{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:JGERARTQ7SSADR7RC6NQDCW6YU","short_pith_number":"pith:JGERARTQ","schema_version":"1.0","canonical_sha256":"4989104670fca401c7f1179b018adec51f28b1ec53554d554e9f9208032d294d","source":{"kind":"arxiv","id":"2402.17991","version":2},"attestation_state":"computed","paper":{"title":"The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 1 < z < 4","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(2) Peking University, (3) Waseda University), Bin Luo (1) ((1) Nanjing University, Luis C. Ho (2), Tao Wang (1), Yijun Wang (1), Yuxing Zhong (3)","submitted_at":"2024-02-28T02:15:52Z","abstract_excerpt":"The fundamental plane of black hole activity (BHFP) describes the correlation between radio luminosity ($L_R$), X-ray luminosity ($L_X$), and black hole mass. It reflects a disc-jet connection. However, dependence of BHFP on various physical properties of active galactic nuclei (AGNs) and host galaxies is unclear, especially for low-luminosity AGNs, which is important for understanding accretion physics in AGNs. Here we explore the dependence of BHFP on radio loudness, Eddington ratio ($\\lambda_E$), redshift, and galaxy star formation properties at 0.1 < z < 4 for radio AGNs. Based on current "},"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":"2402.17991","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-02-28T02:15:52Z","cross_cats_sorted":[],"title_canon_sha256":"c73c6db0c4db86bf8601aca6b51cb8cd88803da183155d38dff3e47190c5ed21","abstract_canon_sha256":"8690ada528f9fca877838e033c8069d170692c0a107e790f915567a8dcef357d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:11:13.319699Z","signature_b64":"dawqC7DHu/sXCfciF7j4tPcx72M7lOIYp8iZLeThEdQA05D1tkvtz4oCb8MArhKtm7j/wCKW85shWPKFBj0PAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4989104670fca401c7f1179b018adec51f28b1ec53554d554e9f9208032d294d","last_reissued_at":"2026-07-05T09:11:13.319167Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:11:13.319167Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 1 < z < 4","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(2) Peking University, (3) Waseda University), Bin Luo (1) ((1) Nanjing University, Luis C. Ho (2), Tao Wang (1), Yijun Wang (1), Yuxing Zhong (3)","submitted_at":"2024-02-28T02:15:52Z","abstract_excerpt":"The fundamental plane of black hole activity (BHFP) describes the correlation between radio luminosity ($L_R$), X-ray luminosity ($L_X$), and black hole mass. It reflects a disc-jet connection. However, dependence of BHFP on various physical properties of active galactic nuclei (AGNs) and host galaxies is unclear, especially for low-luminosity AGNs, which is important for understanding accretion physics in AGNs. Here we explore the dependence of BHFP on radio loudness, Eddington ratio ($\\lambda_E$), redshift, and galaxy star formation properties at 0.1 < z < 4 for radio AGNs. Based on current "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.17991","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/2402.17991/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":"2402.17991","created_at":"2026-07-05T09:11:13.319237+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.17991v2","created_at":"2026-07-05T09:11:13.319237+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.17991","created_at":"2026-07-05T09:11:13.319237+00:00"},{"alias_kind":"pith_short_12","alias_value":"JGERARTQ7SSA","created_at":"2026-07-05T09:11:13.319237+00:00"},{"alias_kind":"pith_short_16","alias_value":"JGERARTQ7SSADR7R","created_at":"2026-07-05T09:11:13.319237+00:00"},{"alias_kind":"pith_short_8","alias_value":"JGERARTQ","created_at":"2026-07-05T09:11:13.319237+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05523","citing_title":"BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\\simeq5.23$","ref_index":279,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU","json":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU.json","graph_json":"https://pith.science/api/pith-number/JGERARTQ7SSADR7RC6NQDCW6YU/graph.json","events_json":"https://pith.science/api/pith-number/JGERARTQ7SSADR7RC6NQDCW6YU/events.json","paper":"https://pith.science/paper/JGERARTQ"},"agent_actions":{"view_html":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU","download_json":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU.json","view_paper":"https://pith.science/paper/JGERARTQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.17991&json=true","fetch_graph":"https://pith.science/api/pith-number/JGERARTQ7SSADR7RC6NQDCW6YU/graph.json","fetch_events":"https://pith.science/api/pith-number/JGERARTQ7SSADR7RC6NQDCW6YU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU/action/storage_attestation","attest_author":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU/action/author_attestation","sign_citation":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU/action/citation_signature","submit_replication":"https://pith.science/pith/JGERARTQ7SSADR7RC6NQDCW6YU/action/replication_record"}},"created_at":"2026-07-05T09:11:13.319237+00:00","updated_at":"2026-07-05T09:11:13.319237+00:00"}