-05T02:16:37.702277+00:00"},{"alias_kind":"pith_short_8","alias_value":"HGNZD4UD","created_at":"2026-07-05T02:16:37.702277+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.30764","citing_title":"Active Galactic Nuclei as high-energy neutrino sources","ref_index":151,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23","json":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23.json","graph_json":"https://pith.science/api/pith-number/HGNZD4UDK3DYQ3QLEH7AHVEV23/graph.json","events_json":"https://pith.science/api/pith-number/HGNZD4UDK3DYQ3QLEH7AHVEV23/events.json","paper":"https://pith.science/paper/HGNZD4UD"},"agent_actions":{"view_html":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23","download_json":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23.json","view_paper":"https://pith.science/paper/HGNZD4UD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.08914&json=true","fetch_graph":"https://pith.science/api/pith-number/HGNZD4UDK3DYQ3QLEH7AHVEV23/graph.json","fetch_events":"https://pith.science/api/pith-number/HGNZD4UDK3DYQ3QLEH7AHVEV23/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23/action/storage_attestation","attest_author":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23/action/author_attestation","sign_citation":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23/action/citation_signature","submit_replication":"https://pith.science/pith/HGNZD4UDK3DYQ3QLEH7AHVEV23/action/replication_record"}},"created_at":"2026-07-05T02:16:37.702277+00:00","updated_at":"2026-07-05T02:16:37.702277+00:00"}