{"as_of":"2026-08-19T02:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:81f521ff79070468d30339feed1e312e7cdd6f4148a3a43889aecbbcff2bb7d3","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T18:51:35.461178Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2208.01031","last_updated":"2022-08-01T17:58:48Z","snapshot_observed_at":"2026-08-16T16:41:54.682967Z","submitted_at":"2022-08-01T17:58:48Z","title":"A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01031","snapshot_observed_at":"2026-08-06T18:51:35.461178Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.07346","last_updated":"2025-07-25T13:32:05Z","snapshot_observed_at":"2026-08-17T22:25:13.071525Z","submitted_at":"2025-07-10T00:19:11Z","title":"CLASS_SZ II: Notes and Examples of Fast and Accurate Calculations of Halo Model, Large Scale Structure and Cosmic Microwave Background Observables","version":3},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-06T18:51:35.461178Z"},"links":{"cited_paper":"/paper/2208.01031","citing_paper":"/paper/2507.07346"},"observation_digest":"sha256:e344191711a7a71df7eeee55fb127518cb3fb10c41aee24205d2f0975c7e0a29","observation_id":"669d0ab2-5abf-4646-9d14-3b791dfd001d","resolution":{"observed_at":"2026-08-06T18:51:35.461178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2208.01031/citation-record","integrity":"/paper/2208.01031/integrity","json":"/paper/2208.01031/citation-record.json","paper":"/paper/2208.01031"},"outbound":[],"paper":{"arxiv_id":"2208.01031","last_updated":"2022-08-01T17:58:48Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T16:41:54.682967Z","submitted_at":"2022-08-01T17:58:48Z","title":"A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2208.01031."}