{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JJRPS2M36QFAOMSSKWF7CERJII","short_pith_number":"pith:JJRPS2M3","schema_version":"1.0","canonical_sha256":"4a62f9699bf40a073252558bf11229420af9d66979eebb26a5c12300e9869243","source":{"kind":"arxiv","id":"1503.08647","version":1},"attestation_state":"computed","paper":{"title":"Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Edo van Uitert, Henk Hoekstra, Marcello Cacciato, Ricardo Herbonnet","submitted_at":"2015-03-30T11:43:26Z","abstract_excerpt":"We study the evolution of the luminosity-to-halo mass relation of Luminous Red Galaxies (LRGs). We select a sample of 52 000 LOWZ and CMASS LRGs from the Baryon Oscillation Spectroscopic Survey (BOSS) SDSS-DR10 in the ~450 deg^2 that overlaps with imaging data from the second Red-sequence Cluster Survey (RCS2), group them into bins of absolute magnitude and redshift and measure their weak lensing signals. The source redshift distribution has a median of 0.7, which allows us to study the lensing signal as a function of lens redshift. We interpret the lensing signal using a halo model, from whic"},"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":"1503.08647","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-03-30T11:43:26Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"1521ec732d6193ae6299e64233ae21b7058848a67299f21f11862d1e8dc4d324","abstract_canon_sha256":"84b351dda7b5233d7a3539efb297f1a954ed0b117657c0b010dd861143c786fc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:58.591489Z","signature_b64":"woF2tEnTUmH3Zt8qQcmj9rR7d87U3wPkIbdWzaVfMGBkcRfpT0zw1mIQ/fIk1WM1V/a03g7eNV7xCU3cHIfuDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a62f9699bf40a073252558bf11229420af9d66979eebb26a5c12300e9869243","last_reissued_at":"2026-05-18T01:40:58.590787Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:58.590787Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Edo van Uitert, Henk Hoekstra, Marcello Cacciato, Ricardo Herbonnet","submitted_at":"2015-03-30T11:43:26Z","abstract_excerpt":"We study the evolution of the luminosity-to-halo mass relation of Luminous Red Galaxies (LRGs). We select a sample of 52 000 LOWZ and CMASS LRGs from the Baryon Oscillation Spectroscopic Survey (BOSS) SDSS-DR10 in the ~450 deg^2 that overlaps with imaging data from the second Red-sequence Cluster Survey (RCS2), group them into bins of absolute magnitude and redshift and measure their weak lensing signals. The source redshift distribution has a median of 0.7, which allows us to study the lensing signal as a function of lens redshift. We interpret the lensing signal using a halo model, from whic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.08647","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":"1503.08647","created_at":"2026-05-18T01:40:58.590896+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.08647v1","created_at":"2026-05-18T01:40:58.590896+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.08647","created_at":"2026-05-18T01:40:58.590896+00:00"},{"alias_kind":"pith_short_12","alias_value":"JJRPS2M36QFA","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JJRPS2M36QFAOMSS","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JJRPS2M3","created_at":"2026-05-18T12:29:27.538025+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/JJRPS2M36QFAOMSSKWF7CERJII","json":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII.json","graph_json":"https://pith.science/api/pith-number/JJRPS2M36QFAOMSSKWF7CERJII/graph.json","events_json":"https://pith.science/api/pith-number/JJRPS2M36QFAOMSSKWF7CERJII/events.json","paper":"https://pith.science/paper/JJRPS2M3"},"agent_actions":{"view_html":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII","download_json":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII.json","view_paper":"https://pith.science/paper/JJRPS2M3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.08647&json=true","fetch_graph":"https://pith.science/api/pith-number/JJRPS2M36QFAOMSSKWF7CERJII/graph.json","fetch_events":"https://pith.science/api/pith-number/JJRPS2M36QFAOMSSKWF7CERJII/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII/action/storage_attestation","attest_author":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII/action/author_attestation","sign_citation":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII/action/citation_signature","submit_replication":"https://pith.science/pith/JJRPS2M36QFAOMSSKWF7CERJII/action/replication_record"}},"created_at":"2026-05-18T01:40:58.590896+00:00","updated_at":"2026-05-18T01:40:58.590896+00:00"}