{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:FFK3NPVBXOLZE26LMV6DMNV4CP","short_pith_number":"pith:FFK3NPVB","schema_version":"1.0","canonical_sha256":"2955b6bea1bb97926bcb657c3636bc13f2618dcccd977989bdf57ade18bbea94","source":{"kind":"arxiv","id":"2411.14154","version":1},"attestation_state":"computed","paper":{"title":"Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Hengyu Wu, Jieci Wang, Shengjia Wang, Tonghua Liu","submitted_at":"2024-11-21T14:18:26Z","abstract_excerpt":"We present an improved model-independent method for determining the cosmic curvature using the observations of Baryon Acoustic Oscillations (BAOs) and the Hubble parameter. The purpose of this work is to provide insights into late-universe curvature measurements using available observational data and techniques. Thus, we use two sources of BAO data sets, BOSS/eBOSS and latest DESI DR1, and two reconstruction methods, Gaussian process (GP) and artificial neural network (ANN). It is important to highlight that our method circumvents influence induced by the sound horizon in BAO observations and "},"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":"2411.14154","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-11-21T14:18:26Z","cross_cats_sorted":[],"title_canon_sha256":"2ba8f274a158e03edb7e2ef30a2396aa304614916e7ff48ce5b5e4debd478c17","abstract_canon_sha256":"405cbb43a948926004e75c3d1b5ec027db786e25558233c253ad622512875fe3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:24:27.923899Z","signature_b64":"3ILO4YL9uoSBmd6+0hlcKChO1BeJTuORYn61FfRZ5P8RCKdYcFAmJ2LC2+OeE8hrbaA1t7VknvqA3/y6fqi4AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2955b6bea1bb97926bcb657c3636bc13f2618dcccd977989bdf57ade18bbea94","last_reissued_at":"2026-07-05T10:24:27.923201Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:24:27.923201Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Hengyu Wu, Jieci Wang, Shengjia Wang, Tonghua Liu","submitted_at":"2024-11-21T14:18:26Z","abstract_excerpt":"We present an improved model-independent method for determining the cosmic curvature using the observations of Baryon Acoustic Oscillations (BAOs) and the Hubble parameter. The purpose of this work is to provide insights into late-universe curvature measurements using available observational data and techniques. Thus, we use two sources of BAO data sets, BOSS/eBOSS and latest DESI DR1, and two reconstruction methods, Gaussian process (GP) and artificial neural network (ANN). It is important to highlight that our method circumvents influence induced by the sound horizon in BAO observations and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.14154","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/2411.14154/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":"2411.14154","created_at":"2026-07-05T10:24:27.923275+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.14154v1","created_at":"2026-07-05T10:24:27.923275+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.14154","created_at":"2026-07-05T10:24:27.923275+00:00"},{"alias_kind":"pith_short_12","alias_value":"FFK3NPVBXOLZ","created_at":"2026-07-05T10:24:27.923275+00:00"},{"alias_kind":"pith_short_16","alias_value":"FFK3NPVBXOLZE26L","created_at":"2026-07-05T10:24:27.923275+00:00"},{"alias_kind":"pith_short_8","alias_value":"FFK3NPVB","created_at":"2026-07-05T10:24:27.923275+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2603.21125","citing_title":"Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23492","citing_title":"The open-Universe signal: A model artifact rather than genuine curvature","ref_index":22,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP","json":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP.json","graph_json":"https://pith.science/api/pith-number/FFK3NPVBXOLZE26LMV6DMNV4CP/graph.json","events_json":"https://pith.science/api/pith-number/FFK3NPVBXOLZE26LMV6DMNV4CP/events.json","paper":"https://pith.science/paper/FFK3NPVB"},"agent_actions":{"view_html":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP","download_json":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP.json","view_paper":"https://pith.science/paper/FFK3NPVB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.14154&json=true","fetch_graph":"https://pith.science/api/pith-number/FFK3NPVBXOLZE26LMV6DMNV4CP/graph.json","fetch_events":"https://pith.science/api/pith-number/FFK3NPVBXOLZE26LMV6DMNV4CP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP/action/storage_attestation","attest_author":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP/action/author_attestation","sign_citation":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP/action/citation_signature","submit_replication":"https://pith.science/pith/FFK3NPVBXOLZE26LMV6DMNV4CP/action/replication_record"}},"created_at":"2026-07-05T10:24:27.923275+00:00","updated_at":"2026-07-05T10:24:27.923275+00:00"}