{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:6O3WNMYWB4EYKX7NSFS46PGMLK","short_pith_number":"pith:6O3WNMYW","schema_version":"1.0","canonical_sha256":"f3b766b3160f09855fed9165cf3ccc5aab41cbeb0b6cf01afef6d74aab385c51","source":{"kind":"arxiv","id":"1412.2137","version":2},"attestation_state":"computed","paper":{"title":"Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z~1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Adam Muzzin, Crist\\'obal Sif\\'on, Henk Hoekstra, Michael L. Balogh, Remco F.J. van der Burg, Sean L. McGee","submitted_at":"2014-12-05T21:00:10Z","abstract_excerpt":"We study the radial number density and stellar mass density distributions of satellite galaxies in a sample of 60 massive clusters at 0.04<z<0.26 selected from the Multi-Epoch Nearby Cluster Survey (MENeaCS) and the Canadian Cluster Comparison Project (CCCP). In addition to ~10,000 spectroscopically confirmed member galaxies, we use deep ugri-band imaging to estimate photometric redshifts and stellar masses, and then statistically subtract fore-, and background sources using data from the COSMOS survey. We measure the galaxy number density and stellar mass density distributions in logarithmica"},"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":"1412.2137","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-12-05T21:00:10Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"7d4d7d941a335f6d594d71b84c8c31aab873b60a76c39767a6a2df6346df097a","abstract_canon_sha256":"8f115a3833bf0863a865cb2e6809419c7f976785da72b7e5986a834fbfcb791c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:17:42.734745Z","signature_b64":"ynxyXwKm3nSWOtwF7COWC3L2kSQFMh0ea9oLl9gZxvsQ1XxP5tviQtihqNQFi7ZLgzcngM2VkU5GZU5/lR2CDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f3b766b3160f09855fed9165cf3ccc5aab41cbeb0b6cf01afef6d74aab385c51","last_reissued_at":"2026-05-18T02:17:42.734303Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:17:42.734303Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z~1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Adam Muzzin, Crist\\'obal Sif\\'on, Henk Hoekstra, Michael L. Balogh, Remco F.J. van der Burg, Sean L. McGee","submitted_at":"2014-12-05T21:00:10Z","abstract_excerpt":"We study the radial number density and stellar mass density distributions of satellite galaxies in a sample of 60 massive clusters at 0.04<z<0.26 selected from the Multi-Epoch Nearby Cluster Survey (MENeaCS) and the Canadian Cluster Comparison Project (CCCP). In addition to ~10,000 spectroscopically confirmed member galaxies, we use deep ugri-band imaging to estimate photometric redshifts and stellar masses, and then statistically subtract fore-, and background sources using data from the COSMOS survey. We measure the galaxy number density and stellar mass density distributions in logarithmica"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.2137","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":"1412.2137","created_at":"2026-05-18T02:17:42.734380+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.2137v2","created_at":"2026-05-18T02:17:42.734380+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.2137","created_at":"2026-05-18T02:17:42.734380+00:00"},{"alias_kind":"pith_short_12","alias_value":"6O3WNMYWB4EY","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_16","alias_value":"6O3WNMYWB4EYKX7N","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_8","alias_value":"6O3WNMYW","created_at":"2026-05-18T12:28:16.859392+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/6O3WNMYWB4EYKX7NSFS46PGMLK","json":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK.json","graph_json":"https://pith.science/api/pith-number/6O3WNMYWB4EYKX7NSFS46PGMLK/graph.json","events_json":"https://pith.science/api/pith-number/6O3WNMYWB4EYKX7NSFS46PGMLK/events.json","paper":"https://pith.science/paper/6O3WNMYW"},"agent_actions":{"view_html":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK","download_json":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK.json","view_paper":"https://pith.science/paper/6O3WNMYW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.2137&json=true","fetch_graph":"https://pith.science/api/pith-number/6O3WNMYWB4EYKX7NSFS46PGMLK/graph.json","fetch_events":"https://pith.science/api/pith-number/6O3WNMYWB4EYKX7NSFS46PGMLK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK/action/storage_attestation","attest_author":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK/action/author_attestation","sign_citation":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK/action/citation_signature","submit_replication":"https://pith.science/pith/6O3WNMYWB4EYKX7NSFS46PGMLK/action/replication_record"}},"created_at":"2026-05-18T02:17:42.734380+00:00","updated_at":"2026-05-18T02:17:42.734380+00:00"}