{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:ELWCV56TC7V3N4LXAWATXHOTYG","short_pith_number":"pith:ELWCV56T","schema_version":"1.0","canonical_sha256":"22ec2af7d317ebb6f17705813b9dd3c1b64e0d81ceec8b6ec0fb52016dad1f68","source":{"kind":"arxiv","id":"1405.6986","version":1},"attestation_state":"computed","paper":{"title":"Low-Mass AGN and Their Relation to the Fundamental Plane of Black Hole Accretion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ashley L. King, Edward M. Cackett, Jason Pinkney, Jon M. Miller, Kayhan Gultekin","submitted_at":"2014-05-27T17:41:54Z","abstract_excerpt":"We put active galactic nuclei (AGNs) with low-mass black holes on the fundamental plane of black hole accretion---the plane that relates X-ray emission, radio emission, and mass of an accreting black hole---to test whether or not the relation is universal for both stellar-mass and supermassive black holes. We use new Chandra X-ray and Very Large Array radio observations of a sample of black holes with masses less than $10^{6.3}\\ M_{\\scriptscriptstyle \\odot}$, which have the best leverage for determining whether supermassive black holes and stellar-mass black holes belong on the same plane. Our"},"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":"1405.6986","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-27T17:41:54Z","cross_cats_sorted":[],"title_canon_sha256":"4e885a2f19ab61d805c27ff0f7d7757eff944fa5ba1ebba411e12e004252a1d9","abstract_canon_sha256":"a0d8ef22abf38849788a096187a4bc673a1ca026fa7edf14c846123b67e17954"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:36.051344Z","signature_b64":"BuyeWBonFFZvKrxbwhfMkr7XDFxBstQoYKGy2gQiX6Wfj4jRSFJu//w+WXVfVMtvjwinrRim0eP7mcLfBuYvDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"22ec2af7d317ebb6f17705813b9dd3c1b64e0d81ceec8b6ec0fb52016dad1f68","last_reissued_at":"2026-05-18T01:36:36.050586Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:36.050586Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Low-Mass AGN and Their Relation to the Fundamental Plane of Black Hole Accretion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ashley L. King, Edward M. Cackett, Jason Pinkney, Jon M. Miller, Kayhan Gultekin","submitted_at":"2014-05-27T17:41:54Z","abstract_excerpt":"We put active galactic nuclei (AGNs) with low-mass black holes on the fundamental plane of black hole accretion---the plane that relates X-ray emission, radio emission, and mass of an accreting black hole---to test whether or not the relation is universal for both stellar-mass and supermassive black holes. We use new Chandra X-ray and Very Large Array radio observations of a sample of black holes with masses less than $10^{6.3}\\ M_{\\scriptscriptstyle \\odot}$, which have the best leverage for determining whether supermassive black holes and stellar-mass black holes belong on the same plane. Our"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.6986","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":"1405.6986","created_at":"2026-05-18T01:36:36.050718+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.6986v1","created_at":"2026-05-18T01:36:36.050718+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.6986","created_at":"2026-05-18T01:36:36.050718+00:00"},{"alias_kind":"pith_short_12","alias_value":"ELWCV56TC7V3","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"ELWCV56TC7V3N4LX","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"ELWCV56T","created_at":"2026-05-18T12:28:28.263976+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/ELWCV56TC7V3N4LXAWATXHOTYG","json":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG.json","graph_json":"https://pith.science/api/pith-number/ELWCV56TC7V3N4LXAWATXHOTYG/graph.json","events_json":"https://pith.science/api/pith-number/ELWCV56TC7V3N4LXAWATXHOTYG/events.json","paper":"https://pith.science/paper/ELWCV56T"},"agent_actions":{"view_html":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG","download_json":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG.json","view_paper":"https://pith.science/paper/ELWCV56T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.6986&json=true","fetch_graph":"https://pith.science/api/pith-number/ELWCV56TC7V3N4LXAWATXHOTYG/graph.json","fetch_events":"https://pith.science/api/pith-number/ELWCV56TC7V3N4LXAWATXHOTYG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG/action/storage_attestation","attest_author":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG/action/author_attestation","sign_citation":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG/action/citation_signature","submit_replication":"https://pith.science/pith/ELWCV56TC7V3N4LXAWATXHOTYG/action/replication_record"}},"created_at":"2026-05-18T01:36:36.050718+00:00","updated_at":"2026-05-18T01:36:36.050718+00:00"}