{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:WGL6P3UERNUHE7A6H57AEJRM4W","short_pith_number":"pith:WGL6P3UE","schema_version":"1.0","canonical_sha256":"b197e7ee848b68727c1e3f7e02262ce5923d46125a6a0b06a6748c11e4532775","source":{"kind":"arxiv","id":"1512.03625","version":1},"attestation_state":"computed","paper":{"title":"RCSLenS: A new estimator for large-scale galaxy-matter correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Buddendiek, A. Choi, C. Blake, C. Heymans, H. Hildebrandt, J. Harnois-Deraps, L. Koens, L. van Waerbeke, M. Viola, P. Schneider, R. Nakajima, T. Erben","submitted_at":"2015-12-11T12:49:01Z","abstract_excerpt":"We present measurements of the galaxy bias $b$ and the galaxy-matter cross-correlation coefficient $r$ for the BOSS LOWZ luminous red galaxy sample. Using a new statistical weak lensing analysis of the Red Sequence Cluster Lensing Survey (RCSLenS) we find the bias properties of this sample to be higher than previously reported with $b=2.45^{+0.05}_{-0.05}$ and $r=1.64^{+0.17}_{-0.16}$ on scales between $3'$ and $20'$. We repeat the measurement for angular scales of $20'\\leq \\vartheta \\leq70'$, which yields $b=2.39^{+0.07}_{-0.07}$ and $r=1.24^{+0.26}_{-0.25}$. This is the first application of "},"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":"1512.03625","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-12-11T12:49:01Z","cross_cats_sorted":[],"title_canon_sha256":"e84e92a6a458fbc66a8c9f11419f3478fd429eeb48e3da1f5782e352f9c1745c","abstract_canon_sha256":"33a1b3147464e716b02348db3c569743a4ef22ef7e3d9e9e896cf1b11aa4a41a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:22:32.411268Z","signature_b64":"11tdEjdu4Q1pWwNU9UAmERejblmCJyt1Y25v+9McXaPjz/1N+W2o7eEBdFoZxquJbGr1Xq4DxjJJXpmR6sO8Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b197e7ee848b68727c1e3f7e02262ce5923d46125a6a0b06a6748c11e4532775","last_reissued_at":"2026-05-18T01:22:32.410842Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:22:32.410842Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"RCSLenS: A new estimator for large-scale galaxy-matter correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Buddendiek, A. Choi, C. Blake, C. Heymans, H. Hildebrandt, J. Harnois-Deraps, L. Koens, L. van Waerbeke, M. Viola, P. Schneider, R. Nakajima, T. Erben","submitted_at":"2015-12-11T12:49:01Z","abstract_excerpt":"We present measurements of the galaxy bias $b$ and the galaxy-matter cross-correlation coefficient $r$ for the BOSS LOWZ luminous red galaxy sample. Using a new statistical weak lensing analysis of the Red Sequence Cluster Lensing Survey (RCSLenS) we find the bias properties of this sample to be higher than previously reported with $b=2.45^{+0.05}_{-0.05}$ and $r=1.64^{+0.17}_{-0.16}$ on scales between $3'$ and $20'$. We repeat the measurement for angular scales of $20'\\leq \\vartheta \\leq70'$, which yields $b=2.39^{+0.07}_{-0.07}$ and $r=1.24^{+0.26}_{-0.25}$. This is the first application of "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.03625","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":"1512.03625","created_at":"2026-05-18T01:22:32.410904+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.03625v1","created_at":"2026-05-18T01:22:32.410904+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.03625","created_at":"2026-05-18T01:22:32.410904+00:00"},{"alias_kind":"pith_short_12","alias_value":"WGL6P3UERNUH","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"WGL6P3UERNUHE7A6","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"WGL6P3UE","created_at":"2026-05-18T12:29:47.479230+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/WGL6P3UERNUHE7A6H57AEJRM4W","json":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W.json","graph_json":"https://pith.science/api/pith-number/WGL6P3UERNUHE7A6H57AEJRM4W/graph.json","events_json":"https://pith.science/api/pith-number/WGL6P3UERNUHE7A6H57AEJRM4W/events.json","paper":"https://pith.science/paper/WGL6P3UE"},"agent_actions":{"view_html":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W","download_json":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W.json","view_paper":"https://pith.science/paper/WGL6P3UE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.03625&json=true","fetch_graph":"https://pith.science/api/pith-number/WGL6P3UERNUHE7A6H57AEJRM4W/graph.json","fetch_events":"https://pith.science/api/pith-number/WGL6P3UERNUHE7A6H57AEJRM4W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W/action/storage_attestation","attest_author":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W/action/author_attestation","sign_citation":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W/action/citation_signature","submit_replication":"https://pith.science/pith/WGL6P3UERNUHE7A6H57AEJRM4W/action/replication_record"}},"created_at":"2026-05-18T01:22:32.410904+00:00","updated_at":"2026-05-18T01:22:32.410904+00:00"}