{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:HXRHVO32MMSVGW6H5MRWQ6IL65","short_pith_number":"pith:HXRHVO32","schema_version":"1.0","canonical_sha256":"3de27abb7a6325535bc7eb2368790bf764dc50f809915d00978ba8a3e01235e1","source":{"kind":"arxiv","id":"2405.10544","version":2},"attestation_state":"computed","paper":{"title":"The Impact of Positive AGN Feedback on the Properties of Galaxies in a Semi-Analytic Model of Galaxy Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Emanuele Contini, Jinsu Rhee, Seyoung Jeon, Sukyoung K. Yi","submitted_at":"2024-05-17T05:15:12Z","abstract_excerpt":"We introduce the state-of-the-art semi-analytic model {\\small FEGA} (Formation and Evolution of GAlaxies), which incorporates updated prescriptions for key physical processes in galaxy formation. Notably, {\\small FEGA} features an unprecedented semi-analytic modeling of positive Active Galactic Nuclei (AGN) feedback. The model combines the latest prescriptions for gas infall and cooling, a revised star formation recipe that incorporates the extended Kennicutt-Schmidt relation, disk instability, updated supernovae feedback, reincorporation of ejected gas, hot gas stripping from satellite galaxi"},"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":"2405.10544","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-05-17T05:15:12Z","cross_cats_sorted":[],"title_canon_sha256":"4adbac8abdf41cd242df29cd11e474b69b362d2eedd02881575f4fe0ebaf029d","abstract_canon_sha256":"145fc73018153b31c511f52eb94631a40e49ddbb3510716670353ed378184593"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:56:19.794291Z","signature_b64":"tkb4FaQ4XuWiFAP2vs39D8Iqu7iRYT9Q7pbyo6EA34sxyXfFaC+3qaQODERa1EjkINVUe/rSejporGofwcuUDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3de27abb7a6325535bc7eb2368790bf764dc50f809915d00978ba8a3e01235e1","last_reissued_at":"2026-07-05T08:56:19.793891Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:56:19.793891Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Impact of Positive AGN Feedback on the Properties of Galaxies in a Semi-Analytic Model of Galaxy Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Emanuele Contini, Jinsu Rhee, Seyoung Jeon, Sukyoung K. Yi","submitted_at":"2024-05-17T05:15:12Z","abstract_excerpt":"We introduce the state-of-the-art semi-analytic model {\\small FEGA} (Formation and Evolution of GAlaxies), which incorporates updated prescriptions for key physical processes in galaxy formation. Notably, {\\small FEGA} features an unprecedented semi-analytic modeling of positive Active Galactic Nuclei (AGN) feedback. The model combines the latest prescriptions for gas infall and cooling, a revised star formation recipe that incorporates the extended Kennicutt-Schmidt relation, disk instability, updated supernovae feedback, reincorporation of ejected gas, hot gas stripping from satellite galaxi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.10544","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/2405.10544/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":"2405.10544","created_at":"2026-07-05T08:56:19.793947+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.10544v2","created_at":"2026-07-05T08:56:19.793947+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.10544","created_at":"2026-07-05T08:56:19.793947+00:00"},{"alias_kind":"pith_short_12","alias_value":"HXRHVO32MMSV","created_at":"2026-07-05T08:56:19.793947+00:00"},{"alias_kind":"pith_short_16","alias_value":"HXRHVO32MMSVGW6H","created_at":"2026-07-05T08:56:19.793947+00:00"},{"alias_kind":"pith_short_8","alias_value":"HXRHVO32","created_at":"2026-07-05T08:56:19.793947+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/HXRHVO32MMSVGW6H5MRWQ6IL65","json":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65.json","graph_json":"https://pith.science/api/pith-number/HXRHVO32MMSVGW6H5MRWQ6IL65/graph.json","events_json":"https://pith.science/api/pith-number/HXRHVO32MMSVGW6H5MRWQ6IL65/events.json","paper":"https://pith.science/paper/HXRHVO32"},"agent_actions":{"view_html":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65","download_json":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65.json","view_paper":"https://pith.science/paper/HXRHVO32","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.10544&json=true","fetch_graph":"https://pith.science/api/pith-number/HXRHVO32MMSVGW6H5MRWQ6IL65/graph.json","fetch_events":"https://pith.science/api/pith-number/HXRHVO32MMSVGW6H5MRWQ6IL65/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65/action/storage_attestation","attest_author":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65/action/author_attestation","sign_citation":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65/action/citation_signature","submit_replication":"https://pith.science/pith/HXRHVO32MMSVGW6H5MRWQ6IL65/action/replication_record"}},"created_at":"2026-07-05T08:56:19.793947+00:00","updated_at":"2026-07-05T08:56:19.793947+00:00"}