{"as_of":"2026-08-04T21:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ad553aed1704a18fec8da27fdbbb2e475aa04a24044bec667af23971475602f3","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T20:23:39.073481Z","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":"2026-05-17T00:21:23.605825Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.02819","snapshot_observed_at":"2026-08-04T20:23:39.073481Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.08657","last_updated":"2026-07-22T12:30:04Z","snapshot_observed_at":"2026-08-04T20:23:35.775557Z","submitted_at":"2025-09-10T14:52:49Z","title":"First Overtone Mode in the Ringdown Signal of GW231028","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T20:23:39.073481Z"},"links":{"cited_paper":"/paper/2402.02819","citing_paper":"/paper/2509.08657"},"observation_digest":"sha256:b06a17949dac231c3599dca39738904b30b6f20e266db5e0f7bcea9f4bfe9e1d","observation_id":"ae64264f-1a06-43b8-8c56-5f083e5d96fe","resolution":{"observed_at":"2026-08-04T20:23:39.073481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.02819","snapshot_observed_at":"2026-08-04T09:43:31.126016Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.13954","last_updated":"2026-06-24T11:08:04Z","snapshot_observed_at":"2026-08-04T09:43:26.558176Z","submitted_at":"2025-10-15T18:00:03Z","title":"Quasinormal mode content of binary black hole ringdowns","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T09:43:31.126016Z"},"links":{"cited_paper":"/paper/2402.02819","citing_paper":"/paper/2510.13954"},"observation_digest":"sha256:ce71e00c5b3098c795ec82d849fa368189c5f9482ee8c61d023e1fa3912c239c","observation_id":"700aabdb-f91c-42a5-9e15-519e15adeebc","resolution":{"observed_at":"2026-08-04T09:43:31.126016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.02819","snapshot_observed_at":"2026-08-04T00:01:17.058760Z","title":"Toward a self-consistent framework for measuring black hole ringdowns,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.03766","last_updated":"2026-06-29T14:21:47Z","snapshot_observed_at":"2026-08-04T00:01:15.294101Z","submitted_at":"2025-11-05T14:57:44Z","title":"Ringdown modulation of acceleration radiation in the Schwarzschild background","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-04T00:01:17.058760Z"},"links":{"cited_paper":"/paper/2402.02819","citing_paper":"/paper/2511.03766"},"observation_digest":"sha256:2954c91cdb4dc7ba750dc845f5d2da0ad4e79240e94cec782a471ff225a3e520","observation_id":"867078d2-a4b1-4c24-b7d7-c4237d6e2eb3","resolution":{"observed_at":"2026-08-04T00:01:17.058760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","version":2},"cited_work":{"arxiv_id":"2402.02819","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.02819","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Toward a self-consistent framework for measuring black hole ringdowns","venue":null,"work_id":"ef9b8abd-36a4-4110-8585-7bcae8e4a931","year":2024},"citing_paper":{"arxiv_id":"2512.08598","last_updated":"2026-04-16T14:35:03Z","snapshot_observed_at":"2026-07-06T22:38:13.359449Z","submitted_at":"2025-12-09T13:36:27Z","title":"Horizon brightened acceleration radiation from massive vector fields","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-17T00:20:09.677514Z"},"links":{"cited_paper":"/paper/2402.02819","citing_paper":"/paper/2512.08598"},"observation_digest":"sha256:998ed9ae1df201066fb1f7bb4b84a3d294c7413daddb404ccb655b7f2b6789c2","observation_id":"e6167ceb-e9d2-4d1c-98dd-9b860a631719","resolution":{"observed_at":"2026-05-17T00:21:23.608754Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","version":2},"cited_work":{"arxiv_id":"2402.02819","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.02819","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Toward a self-consistent framework for measuring black hole ringdowns","venue":null,"work_id":"ef9b8abd-36a4-4110-8585-7bcae8e4a931","year":2024},"citing_paper":{"arxiv_id":"2605.03576","last_updated":"2026-05-05T09:45:08Z","snapshot_observed_at":"2026-07-06T23:16:30.147006Z","submitted_at":"2026-05-05T09:45:08Z","title":"Ringdown Analysis of GW250114 with Orthonormal Modes","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-07T04:06:51.511923Z"},"links":{"cited_paper":"/paper/2402.02819","citing_paper":"/paper/2605.03576"},"observation_digest":"sha256:e81ba636af9cd836510acfc4b1d377825c0d324bb245d9535cd0c96a5bb7b468","observation_id":"9d0ef981-5aba-4161-8d12-f36e95df9f77","resolution":{"observed_at":"2026-05-12T11:01:31.165157Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.02819","snapshot_observed_at":"2026-07-11T06:56:40.482817Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.05486","last_updated":"2026-07-06T18:00:00Z","snapshot_observed_at":"2026-07-11T06:56:40.253869Z","submitted_at":"2026-07-06T18:00:00Z","title":"Finite signal-to-noise ratio bias in parameter estimation for damped oscillations: cautionary remark about catalog-level black-hole spectroscopy","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-11T06:56:40.482817Z"},"links":{"cited_paper":"/paper/2402.02819","citing_paper":"/paper/2607.05486"},"observation_digest":"sha256:a443d989ea9de2852e9b26638ac34c3870dd1329100c79363d3bbdcf2dd8a8ee","observation_id":"57c9656c-6d1e-4dfe-b789-7e398df60608","resolution":{"observed_at":"2026-07-11T06:56:40.482817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2402.02819/citation-record","integrity":"/paper/2402.02819/integrity","json":"/paper/2402.02819/citation-record.json","paper":"/paper/2402.02819"},"outbound":[],"paper":{"arxiv_id":"2402.02819","last_updated":"2024-06-12T00:38:18Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T17:25:18.238343Z","submitted_at":"2024-02-05T09:03:45Z","title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2402.02819."}