{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:PP3BWMWYDVR5UUWRRWEZGVILOD","short_pith_number":"pith:PP3BWMWY","schema_version":"1.0","canonical_sha256":"7bf61b32d81d63da52d18d8993550b70f1e0a37e769b9a56ab4f641e4c1cfc2e","source":{"kind":"arxiv","id":"2506.23105","version":1},"attestation_state":"computed","paper":{"title":"How Do Ionizing Photons Escape from Star-Forming Galaxies?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"Allison Strom, Cody Carr, Renyue Cen, Sally Oey, Sophia Flury, Stephan McCandliss","submitted_at":"2025-06-29T06:10:36Z","abstract_excerpt":"The Epoch of Reionization marks the last major phase transition in the early Universe, during which the majority of neutral hydrogen once filling the intergalactic medium was ionized by the first galaxies. The James Webb Space Telescope is now identifying promising galaxy candidates capable of producing sufficient ionizing photons to drive this transformation. However, the fraction of these photons that escape into intergalactic space--the escape fraction--remains highly uncertain. Stellar feedback is thought to play a critical role in carving low-density channels that allow ionizing radiation"},"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":"2506.23105","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-06-29T06:10:36Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"8917acfe8978edd9378e79848ac97ecebf8737b9996c85ff74b78f1c4081dbae","abstract_canon_sha256":"694a892c0bfeb6ddcc2f279a64bf293def49e09cf1b607bce87971bdb70371ad"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:29:15.452414Z","signature_b64":"ik5N/TCjCM5MV1JMTtZhUYKlP8KbSbTSFv+Pp9rtw+j5FZwHTtOqWzBiEOwzr6+D5Iqa0paXs8cK178ZPM4sAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7bf61b32d81d63da52d18d8993550b70f1e0a37e769b9a56ab4f641e4c1cfc2e","last_reissued_at":"2026-07-05T11:29:15.451906Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:29:15.451906Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How Do Ionizing Photons Escape from Star-Forming Galaxies?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"Allison Strom, Cody Carr, Renyue Cen, Sally Oey, Sophia Flury, Stephan McCandliss","submitted_at":"2025-06-29T06:10:36Z","abstract_excerpt":"The Epoch of Reionization marks the last major phase transition in the early Universe, during which the majority of neutral hydrogen once filling the intergalactic medium was ionized by the first galaxies. The James Webb Space Telescope is now identifying promising galaxy candidates capable of producing sufficient ionizing photons to drive this transformation. However, the fraction of these photons that escape into intergalactic space--the escape fraction--remains highly uncertain. Stellar feedback is thought to play a critical role in carving low-density channels that allow ionizing radiation"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.23105","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2506.23105/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":"2506.23105","created_at":"2026-07-05T11:29:15.451969+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.23105v1","created_at":"2026-07-05T11:29:15.451969+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.23105","created_at":"2026-07-05T11:29:15.451969+00:00"},{"alias_kind":"pith_short_12","alias_value":"PP3BWMWYDVR5","created_at":"2026-07-05T11:29:15.451969+00:00"},{"alias_kind":"pith_short_16","alias_value":"PP3BWMWYDVR5UUWR","created_at":"2026-07-05T11:29:15.451969+00:00"},{"alias_kind":"pith_short_8","alias_value":"PP3BWMWY","created_at":"2026-07-05T11:29:15.451969+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.12482","citing_title":"CLASSY. XV. Kinematics and Spatial Distributions of Outflows in Local Highly Star-Forming Galaxies","ref_index":3,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD","json":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD.json","graph_json":"https://pith.science/api/pith-number/PP3BWMWYDVR5UUWRRWEZGVILOD/graph.json","events_json":"https://pith.science/api/pith-number/PP3BWMWYDVR5UUWRRWEZGVILOD/events.json","paper":"https://pith.science/paper/PP3BWMWY"},"agent_actions":{"view_html":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD","download_json":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD.json","view_paper":"https://pith.science/paper/PP3BWMWY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.23105&json=true","fetch_graph":"https://pith.science/api/pith-number/PP3BWMWYDVR5UUWRRWEZGVILOD/graph.json","fetch_events":"https://pith.science/api/pith-number/PP3BWMWYDVR5UUWRRWEZGVILOD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD/action/storage_attestation","attest_author":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD/action/author_attestation","sign_citation":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD/action/citation_signature","submit_replication":"https://pith.science/pith/PP3BWMWYDVR5UUWRRWEZGVILOD/action/replication_record"}},"created_at":"2026-07-05T11:29:15.451969+00:00","updated_at":"2026-07-05T11:29:15.451969+00:00"}