{"as_of":"2026-08-09T06:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9025b5ec4d9e6fe783e0ce479179cf772f1f69fc0d35d76d36e5837968526cac","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T22:39:17.934938Z","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":"2026-07-04T18:20:04.706010Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2205.14808","last_updated":"2022-05-30T02:09:43Z","snapshot_observed_at":"2026-07-06T13:15:14.206185Z","submitted_at":"2022-05-30T02:09:43Z","title":"Wave equations estimates and the nonlinear stability of slowly rotating Kerr black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.14808","snapshot_observed_at":"2026-08-06T22:39:17.934938Z","title":"W ave equations estimates and the nonlinear stability of slowly rotating K err black holes","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.21183","last_updated":"2025-06-26T12:43:18Z","snapshot_observed_at":"2026-08-06T22:30:06.281678Z","submitted_at":"2025-06-26T12:43:18Z","title":"Linear stability of Kerr black holes in the full subextremal range","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-06T22:39:17.934938Z"},"links":{"cited_paper":"/paper/2205.14808","citing_paper":"/paper/2506.21183"},"observation_digest":"sha256:d53ce1a34d9bc4a29e0a6f34c3a7aee9830314a7ac6417523a8ec315c06ba27f","observation_id":"aee8b989-06fe-44a5-a7bb-fe1863491f24","resolution":{"observed_at":"2026-08-06T22:39:17.934938Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.14808","last_updated":"2022-05-30T02:09:43Z","snapshot_observed_at":"2026-07-06T13:15:14.206185Z","submitted_at":"2022-05-30T02:09:43Z","title":"Wave equations estimates and the nonlinear stability of slowly rotating Kerr black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.14808","snapshot_observed_at":"2026-08-06T18:31:08.937333Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.08326","last_updated":"2025-07-11T05:33:54Z","snapshot_observed_at":"2026-08-08T06:26:29.385101Z","submitted_at":"2025-07-11T05:33:54Z","title":"On Axially Symmetric Perturbations of Kerr Black Hole Spacetimes","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T18:31:08.937333Z"},"links":{"cited_paper":"/paper/2205.14808","citing_paper":"/paper/2507.08326"},"observation_digest":"sha256:2baf9ef71c7e21ed1f588a0b299a9ee59dd28f62565fcac2133fadcda2cf089b","observation_id":"20e3a173-4476-4420-9a24-9c929b693adb","resolution":{"observed_at":"2026-08-06T18:31:08.937333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.14808","last_updated":"2022-05-30T02:09:43Z","snapshot_observed_at":"2026-07-06T13:15:14.206185Z","submitted_at":"2022-05-30T02:09:43Z","title":"Wave equations estimates and the nonlinear stability of slowly rotating Kerr black holes","version":1},"cited_work":{"arxiv_id":"2205.14808","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2205.14808","snapshot_observed_at":"2026-07-04T18:20:04.706010Z","title":"Giorgi, S","venue":null,"work_id":"480937df-1b8d-4aa9-84a6-7e0f391d7c84","year":null},"citing_paper":{"arxiv_id":"2606.24642","last_updated":"2026-06-24T17:40:35Z","snapshot_observed_at":"2026-07-06T23:59:13.320720Z","submitted_at":"2026-06-23T14:39:40Z","title":"When Black Holes Can Wear Pants","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-25T22:56:01.698250Z"},"links":{"cited_paper":"/paper/2205.14808","citing_paper":"/paper/2606.24642"},"observation_digest":"sha256:1ab3c80e64e8c617d8019df8d4e376d1bf3231506969834d83a3e62ef6024a22","observation_id":"e1e50cdd-8505-4a0e-955b-ceea71a5b3ba","resolution":{"observed_at":"2026-07-04T18:20:04.708025Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.14808","last_updated":"2022-05-30T02:09:43Z","snapshot_observed_at":"2026-07-06T13:15:14.206185Z","submitted_at":"2022-05-30T02:09:43Z","title":"Wave equations estimates and the nonlinear stability of slowly rotating Kerr black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.14808","snapshot_observed_at":"2026-07-13T05:30:50.076813Z","title":"Giorgi, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.08958","last_updated":"2026-07-09T21:48:50Z","snapshot_observed_at":"2026-08-07T23:50:08.435416Z","submitted_at":"2026-07-09T21:48:50Z","title":"A Physical space derivation of Morawetz-Energy estimates in Kerr spacetimes with large angular momentum","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-13T05:30:50.076813Z"},"links":{"cited_paper":"/paper/2205.14808","citing_paper":"/paper/2607.08958"},"observation_digest":"sha256:7cb5d161bbea554de22f637885348a43f4d88d1dfb03f5bc07f11491fe174018","observation_id":"19fc5939-2b36-406a-87ea-c9a4b9cf142c","resolution":{"observed_at":"2026-07-13T05:30:50.076813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2205.14808/citation-record","integrity":"/paper/2205.14808/integrity","json":"/paper/2205.14808/citation-record.json","paper":"/paper/2205.14808"},"outbound":[],"paper":{"arxiv_id":"2205.14808","last_updated":"2022-05-30T02:09:43Z","latest_version":1,"primary_category":"math.AP","snapshot_observed_at":"2026-07-06T13:15:14.206185Z","submitted_at":"2022-05-30T02:09:43Z","title":"Wave equations estimates and the nonlinear stability of slowly rotating Kerr black holes"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2205.14808."}