{"as_of":"2026-08-09T15:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3e674c341e488634b1e129e807d35ac2d11c2e1feea95da10c320ea6591d68c0","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":24,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":24,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":24,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":24,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:46:17.866596Z","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":"2026-07-02T22:07:26.280218Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-07T04:46:17.866596Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.866596Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:7c9a5ac541e0ca30f14a071959e68f989e7c306f9c174ed88eb16145079a5c72","observation_id":"9ed3de29-3a7b-4b13-9265-184bd5f0de49","resolution":{"observed_at":"2026-08-07T04:46:17.866596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-06T14:09:33.295680Z","title":"Skvortsova, Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer–Snyder Model of Black Holes, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-09T06:31:42.540197Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.295680Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:32652dcabacb117fc81f6fba87f4563c85f3d25da758d79556ee0a937488b7c8","observation_id":"2fd02827-d5bf-4227-b7a7-3f3ff0411be2","resolution":{"observed_at":"2026-08-06T14:09:33.295680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-05T19:07:37.520118Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.13366","last_updated":"2026-07-22T14:35:30Z","snapshot_observed_at":"2026-08-07T18:18:39.515438Z","submitted_at":"2025-08-18T21:17:11Z","title":"Where Do the Returns to Schooling Come From? Educational Transitions and Labor Market Payoffs","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-05T19:07:37.520118Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2508.13366"},"observation_digest":"sha256:912058ccfe663b4e94b5ac30afd75f31bbe9406a68a88a49ee8eddc8a9396a95","observation_id":"b586a199-c800-4ae9-8c48-293929b75d39","resolution":{"observed_at":"2026-08-05T19:07:37.520118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-04T11:09:55.462931Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.06689","last_updated":"2026-05-28T09:50:09Z","snapshot_observed_at":"2026-08-04T11:09:41.169992Z","submitted_at":"2025-10-08T06:25:32Z","title":"Bonanno-Reuter regular black hole: quasi-resonances, grey-body factors and absorption cross-sections of a massive scalar field","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-04T11:09:55.462931Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2510.06689"},"observation_digest":"sha256:86a000564b947407ec766fdd7a20e2979cb9be866f88b845d67b6505790aecae","observation_id":"14afa632-9d47-4eef-a266-82a6d9471e8d","resolution":{"observed_at":"2026-08-04T11:09:55.462931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2510.27320","last_updated":"2026-04-06T06:53:03Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-31T09:47:10Z","title":"The quasinormal modes of the rotating quantum corrected black holes","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-18T03:07:46.828770Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2510.27320"},"observation_digest":"sha256:24c50000bb31b88a8f7198dc426f4b7da8178fcedbf270e8681eb59c336d30d4","observation_id":"0724c1b7-c9a5-48ac-a04f-ee2c320e4baf","resolution":{"observed_at":"2026-05-18T03:10:49.291353Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-03T22:11:07.911772Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.12335","last_updated":"2026-05-28T09:58:14Z","snapshot_observed_at":"2026-08-03T22:11:04.419217Z","submitted_at":"2025-11-15T19:28:44Z","title":"Long-lived quasinormal modes and grey-body factors of supermassive black holes with a dark matter halo","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-03T22:11:07.911772Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2511.12335"},"observation_digest":"sha256:9c6ad328e94077cc334203fd652c5ce211569a863ee47b6b2dc98488a6bf416e","observation_id":"b1ae3f11-68ef-4e0c-b38a-ab1f7b92ac05","resolution":{"observed_at":"2026-08-03T22:11:07.911772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2601.17906","last_updated":"2026-04-02T18:11:47Z","snapshot_observed_at":"2026-07-06T22:42:57.796038Z","submitted_at":"2026-01-25T16:54:41Z","title":"Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole","version":2},"reference_index":157,"source":"pdf_text","source_observed_at":"2026-05-16T11:06:54.209646Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2601.17906"},"observation_digest":"sha256:cf92f030afe24943c4aeac313a9e8b5e0f20e293a4cf28bef3c0f6abc721b394","observation_id":"6b3c6ea5-7c1e-4c2b-9cd4-9a0cf1a9a65c","resolution":{"observed_at":"2026-05-16T11:07:47.501732Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2602.11001","last_updated":"2026-04-17T10:43:09Z","snapshot_observed_at":"2026-07-06T22:45:29.609382Z","submitted_at":"2026-02-11T16