{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:FNR6DLTVAJAP2EQ6UE5R35MTZF","short_pith_number":"pith:FNR6DLTV","schema_version":"1.0","canonical_sha256":"2b63e1ae750240fd121ea13b1df593c94b82069ac331dd461e4d435ccaf6a2d2","source":{"kind":"arxiv","id":"2401.07580","version":2},"attestation_state":"computed","paper":{"title":"Upper Limit on the Coronal Cosmic Ray Energy Budget in Seyfert Galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Dmitry Khangulyan, Shinsuke Takasao, Yoshiyuki Inoue","submitted_at":"2024-01-15T10:27:52Z","abstract_excerpt":"The IceCube collaboration has reported possible detections of high-energy neutrinos from nearby Seyfert galaxies. While central hot coronae are proposed as the primary neutrino production site, the exact coronal cosmic-ray energy budget has been loosely constrained. In this study, we propose a new stringent upper bound on the coronal cosmic-ray energy budget of Seyfert galaxies, considering both accretion dynamics and observed properties of radio-quiet Seyfert galaxies. Notably, even under the calorimetric condition where cosmic rays lose all their energies, our limit indicates that the corona"},"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":"2401.07580","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-01-15T10:27:52Z","cross_cats_sorted":[],"title_canon_sha256":"9d9d7cd6bf17e0459e40f33d0db1c8b3dcf3a7e289786103453ff0c1b06bb1e0","abstract_canon_sha256":"b0a8541d22e8632f774bf824f5b72954a05d1b6f10d8c24c8b69b64a92d6b540"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:40:58.484294Z","signature_b64":"apivLwNHjUg1f1NdjtyZp10TkUwdb1HBEWQMhoGP6avaA3osi6aIsx3l6FCu72m8wtbUJU2Hfq7kAkgIMHCYBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b63e1ae750240fd121ea13b1df593c94b82069ac331dd461e4d435ccaf6a2d2","last_reissued_at":"2026-07-05T08:40:58.483776Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:40:58.483776Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Upper Limit on the Coronal Cosmic Ray Energy Budget in Seyfert Galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Dmitry Khangulyan, Shinsuke Takasao, Yoshiyuki Inoue","submitted_at":"2024-01-15T10:27:52Z","abstract_excerpt":"The IceCube collaboration has reported possible detections of high-energy neutrinos from nearby Seyfert galaxies. While central hot coronae are proposed as the primary neutrino production site, the exact coronal cosmic-ray energy budget has been loosely constrained. In this study, we propose a new stringent upper bound on the coronal cosmic-ray energy budget of Seyfert galaxies, considering both accretion dynamics and observed properties of radio-quiet Seyfert galaxies. Notably, even under the calorimetric condition where cosmic rays lose all their energies, our limit indicates that the corona"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2401.07580","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2401.07580/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":"2401.07580","created_at":"2026-07-05T08:40:58.483833+00:00"},{"alias_kind":"arxiv_version","alias_value":"2401.07580v2","created_at":"2026-07-05T08:40:58.483833+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2401.07580","created_at":"2026-07-05T08:40:58.483833+00:00"},{"alias_kind":"pith_short_12","alias_value":"FNR6DLTVAJAP","created_at":"2026-07-05T08:40:58.483833+00:00"},{"alias_kind":"pith_short_16","alias_value":"FNR6DLTVAJAP2EQ6","created_at":"2026-07-05T08:40:58.483833+00:00"},{"alias_kind":"pith_short_8","alias_value":"FNR6DLTV","created_at":"2026-07-05T08:40:58.483833+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/FNR6DLTVAJAP2EQ6UE5R35MTZF","json":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF.json","graph_json":"https://pith.science/api/pith-number/FNR6DLTVAJAP2EQ6UE5R35MTZF/graph.json","events_json":"https://pith.science/api/pith-number/FNR6DLTVAJAP2EQ6UE5R35MTZF/events.json","paper":"https://pith.science/paper/FNR6DLTV"},"agent_actions":{"view_html":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF","download_json":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF.json","view_paper":"https://pith.science/paper/FNR6DLTV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2401.07580&json=true","fetch_graph":"https://pith.science/api/pith-number/FNR6DLTVAJAP2EQ6UE5R35MTZF/graph.json","fetch_events":"https://pith.science/api/pith-number/FNR6DLTVAJAP2EQ6UE5R35MTZF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF/action/storage_attestation","attest_author":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF/action/author_attestation","sign_citation":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF/action/citation_signature","submit_replication":"https://pith.science/pith/FNR6DLTVAJAP2EQ6UE5R35MTZF/action/replication_record"}},"created_at":"2026-07-05T08:40:58.483833+00:00","updated_at":"2026-07-05T08:40:58.483833+00:00"}