{"as_of":"2026-08-22T17:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c154f4dfb1d6c0ad60e06b1e2c4de5dc070d84bba6d5a088b8d7ea76757604b9","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":"2026-08-22T06:32:14.747728+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":"2026-08-01T22:12:34.298039Z","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":"2202.11332","last_updated":"2022-02-23T07:27:25Z","snapshot_observed_at":"2026-08-17T17:09:48.735213Z","submitted_at":"2022-02-23T07:27:25Z","title":"Measuring the cosmological density field twice: A novel test of dark energy using the CMB quadrupole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.11332","snapshot_observed_at":"2026-08-01T22:12:34.298039Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15850","last_updated":"2026-07-17T11:08:01Z","snapshot_observed_at":"2026-08-15T22:59:01.066728Z","submitted_at":"2026-07-17T11:08:01Z","title":"Standard Reconstruction Shifts the Optimal Input Scale for CNN-Based Density-Field Reconstruction","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-01T22:12:34.298039Z"},"links":{"cited_paper":"/paper/2202.11332","citing_paper":"/paper/2607.15850"},"observation_digest":"sha256:64dc5881047cf431941b4d80f5c706b355301a271abd93a3b0b79d09fd1a7ed0","observation_id":"bc371e4a-5f59-497d-beea-bff60160d5d8","resolution":{"observed_at":"2026-08-01T22:12:34.298039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2202.11332/citation-record","integrity":"/paper/2202.11332/integrity","json":"/paper/2202.11332/citation-record.json","paper":"/paper/2202.11332"},"outbound":[],"paper":{"arxiv_id":"2202.11332","last_updated":"2022-02-23T07:27:25Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T17:09:48.735213Z","submitted_at":"2022-02-23T07:27:25Z","title":"Measuring the cosmological density field twice: A novel test of dark energy using the CMB quadrupole"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2202.11332."}