{"as_of":"2026-08-15T16:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:25159624ad15781729e3bdb3e6457d3073f7ff429731f22ebd13cbf73dc63d09","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-31T23:27:07.692013Z","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":"2026-05-18T17:42:46.910335Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2210.10435","last_updated":"2024-09-20T05:25:02Z","snapshot_observed_at":"2026-08-13T14:02:08.341224Z","submitted_at":"2022-10-19T10:06:48Z","title":"Integrated perturbation theory for cosmological tensor fields. I. Basic formulation","version":5},"cited_work":{"arxiv_id":"2210.10435","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.10435","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Matsubara, The integrated perturbation theory for cosmological tensor fields I: Basic formulation, arXiv e-prints , arXiv:2210.10435 (2022), arXiv:2210.10435 [astro-ph.CO]","venue":null,"work_id":"bb22e00b-ea97-422f-a84a-e8d21ff141cb","year":2022},"citing_paper":{"arxiv_id":"2509.08787","last_updated":"2026-04-13T10:52:50Z","snapshot_observed_at":"2026-08-06T22:16:50.270614Z","submitted_at":"2025-09-10T17:15:21Z","title":"Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity","version":2},"reference_index":122,"source":"pdf_text","source_observed_at":"2026-05-18T17:42:09.607777Z"},"links":{"cited_paper":"/paper/2210.10435","citing_paper":"/paper/2509.08787"},"observation_digest":"sha256:8dc63e3e958ed4303abd191293bc63f1540578d54ccf353a44c428c8e440e653","observation_id":"4ea6480e-aa0a-4761-bdb2-36a06b86f378","resolution":{"observed_at":"2026-05-18T17:42:46.913563Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.10435","last_updated":"2024-09-20T05:25:02Z","snapshot_observed_at":"2026-08-13T14:02:08.341224Z","submitted_at":"2022-10-19T10:06:48Z","title":"Integrated perturbation theory for cosmological tensor fields. I. Basic formulation","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.10435","snapshot_observed_at":"2026-07-31T23:27:07.692013Z","title":"Matsubara,Integrated perturbation theory for cosmological tensor fields","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.23973","last_updated":"2026-07-27T03:49:28Z","snapshot_observed_at":"2026-08-15T13:24:15.486733Z","submitted_at":"2026-07-27T03:49:28Z","title":"Testing Statistical Isotropy on the Sphere with Minkowski Tensors","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-31T23:27:07.692013Z"},"links":{"cited_paper":"/paper/2210.10435","citing_paper":"/paper/2607.23973"},"observation_digest":"sha256:1c3595baf73acc9a5f1ebc057f68dde7d86f80e842c32cc582b796ef0cea3438","observation_id":"cc67ba6a-55cc-4a9f-b7ef-898723894cc0","resolution":{"observed_at":"2026-07-31T23:27:07.692013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2210.10435/citation-record","integrity":"/paper/2210.10435/integrity","json":"/paper/2210.10435/citation-record.json","paper":"/paper/2210.10435"},"outbound":[],"paper":{"arxiv_id":"2210.10435","last_updated":"2024-09-20T05:25:02Z","latest_version":5,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T14:02:08.341224Z","submitted_at":"2022-10-19T10:06:48Z","title":"Integrated perturbation theory for cosmological tensor fields. I. Basic formulation"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2210.10435."}