{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:XG7A53CMBJMPJMNZ55MN7YMI4N","short_pith_number":"pith:XG7A53CM","schema_version":"1.0","canonical_sha256":"b9be0eec4c0a58f4b1b9ef58dfe188e3780244805784065f42bd6b595f8d1561","source":{"kind":"arxiv","id":"1407.5621","version":2},"attestation_state":"computed","paper":{"title":"The influence of the environmental history on quenching star formation in a $\\Lambda$CDM universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"\\'Alvaro Villalobos, Angela Iovino, Dave Wilman, Gabriella De Lucia, Michaela Hirschmann, Olga Cucciati, Simone Weinmann, Stefano Zibetti","submitted_at":"2014-07-21T20:00:03Z","abstract_excerpt":"We present a detailed analysis of the influence of the environment and of the environmental history on quenching star formation in central and satellite galaxies in the local Universe. We take advantage of publicly available galaxy catalogues obtained from applying a galaxy formation model to the Millennium simulation. In addition to halo mass, we consider the local density of galaxies within various fixed scales. Comparing our model predictions to observational data (SDSS), we demonstrate that the models are failing to reproduce the observed density dependence of the quiescent galaxy fraction"},"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":"1407.5621","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-21T20:00:03Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"69ed1291651fcafdc85dc0fdf933605e9ff00f9adc7512090e04cf3bd8eef263","abstract_canon_sha256":"c8f5facb8a7a9abe12cf4935e3d4640fb95375e2e8c075162d8560bd28819ea7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:33.446190Z","signature_b64":"mPAo1CgricBtPWTGr9nelqdq0g5cAaJ/349U0s2baPAxljLekidp56bN1hc7xOajtWmrCtaeSfISqf2AEJkPCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b9be0eec4c0a58f4b1b9ef58dfe188e3780244805784065f42bd6b595f8d1561","last_reissued_at":"2026-05-18T01:42:33.445708Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:33.445708Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The influence of the environmental history on quenching star formation in a $\\Lambda$CDM universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"\\'Alvaro Villalobos, Angela Iovino, Dave Wilman, Gabriella De Lucia, Michaela Hirschmann, Olga Cucciati, Simone Weinmann, Stefano Zibetti","submitted_at":"2014-07-21T20:00:03Z","abstract_excerpt":"We present a detailed analysis of the influence of the environment and of the environmental history on quenching star formation in central and satellite galaxies in the local Universe. We take advantage of publicly available galaxy catalogues obtained from applying a galaxy formation model to the Millennium simulation. In addition to halo mass, we consider the local density of galaxies within various fixed scales. Comparing our model predictions to observational data (SDSS), we demonstrate that the models are failing to reproduce the observed density dependence of the quiescent galaxy fraction"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.5621","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":"1407.5621","created_at":"2026-05-18T01:42:33.445786+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.5621v2","created_at":"2026-05-18T01:42:33.445786+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.5621","created_at":"2026-05-18T01:42:33.445786+00:00"},{"alias_kind":"pith_short_12","alias_value":"XG7A53CMBJMP","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"XG7A53CMBJMPJMNZ","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"XG7A53CM","created_at":"2026-05-18T12:28:57.508820+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/XG7A53CMBJMPJMNZ55MN7YMI4N","json":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N.json","graph_json":"https://pith.science/api/pith-number/XG7A53CMBJMPJMNZ55MN7YMI4N/graph.json","events_json":"https://pith.science/api/pith-number/XG7A53CMBJMPJMNZ55MN7YMI4N/events.json","paper":"https://pith.science/paper/XG7A53CM"},"agent_actions":{"view_html":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N","download_json":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N.json","view_paper":"https://pith.science/paper/XG7A53CM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.5621&json=true","fetch_graph":"https://pith.science/api/pith-number/XG7A53CMBJMPJMNZ55MN7YMI4N/graph.json","fetch_events":"https://pith.science/api/pith-number/XG7A53CMBJMPJMNZ55MN7YMI4N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N/action/storage_attestation","attest_author":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N/action/author_attestation","sign_citation":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N/action/citation_signature","submit_replication":"https://pith.science/pith/XG7A53CMBJMPJMNZ55MN7YMI4N/action/replication_record"}},"created_at":"2026-05-18T01:42:33.445786+00:00","updated_at":"2026-05-18T01:42:33.445786+00:00"}