{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:HW7VB6YRVQMCPB76KIW5ENQ57L","short_pith_number":"pith:HW7VB6YR","schema_version":"1.0","canonical_sha256":"3dbf50fb11ac182787fe522dd2361dfaefdfdfa04e341372b5e3ba5c888feb43","source":{"kind":"arxiv","id":"1405.4856","version":1},"attestation_state":"computed","paper":{"title":"Cookie-cutter halos: the remarkable constancy of the stellar mass function of satellite galaxies at 0.2<z<1.2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Danilo Marchesini, Mauro Stefanon, Ryan F. Quadri, Tomer Tal","submitted_at":"2014-05-19T20:00:00Z","abstract_excerpt":"We present an observational study of the stellar mass function of satellite galaxies around central galaxies at 0.2<z<1.2. Using statistical background subtraction of contaminating sources we derive satellite stellar mass distributions in four bins of central galaxy mass in three redshift ranges. Our results show that the stellar mass function of satellite galaxies increases with central galaxy mass, and that the distribution of satellite masses at fixed central mass is at most weakly dependent on redshift. We conclude that the average mass distribution of galaxies in groups is remarkably univ"},"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":"1405.4856","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-05-19T20:00:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"336bf09f7ca319d3a64c93698207054818d75cef832ad44e8d8ec59d292cbff3","abstract_canon_sha256":"e44330acbf162c0eaba4fc5d1c26010991ae020b49d4674cc805b6a067b60420"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:51:32.825831Z","signature_b64":"81TfECSZiN6I5v6NW/uykLOAJEwjttexpp9z2ZQdWrHzgBhf8YqclQ7XXFPMtJqCA9NDbTsKBJZSHoEx1NSaAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3dbf50fb11ac182787fe522dd2361dfaefdfdfa04e341372b5e3ba5c888feb43","last_reissued_at":"2026-05-18T02:51:32.825292Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:51:32.825292Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cookie-cutter halos: the remarkable constancy of the stellar mass function of satellite galaxies at 0.2<z<1.2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Danilo Marchesini, Mauro Stefanon, Ryan F. Quadri, Tomer Tal","submitted_at":"2014-05-19T20:00:00Z","abstract_excerpt":"We present an observational study of the stellar mass function of satellite galaxies around central galaxies at 0.2<z<1.2. Using statistical background subtraction of contaminating sources we derive satellite stellar mass distributions in four bins of central galaxy mass in three redshift ranges. Our results show that the stellar mass function of satellite galaxies increases with central galaxy mass, and that the distribution of satellite masses at fixed central mass is at most weakly dependent on redshift. We conclude that the average mass distribution of galaxies in groups is remarkably univ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.4856","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":"1405.4856","created_at":"2026-05-18T02:51:32.825389+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.4856v1","created_at":"2026-05-18T02:51:32.825389+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.4856","created_at":"2026-05-18T02:51:32.825389+00:00"},{"alias_kind":"pith_short_12","alias_value":"HW7VB6YRVQMC","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_16","alias_value":"HW7VB6YRVQMCPB76","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_8","alias_value":"HW7VB6YR","created_at":"2026-05-18T12:28:30.664211+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/HW7VB6YRVQMCPB76KIW5ENQ57L","json":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L.json","graph_json":"https://pith.science/api/pith-number/HW7VB6YRVQMCPB76KIW5ENQ57L/graph.json","events_json":"https://pith.science/api/pith-number/HW7VB6YRVQMCPB76KIW5ENQ57L/events.json","paper":"https://pith.science/paper/HW7VB6YR"},"agent_actions":{"view_html":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L","download_json":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L.json","view_paper":"https://pith.science/paper/HW7VB6YR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.4856&json=true","fetch_graph":"https://pith.science/api/pith-number/HW7VB6YRVQMCPB76KIW5ENQ57L/graph.json","fetch_events":"https://pith.science/api/pith-number/HW7VB6YRVQMCPB76KIW5ENQ57L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L/action/storage_attestation","attest_author":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L/action/author_attestation","sign_citation":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L/action/citation_signature","submit_replication":"https://pith.science/pith/HW7VB6YRVQMCPB76KIW5ENQ57L/action/replication_record"}},"created_at":"2026-05-18T02:51:32.825389+00:00","updated_at":"2026-05-18T02:51:32.825389+00:00"}