{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:SDJ4KRTNXWVH7MFLFPFKYU4IBQ","short_pith_number":"pith:SDJ4KRTN","schema_version":"1.0","canonical_sha256":"90d3c5466dbdaa7fb0ab2bcaac53880c19a8ee013afc0092ac8da25c12fc19b4","source":{"kind":"arxiv","id":"astro-ph/0503584","version":1},"attestation_state":"computed","paper":{"title":"Effects of Gravitational Evolution, Biasing, and Redshift Space Distortion on Topology","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Changbom Park, J. Richard Gott III, Juhan Kim","submitted_at":"2005-03-28T03:53:13Z","abstract_excerpt":"We have studied the dependence of topology of large scale structure on tracer, gravitational evolution, redshift space distortion, and cosmology. A series of large N-body simulations of the $\\Lambda$CDM and SCDM models that have evolved 1.1 or 8.6 billion particles, are used in the study. Evolution of the genus statistic, used as a topology measure, from redshift 8 to 0 is accurately calculated over a wide range of smoothing scales using the simulations. The tracers of large scale structure considered are the CDM matter, biased peaks in the initial density field, dark halos, and `galaxies' pop"},"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":"astro-ph/0503584","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-03-28T03:53:13Z","cross_cats_sorted":[],"title_canon_sha256":"9baf98ab706adf84606630002b7ff9742fe19899958e578a1646edee95474503","abstract_canon_sha256":"60ec1c11f3a0d56d11b0ac0ef2e8f8ca156239f0e550b2f69862736fe0b28512"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:51:05.006760Z","signature_b64":"dkigC86X0YH/qK8SvcpYdWK0ZvdeK4TBzrQquZxs7MgVCFwVR6clO06sXBCEvLFrBCqXUJJBysClVsKfSitLAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"90d3c5466dbdaa7fb0ab2bcaac53880c19a8ee013afc0092ac8da25c12fc19b4","last_reissued_at":"2026-07-04T16:51:05.006347Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:51:05.006347Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Effects of Gravitational Evolution, Biasing, and Redshift Space Distortion on Topology","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Changbom Park, J. Richard Gott III, Juhan Kim","submitted_at":"2005-03-28T03:53:13Z","abstract_excerpt":"We have studied the dependence of topology of large scale structure on tracer, gravitational evolution, redshift space distortion, and cosmology. A series of large N-body simulations of the $\\Lambda$CDM and SCDM models that have evolved 1.1 or 8.6 billion particles, are used in the study. Evolution of the genus statistic, used as a topology measure, from redshift 8 to 0 is accurately calculated over a wide range of smoothing scales using the simulations. The tracers of large scale structure considered are the CDM matter, biased peaks in the initial density field, dark halos, and `galaxies' pop"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0503584","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/astro-ph/0503584/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":"astro-ph/0503584","created_at":"2026-07-04T16:51:05.006411+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0503584v1","created_at":"2026-07-04T16:51:05.006411+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0503584","created_at":"2026-07-04T16:51:05.006411+00:00"},{"alias_kind":"pith_short_12","alias_value":"SDJ4KRTNXWVH","created_at":"2026-07-04T16:51:05.006411+00:00"},{"alias_kind":"pith_short_16","alias_value":"SDJ4KRTNXWVH7MFL","created_at":"2026-07-04T16:51:05.006411+00:00"},{"alias_kind":"pith_short_8","alias_value":"SDJ4KRTN","created_at":"2026-07-04T16:51:05.006411+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.01698","citing_title":"Cosmological constraints from the Minkowski functionals of the BOSS CMASS galaxy sample","ref_index":123,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ","json":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ.json","graph_json":"https://pith.science/api/pith-number/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/graph.json","events_json":"https://pith.science/api/pith-number/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/events.json","paper":"https://pith.science/paper/SDJ4KRTN"},"agent_actions":{"view_html":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ","download_json":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ.json","view_paper":"https://pith.science/paper/SDJ4KRTN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0503584&json=true","fetch_graph":"https://pith.science/api/pith-number/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/graph.json","fetch_events":"https://pith.science/api/pith-number/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/action/storage_attestation","attest_author":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/action/author_attestation","sign_citation":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/action/citation_signature","submit_replication":"https://pith.science/pith/SDJ4KRTNXWVH7MFLFPFKYU4IBQ/action/replication_record"}},"created_at":"2026-07-04T16:51:05.006411+00:00","updated_at":"2026-07-04T16:51:05.006411+00:00"}