{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:REP2CSHG56JNXDTFKEJCLMWT3X","short_pith_number":"pith:REP2CSHG","schema_version":"1.0","canonical_sha256":"891fa148e6ef92db8e65511225b2d3ddfc2254a50e5282359f14a7ad7172bc4f","source":{"kind":"arxiv","id":"2306.11124","version":2},"attestation_state":"computed","paper":{"title":"KiDS-1000: Cosmology with improved cosmic shear measurements","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Angus H. Wright, Arun Kannawadi, Benjamin Giblin, Benjamin Joachimi, Catherine Heymans, Hendrik Hildebrandt, Henk Hoekstra, Huanyuan Shan, Jan Luca van den Busch, Konrad Kuijken, Lance Miller, Maciej Bilicki, Marika Asgari, Robert Reischke, Shun-Sheng Li","submitted_at":"2023-06-19T19:00:57Z","abstract_excerpt":"We present refined cosmological parameter constraints derived from a cosmic shear analysis of the fourth data release of the Kilo-Degree Survey (KiDS-1000). Our main improvements include enhanced galaxy shape measurements made possible by an updated version of the lensfit code and improved shear calibration achieved with a newly developed suite of multi-band image simulations. Additionally, we incorporated recent advancements in cosmological inference from the joint Dark Energy Survey Year 3 and KiDS-1000 cosmic shear analysis. Assuming a spatially flat standard cosmological model, we constrai"},"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":"2306.11124","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-06-19T19:00:57Z","cross_cats_sorted":[],"title_canon_sha256":"4268e0c02a7980a87bed40cbdba18dc41bbff15ca40d443390b33e1abb3744c0","abstract_canon_sha256":"c565fea43a077c28fe3d1b11d7e43699bdb738a6c94c8730f9c0dcc9c15aeb9f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:17:27.170410Z","signature_b64":"+YG9qv3WN9SV1QJE1ouW+DUdAu4E7PYBXQ+sGiaEvfuUiNg3y+mbbDd3h6Dwf14rR/ztagyCrIgaxE0dmjtRAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"891fa148e6ef92db8e65511225b2d3ddfc2254a50e5282359f14a7ad7172bc4f","last_reissued_at":"2026-07-05T07:17:27.169930Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:17:27.169930Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"KiDS-1000: Cosmology with improved cosmic shear measurements","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Angus H. Wright, Arun Kannawadi, Benjamin Giblin, Benjamin Joachimi, Catherine Heymans, Hendrik Hildebrandt, Henk Hoekstra, Huanyuan Shan, Jan Luca van den Busch, Konrad Kuijken, Lance Miller, Maciej Bilicki, Marika Asgari, Robert Reischke, Shun-Sheng Li","submitted_at":"2023-06-19T19:00:57Z","abstract_excerpt":"We present refined cosmological parameter constraints derived from a cosmic shear analysis of the fourth data release of the Kilo-Degree Survey (KiDS-1000). Our main improvements include enhanced galaxy shape measurements made possible by an updated version of the lensfit code and improved shear calibration achieved with a newly developed suite of multi-band image simulations. Additionally, we incorporated recent advancements in cosmological inference from the joint Dark Energy Survey Year 3 and KiDS-1000 cosmic shear analysis. Assuming a spatially flat standard cosmological model, we constrai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.11124","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/2306.11124/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":"2306.11124","created_at":"2026-07-05T07:17:27.169986+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.11124v2","created_at":"2026-07-05T07:17:27.169986+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.11124","created_at":"2026-07-05T07:17:27.169986+00:00"},{"alias_kind":"pith_short_12","alias_value":"REP2CSHG56JN","created_at":"2026-07-05T07:17:27.169986+00:00"},{"alias_kind":"pith_short_16","alias_value":"REP2CSHG56JNXDTF","created_at":"2026-07-05T07:17:27.169986+00:00"},{"alias_kind":"pith_short_8","alias_value":"REP2CSHG","created_at":"2026-07-05T07:17:27.169986+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05784","citing_title":"CMB Lensing Reconstruction Using Two Years of Temperature Data from the SPT-3G Summer Survey","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.27221","citing_title":"Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2511.18134","citing_title":"Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI","ref_index":14,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X","json":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X.json","graph_json":"https://pith.science/api/pith-number/REP2CSHG56JNXDTFKEJCLMWT3X/graph.json","events_json":"https://pith.science/api/pith-number/REP2CSHG56JNXDTFKEJCLMWT3X/events.json","paper":"https://pith.science/paper/REP2CSHG"},"agent_actions":{"view_html":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X","download_json":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X.json","view_paper":"https://pith.science/paper/REP2CSHG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.11124&json=true","fetch_graph":"https://pith.science/api/pith-number/REP2CSHG56JNXDTFKEJCLMWT3X/graph.json","fetch_events":"https://pith.science/api/pith-number/REP2CSHG56JNXDTFKEJCLMWT3X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X/action/storage_attestation","attest_author":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X/action/author_attestation","sign_citation":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X/action/citation_signature","submit_replication":"https://pith.science/pith/REP2CSHG56JNXDTFKEJCLMWT3X/action/replication_record"}},"created_at":"2026-07-05T07:17:27.169986+00:00","updated_at":"2026-07-05T07:17:27.169986+00:00"}