{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:LYJV6IOTZ2ERD3ZKQ2UMTX4J27","short_pith_number":"pith:LYJV6IOT","schema_version":"1.0","canonical_sha256":"5e135f21d3ce8911ef2a86a8c9df89d7c9226102896e8adcf43df3accee181b2","source":{"kind":"arxiv","id":"astro-ph/0612212","version":1},"attestation_state":"computed","paper":{"title":"Relativistic effects on the observed AGN luminosity distribution","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Shuang Nan Zhang, Xiao Ling Zhang, Yuan Liu","submitted_at":"2006-12-08T12:14:10Z","abstract_excerpt":"Recently Zhang (2005) has proposed a model to account for the well established effect that the fraction of type-II AGNs is anti-correlated with the observed X-ray luminosity; the model consists of an X-ray emitting accretion disk coaligned to the dusty torus within the standard AGN unification model. In this paper the model is refined by including relativistic effects of the observed X-ray radiations from the vicinity of the supermassive black hole in an AGN. The relativistic corrections improve the combined fitting results of the observed luminosity distribution and the type-II AGN fraction, "},"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":"astro-ph/0612212","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-08T12:14:10Z","cross_cats_sorted":[],"title_canon_sha256":"5c25545be899b03967816cc599418486c73a6b7ca49fff73689e3f55133d115d","abstract_canon_sha256":"576e2a297799d56b0d40112fb2a598a960250374c345f91f55e7be5d13e4ce0e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:28.549265Z","signature_b64":"5bp9HYWfGteu+jDh8EmOX2YNPhrk/MfVwalKBDU6JPP7dzR/8KKPX6PN1uCKJ4goNJrGk4q9yBTnC6b0OXMEBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5e135f21d3ce8911ef2a86a8c9df89d7c9226102896e8adcf43df3accee181b2","last_reissued_at":"2026-05-18T01:40:28.548778Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:28.548778Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relativistic effects on the observed AGN luminosity distribution","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Shuang Nan Zhang, Xiao Ling Zhang, Yuan Liu","submitted_at":"2006-12-08T12:14:10Z","abstract_excerpt":"Recently Zhang (2005) has proposed a model to account for the well established effect that the fraction of type-II AGNs is anti-correlated with the observed X-ray luminosity; the model consists of an X-ray emitting accretion disk coaligned to the dusty torus within the standard AGN unification model. In this paper the model is refined by including relativistic effects of the observed X-ray radiations from the vicinity of the supermassive black hole in an AGN. The relativistic corrections improve the combined fitting results of the observed luminosity distribution and the type-II AGN fraction, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612212","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":""},"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":"astro-ph/0612212","created_at":"2026-05-18T01:40:28.548842+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612212v1","created_at":"2026-05-18T01:40:28.548842+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612212","created_at":"2026-05-18T01:40:28.548842+00:00"},{"alias_kind":"pith_short_12","alias_value":"LYJV6IOTZ2ER","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"LYJV6IOTZ2ERD3ZK","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"LYJV6IOT","created_at":"2026-05-18T12:25:54.717736+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/LYJV6IOTZ2ERD3ZKQ2UMTX4J27","json":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27.json","graph_json":"https://pith.science/api/pith-number/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/graph.json","events_json":"https://pith.science/api/pith-number/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/events.json","paper":"https://pith.science/paper/LYJV6IOT"},"agent_actions":{"view_html":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27","download_json":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27.json","view_paper":"https://pith.science/paper/LYJV6IOT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0612212&json=true","fetch_graph":"https://pith.science/api/pith-number/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/graph.json","fetch_events":"https://pith.science/api/pith-number/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/action/storage_attestation","attest_author":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/action/author_attestation","sign_citation":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/action/citation_signature","submit_replication":"https://pith.science/pith/LYJV6IOTZ2ERD3ZKQ2UMTX4J27/action/replication_record"}},"created_at":"2026-05-18T01:40:28.548842+00:00","updated_at":"2026-05-18T01:40:28.548842+00:00"}