{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:LU6HSGMPTDGZX6ALSQKL5KOXWI","short_pith_number":"pith:LU6HSGMP","schema_version":"1.0","canonical_sha256":"5d3c79198f98cd9bf80b9414bea9d7b205bda1119448c8c963d42c78dd0345e9","source":{"kind":"arxiv","id":"2411.18722","version":2},"attestation_state":"computed","paper":{"title":"On the universality of the halo mass function beyond ${\\Lambda}$CDM cosmology","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Robert E. Smith, Yuhao Li","submitted_at":"2024-11-27T19:52:14Z","abstract_excerpt":"Theoretical frameworks based on Press-Schechter formalism and excursion set arguments suggest that the abundance of dark matter haloes exhibits universal behaviour when expressed in terms of peak height. If true, this implies that a single high-accuracy cosmological simulation could serve as a basis for constructing an emulator applicable to any other cosmology of interest. This tantalising possibility has inspired numerous studies over the years. However, in practice, different ways of defining haloes have led to mixed results concerning this issue. In this work, we utilise a suite of high-re"},"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":"2411.18722","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-11-27T19:52:14Z","cross_cats_sorted":[],"title_canon_sha256":"d163526b9e64b3d6a1e4ce7fef624badc0db76e26b2f253fa22e8056a559f9c7","abstract_canon_sha256":"e356e4df619b46f8dd59cfde4766f08b438b4b196beca13436726063d98be960"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:29:52.411619Z","signature_b64":"JppwuYrwDfiuohbm3QCneKgRONLRU+cGdnbWHq9Q9LPEWGk+geFrY+7kHpuu+j8UpCYgw30PUOJE1SVYqXBbCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d3c79198f98cd9bf80b9414bea9d7b205bda1119448c8c963d42c78dd0345e9","last_reissued_at":"2026-07-05T11:29:52.411146Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:29:52.411146Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the universality of the halo mass function beyond ${\\Lambda}$CDM cosmology","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Robert E. Smith, Yuhao Li","submitted_at":"2024-11-27T19:52:14Z","abstract_excerpt":"Theoretical frameworks based on Press-Schechter formalism and excursion set arguments suggest that the abundance of dark matter haloes exhibits universal behaviour when expressed in terms of peak height. If true, this implies that a single high-accuracy cosmological simulation could serve as a basis for constructing an emulator applicable to any other cosmology of interest. This tantalising possibility has inspired numerous studies over the years. However, in practice, different ways of defining haloes have led to mixed results concerning this issue. In this work, we utilise a suite of high-re"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.18722","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.18722/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":"2411.18722","created_at":"2026-07-05T11:29:52.411201+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.18722v2","created_at":"2026-07-05T11:29:52.411201+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.18722","created_at":"2026-07-05T11:29:52.411201+00:00"},{"alias_kind":"pith_short_12","alias_value":"LU6HSGMPTDGZ","created_at":"2026-07-05T11:29:52.411201+00:00"},{"alias_kind":"pith_short_16","alias_value":"LU6HSGMPTDGZX6AL","created_at":"2026-07-05T11:29:52.411201+00:00"},{"alias_kind":"pith_short_8","alias_value":"LU6HSGMP","created_at":"2026-07-05T11:29:52.411201+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26237","citing_title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17660","citing_title":"Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23236","citing_title":"The functional form of galaxy and halo luminosity and mass functions","ref_index":45,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI","json":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI.json","graph_json":"https://pith.science/api/pith-number/LU6HSGMPTDGZX6ALSQKL5KOXWI/graph.json","events_json":"https://pith.science/api/pith-number/LU6HSGMPTDGZX6ALSQKL5KOXWI/events.json","paper":"https://pith.science/paper/LU6HSGMP"},"agent_actions":{"view_html":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI","download_json":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI.json","view_paper":"https://pith.science/paper/LU6HSGMP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.18722&json=true","fetch_graph":"https://pith.science/api/pith-number/LU6HSGMPTDGZX6ALSQKL5KOXWI/graph.json","fetch_events":"https://pith.science/api/pith-number/LU6HSGMPTDGZX6ALSQKL5KOXWI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI/action/storage_attestation","attest_author":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI/action/author_attestation","sign_citation":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI/action/citation_signature","submit_replication":"https://pith.science/pith/LU6HSGMPTDGZX6ALSQKL5KOXWI/action/replication_record"}},"created_at":"2026-07-05T11:29:52.411201+00:00","updated_at":"2026-07-05T11:29:52.411201+00:00"}