{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:NOM7KAR5CY3HPGGCRCKFIO6TQZ","short_pith_number":"pith:NOM7KAR5","schema_version":"1.0","canonical_sha256":"6b99f5023d16367798c28894543bd3864caafc5d20497606b71df54766c33c0e","source":{"kind":"arxiv","id":"1709.00834","version":1},"attestation_state":"computed","paper":{"title":"How does the cosmic web impact assembly bias?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"C. Cadiou, C. Pichon, K. Kraljic, M. Musso, S. Codis, Y. Dubois","submitted_at":"2017-09-04T06:34:13Z","abstract_excerpt":"The mass, accretion rate and formation time of dark matter haloes near proto-filaments (identified as saddle points of the potential) are analytically predicted using a conditional version of the excursion set approach in its so-called \"upcrossing\" approximation. The model predicts that at fixed mass, mass accretion rate and formation time vary with orientation and distance from the saddle, demonstrating that assembly bias is indeed influenced by the tides imposed by the cosmic web. Starved, early forming haloes of smaller mass lie preferentially along the main axis of filaments, while more ma"},"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":"1709.00834","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-09-04T06:34:13Z","cross_cats_sorted":[],"title_canon_sha256":"b857e461157dc0b886e9a1bdfebc352eb914ed1baecf6fb2a4d88a469f63d9c5","abstract_canon_sha256":"b244d4497790c7eb55c475cc1ad1ffc222465ef4e892d2556641f4fc2038504e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:26:11.191204Z","signature_b64":"p0FBRjPeSRgQMXhN0IJte31Boiq9Ph8NrIOKYt38uNyBbVeympu2qNmCNZ8F2N/W6/SC+KDSbXNf7c4s+z+zCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6b99f5023d16367798c28894543bd3864caafc5d20497606b71df54766c33c0e","last_reissued_at":"2026-07-05T03:26:11.190751Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:26:11.190751Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How does the cosmic web impact assembly bias?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"C. Cadiou, C. Pichon, K. Kraljic, M. Musso, S. Codis, Y. Dubois","submitted_at":"2017-09-04T06:34:13Z","abstract_excerpt":"The mass, accretion rate and formation time of dark matter haloes near proto-filaments (identified as saddle points of the potential) are analytically predicted using a conditional version of the excursion set approach in its so-called \"upcrossing\" approximation. The model predicts that at fixed mass, mass accretion rate and formation time vary with orientation and distance from the saddle, demonstrating that assembly bias is indeed influenced by the tides imposed by the cosmic web. Starved, early forming haloes of smaller mass lie preferentially along the main axis of filaments, while more ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.00834","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1709.00834/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"1709.00834","created_at":"2026-07-05T03:26:11.190808+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.00834v1","created_at":"2026-07-05T03:26:11.190808+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.00834","created_at":"2026-07-05T03:26:11.190808+00:00"},{"alias_kind":"pith_short_12","alias_value":"NOM7KAR5CY3H","created_at":"2026-07-05T03:26:11.190808+00:00"},{"alias_kind":"pith_short_16","alias_value":"NOM7KAR5CY3HPGGC","created_at":"2026-07-05T03:26:11.190808+00:00"},{"alias_kind":"pith_short_8","alias_value":"NOM7KAR5","created_at":"2026-07-05T03:26:11.190808+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/NOM7KAR5CY3HPGGCRCKFIO6TQZ","json":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ.json","graph_json":"https://pith.science/api/pith-number/NOM7KAR5CY3HPGGCRCKFIO6TQZ/graph.json","events_json":"https://pith.science/api/pith-number/NOM7KAR5CY3HPGGCRCKFIO6TQZ/events.json","paper":"https://pith.science/paper/NOM7KAR5"},"agent_actions":{"view_html":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ","download_json":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ.json","view_paper":"https://pith.science/paper/NOM7KAR5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.00834&json=true","fetch_graph":"https://pith.science/api/pith-number/NOM7KAR5CY3HPGGCRCKFIO6TQZ/graph.json","fetch_events":"https://pith.science/api/pith-number/NOM7KAR5CY3HPGGCRCKFIO6TQZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ/action/storage_attestation","attest_author":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ/action/author_attestation","sign_citation":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ/action/citation_signature","submit_replication":"https://pith.science/pith/NOM7KAR5CY3HPGGCRCKFIO6TQZ/action/replication_record"}},"created_at":"2026-07-05T03:26:11.190808+00:00","updated_at":"2026-07-05T03:26:11.190808+00:00"}