{"as_of":"2026-08-23T17:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:42afc362de34c8965f4116bd50f5a0a94360d01890801dbe31891d2eeabca4fe","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":"2026-08-23T06:30:58.430688+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":"2026-08-11T14:26:32.091190Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-05T14:45:52.135636Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.08574","last_updated":"2024-09-25T18:44:21Z","snapshot_observed_at":"2026-08-16T14:01:22.794507Z","submitted_at":"2024-04-12T16:21:49Z","title":"Cosmic variance of the Hellings and Downs correlation for ensembles of universes having nonzero angular power spectra","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.08574","snapshot_observed_at":"2026-08-11T14:26:32.091190Z","title":"Agarwal and J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12073","last_updated":"2025-04-24T14:49:59Z","snapshot_observed_at":"2026-08-18T20:11:59.605954Z","submitted_at":"2024-12-16T18:46:25Z","title":"Mitigating cosmic variance in the Hellings-Downs curve: a Cosmic Microwave Background analogy","version":4},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T14:26:32.091190Z"},"links":{"cited_paper":"/paper/2404.08574","citing_paper":"/paper/2412.12073"},"observation_digest":"sha256:75402644f3613452876a22efa297bac98e9068ca2783544c16af0402bbb47234","observation_id":"409231ff-dcc1-40c2-a7a9-5d5669b4b742","resolution":{"observed_at":"2026-08-11T14:26:32.091190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08574","last_updated":"2024-09-25T18:44:21Z","snapshot_observed_at":"2026-08-16T14:01:22.794507Z","submitted_at":"2024-04-12T16:21:49Z","title":"Cosmic variance of the Hellings and Downs correlation for ensembles of universes having nonzero angular power spectra","version":3},"cited_work":{"arxiv_id":"2404.08574","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.08574","snapshot_observed_at":"2026-08-05T14:45:52.135636Z","title":"Cosmic variance of the Hellings and Downs correlation for ensembles of universes having nonzero angular power spectra","venue":"gr-qc","work_id":"05e94d0c-6b02-4002-955b-66948829f6c4","year":2024},"citing_paper":{"arxiv_id":"2508.21131","last_updated":"2025-08-28T18:05:44Z","snapshot_observed_at":"2026-08-20T02:06:16.790193Z","submitted_at":"2025-08-28T18:05:44Z","title":"Cosmic Variance in Anisotropy Searches at Pulsar Timing Arrays","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-05T14:45:51.161981Z"},"links":{"cited_paper":"/paper/2404.08574","citing_paper":"/paper/2508.21131"},"observation_digest":"sha256:750df1582a4d91a1c6e70da52923836985c56940421699106272a23ecd8983e8","observation_id":"ff5e11de-3244-48c1-8626-82f0f828e1b3","resolution":{"observed_at":"2026-08-05T14:45:52.141996Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2404.08574/citation-record","integrity":"/paper/2404.08574/integrity","json":"/paper/2404.08574/citation-record.json","paper":"/paper/2404.08574"},"outbound":[],"paper":{"arxiv_id":"2404.08574","last_updated":"2024-09-25T18:44:21Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T14:01:22.794507Z","submitted_at":"2024-04-12T16:21:49Z","title":"Cosmic variance of the Hellings and Downs correlation for ensembles of universes having nonzero angular power spectra"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2404.08574."}