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Komiyama","submitted_at":"2003-09-24T04:42:15Z","abstract_excerpt":"We investigate the clustering properties of 2,600 Lyman Break Galaxies (LBGs) at z=3.5-5.2 in two large blank fields, the Subaru Deep Field and the Subaru/XMM Deep Field (600arcmin^2 each). The angular correlation functions of these LBGs show a clear clustering at both z~4 and 5. The correlation lengths are r_0= 4.1^{+0.2}_{-0.2} and 5.9^{+1.3}_{-1.7} h_{100}^{-1} Mpc (r_0= 5.1^{+1.0}_{-1.1} and 5.9^{+1.3}_{-1.7} h_{100}^{-1} Mpc) for all the detected LBGs (for L>L* LBGs) at z~4 and 5, respectively. These correlation lengths correspond to galaxy-dark matter biases of b_g= 2.9^{+0.1}_{-0.1} and"},"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/0309657","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-09-24T04:42:15Z","cross_cats_sorted":[],"title_canon_sha256":"ad72eaa4980c50d13ea4a8cdf4dc382f881a5c4a0f552beccb55c97fbaa442d7","abstract_canon_sha256":"3478850efd16123c83b7c15af208843dd87271123682409b394eb0e7ca772747"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:19:41.626845Z","signature_b64":"CR0E10+c+MeN2KPQfB6zuhIUPE6JzSSAop4LmWSj4VFlsG45WSGLKLaFSsrLVgWcq/hhkx84dhX3GabyYjVbBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f8a9821436ddb764e9d5d630e3a5dcc277e32e834141de490adc2d344f736133","last_reissued_at":"2026-05-18T04:19:41.626158Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:19:41.626158Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Subaru Deep Survey VI. 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