{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LNTUP4TKSMGWLHAFTE4FBJ2CZT","short_pith_number":"pith:LNTUP4TK","schema_version":"1.0","canonical_sha256":"5b6747f26a930d659c05993850a742ccd2f7c7e3ff18c757adf26405981e7f92","source":{"kind":"arxiv","id":"1703.02049","version":2},"attestation_state":"computed","paper":{"title":"The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Durkalec, A. Koekemoer, A. Pollo, B.C. Lemaux, B. Garilli, E. Zucca, G. Zamorani, J. Pforr, N. Hathi, O. Le F\\'evre, S. Bardelli","submitted_at":"2017-03-06T19:00:03Z","abstract_excerpt":"We present the study of the dependence of galaxy clustering on luminosity and stellar mass in the redshift range 2$<$z$<$3.5 using 3236 galaxies with robust spectroscopic redshifts from the VIMOS Ultra Deep Survey (VUDS). We measure the two-point real-space correlation function $w_p(r_p)$ for four volume-limited stellar mass and four luminosity, M$_{UV}$ absolute magnitude selected, sub-samples. We find that the scale dependent clustering amplitude $r_0$ significantly increases with increasing luminosity and stellar mass indicating a strong galaxy clustering dependence on these properties. Thi"},"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":"1703.02049","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-03-06T19:00:03Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"2f38c5ece2f6735f3ca6a6867c966c50ef010ffa54f18c197106a74ea15945fd","abstract_canon_sha256":"867c3a22adb4f31b6aba146a3371ac8021fd05382ce4a9bfea2b45e51f60a861"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:17:43.944236Z","signature_b64":"cqxpuTLcU7PuF5i2PpO2C/V7r5FAnjVZT19Vm+51BCAYSifrJVGXe2fOGhFsuK8zlK7x11+1cEPpo4nOHPmpBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b6747f26a930d659c05993850a742ccd2f7c7e3ff18c757adf26405981e7f92","last_reissued_at":"2026-05-18T00:17:43.943692Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:17:43.943692Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Durkalec, A. Koekemoer, A. Pollo, B.C. Lemaux, B. Garilli, E. Zucca, G. Zamorani, J. Pforr, N. Hathi, O. Le F\\'evre, S. Bardelli","submitted_at":"2017-03-06T19:00:03Z","abstract_excerpt":"We present the study of the dependence of galaxy clustering on luminosity and stellar mass in the redshift range 2$<$z$<$3.5 using 3236 galaxies with robust spectroscopic redshifts from the VIMOS Ultra Deep Survey (VUDS). We measure the two-point real-space correlation function $w_p(r_p)$ for four volume-limited stellar mass and four luminosity, M$_{UV}$ absolute magnitude selected, sub-samples. We find that the scale dependent clustering amplitude $r_0$ significantly increases with increasing luminosity and stellar mass indicating a strong galaxy clustering dependence on these properties. Thi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.02049","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":"1703.02049","created_at":"2026-05-18T00:17:43.943756+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.02049v2","created_at":"2026-05-18T00:17:43.943756+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.02049","created_at":"2026-05-18T00:17:43.943756+00:00"},{"alias_kind":"pith_short_12","alias_value":"LNTUP4TKSMGW","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LNTUP4TKSMGWLHAF","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LNTUP4TK","created_at":"2026-05-18T12:31:28.150371+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/LNTUP4TKSMGWLHAFTE4FBJ2CZT","json":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT.json","graph_json":"https://pith.science/api/pith-number/LNTUP4TKSMGWLHAFTE4FBJ2CZT/graph.json","events_json":"https://pith.science/api/pith-number/LNTUP4TKSMGWLHAFTE4FBJ2CZT/events.json","paper":"https://pith.science/paper/LNTUP4TK"},"agent_actions":{"view_html":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT","download_json":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT.json","view_paper":"https://pith.science/paper/LNTUP4TK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.02049&json=true","fetch_graph":"https://pith.science/api/pith-number/LNTUP4TKSMGWLHAFTE4FBJ2CZT/graph.json","fetch_events":"https://pith.science/api/pith-number/LNTUP4TKSMGWLHAFTE4FBJ2CZT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT/action/storage_attestation","attest_author":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT/action/author_attestation","sign_citation":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT/action/citation_signature","submit_replication":"https://pith.science/pith/LNTUP4TKSMGWLHAFTE4FBJ2CZT/action/replication_record"}},"created_at":"2026-05-18T00:17:43.943756+00:00","updated_at":"2026-05-18T00:17:43.943756+00:00"}