{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:NLIXWET23SZ4YJJRGPORPUQFWD","short_pith_number":"pith:NLIXWET2","schema_version":"1.0","canonical_sha256":"6ad17b127adcb3cc253133dd17d205b0d0f60d415e48781492710c9a922da553","source":{"kind":"arxiv","id":"2006.05997","version":2},"attestation_state":"computed","paper":{"title":"Powering galactic super-winds with small-scale AGN winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Garching), R\\\"udiger Pakmor, Tiago Costa, Volker Springel (MPA","submitted_at":"2020-06-10T18:00:01Z","abstract_excerpt":"We present a new implementation for active galactic nucleus (AGN) feedback through small-scale, ultra-fast winds in the moving-mesh hydrodynamic code AREPO. The wind is injected by prescribing mass, momentum and energy fluxes across a spherical boundary centred on a supermassive black hole according to available constraints for accretion disc winds. After sweeping-up a mass equal to their own, small-scale winds thermalise, powering energy-driven outflows with dynamics, structure and cooling properties in excellent agreement with those of analytic wind solutions. Momentum-driven solutions do no"},"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":"2006.05997","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-06-10T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"8cda937888ed5419e82cd76da9788c254ab4bd0be49836eb404f7c650fcc806f","abstract_canon_sha256":"aaac30be154fbdde221d397955b972eebeb6189f365635080e3c7aa85c5c08b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:28:12.008220Z","signature_b64":"CH264eseTK00QAzMtds4aXuDBonxlHlGEs1VZSJZon+M3JO6xQ/2u15wOV4Exk22KmBFdxJsUrPjf3CSj8ylAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ad17b127adcb3cc253133dd17d205b0d0f60d415e48781492710c9a922da553","last_reissued_at":"2026-07-05T01:28:12.007752Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:28:12.007752Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Powering galactic super-winds with small-scale AGN winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Garching), R\\\"udiger Pakmor, Tiago Costa, Volker Springel (MPA","submitted_at":"2020-06-10T18:00:01Z","abstract_excerpt":"We present a new implementation for active galactic nucleus (AGN) feedback through small-scale, ultra-fast winds in the moving-mesh hydrodynamic code AREPO. The wind is injected by prescribing mass, momentum and energy fluxes across a spherical boundary centred on a supermassive black hole according to available constraints for accretion disc winds. After sweeping-up a mass equal to their own, small-scale winds thermalise, powering energy-driven outflows with dynamics, structure and cooling properties in excellent agreement with those of analytic wind solutions. Momentum-driven solutions do no"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.05997","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/2006.05997/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":"2006.05997","created_at":"2026-07-05T01:28:12.007809+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.05997v2","created_at":"2026-07-05T01:28:12.007809+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.05997","created_at":"2026-07-05T01:28:12.007809+00:00"},{"alias_kind":"pith_short_12","alias_value":"NLIXWET23SZ4","created_at":"2026-07-05T01:28:12.007809+00:00"},{"alias_kind":"pith_short_16","alias_value":"NLIXWET23SZ4YJJR","created_at":"2026-07-05T01:28:12.007809+00:00"},{"alias_kind":"pith_short_8","alias_value":"NLIXWET2","created_at":"2026-07-05T01:28:12.007809+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/NLIXWET23SZ4YJJRGPORPUQFWD","json":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD.json","graph_json":"https://pith.science/api/pith-number/NLIXWET23SZ4YJJRGPORPUQFWD/graph.json","events_json":"https://pith.science/api/pith-number/NLIXWET23SZ4YJJRGPORPUQFWD/events.json","paper":"https://pith.science/paper/NLIXWET2"},"agent_actions":{"view_html":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD","download_json":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD.json","view_paper":"https://pith.science/paper/NLIXWET2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.05997&json=true","fetch_graph":"https://pith.science/api/pith-number/NLIXWET23SZ4YJJRGPORPUQFWD/graph.json","fetch_events":"https://pith.science/api/pith-number/NLIXWET23SZ4YJJRGPORPUQFWD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD/action/storage_attestation","attest_author":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD/action/author_attestation","sign_citation":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD/action/citation_signature","submit_replication":"https://pith.science/pith/NLIXWET23SZ4YJJRGPORPUQFWD/action/replication_record"}},"created_at":"2026-07-05T01:28:12.007809+00:00","updated_at":"2026-07-05T01:28:12.007809+00:00"}