{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:MI3TVHVFLIC3CNR4F2CKC2LMER","short_pith_number":"pith:MI3TVHVF","schema_version":"1.0","canonical_sha256":"62373a9ea55a05b1363c2e84a1696c245f5e20f1ba61724f3a238e6dc7167ca9","source":{"kind":"arxiv","id":"2512.14486","version":2},"attestation_state":"computed","paper":{"title":"A first systematic study of [OIII] 88$\\mu$m at $z>8$: two luminous oxygen lines and a powerful ionized outflow in the first 600 million years","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akio K. Inoue, Andrea Ferrara, Andrea Pallottini, Andreas Faisst, Bovornpratch Vijarnwannaluk, Chayan Mondal, Chian-Chou Chen, Daniel P. Stark, Elisabete da Cunha, Hanae Inami, Hiddo S. B. Algera, Huub R\\\"ottgering, Jacqueline Hodge, John R. Weaver, Joris Witstok, Jorryt Matthee, Karin Cescon, Kasper Heintz, Laura Sommovigo, Livia Vallini, Lucie E. Rowland, Manuel Aravena, Mengyuan Xiao, Norbert Werner, Pascal A. Oesch, Paul van der Werf, Pratika Dayal, Renske Smit, Rodrigo Herrera-Camus, Romain Meyer, Rychard J. Bouwens, Sander Schouws, Seiji Fujimoto, Shoichiro Mizukoshi, Takuya Hashimoto, Themiya Nanayakkara, Tom J. L. C. Bakx, Yuma Sugahara","submitted_at":"2025-12-16T15:17:11Z","abstract_excerpt":"We present deep ALMA Band 7 observations of the [OIII] $88\\mu$m line and underlying dust continuum emission in four UV-bright, gravitationally lensed (magnification $\\mu = 1.4-3.8$), JWST-selected galaxies at $z = 8.5 - 10.3$, with observed magnitudes $-22.5 \\lesssim M_\\mathrm{UV} \\lesssim -20.5$. [OIII] $88\\mu$m is confidently detected in UNCOVER-10646 at $z=8.5080 \\pm 0.0011$ ($15\\sigma$) and DHZ1 at $z=9.3113 \\pm 0.0006$ ($6\\sigma$), with both being intrinsically luminous systems [$L_\\text{[OIII]} = (1.1 - 1.6) \\times 10^9\\,L_\\odot$] that follow the local [OIII]-SFR relation. [OIII] $88\\mu$"},"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":"2512.14486","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-12-16T15:17:11Z","cross_cats_sorted":[],"title_canon_sha256":"4017a4dbf9d825f6aeda8ceb475e538a7f73e08ec05fdfebd2e93ee809fa83ee","abstract_canon_sha256":"5344f64fc85eade1c865a42669f9eb51f886b647d4ba375aded7f6bec8cd3fff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-21T01:21:41.522388Z","signature_b64":"0f32jhkHysW9SQ3Qw4rMRUgzTgyqDaRQ7Z+B8WmTXS4Dps3acCQSYJQ/yvb+4l6CoxJCBkxFTwYJcNAzNwA8Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"62373a9ea55a05b1363c2e84a1696c245f5e20f1ba61724f3a238e6dc7167ca9","last_reissued_at":"2026-07-21T01:21:41.521449Z","signature_status":"signed_v1","first_computed_at":"2026-07-21T01:21:41.521449Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A first systematic study of [OIII] 88$\\mu$m at $z>8$: two luminous oxygen lines and a powerful ionized outflow in the first 600 million years","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akio K. Inoue, Andrea Ferrara, Andrea Pallottini, Andreas Faisst, Bovornpratch Vijarnwannaluk, Chayan Mondal, Chian-Chou Chen, Daniel P. Stark, Elisabete da Cunha, Hanae Inami, Hiddo S. B. Algera, Huub R\\\"ottgering, Jacqueline Hodge, John R. Weaver, Joris Witstok, Jorryt Matthee, Karin Cescon, Kasper Heintz, Laura Sommovigo, Livia Vallini, Lucie E. Rowland, Manuel Aravena, Mengyuan Xiao, Norbert Werner, Pascal A. Oesch, Paul van der Werf, Pratika Dayal, Renske Smit, Rodrigo Herrera-Camus, Romain Meyer, Rychard J. Bouwens, Sander Schouws, Seiji Fujimoto, Shoichiro Mizukoshi, Takuya Hashimoto, Themiya Nanayakkara, Tom J. L. C. Bakx, Yuma Sugahara","submitted_at":"2025-12-16T15:17:11Z","abstract_excerpt":"We