{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:WH7CLZK3FE566IWN7B3RBTOG4P","short_pith_number":"pith:WH7CLZK3","schema_version":"1.0","canonical_sha256":"b1fe25e55b293bef22cdf87710cdc6e3f77f5980d8c275f5302e2639fd7f1161","source":{"kind":"arxiv","id":"2512.20132","version":2},"attestation_state":"computed","paper":{"title":"Parity-odd Four-Point Correlation Function from DESI Data Release 1 Luminous Red Galaxy Sample","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"A. de la Macorra, A. Kremin, B. A. Weaver, C. Howlett, C. Lamman, D. Bianchi, D. Brooks, D. Schlegel, D. Sprayberry, E. Gazta\\~naga, E. Sanchez, F. Prada, G. Gutierrez, G. Niz, G. Rossi, G. Tarl\\'e, H.-J. Seo, H. Zou, I. P\\'erez-R\\`afols, J. Aguilar, J. E. Forero-Romero, J. Hou, J. Silber, L. Le Guillou, M. Ishak, M. Landriau, M. Schubnell, O. Lahav, P. Doel, R. Joyce, R. Miquel, R. N. Cahn, S. Ahlen, S. Nadathur, T. Claybaugh, W. J. Percival","submitted_at":"2025-12-23T07:50:23Z","abstract_excerpt":"The parity-odd four-point function provides a unique probe of fundamental symmetries and potential new physics in the large-scale structure of the Universe. We present measurements of the parity-odd four-point function using the DESI DR1 LRG sample and assess its detection significance. Our analysis considers both auto- and cross-correlations, using two complementary approaches to the covariance: (i) the full analytic covariance matrix applied to the uncompressed data vector, and (ii) a compressed data vector combined with a hybrid covariance matrix constructed from simulations and analytic es"},"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":"2512.20132","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-12-23T07:50:23Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"8187a76b13bd0560f788ee24822335a18bd9bd3483a504f3cf469c01087143ac","abstract_canon_sha256":"25df17ea62eefa5431dfb685ea8be9500f7019531f0832aebb32b0b33f2a708c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-09T01:05:12.074266Z","signature_b64":"1sP+WrKA0EeeVT0wJSCqExuR2T02S53YcTek97MpfQV0n7yoR9kOkNaGO1ZeudC5hclHd15mKvrcFWpyKCdYBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b1fe25e55b293bef22cdf87710cdc6e3f77f5980d8c275f5302e2639fd7f1161","last_reissued_at":"2026-06-09T01:05:12.073693Z","signature_status":"signed_v1","first_computed_at":"2026-06-09T01:05:12.073693Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Parity-odd Four-Point Correlation Function from DESI Data Release 1 Luminous Red Galaxy Sample","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"A. de la Macorra, A. Kremin, B. A. Weaver, C. Howlett, C. Lamman, D. Bianchi, D. Brooks, D. Schlegel, D. Sprayberry, E. Gazta\\~naga, E. Sanchez, F. Prada, G. Gutierrez, G. Niz, G. Rossi, G. Tarl\\'e, H.-J. Seo, H. Zou, I. P\\'erez-R\\`afols, J. Aguilar, J. E. Forero-Romero, J. Hou, J. Silber, L. Le Guillou, M. Ishak, M. Landriau, M. Schubnell, O. Lahav, P. Doel, R. Joyce, R. Miquel, R. N. Cahn, S. Ahlen, S. Nadathur, T. Claybaugh, W. J. Percival","submitted_at":"2025-12-23T07:50:23Z","abstract_excerpt":"The parity-odd four-point function provides a unique probe of fundamental symmetries and potential new physics in the large-scale structure of the Universe. We present measurements of the parity-odd four-point function using the DESI DR1 LRG sample and assess its detection significance. Our analysis considers both auto- and cross-correlations, using two complementary approaches to the covariance: (i) the full analytic covariance matrix applied to the uncompressed data vector, and (ii) a compressed data vector combined with a hybrid covariance matrix constructed from simulations and analytic es"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2512.20132","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/2512.20132/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":"2512.20132","created_at":"2026-06-09T01:05:12.073754+00:00"},{"alias_kind":"arxiv_version","alias_value":"2512.20132v2","created_at":"2026-06-09T01:05:12.073754+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2512.20132","created_at":"2026-06-09T01:05:12.073754+00:00"},{"alias_kind":"pith_short_12","alias_value":"WH7CLZK3FE56","created_at":"2026-06-09T01:05:12.073754+00:00"},{"alias_kind":"pith_short_16","alias_value":"WH7CLZK3FE566IWN","created_at":"2026-06-09T01:05:12.073754+00:00"},{"alias_kind":"pith_short_8","alias_value":"WH7CLZK3","created_at":"2026-06-09T01:05:12.073754+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.06021","citing_title":"Testing parity with composite-field spectra of BOSS and DESI luminous red galaxies","ref_index":46,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P","json":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P.json","graph_json":"https://pith.science/api/pith-number/WH7CLZK3FE566IWN7B3RBTOG4P/graph.json","events_json":"https://pith.science/api/pith-number/WH7CLZK3FE566IWN7B3RBTOG4P/events.json","paper":"https://pith.science/paper/WH7CLZK3"},"agent_actions":{"view_html":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P","download_json":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P.json","view_paper":"https://pith.science/paper/WH7CLZK3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2512.20132&json=true","fetch_graph":"https://pith.science/api/pith-number/WH7CLZK3FE566IWN7B3RBTOG4P/graph.json","fetch_events":"https://pith.science/api/pith-number/WH7CLZK3FE566IWN7B3RBTOG4P/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P/action/storage_attestation","attest_author":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P/action/author_attestation","sign_citation":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P/action/citation_signature","submit_replication":"https://pith.science/pith/WH7CLZK3FE566IWN7B3RBTOG4P/action/replication_record"}},"created_at":"2026-06-09T01:05:12.073754+00:00","updated_at":"2026-06-09T01:05:12.073754+00:00"}