{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:4ZTFOGYAAJ2SUTKPOWIKFUVCWG","short_pith_number":"pith:4ZTFOGYA","schema_version":"1.0","canonical_sha256":"e666571b0002752a4d4f7590a2d2a2b18d6417d80a317a06a3b45d4969bce958","source":{"kind":"arxiv","id":"1608.04762","version":3},"attestation_state":"computed","paper":{"title":"Feedback-regulated star formation and escape of LyC photons from mini-haloes during reionisation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adrianne Slyz, Harley Katz, Joakim Rosdahl, Julien Devriendt, Martin Haehnelt, Taysun Kimm","submitted_at":"2016-08-16T20:08:03Z","abstract_excerpt":"Reionisation in the early Universe is likely driven by dwarf galaxies. Using cosmological radiation-hydrodynamic simulations, we study star formation and the escape of Lyman continuum (LyC) photons from mini-haloes with $M_{\\rm halo} \\le 10^8\\,M_\\odot$. Our simulations include a new thermo-turbulent star formation model, non-equilibrium chemistry, and relevant stellar feedback processes (photoionisation by young massive stars, radiation pressure, and mechanical supernova explosions). We find that feedback reduces star formation very efficiently in mini-haloes, resulting in the stellar mass con"},"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":"1608.04762","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-08-16T20:08:03Z","cross_cats_sorted":[],"title_canon_sha256":"d5192ed205bdb59548fd968b2d946b4cc45f454b4b62c8b63a3c9c74c9739753","abstract_canon_sha256":"09a7c5beb1c448e6bd62a9ca3efc83c6448a9a9007c51368586acd82e14d1a09"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:38.993834Z","signature_b64":"XaEFWmEavTxVu9yDhbH/PdqHavCUrrnKNndbmqYxxUhtkOL1evhMML/9JCtmcGyoojHp5I+pfUV7y6tkm0PhCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e666571b0002752a4d4f7590a2d2a2b18d6417d80a317a06a3b45d4969bce958","last_reissued_at":"2026-05-18T00:52:38.993275Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:38.993275Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Feedback-regulated star formation and escape of LyC photons from mini-haloes during reionisation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adrianne Slyz, Harley Katz, Joakim Rosdahl, Julien Devriendt, Martin Haehnelt, Taysun Kimm","submitted_at":"2016-08-16T20:08:03Z","abstract_excerpt":"Reionisation in the early Universe is likely driven by dwarf galaxies. Using cosmological radiation-hydrodynamic simulations, we study star formation and the escape of Lyman continuum (LyC) photons from mini-haloes with $M_{\\rm halo} \\le 10^8\\,M_\\odot$. Our simulations include a new thermo-turbulent star formation model, non-equilibrium chemistry, and relevant stellar feedback processes (photoionisation by young massive stars, radiation pressure, and mechanical supernova explosions). We find that feedback reduces star formation very efficiently in mini-haloes, resulting in the stellar mass con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.04762","kind":"arxiv","version":3},"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":"1608.04762","created_at":"2026-05-18T00:52:38.993384+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.04762v3","created_at":"2026-05-18T00:52:38.993384+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.04762","created_at":"2026-05-18T00:52:38.993384+00:00"},{"alias_kind":"pith_short_12","alias_value":"4ZTFOGYAAJ2S","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_16","alias_value":"4ZTFOGYAAJ2SUTKP","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_8","alias_value":"4ZTFOGYA","created_at":"2026-05-18T12:29:58.707656+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/4ZTFOGYAAJ2SUTKPOWIKFUVCWG","json":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG.json","graph_json":"https://pith.science/api/pith-number/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/graph.json","events_json":"https://pith.science/api/pith-number/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/events.json","paper":"https://pith.science/paper/4ZTFOGYA"},"agent_actions":{"view_html":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG","download_json":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG.json","view_paper":"https://pith.science/paper/4ZTFOGYA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.04762&json=true","fetch_graph":"https://pith.science/api/pith-number/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/graph.json","fetch_events":"https://pith.science/api/pith-number/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/action/storage_attestation","attest_author":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/action/author_attestation","sign_citation":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/action/citation_signature","submit_replication":"https://pith.science/pith/4ZTFOGYAAJ2SUTKPOWIKFUVCWG/action/replication_record"}},"created_at":"2026-05-18T00:52:38.993384+00:00","updated_at":"2026-05-18T00:52:38.993384+00:00"}