present deep ALMA Band 7 observations of the [OIII] $88\\mu$m line and underlying dust continuum emission in four UV-bright, gravitationally lensed (magnification $\\mu = 1.4-3.8$), JWST-selected galaxies at $z = 8.5 - 10.3$, with observed magnitudes $-22.5 \\lesssim M_\\mathrm{UV} \\lesssim -20.5$. [OIII] $88\\mu$m is confidently detected in UNCOVER-10646 at $z=8.5080 \\pm 0.0011$ ($15\\sigma$) and DHZ1 at $z=9.3113 \\pm 0.0006$ ($6\\sigma$), with both being intrinsically luminous systems [$L_\\text{[OIII]} = (1.1 - 1.6) \\times 10^9\\,L_\\odot$] that follow the local [OIII]-SFR relation. [OIII] $88\\mu$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2512.14486","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/2512.14486/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":"2512.14486","created_at":"2026-07-21T01:21:41.521883+00:00"},{"alias_kind":"arxiv_version","alias_value":"2512.14486v2","created_at":"2026-07-21T01:21:41.521883+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2512.14486","created_at":"2026-07-21T01:21:41.521883+00:00"},{"alias_kind":"pith_short_12","alias_value":"MI3TVHVFLIC3","created_at":"2026-07-21T01:21:41.521883+00:00"},{"alias_kind":"pith_short_16","alias_value":"MI3TVHVFLIC3CNR4","created_at":"2026-07-21T01:21:41.521883+00:00"},{"alias_kind":"pith_short_8","alias_value":"MI3TVHVF","created_at":"2026-07-21T01:21:41.521883+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2606.13078","citing_title":"Chemical signatures from the first stars embedded in metal-poor gas in galaxies at cosmic dawn","ref_index":74,"is_internal_anchor":true},{"citing_arxiv_id":"2606.06108","citing_title":"Grain-size evolution and rapid dust growth in high-redshift galaxies","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2606.06609","citing_title":"JWST absorption line spectroscopy with SPURS: ISM covering fractions and kinematics in individual galaxies at $z=5-9$","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2606.10271","citing_title":"Multiphase images of a powerful supernova-driven wind in the early Universe","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2604.22460","citing_title":"Spatially resolved metallicity and ionization in the merging system Gz9p3 at z=9.3","ref_index":1,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER","json":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER.json","graph_json":"https://pith.science/api/pith-number/MI3TVHVFLIC3CNR4F2CKC2LMER/graph.json","events_json":"https://pith.science/api/pith-number/MI3TVHVFLIC3CNR4F2CKC2LMER/events.json","paper":"https://pith.science/paper/MI3TVHVF"},"agent_actions":{"view_html":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER","download_json":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER.json","view_paper":"https://pith.science/paper/MI3TVHVF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2512.14486&json=true","fetch_graph":"https://pith.science/api/pith-number/MI3TVHVFLIC3CNR4F2CKC2LMER/graph.json","fetch_events":"https://pith.science/api/pith-number/MI3TVHVFLIC3CNR4F2CKC2LMER/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER/action/storage_attestation","attest_author":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER/action/author_attestation","sign_citation":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER/action/citation_signature","submit_replication":"https://pith.science/pith/MI3TVHVFLIC3CNR4F2CKC2LMER/action/replication_record"}},"created_at":"2026-07-21T01:21:41.521883+00:00","updated_at":"2026-07-21T01:21:41.521883+00:00"}