{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:NLICRCOQZ7RPOJBIZ4NQZ2BRRH","short_pith_number":"pith:NLICRCOQ","schema_version":"1.0","canonical_sha256":"6ad02889d0cfe2f72428cf1b0ce83189e12f1b687cf4e32c6761cb84edc5427b","source":{"kind":"arxiv","id":"astro-ph/0302466","version":1},"attestation_state":"computed","paper":{"title":"Subaru Deep Survey. IV. Discovery of a Large-Scale Structure at Redshift \\simeq 5","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Nakata, H. Furusawa, H. Tamura, K. Kawabata, K. Kodaira, K. Ohta, K. Shimasaku, M. Doi, M. Hamabe, M. Kimura, M. Miyazaki, M. Ouchi, M. Sekiguchi, M. Yagi, N. Kashikawa, N. Yasuda, S. Miyazaki, S. Okamura, T. Hayashino, T. Yamada, Y. Komiyama, Y. Matsuda, Y. Ohyama, Y. Shioya, Y. Taniguchi","submitted_at":"2003-02-22T07:18:11Z","abstract_excerpt":"We report the discovery of a large-scale structure of Lyman alpha emitters (LAEs) at z=4.86 based on wide-field imaging with the prime-focus camera (Suprime-Cam) on the Subaru telescope. We observed a 25' x 45' area of the Subaru Deep Field in a narrow band (NB, lambdaC=7126 A and FWHM=73 A) together with R and i'. We isolate from these data 43 LAE candidates down to NB=25.5 mag using color criteria. Follow-up spectroscopy of five candidates suggests the contamination by low-z objects to be ~ 20%. We find that the LAE candidates are clustered in an elongated region on the sky of 20 Mpc in widt"},"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":"astro-ph/0302466","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-02-22T07:18:11Z","cross_cats_sorted":[],"title_canon_sha256":"f0cc2245f1c6125b779af49b41843a6b46f2f5cc6b9494a20c3b0e4d8212ecbe","abstract_canon_sha256":"56f18b3e930a5105cc1b57f7bdf57abd8a8f5e2d1aebff86973db9759237c786"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:36:32.058360Z","signature_b64":"jcJN0HLWoJecTiOk1JUeMGmvy7yGPfjeqj5P613TQoEiS2gO8oclKbmnJGVvEmS0HVf8i8RqrggV0PFUS6SYAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ad02889d0cfe2f72428cf1b0ce83189e12f1b687cf4e32c6761cb84edc5427b","last_reissued_at":"2026-07-04T16:36:32.057877Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:36:32.057877Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Subaru Deep Survey. IV. Discovery of a Large-Scale Structure at Redshift \\simeq 5","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Nakata, H. Furusawa, H. Tamura, K. Kawabata, K. Kodaira, K. Ohta, K. Shimasaku, M. Doi, M. Hamabe, M. Kimura, M. Miyazaki, M. Ouchi, M. Sekiguchi, M. Yagi, N. Kashikawa, N. Yasuda, S. Miyazaki, S. Okamura, T. Hayashino, T. Yamada, Y. Komiyama, Y. Matsuda, Y. Ohyama, Y. Shioya, Y. Taniguchi","submitted_at":"2003-02-22T07:18:11Z","abstract_excerpt":"We report the discovery of a large-scale structure of Lyman alpha emitters (LAEs) at z=4.86 based on wide-field imaging with the prime-focus camera (Suprime-Cam) on the Subaru telescope. We observed a 25' x 45' area of the Subaru Deep Field in a narrow band (NB, lambdaC=7126 A and FWHM=73 A) together with R and i'. We isolate from these data 43 LAE candidates down to NB=25.5 mag using color criteria. Follow-up spectroscopy of five candidates suggests the contamination by low-z objects to be ~ 20%. We find that the LAE candidates are clustered in an elongated region on the sky of 20 Mpc in widt"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0302466","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/astro-ph/0302466/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":"astro-ph/0302466","created_at":"2026-07-04T16:36:32.057939+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0302466v1","created_at":"2026-07-04T16:36:32.057939+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0302466","created_at":"2026-07-04T16:36:32.057939+00:00"},{"alias_kind":"pith_short_12","alias_value":"NLICRCOQZ7RP","created_at":"2026-07-04T16:36:32.057939+00:00"},{"alias_kind":"pith_short_16","alias_value":"NLICRCOQZ7RPOJBI","created_at":"2026-07-04T16:36:32.057939+00:00"},{"alias_kind":"pith_short_8","alias_value":"NLICRCOQ","created_at":"2026-07-04T16:36:32.057939+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.23790","citing_title":"Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters","ref_index":254,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH","json":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH.json","graph_json":"https://pith.science/api/pith-number/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/graph.json","events_json":"https://pith.science/api/pith-number/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/events.json","paper":"https://pith.science/paper/NLICRCOQ"},"agent_actions":{"view_html":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH","download_json":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH.json","view_paper":"https://pith.science/paper/NLICRCOQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0302466&json=true","fetch_graph":"https://pith.science/api/pith-number/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/graph.json","fetch_events":"https://pith.science/api/pith-number/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/action/storage_attestation","attest_author":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/action/author_attestation","sign_citation":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/action/citation_signature","submit_replication":"https://pith.science/pith/NLICRCOQZ7RPOJBIZ4NQZ2BRRH/action/replication_record"}},"created_at":"2026-07-04T16:36:32.057939+00:00","updated_at":"2026-07-04T16:36:32.057939+00:00"}