{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:DOE5Q2M7MR6PFCJQPFXDEUJ5FW","short_pith_number":"pith:DOE5Q2M7","schema_version":"1.0","canonical_sha256":"1b89d8699f647cf28930796e32513d2d8516035570e1fde9fe573b097455b83f","source":{"kind":"arxiv","id":"2211.08254","version":1},"attestation_state":"computed","paper":{"title":"EIGER I. a large sample of [OIII]-emitting galaxies at $5.3 < z < 6.9$ and direct evidence for local reionization by galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Anna-Christina Eilers, Daichi Kashino, Jorryt Matthee, Robert A. Simcoe, Rongmon Bordoloi, Ruari Mackenzie, Simon J. Lilly","submitted_at":"2022-11-15T16:00:24Z","abstract_excerpt":"We present a first sample of 117 [OIII]$\\lambda\\lambda$4960,5008-selected star-forming galaxies at $5.33 < z < 6.93$ detected in JWST/NIRCam 3.5$\\mu$m slitless spectroscopy of a $6.5 \\times 3.4$ arcmin$^2$ field centered on the hyperluminous quasar SDSS J0100+2802, obtained as part of the EIGER (Emission-line galaxies and Intergalactic Gas in the Epoch of Reionization) survey. Three prominent galaxy overdensities are observed, one of them at the redshift of the quasar. Galaxies are found within 200 pkpc and 105 km s$^{-1}$ of four known metal absorption-line systems in this redshift range. We "},"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":"2211.08254","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-11-15T16:00:24Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"d4bb3bf4063d8fa7766189844d2b9e1c4d095f12697db835a082091abbd8d418","abstract_canon_sha256":"4cd54ce8867a735a5f97ce31adb901d0d6c376698405c3740238a34bbfa3d76d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:25:15.424608Z","signature_b64":"f7nb7/FctgBO8ZprN2XzAgqdU0GWAwyrawZvrna5pVj2dxWkn3dIB0C0zhTUC/188emZyyMazIP4boTKwfd/AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b89d8699f647cf28930796e32513d2d8516035570e1fde9fe573b097455b83f","last_reissued_at":"2026-07-05T06:25:15.424121Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:25:15.424121Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"EIGER I. a large sample of [OIII]-emitting galaxies at $5.3 < z < 6.9$ and direct evidence for local reionization by galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Anna-Christina Eilers, Daichi Kashino, Jorryt Matthee, Robert A. Simcoe, Rongmon Bordoloi, Ruari Mackenzie, Simon J. Lilly","submitted_at":"2022-11-15T16:00:24Z","abstract_excerpt":"We present a first sample of 117 [OIII]$\\lambda\\lambda$4960,5008-selected star-forming galaxies at $5.33 < z < 6.93$ detected in JWST/NIRCam 3.5$\\mu$m slitless spectroscopy of a $6.5 \\times 3.4$ arcmin$^2$ field centered on the hyperluminous quasar SDSS J0100+2802, obtained as part of the EIGER (Emission-line galaxies and Intergalactic Gas in the Epoch of Reionization) survey. Three prominent galaxy overdensities are observed, one of them at the redshift of the quasar. Galaxies are found within 200 pkpc and 105 km s$^{-1}$ of four known metal absorption-line systems in this redshift range. We "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.08254","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/2211.08254/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":"2211.08254","created_at":"2026-07-05T06:25:15.424178+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.08254v1","created_at":"2026-07-05T06:25:15.424178+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.08254","created_at":"2026-07-05T06:25:15.424178+00:00"},{"alias_kind":"pith_short_12","alias_value":"DOE5Q2M7MR6P","created_at":"2026-07-05T06:25:15.424178+00:00"},{"alias_kind":"pith_short_16","alias_value":"DOE5Q2M7MR6PFCJQ","created_at":"2026-07-05T06:25:15.424178+00:00"},{"alias_kind":"pith_short_8","alias_value":"DOE5Q2M7","created_at":"2026-07-05T06:25:15.424178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05523","citing_title":"BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\\simeq5.23$","ref_index":46,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW","json":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW.json","graph_json":"https://pith.science/api/pith-number/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/graph.json","events_json":"https://pith.science/api/pith-number/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/events.json","paper":"https://pith.science/paper/DOE5Q2M7"},"agent_actions":{"view_html":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW","download_json":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW.json","view_paper":"https://pith.science/paper/DOE5Q2M7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.08254&json=true","fetch_graph":"https://pith.science/api/pith-number/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/graph.json","fetch_events":"https://pith.science/api/pith-number/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/action/storage_attestation","attest_author":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/action/author_attestation","sign_citation":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/action/citation_signature","submit_replication":"https://pith.science/pith/DOE5Q2M7MR6PFCJQPFXDEUJ5FW/action/replication_record"}},"created_at":"2026-07-05T06:25:15.424178+00:00","updated_at":"2026-07-05T06:25:15.424178+00:00"}