{"as_of":"2026-08-19T09:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:986de0242a12ac212b06f12deb94fed6de35c3b7673c75169225f0bef3cb8259","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":"2026-08-19T06:32:44.657259+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":"2026-08-04T19:41:19.138000Z","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":"2408.16747","last_updated":"2024-12-12T15:43:15Z","snapshot_observed_at":"2026-08-16T13:22:50.216123Z","submitted_at":"2024-08-29T17:40:06Z","title":"Ringdown of a postinnermost stable circular orbit of a rapidly spinning black hole: Mass ratio dependence of higher harmonic quasinormal mode excitation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.16747","snapshot_observed_at":"2026-08-04T19:41:19.138000Z","title":"Watarai, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.09165","last_updated":"2025-09-11T05:48:16Z","snapshot_observed_at":"2026-08-17T06:45:07.023326Z","submitted_at":"2025-09-11T05:48:16Z","title":"Probing Direct Waves in Black Hole Ringdowns","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-04T19:41:19.138000Z"},"links":{"cited_paper":"/paper/2408.16747","citing_paper":"/paper/2509.09165"},"observation_digest":"sha256:22c80f90c0cbd293d6ed4d09ed9514627dcba6a30b99c627dcbf022dc1cc5bee","observation_id":"f541b340-cf01-4e02-9cae-0cbc04fccde4","resolution":{"observed_at":"2026-08-04T19:41:19.138000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.16747","last_updated":"2024-12-12T15:43:15Z","snapshot_observed_at":"2026-08-16T13:22:50.216123Z","submitted_at":"2024-08-29T17:40:06Z","title":"Ringdown of a postinnermost stable circular orbit of a rapidly spinning black hole: Mass ratio dependence of higher harmonic quasinormal mode excitation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.16747","snapshot_observed_at":"2026-08-03T22:53:00.959379Z","title":"Watarai, Ringdown of a postinnermost stable circular orbit of a rapidly spinning black hole: Mass ratio depen- dence of higher harmonic quasinormal mode excitation, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.08673","last_updated":"2026-06-02T15:50:35Z","snapshot_observed_at":"2026-08-13T14:35:58.879151Z","submitted_at":"2025-11-11T19:00:01Z","title":"Gravitational radiation from Kerr black holes using the Sasaki-Nakamura formalism: Waveforms and fluxes at infinity","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T22:53:00.959379Z"},"links":{"cited_paper":"/paper/2408.16747","citing_paper":"/paper/2511.08673"},"observation_digest":"sha256:94e1e26934ec3c80b42a2b3eb77a2fa7c104f403d954801d6507aba3d9f66fa8","observation_id":"101dc68d-0057-4dd7-b599-79fa0aa15109","resolution":{"observed_at":"2026-08-03T22:53:00.959379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2408.16747/citation-record","integrity":"/paper/2408.16747/integrity","json":"/paper/2408.16747/citation-record.json","paper":"/paper/2408.16747"},"outbound":[],"paper":{"arxiv_id":"2408.16747","last_updated":"2024-12-12T15:43:15Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T13:22:50.216123Z","submitted_at":"2024-08-29T17:40:06Z","title":"Ringdown of a postinnermost stable circular orbit of a rapidly spinning black hole: Mass ratio dependence of higher harmonic quasinormal mode excitation"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2408.16747."}