{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:6AOIX5SX4PZVANMJ5CTIMKKOGR","short_pith_number":"pith:6AOIX5SX","schema_version":"1.0","canonical_sha256":"f01c8bf657e3f3503589e8a686294e3452c41b8026de7d0b2b221b2bec0b191e","source":{"kind":"arxiv","id":"2507.16231","version":2},"attestation_state":"computed","paper":{"title":"Ly$\\alpha$ Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly$\\alpha$ detection","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"George D. Becker, Hui Hong, Seyedazim Hashemi, Yongda Zhu","submitted_at":"2025-07-22T05:04:30Z","abstract_excerpt":"Using galaxy Ly$\\alpha$ emission to probe reionization relies on establishing baseline expectations for its detectability in the absence of attenuation by neutral gas in the IGM. Towards this end, the growing numbers of $z \\sim 5$--6 star-forming galaxies spectroscopically selected by JWST provide an ideal sample for determining how Ly$\\alpha$ emission depends on galaxy properties and environment after reionization has largely completed. In this study, we use Keck LRIS to measure the Ly$\\alpha$ emission of 46 JWST-selected [OIII]-emitting galaxies over $5.3 \\lesssim z \\lesssim 6.2$ in the fore"},"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":"2507.16231","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-07-22T05:04:30Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"602d33fa9f93279c583b98481ecc5473ce378b748c5a50f30dffc9766338c506","abstract_canon_sha256":"0df70c4f2001b8f06f5eb7bb7decd9b9f0a50f20daeac3368ddcf0e3440e8e3a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:45:37.924271Z","signature_b64":"aq2XycWaMO8ZoerkoP/Ynr6+Be2Kivp7tcRz3Opr4ZLtUfvutiUqT4qOhr2gsFGZ+08IUyCz+LxnnvwxoIs0Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f01c8bf657e3f3503589e8a686294e3452c41b8026de7d0b2b221b2bec0b191e","last_reissued_at":"2026-07-05T11:45:37.923785Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:45:37.923785Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ly$\\alpha$ Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly$\\alpha$ detection","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"George D. Becker, Hui Hong, Seyedazim Hashemi, Yongda Zhu","submitted_at":"2025-07-22T05:04:30Z","abstract_excerpt":"Using galaxy Ly$\\alpha$ emission to probe reionization relies on establishing baseline expectations for its detectability in the absence of attenuation by neutral gas in the IGM. Towards this end, the growing numbers of $z \\sim 5$--6 star-forming galaxies spectroscopically selected by JWST provide an ideal sample for determining how Ly$\\alpha$ emission depends on galaxy properties and environment after reionization has largely completed. In this study, we use Keck LRIS to measure the Ly$\\alpha$ emission of 46 JWST-selected [OIII]-emitting galaxies over $5.3 \\lesssim z \\lesssim 6.2$ in the fore"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.16231","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/2507.16231/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":"2507.16231","created_at":"2026-07-05T11:45:37.923845+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.16231v2","created_at":"2026-07-05T11:45:37.923845+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.16231","created_at":"2026-07-05T11:45:37.923845+00:00"},{"alias_kind":"pith_short_12","alias_value":"6AOIX5SX4PZV","created_at":"2026-07-05T11:45:37.923845+00:00"},{"alias_kind":"pith_short_16","alias_value":"6AOIX5SX4PZVANMJ","created_at":"2026-07-05T11:45:37.923845+00:00"},{"alias_kind":"pith_short_8","alias_value":"6AOIX5SX","created_at":"2026-07-05T11:45:37.923845+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/6AOIX5SX4PZVANMJ5CTIMKKOGR","json":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR.json","graph_json":"https://pith.science/api/pith-number/6AOIX5SX4PZVANMJ5CTIMKKOGR/graph.json","events_json":"https://pith.science/api/pith-number/6AOIX5SX4PZVANMJ5CTIMKKOGR/events.json","paper":"https://pith.science/paper/6AOIX5SX"},"agent_actions":{"view_html":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR","download_json":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR.json","view_paper":"https://pith.science/paper/6AOIX5SX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.16231&json=true","fetch_graph":"https://pith.science/api/pith-number/6AOIX5SX4PZVANMJ5CTIMKKOGR/graph.json","fetch_events":"https://pith.science/api/pith-number/6AOIX5SX4PZVANMJ5CTIMKKOGR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR/action/storage_attestation","attest_author":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR/action/author_attestation","sign_citation":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR/action/citation_signature","submit_replication":"https://pith.science/pith/6AOIX5SX4PZVANMJ5CTIMKKOGR/action/replication_record"}},"created_at":"2026-07-05T11:45:37.923845+00:00","updated_at":"2026-07-05T11:45:37.923845+00:00"}