{"as_of":"2026-08-19T09:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c8d05ce8e3077a9beeeb1a3aa3333c8541e9675207ef03a1f2704ded093be463","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:21:13.893875Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T15:29:56.603874Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2402.13783","last_updated":"2025-01-21T11:02:11Z","snapshot_observed_at":"2026-08-17T02:23:05.262314Z","submitted_at":"2024-02-21T13:07:43Z","title":"A comparison of shrinkage estimators of the cosmological precision matrix","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.13783","snapshot_observed_at":"2026-08-16T05:21:13.893875Z","title":"Looijmans, M.S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.21133","last_updated":"2025-07-01T17:51:09Z","snapshot_observed_at":"2026-08-17T08:45:05.607427Z","submitted_at":"2025-04-29T19:28:30Z","title":"Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation","version":2},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-08-16T05:21:13.893875Z"},"links":{"cited_paper":"/paper/2402.13783","citing_paper":"/paper/2504.21133"},"observation_digest":"sha256:f033ab67b80ae4c1ada0367beae74b726a1a88107de476ad94c3b2e82448d6c8","observation_id":"9ad71e84-8f75-4266-9016-32e5ebd803ea","resolution":{"observed_at":"2026-08-16T05:21:13.893875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13783","last_updated":"2025-01-21T11:02:11Z","snapshot_observed_at":"2026-08-17T02:23:05.262314Z","submitted_at":"2024-02-21T13:07:43Z","title":"A comparison of shrinkage estimators of the cosmological precision matrix","version":2},"cited_work":{"arxiv_id":"2402.13783","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.13783","snapshot_observed_at":"2026-07-04T15:29:56.603874Z","title":"J., Wang, M","venue":null,"work_id":"376f7a9a-5652-4031-bfeb-832cf4e5ee02","year":2024},"citing_paper":{"arxiv_id":"2506.09118","last_updated":"2026-04-13T09:38:31Z","snapshot_observed_at":"2026-07-06T21:39:56.824255Z","submitted_at":"2025-06-10T18:00:00Z","title":"Euclid preparation. LXXXIX. Accurate and precise data-driven angular power spectrum covariances","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-19T10:06:03.372802Z"},"links":{"cited_paper":"/paper/2402.13783","citing_paper":"/paper/2506.09118"},"observation_digest":"sha256:fc6767d2bedfa3766ee2693a23c4fa84e6bf62ca2788d0e6d5708c35f92823dd","observation_id":"c87e802c-2ccb-4e2e-8839-e235cdaf42dc","resolution":{"observed_at":"2026-05-19T10:07:14.230712Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13783","last_updated":"2025-01-21T11:02:11Z","snapshot_observed_at":"2026-08-17T02:23:05.262314Z","submitted_at":"2024-02-21T13:07:43Z","title":"A comparison of shrinkage estimators of the cosmological precision matrix","version":2},"cited_work":{"arxiv_id":"2402.13783","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.13783","snapshot_observed_at":"2026-07-04T15:29:56.603874Z","title":"J., Wang, M","venue":null,"work_id":"376f7a9a-5652-4031-bfeb-832cf4e5ee02","year":2024},"citing_paper":{"arxiv_id":"2606.26237","last_updated":"2026-06-24T18:00:03Z","snapshot_observed_at":"2026-07-07T00:00:36.766142Z","submitted_at":"2026-06-24T18:00:03Z","title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","version":1},"reference_index":238,"source":"arxiv_source","source_observed_at":"2026-06-26T01:35:05.451125Z"},"links":{"cited_paper":"/paper/2402.13783","citing_paper":"/paper/2606.26237"},"observation_digest":"sha256:ff6c1e8cff260574df24d3c0027ed3ddf288158c1d2e330e1df22f61c6d421fa","observation_id":"e76158b9-b09a-4e69-b142-a49fb4ac3cfe","resolution":{"observed_at":"2026-07-04T15:29:56.605438Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2402.13783/citation-record","integrity":"/paper/2402.13783/integrity","json":"/paper/2402.13783/citation-record.json","paper":"/paper/2402.13783"},"outbound":[],"paper":{"arxiv_id":"2402.13783","last_updated":"2025-01-21T11:02:11Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T02:23:05.262314Z","submitted_at":"2024-02-21T13:07:43Z","title":"A comparison of shrinkage estimators of the cosmological precision matrix"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2402.13783."}