{"as_of":"2026-08-08T07:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:60268c77b1b8f34a17eba2ceff4691e3e8a297dadfe17553e30d8cda1aef7ab2","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:55:32.921961Z","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":"2026-07-01T20:06:12.143097Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":"2404.01374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-07-01T20:06:12.143097Z","title":"Cardoso, S","venue":null,"work_id":"40b0bcfa-1e4a-4dc9-b1e3-8bd4f8ef771a","year":2024},"citing_paper":{"arxiv_id":"2501.16433","last_updated":"2026-05-13T15:28:20Z","snapshot_observed_at":"2026-08-02T14:23:16.098022Z","submitted_at":"2025-01-27T19:00:06Z","title":"Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-23T04:43:04.006726Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2501.16433"},"observation_digest":"sha256:dbb08e4c466a226006f80ff61e71e26ebc89478a4232cd15d4936da3960b2df8","observation_id":"687cf8b9-6e72-435e-ae52-cd84c04deaf1","resolution":{"observed_at":"2026-05-23T04:45:25.396837Z","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":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-08-07T14:55:32.921961Z","title":"Cardoso, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.17186","last_updated":"2025-06-26T08:22:36Z","snapshot_observed_at":"2026-08-07T15:11:40.044873Z","submitted_at":"2025-05-22T18:00:03Z","title":"Bound States of the Schwarzschild Black Hole","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T14:55:32.921961Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2505.17186"},"observation_digest":"sha256:255e1b76510a337009be470f70fc23b7266a27f48dbaed4e78e6507738ed10e3","observation_id":"83961054-b024-43c2-b519-dcc3208dc309","resolution":{"observed_at":"2026-08-07T14:55:32.921961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-08-07T13:41:51.067451Z","title":"Cardoso, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.21303","last_updated":"2025-07-03T13:24:54Z","snapshot_observed_at":"2026-08-07T13:28:11.475614Z","submitted_at":"2025-05-27T15:05:21Z","title":"Spectrum instability and greybody factor stability for parabolic approximation of Regge-Wheeler potential","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T13:41:51.067451Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2505.21303"},"observation_digest":"sha256:faf4ff828e381cef35957d1ecb25fba42d30f1a93ec14787b8ca50d5a5422404","observation_id":"83f8b5d2-536d-4a0a-a9fb-c9cfb4b63247","resolution":{"observed_at":"2026-08-07T13:41:51.067451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-08-07T05:36:04.929913Z","title":"Physical significance of the black hole quasinormal mode spectra instability,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.07562","last_updated":"2026-07-15T17:25:26Z","snapshot_observed_at":"2026-08-08T00:20:30.638303Z","submitted_at":"2025-06-09T08:57:53Z","title":"Numerical study on the robustness of the stability for stable black holes","version":4},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T05:36:04.929913Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2506.07562"},"observation_digest":"sha256:d84b912062aecb22d3a606d41d109090988e5964506e5bfdde276de0cf4baf49","observation_id":"d3350d1c-9239-4e14-8001-fcdf39dfe242","resolution":{"observed_at":"2026-08-07T05:36:04.929913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":"2404.01374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-07-01T20:06:12.143097Z","title":"Cardoso, S","venue":null,"work_id":"40b0bcfa-1e4a-4dc9-b1e3-8bd4f8ef771a","year":2024},"citing_paper":{"arxiv_id":"2511.00565","last_updated":"2026-04-15T22:30:45Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-11-01T14:05:54Z","title":"Reflectionless and echo modes in asymmetric Damour-Solodukhin wormholes","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-18T01:34:45.033342Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2511.00565"},"observation_digest":"sha256:5058bf95d9d13c40baae514a0fbffee8dd44251444eb37956da82ce5b5297f29","observation_id":"99949631-d27c-4b52-ba70-cb0463da3a2f","resolution":{"observed_at":"2026-05-18T01:35:36.266219Z","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":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":"2404.01374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-07-01T20:06:12.143097Z","title":"Cardoso, S","venue":null,"work_id":"40b0bcfa-1e4a-4dc9-b1e3-8bd4f8ef771a","year":2024},"citing_paper":{"arxiv_id":"2511.08692","last_updated":"2026-05-13T14:11:56Z","snapshot_observed_at":"2026-07-06T22:35:31.750339Z","submitted_at":"2025-11-11T19:00:08Z","title":"Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-17T23:20:36.030481Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2511.08692"},"observation_digest":"sha256:1bcdc6179586d27b9c8adbf10349a670c4ff09d75d221d0e15bb175d93b92bbf","observation_id":"ba3cf397-60f7-4288-bf17-b5a836f56b60","resolution":{"observed_at":"2026-05-17T23:22:13.114761Z","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":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-08-03T15:08:53.731565Z","title":"Cardoso, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.18631","last_updated":"2026-06-03T12:09:17Z","snapshot_observed_at":"2026-08-06T17:08:32.113965Z","submitted_at":"2025-12-21T08:01:08Z","title":"Spectral instability of parametrized black hole quasinormal modes in the high-overtone limit via the exact WKB analysis","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T15:08:53.731565Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2512.18631"},"observation_digest":"sha256:653b96312f86ce39721a0c4bfc54c4d296534c5362b06e4801dc295094809240","observation_id":"85608426-b71c-4bb4-b6b3-64e91949306c","resolution":{"observed_at":"2026-08-03T15:08:53.731565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":"2404.01374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-07-01T20:06:12.143097Z","title":"Cardoso, S","venue":null,"work_id":"40b0bcfa-1e4a-4dc9-b1e3-8bd4f8ef771a","year":2024},"citing_paper":{"arxiv_id":"2606.00166","last_updated":"2026-05-29T12:13:09Z","snapshot_observed_at":"2026-07-06T23:40:56.510371Z","submitted_at":"2026-05-29T12:13:09Z","title":"Cascading amplification of gravitational waves triggered by environment in dynamical Chern-Simons gravity","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-06-28T21:36:52.517617Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2606.00166"},"observation_digest":"sha256:374e291d4866030824645d3f1b3de3982932edf6bf13aa9544e5d25c239ff76e","observation_id":"0ea8be85-8cd1-4fcd-8ccc-99379a0f101e","resolution":{"observed_at":"2026-07-01T20:06:12.144331Z","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":"2404.01374","last_updated":"2024-04-01T18:00:01Z","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01374","snapshot_observed_at":"2026-08-04T04:35:28.430501Z","title":"On the physical significance of black hole quasinormal mode spectra instability","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03434","last_updated":"2026-08-03T11:58:44Z","snapshot_observed_at":"2026-08-06T23:31:36.448133Z","submitted_at":"2026-07-03T15:46:30Z","title":"Berry Picking: Random Wave Chaos Hierarchy for BPS Microstate Geometries","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-04T04:35:28.430501Z"},"links":{"cited_paper":"/paper/2404.01374","citing_paper":"/paper/2607.03434"},"observation_digest":"sha256:4144b0ec5c57685918277442c4203234f00d738ef01ddba1ce876709835efe45","observation_id":"254f9555-9cce-4fc1-864a-90009f736a70","resolution":{"observed_at":"2026-08-04T04:35:28.430501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.01374/citation-record","integrity":"/paper/2404.01374/integrity","json":"/paper/2404.01374/citation-record.json","paper":"/paper/2404.01374"},"outbound":[],"paper":{"arxiv_id":"2404.01374","last_updated":"2024-04-01T18:00:01Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T17:54:11.726535Z","submitted_at":"2024-04-01T18:00:01Z","title":"On the physical significance of black hole quasinormal mode spectra instability"},"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 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2404.01374."}