{"as_of":"2026-08-13T17:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4b185894e349c7a1631d664bd735b3a4ad0f3592b353c07fd5409ccd058d2d6e","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":"2026-08-13T06:32:02.005865+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":"2026-08-12T04:42:52.311521Z","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":"2026-05-22T01:55:55.918132Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2309.01643","last_updated":"2024-02-10T15:11:34Z","snapshot_observed_at":"2026-08-13T10:20:44.491540Z","submitted_at":"2023-09-04T14:54:15Z","title":"On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.01643","snapshot_observed_at":"2026-08-12T04:42:52.311521Z","title":"Ding and C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.01219","last_updated":"2025-08-16T12:12:35Z","snapshot_observed_at":"2026-08-12T18:26:32.988596Z","submitted_at":"2024-12-02T07:38:18Z","title":"Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T04:42:52.311521Z"},"links":{"cited_paper":"/paper/2309.01643","citing_paper":"/paper/2412.01219"},"observation_digest":"sha256:dfc12c0cc5fe4a86c2ebc94d4157b41449ff6c0d1eda4bfff1afd09638d99c40","observation_id":"6bfc2caf-be03-4ab4-90ed-bb6f20b421d3","resolution":{"observed_at":"2026-08-12T04:42:52.311521Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.01643","last_updated":"2024-02-10T15:11:34Z","snapshot_observed_at":"2026-08-13T10:20:44.491540Z","submitted_at":"2023-09-04T14:54:15Z","title":"On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations","version":2},"cited_work":{"arxiv_id":"2309.01643","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2309.01643","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ding and C","venue":null,"work_id":"ec0146fc-3ca8-4db1-9063-8ad2e73e3227","year":2024},"citing_paper":{"arxiv_id":"2505.16820","last_updated":"2026-04-13T03:10:33Z","snapshot_observed_at":"2026-07-06T21:28:38.694043Z","submitted_at":"2025-05-22T15:55:50Z","title":"Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order","version":3},"reference_index":212,"source":"pdf_text","source_observed_at":"2026-05-22T01:55:13.345095Z"},"links":{"cited_paper":"/paper/2309.01643","citing_paper":"/paper/2505.16820"},"observation_digest":"sha256:39df8f88847eac5ecc437b3c3c124f434752d3607aa54d2bf5a62f49cd73ddb9","observation_id":"9de6cd6a-9f2e-43e2-a3c2-382bfcf57de4","resolution":{"observed_at":"2026-05-22T01:55:55.920716Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2309.01643/citation-record","integrity":"/paper/2309.01643/integrity","json":"/paper/2309.01643/citation-record.json","paper":"/paper/2309.01643"},"outbound":[],"paper":{"arxiv_id":"2309.01643","last_updated":"2024-02-10T15:11:34Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T10:20:44.491540Z","submitted_at":"2023-09-04T14:54:15Z","title":"On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2309.01643."}