{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:2PBXZRKNKMPS3GLWCSZLYESTS7","short_pith_number":"pith:2PBXZRKN","schema_version":"1.0","canonical_sha256":"d3c37cc54d531f2d997614b2bc125397d8bcba881cd0886f2b275d6ed6933993","source":{"kind":"arxiv","id":"2502.00504","version":1},"attestation_state":"computed","paper":{"title":"A New Interpretation for the Hot Corona in Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jian-Min Wang, Yan-Rong Li, Yu Zhao","submitted_at":"2025-02-01T17:52:05Z","abstract_excerpt":"This work attempts to provide a new interpretation for the hot corona in active galactic nuclei (AGNs). A thin\n  parabolic magnetic reconnection layer, anchored at the innermost disk and extending along the boundary of the\n  magnetic tower for a few tens of gravitational radii, serves as a hard-X-ray source above the disk. Within this\n  reconnection layer, the tearing instability leads to the formation of a chain of plasmoids, which contain relativistic\n  electrons that generate X-ray radiation through inverse-Compton (IC) scattering of soft photons emitted by the\n  accretion disk. Based on pr"},"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":"2502.00504","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-02-01T17:52:05Z","cross_cats_sorted":[],"title_canon_sha256":"a1d91087bc607b9f257ae0f1972cd8a79f741ea5c4d623bbe1008eabfc8b6329","abstract_canon_sha256":"6bf387ccd7d9d31d612896f1d93c5154ae1a7e7ecfbc4196a151a90df0cdb7f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:08:34.610961Z","signature_b64":"RbuXhe9F+fGUuuUIObKzxBltlJP5rO7toKtF8F57NOHimp+KVvudokB7HkNmGOa4ADIy8oU7w7NGal4yQ6QgBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3c37cc54d531f2d997614b2bc125397d8bcba881cd0886f2b275d6ed6933993","last_reissued_at":"2026-07-05T10:08:34.610506Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:08:34.610506Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A New Interpretation for the Hot Corona in Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jian-Min Wang, Yan-Rong Li, Yu Zhao","submitted_at":"2025-02-01T17:52:05Z","abstract_excerpt":"This work attempts to provide a new interpretation for the hot corona in active galactic nuclei (AGNs). A thin\n  parabolic magnetic reconnection layer, anchored at the innermost disk and extending along the boundary of the\n  magnetic tower for a few tens of gravitational radii, serves as a hard-X-ray source above the disk. Within this\n  reconnection layer, the tearing instability leads to the formation of a chain of plasmoids, which contain relativistic\n  electrons that generate X-ray radiation through inverse-Compton (IC) scattering of soft photons emitted by the\n  accretion disk. Based on pr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.00504","kind":"arxiv","version":1},"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/2502.00504/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":"2502.00504","created_at":"2026-07-05T10:08:34.610560+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.00504v1","created_at":"2026-07-05T10:08:34.610560+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.00504","created_at":"2026-07-05T10:08:34.610560+00:00"},{"alias_kind":"pith_short_12","alias_value":"2PBXZRKNKMPS","created_at":"2026-07-05T10:08:34.610560+00:00"},{"alias_kind":"pith_short_16","alias_value":"2PBXZRKNKMPS3GLW","created_at":"2026-07-05T10:08:34.610560+00:00"},{"alias_kind":"pith_short_8","alias_value":"2PBXZRKN","created_at":"2026-07-05T10:08:34.610560+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/2PBXZRKNKMPS3GLWCSZLYESTS7","json":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7.json","graph_json":"https://pith.science/api/pith-number/2PBXZRKNKMPS3GLWCSZLYESTS7/graph.json","events_json":"https://pith.science/api/pith-number/2PBXZRKNKMPS3GLWCSZLYESTS7/events.json","paper":"https://pith.science/paper/2PBXZRKN"},"agent_actions":{"view_html":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7","download_json":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7.json","view_paper":"https://pith.science/paper/2PBXZRKN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.00504&json=true","fetch_graph":"https://pith.science/api/pith-number/2PBXZRKNKMPS3GLWCSZLYESTS7/graph.json","fetch_events":"https://pith.science/api/pith-number/2PBXZRKNKMPS3GLWCSZLYESTS7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7/action/storage_attestation","attest_author":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7/action/author_attestation","sign_citation":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7/action/citation_signature","submit_replication":"https://pith.science/pith/2PBXZRKNKMPS3GLWCSZLYESTS7/action/replication_record"}},"created_at":"2026-07-05T10:08:34.610560+00:00","updated_at":"2026-07-05T10:08:34.610560+00:00"}