{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:JAMPC2WOB23UWJC2IVBHESTCHX","short_pith_number":"pith:JAMPC2WO","schema_version":"1.0","canonical_sha256":"4818f16ace0eb74b245a4542724a623dc5be45b865f66e30823eca0af73117ac","source":{"kind":"arxiv","id":"astro-ph/0412460","version":1},"attestation_state":"computed","paper":{"title":"Discovery of a Large Scale Clumpy Structure around the Lynx Supercluster at z~1.27","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Fumiaki Nakata, Hisanori Furusawa, Kazuhiro Shimasaku, Maki Sekiguchi, Mamoru Doi, Masafumi Yagi, Masahiko Kimura, Masami Ouchi, Masaru Hamabe, Naoki Yasuda, Sadanori Okamura, Satoshi Miyazaki, Tadayuki Kodama, Yoshihiro Ueda, Yutaka Komiyama","submitted_at":"2004-12-17T12:50:44Z","abstract_excerpt":"We report the discovery of a probable large scale structure composed of many galaxy clumps around the known twin clusters at z=1.26 and z=1.27 in the Lynx region. Our analysis is based on deep, panoramic, and multi-colour imaging (26.4'x24.1') in VRi'z'-bands with the Suprime-Cam on the 8.2m Subaru telescope. This unique, deep and wide-field imaging data-set allows us for the first time to map out the galaxy distribution in the highest redshift supercluster known. We apply a photometric redshift technique to extract plausible cluster members at z~1.27 down to i'=26.15 (5sigma) corresponding to"},"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/0412460","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-12-17T12:50:44Z","cross_cats_sorted":[],"title_canon_sha256":"58d257390d1316dd064e9ee7737136cd9ad179b3b6d4eb4f3111abb026f852a2","abstract_canon_sha256":"7149b8de873b941a4b195d3096be45112689be7c7e8ddef36bb33066ea7706c1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:45:26.497891Z","signature_b64":"z/61uQMLzl85TTpvKcs1UsRxXqxF+mDH3Zy+mhNN364fOUAMNk8gGkj+Ut9f8YEsJTiShT/Fag95jCQSan0hAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4818f16ace0eb74b245a4542724a623dc5be45b865f66e30823eca0af73117ac","last_reissued_at":"2026-07-04T16:45:26.497535Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:45:26.497535Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of a Large Scale Clumpy Structure around the Lynx Supercluster at z~1.27","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Fumiaki Nakata, Hisanori Furusawa, Kazuhiro Shimasaku, Maki Sekiguchi, Mamoru Doi, Masafumi Yagi, Masahiko Kimura, Masami Ouchi, Masaru Hamabe, Naoki Yasuda, Sadanori Okamura, Satoshi Miyazaki, Tadayuki Kodama, Yoshihiro Ueda, Yutaka Komiyama","submitted_at":"2004-12-17T12:50:44Z","abstract_excerpt":"We report the discovery of a probable large scale structure composed of many galaxy clumps around the known twin clusters at z=1.26 and z=1.27 in the Lynx region. Our analysis is based on deep, panoramic, and multi-colour imaging (26.4'x24.1') in VRi'z'-bands with the Suprime-Cam on the 8.2m Subaru telescope. This unique, deep and wide-field imaging data-set allows us for the first time to map out the galaxy distribution in the highest redshift supercluster known. We apply a photometric redshift technique to extract plausible cluster members at z~1.27 down to i'=26.15 (5sigma) corresponding to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0412460","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/0412460/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/0412460","created_at":"2026-07-04T16:45:26.497589+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0412460v1","created_at":"2026-07-04T16:45:26.497589+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0412460","created_at":"2026-07-04T16:45:26.497589+00:00"},{"alias_kind":"pith_short_12","alias_value":"JAMPC2WOB23U","created_at":"2026-07-04T16:45:26.497589+00:00"},{"alias_kind":"pith_short_16","alias_value":"JAMPC2WOB23UWJC2","created_at":"2026-07-04T16:45:26.497589+00:00"},{"alias_kind":"pith_short_8","alias_value":"JAMPC2WO","created_at":"2026-07-04T16:45:26.497589+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/JAMPC2WOB23UWJC2IVBHESTCHX","json":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX.json","graph_json":"https://pith.science/api/pith-number/JAMPC2WOB23UWJC2IVBHESTCHX/graph.json","events_json":"https://pith.science/api/pith-number/JAMPC2WOB23UWJC2IVBHESTCHX/events.json","paper":"https://pith.science/paper/JAMPC2WO"},"agent_actions":{"view_html":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX","download_json":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX.json","view_paper":"https://pith.science/paper/JAMPC2WO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0412460&json=true","fetch_graph":"https://pith.science/api/pith-number/JAMPC2WOB23UWJC2IVBHESTCHX/graph.json","fetch_events":"https://pith.science/api/pith-number/JAMPC2WOB23UWJC2IVBHESTCHX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX/action/storage_attestation","attest_author":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX/action/author_attestation","sign_citation":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX/action/citation_signature","submit_replication":"https://pith.science/pith/JAMPC2WOB23UWJC2IVBHESTCHX/action/replication_record"}},"created_at":"2026-07-04T16:45:26.497589+00:00","updated_at":"2026-07-04T16:45:26.497589+00:00"}