{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:BP5QUJ7PYGLM7QCVTN5CBH7L4I","short_pith_number":"pith:BP5QUJ7P","schema_version":"1.0","canonical_sha256":"0bfb0a27efc196cfc0559b7a209febe20da077c251933e3cc9454d213bc77be9","source":{"kind":"arxiv","id":"1005.1661","version":2},"attestation_state":"computed","paper":{"title":"The Evolution of the UV Luminosity Function from z ~ 0.75 to z ~ 2.5 using HST ERS WFC3/UVIS Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Santa Cruz, 3), (3) Leiden, (4) Colorado, (5) STScI, (6) Carnegie, (7) Yale), C. M. Carollo (1), D. Magee (2), G. D. Illingworth (2), I. Labbe (6), M. Franx (3), M. Stiavelli (5), M. Trenti (4), P. A. Oesch (1), P. G. van Dokkum (7) ((1) ETH Zurich, R. J. Bouwens (2","submitted_at":"2010-05-10T20:17:05Z","abstract_excerpt":"We present UV luminosity functions (LFs) at 1500 Angstrom derived from the HST Early Release Science WFC3/UVIS data acquired over ~50 arcmin^2 of the GOODS-South field. The LFs are determined over the entire redshift range z=0.75-2.5 using two methods, similar to those used at higher redshifts for Lyman Break Galaxies (LBGs): (1) 13-band UV+optical+NIR photometric redshifts to study galaxies in the range z=0.5-2 in three bins of dz=0.5, and (2) dropout samples in three redshift windows centered at z~1.5, z~1.9, and z~2.5. The characteristic luminosity dims by ~1.5 mag from z=2.5 to z=0.75, con"},"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":"1005.1661","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-05-10T20:17:05Z","cross_cats_sorted":[],"title_canon_sha256":"a0981122283c28bdb18a1295d0bbc8044a40cbcbf3c44746979c20d5df2778ba","abstract_canon_sha256":"8098d8dca8ecd5ece9e9d711a1718e2645659fd75a1a89d22e8fa2e64925ef4f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:34:27.540436Z","signature_b64":"JvOJP6EHmbWSnOp8o1we0Wx7E0LAGM/UtEmEKNINAbzS663P07kTIQP7zHSOpKkX65bIy0x5aQ8bpN1M2mFQDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0bfb0a27efc196cfc0559b7a209febe20da077c251933e3cc9454d213bc77be9","last_reissued_at":"2026-05-18T04:34:27.539734Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:34:27.539734Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Evolution of the UV Luminosity Function from z ~ 0.75 to z ~ 2.5 using HST ERS WFC3/UVIS Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Santa Cruz, 3), (3) Leiden, (4) Colorado, (5) STScI, (6) Carnegie, (7) Yale), C. M. Carollo (1), D. Magee (2), G. D. Illingworth (2), I. Labbe (6), M. Franx (3), M. Stiavelli (5), M. Trenti (4), P. A. Oesch (1), P. G. van Dokkum (7) ((1) ETH Zurich, R. J. Bouwens (2","submitted_at":"2010-05-10T20:17:05Z","abstract_excerpt":"We present UV luminosity functions (LFs) at 1500 Angstrom derived from the HST Early Release Science WFC3/UVIS data acquired over ~50 arcmin^2 of the GOODS-South field. The LFs are determined over the entire redshift range z=0.75-2.5 using two methods, similar to those used at higher redshifts for Lyman Break Galaxies (LBGs): (1) 13-band UV+optical+NIR photometric redshifts to study galaxies in the range z=0.5-2 in three bins of dz=0.5, and (2) dropout samples in three redshift windows centered at z~1.5, z~1.9, and z~2.5. The characteristic luminosity dims by ~1.5 mag from z=2.5 to z=0.75, con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1661","kind":"arxiv","version":2},"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":"1005.1661","created_at":"2026-05-18T04:34:27.539854+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.1661v2","created_at":"2026-05-18T04:34:27.539854+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.1661","created_at":"2026-05-18T04:34:27.539854+00:00"},{"alias_kind":"pith_short_12","alias_value":"BP5QUJ7PYGLM","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BP5QUJ7PYGLM7QCV","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BP5QUJ7P","created_at":"2026-05-18T12:26:05.355336+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/BP5QUJ7PYGLM7QCVTN5CBH7L4I","json":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I.json","graph_json":"https://pith.science/api/pith-number/BP5QUJ7PYGLM7QCVTN5CBH7L4I/graph.json","events_json":"https://pith.science/api/pith-number/BP5QUJ7PYGLM7QCVTN5CBH7L4I/events.json","paper":"https://pith.science/paper/BP5QUJ7P"},"agent_actions":{"view_html":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I","download_json":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I.json","view_paper":"https://pith.science/paper/BP5QUJ7P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.1661&json=true","fetch_graph":"https://pith.science/api/pith-number/BP5QUJ7PYGLM7QCVTN5CBH7L4I/graph.json","fetch_events":"https://pith.science/api/pith-number/BP5QUJ7PYGLM7QCVTN5CBH7L4I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I/action/storage_attestation","attest_author":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I/action/author_attestation","sign_citation":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I/action/citation_signature","submit_replication":"https://pith.science/pith/BP5QUJ7PYGLM7QCVTN5CBH7L4I/action/replication_record"}},"created_at":"2026-05-18T04:34:27.539854+00:00","updated_at":"2026-05-18T04:34:27.539854+00:00"}