:23:23Z","title":"Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes","version":2},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-05-16T02:41:01.645151Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2602.11001"},"observation_digest":"sha256:2972a3e261adc673a65430cd12c8aa1c8ca5f9b336a5c612eecda6ed6fda40b9","observation_id":"ddb5b252-8fb8-477b-85ad-77d66708c5a9","resolution":{"observed_at":"2026-05-16T02:42:10.741726Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2603.10844","last_updated":"2026-04-16T17:09:38Z","snapshot_observed_at":"2026-07-06T22:48:39.649787Z","submitted_at":"2026-03-11T14:52:37Z","title":"Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity","version":2},"reference_index":182,"source":"pdf_text","source_observed_at":"2026-05-15T13:15:54.975020Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2603.10844"},"observation_digest":"sha256:8fd29e1a96c2044ba6daebc8827974cfc68b6ef6afcbec463b2eeb7a580037a2","observation_id":"46078520-0d36-410f-ae58-370747b8efd7","resolution":{"observed_at":"2026-05-15T13:20:02.647522Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-04T05:43:13.506509Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.28415","last_updated":"2026-08-03T09:20:37Z","snapshot_observed_at":"2026-08-08T18:53:35.806470Z","submitted_at":"2026-03-30T13:27:04Z","title":"Long-lived quasinormal frequencies for regular black hole supported by the Einasto profile in the presence of the magnetic field","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:13.506509Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2603.28415"},"observation_digest":"sha256:6d1656be60024bb6c5ada9f4408917f8d4f531a950b1a277b5103151088fa06b","observation_id":"23c2699a-4903-42ae-8224-5f69a145d83e","resolution":{"observed_at":"2026-08-04T05:43:13.506509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2604.11845","last_updated":"2026-04-12T21:06:27Z","snapshot_observed_at":"2026-07-06T23:00:08.171601Z","submitted_at":"2026-04-12T21:06:27Z","title":"Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-10T15:10:05.638518Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2604.11845"},"observation_digest":"sha256:a2bebf1cffd46831bdce20cb6cda5974ea2be60a647b0c3ddf8a568f51cb6ba9","observation_id":"97059b4a-e6e0-42fd-b037-e8fbe8533e1d","resolution":{"observed_at":"2026-05-11T11:06:02.620406Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-07-06T23:10:24.992210Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-08T02:18:25.796367Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:0fead33a3b7f966b51ce770237e60c3ece43f2b5b5869132f09859bfb2373c3a","observation_id":"03cb8bb1-19c7-44cf-90bb-dd70a94ba0f6","resolution":{"observed_at":"2026-05-11T22:51:26.551379Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-07-06T23:10:24.992210Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-14T22:18:47.797399Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:953135e48c8f76e4ae8d3685f4354965616f6c3fc5e82edc386562c99628d306","observation_id":"630769ad-0d2a-4f68-90c4-e13bf99bdcac","resolution":{"observed_at":"2026-05-14T22:19:31.416758Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2604.25471","last_updated":"2026-04-28T10:23:30Z","snapshot_observed_at":"2026-08-02T11:44:34.483229Z","submitted_at":"2026-04-28T10:23:30Z","title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","version":1},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-05-07T15:29:43.270538Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2604.25471"},"observation_digest":"sha256:da06cf397c17f33db96afefcf75a4be557c2844b815c256420661993d1713612","observation_id":"25f0749e-794d-47a9-b800-072de02d5e90","resolution":{"observed_at":"2026-05-12T00:21:15.756350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.03659","last_updated":"2026-05-05T11:41:14Z","snapshot_observed_at":"2026-07-06T23:16:34.988490Z","submitted_at":"2026-05-05T11:41:14Z","title":"Long-lived massive scalar modes, grey-body factors, and absorption cross sections of the Reissner--Nordstr\\\"om-like brane-world black hole","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-07T14:06:56.581854Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.03659"},"observation_digest":"sha256:ff022bd49deddcb82e97bf85142031cf07025104107e903785cb485126759e55","observation_id":"38f6412e-9a0c-4967-8561-09f011d48a0d","resolution":{"observed_at":"2026-05-12T08:41:24.722760Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.11013","last_updated":"2026-05-10T12:56:40Z","snapshot_observed_at":"2026-07-06T23:22:52.369277Z","submitted_at":"2026-05-10T12:56:40Z","title":"Massive Scalar Quasinormal Modes, Greybody Factors, and Absorption Cross Section of a Parity-Symmetric Beyond-Horndeski Black