{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:H6GEMAHDNEO7ZRGKEPUHE7YQJR","short_pith_number":"pith:H6GEMAHD","schema_version":"1.0","canonical_sha256":"3f8c4600e3691dfcc4ca23e8727f104c6064a86ed24e658a7ba314b792f91bcb","source":{"kind":"arxiv","id":"1503.05206","version":1},"attestation_state":"computed","paper":{"title":"Powerful Outflows and Feedback from Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Andrew King, Ken Pounds","submitted_at":"2015-03-17T20:04:52Z","abstract_excerpt":"Active Galactic Nuclei (AGN) represent the growth phases of the supermassive black holes in the center of almost every galaxy. Powerful, highly ionized winds, with velocities $\\sim 0.1- 0.2c$ are a common feature in X--ray spectra of luminous AGN, offering a plausible physical origin for the well known connections between the hole and properties of its host. Observability constraints suggest that the winds must be episodic, and detectable only for a few percent of their lifetimes. The most powerful wind feedback, establishing the $M -\\sigma$ relation, is probably not directly observable at all"},"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":"1503.05206","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-03-17T20:04:52Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"00b9a9b1f28b0fac837be66f7ee03b152a28b27ed3c12f5017b0de3a997a9319","abstract_canon_sha256":"c51fe50a4904d54973095baa99682a4062de0b07325bfbf965414b42b782908a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:32:30.023745Z","signature_b64":"Pb8FyUUknMxF1wFx2o+9xQ793pC/4quWK5ZPsyfIWe9LzD7fLKltOcMRzHMdlbGYb4fQK95huZx6kl8RwBIBAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3f8c4600e3691dfcc4ca23e8727f104c6064a86ed24e658a7ba314b792f91bcb","last_reissued_at":"2026-05-18T01:32:30.023287Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:32:30.023287Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Powerful Outflows and Feedback from Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Andrew King, Ken Pounds","submitted_at":"2015-03-17T20:04:52Z","abstract_excerpt":"Active Galactic Nuclei (AGN) represent the growth phases of the supermassive black holes in the center of almost every galaxy. Powerful, highly ionized winds, with velocities $\\sim 0.1- 0.2c$ are a common feature in X--ray spectra of luminous AGN, offering a plausible physical origin for the well known connections between the hole and properties of its host. Observability constraints suggest that the winds must be episodic, and detectable only for a few percent of their lifetimes. The most powerful wind feedback, establishing the $M -\\sigma$ relation, is probably not directly observable at all"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.05206","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":"1503.05206","created_at":"2026-05-18T01:32:30.023369+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.05206v1","created_at":"2026-05-18T01:32:30.023369+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.05206","created_at":"2026-05-18T01:32:30.023369+00:00"},{"alias_kind":"pith_short_12","alias_value":"H6GEMAHDNEO7","created_at":"2026-05-18T12:29:22.688609+00:00"},{"alias_kind":"pith_short_16","alias_value":"H6GEMAHDNEO7ZRGK","created_at":"2026-05-18T12:29:22.688609+00:00"},{"alias_kind":"pith_short_8","alias_value":"H6GEMAHD","created_at":"2026-05-18T12:29:22.688609+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":16,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22918","citing_title":"Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds","ref_index":119,"is_internal_anchor":true},{"citing_arxiv_id":"1907.05323","citing_title":"Extragalactic astrophysics with next-generation CMB experiments","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2510.08997","citing_title":"Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"1902.05554","citing_title":"First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback","ref_index":270,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02663","citing_title":"Jet-driven shocks and turbulence in radio-loud Active Galactic Nuclei observed with JWST MIRI/MRS","ref_index":148,"is_internal_anchor":false},{"citing_arxiv_id":"2605.10557","citing_title":"Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2605.10024","citing_title":"Hydrodynamical simulation of wind production from hot accretion flows in tidal disruption events","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18522","citing_title":"A Census of Na D-traced neutral ISM and outflows at $0.6