{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:7SPX7HUDLBYMWRUDAOBEOFF2OJ","short_pith_number":"pith:7SPX7HUD","schema_version":"1.0","canonical_sha256":"fc9f7f9e835870cb468303824714ba72424ea2ad13c6d6411197c956fe784042","source":{"kind":"arxiv","id":"1711.04787","version":1},"attestation_state":"computed","paper":{"title":"Lyman-Break Galaxies at $z\\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chun Ly, Daniel P. Cohen, Kazuhiro Shimasaku, Kentaro Motohara, Masao Hayashi, Matthew A. Malkan, Miyoko Maruyama, Nobunari Kashikawa, Shogo Ishikawa","submitted_at":"2017-11-13T19:00:38Z","abstract_excerpt":"We combined deep U-band imaging from the KPNO-4m/MOSAIC camera with very deep multi-waveband data from the optical to infrared, to select Lyman Break Galaxies (LBGs) at z~3 using U-V and V-R colors in the Subaru Deep Field. With the resulting sample of 5161 LBGs, we construct the UV luminosity function down to $M_{UV} = -18$ and find a steep faint-end slope of $\\alpha=-1.78 \\pm 0.05$. We analyze rest-frame UV-to-IR spectral energy distributions generated from the median optical photometry and photometry on median-stacked IR images. In the stacks of faint LBGs, we find a background depression c"},"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":"1711.04787","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-13T19:00:38Z","cross_cats_sorted":[],"title_canon_sha256":"b737035bc2c0f53b30dd913bd6fdd5ae65e765573afeb7ec4cfc7f0b7adcb173","abstract_canon_sha256":"6ef1235218b1232ab978ca60a482bb89928d7844b290b777a3d4e1c7760bd56b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:30:35.736752Z","signature_b64":"U3GWP6g2fFxoGx38cl7SLuB1QcP/qM4FCVCUbf5hbK4IXvptZVwQlYuoY+rS4HWzzl65YxW2VRUj11OeXOVUAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fc9f7f9e835870cb468303824714ba72424ea2ad13c6d6411197c956fe784042","last_reissued_at":"2026-05-18T00:30:35.736126Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:30:35.736126Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Lyman-Break Galaxies at $z\\sim 3$ in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Chun Ly, Daniel P. Cohen, Kazuhiro Shimasaku, Kentaro Motohara, Masao Hayashi, Matthew A. Malkan, Miyoko Maruyama, Nobunari Kashikawa, Shogo Ishikawa","submitted_at":"2017-11-13T19:00:38Z","abstract_excerpt":"We combined deep U-band imaging from the KPNO-4m/MOSAIC camera with very deep multi-waveband data from the optical to infrared, to select Lyman Break Galaxies (LBGs) at z~3 using U-V and V-R colors in the Subaru Deep Field. With the resulting sample of 5161 LBGs, we construct the UV luminosity function down to $M_{UV} = -18$ and find a steep faint-end slope of $\\alpha=-1.78 \\pm 0.05$. We analyze rest-frame UV-to-IR spectral energy distributions generated from the median optical photometry and photometry on median-stacked IR images. In the stacks of faint LBGs, we find a background depression c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.04787","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":""},"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":"1711.04787","created_at":"2026-05-18T00:30:35.736199+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.04787v1","created_at":"2026-05-18T00:30:35.736199+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.04787","created_at":"2026-05-18T00:30:35.736199+00:00"},{"alias_kind":"pith_short_12","alias_value":"7SPX7HUDLBYM","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"7SPX7HUDLBYMWRUD","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"7SPX7HUD","created_at":"2026-05-18T12:31:05.417338+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/7SPX7HUDLBYMWRUDAOBEOFF2OJ","json":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ.json","graph_json":"https://pith.science/api/pith-number/7SPX7HUDLBYMWRUDAOBEOFF2OJ/graph.json","events_json":"https://pith.science/api/pith-number/7SPX7HUDLBYMWRUDAOBEOFF2OJ/events.json","paper":"https://pith.science/paper/7SPX7HUD"},"agent_actions":{"view_html":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ","download_json":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ.json","view_paper":"https://pith.science/paper/7SPX7HUD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.04787&json=true","fetch_graph":"https://pith.science/api/pith-number/7SPX7HUDLBYMWRUDAOBEOFF2OJ/graph.json","fetch_events":"https://pith.science/api/pith-number/7SPX7HUDLBYMWRUDAOBEOFF2OJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ/action/storage_attestation","attest_author":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ/action/author_attestation","sign_citation":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ/action/citation_signature","submit_replication":"https://pith.science/pith/7SPX7HUDLBYMWRUDAOBEOFF2OJ/action/replication_record"}},"created_at":"2026-05-18T00:30:35.736199+00:00","updated_at":"2026-05-18T00:30:35.736199+00:00"}