Hole","version":1},"reference_index":139,"source":"pdf_text","source_observed_at":"2026-05-13T01:58:50.185004Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.11013"},"observation_digest":"sha256:f19a5bbfb32cad03bed68a86c98195085b65c01696662c6da38ab395ed46c34b","observation_id":"9e9c5936-92c3-447e-b7d2-e2ea5b160080","resolution":{"observed_at":"2026-05-13T02:07:08.566501Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.11364","last_updated":"2026-05-12T00:34:59Z","snapshot_observed_at":"2026-08-03T00:14:03.960316Z","submitted_at":"2026-05-12T00:34:59Z","title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","version":1},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-05-13T02:39:27.974688Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.11364"},"observation_digest":"sha256:fd23e58d14578141221144eb297e525574af82b9a846bf15007f22e7a104b411","observation_id":"ccf5f620-2907-4fb6-94c4-799c1a42241c","resolution":{"observed_at":"2026-05-13T02:47:08.235621Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.12113","last_updated":"2026-05-12T13:29:10Z","snapshot_observed_at":"2026-08-04T03:37:25.006389Z","submitted_at":"2026-05-12T13:29:10Z","title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-13T04:51:34.508568Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.12113"},"observation_digest":"sha256:b67ec5e1d30fc5fcedd0c04bca20abbf30fa37fc93a6eebdc8fc7e55550ceeb1","observation_id":"ac90f6a5-cc9c-439e-8548-f698bcd1c7f9","resolution":{"observed_at":"2026-05-13T04:52:16.593822Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.21533","last_updated":"2026-05-19T22:29:19Z","snapshot_observed_at":"2026-08-02T05:35:23.334080Z","submitted_at":"2026-05-19T22:29:19Z","title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","version":1},"reference_index":106,"source":"pdf_text","source_observed_at":"2026-05-22T00:57:40.683341Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.21533"},"observation_digest":"sha256:bca567cbacf56a6e1b2b85ae3b5273d1bf4090f5e470d852579d7b10ac319a42","observation_id":"dc0f8f2a-b68e-423f-88b8-454ee164a6a7","resolution":{"observed_at":"2026-05-22T01:00:51.658248Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.25076","last_updated":"2026-05-24T13:39:39Z","snapshot_observed_at":"2026-08-02T03:13:12.097021Z","submitted_at":"2026-05-24T13:39:39Z","title":"Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-06-29T23:58:23.049086Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.25076"},"observation_digest":"sha256:6b2571a072265f334beca9fd35b130501128dbfaf73c211bc0c2c045bce6b6af","observation_id":"49a8b4b4-7712-4e70-a4be-7b10f932a414","resolution":{"observed_at":"2026-06-30T00:04:06.247394Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2605.25705","last_updated":"2026-05-25T11:03:23Z","snapshot_observed_at":"2026-07-06T23:35:36.158984Z","submitted_at":"2026-05-25T11:03:23Z","title":"Ces\\`aro convergence of the high-order WKB method and its applications to black-hole overtones and long-lived modes","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-29T20:43:00.569439Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2605.25705"},"observation_digest":"sha256:9bc1c3d3633c2405cd5a30307795263b6f96f460adaeb5cf5e66e01720a058f9","observation_id":"a212e6a5-5fd9-4db5-8b3d-ce566bf973f2","resolution":{"observed_at":"2026-06-29T20:43:58.811190Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2606.03842","last_updated":"2026-06-02T16:21:06Z","snapshot_observed_at":"2026-08-08T00:18:33.937793Z","submitted_at":"2026-06-02T16:21:06Z","title":"Scattering and Hawking Radiation from Einstein--Euler--Heisenberg--de Sitter Black Holes","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-06-28T08:52:29.167858Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2606.03842"},"observation_digest":"sha256:1c49c1c08cb5eb318e67ed3079817ee7a4726f24b5754507d44b2f507b71ed44","observation_id":"06cfc2b0-ae24-445c-923e-8bc03c0aa7c5","resolution":{"observed_at":"2026-07-02T04:46:38.398146Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":"2405.06390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-07-02T22:07:26.280218Z","title":"Skvortsova, Fortsch","venue":null,"work_id":"8a1dd7ca-e3fc-42a2-b4fe-d8654d8f4514","year":2024},"citing_paper":{"arxiv_id":"2606.08351","last_updated":"2026-07-18T16:56:07Z","snapshot_observed_at":"2026-08-02T12:12:04.199571Z","submitted_at":"2026-06-06T21:52:07Z","title":"Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-06-27T19:13:05.039350Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2606.08351"},"observation_digest":"sha256:8f68a6a644d6e6bb8e6e0bf4ed0e71c81a1459186b42e5cc93b7ab580c243a0e","observation_id":"ab62e6fb-2fa6-4f49-b7e6-3e07d9f2a773","resolution":{"observed_at":"2026-07-02T22:07:26.281935Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-02T12:12:04.979800Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.08351","last_updated":"2026-07-18T16:56:07Z","snapshot_observed_at":"2026-08-02T12:12:04.199571Z","submitted_at":"2026-06-06T21:52:07Z","title":"Hawking Emission from Black Holes Evaporating toward Wormholes and the Accuracy of the WKB Approximation","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-02T12:12:04.979800Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2606.08351"},"observation_digest":"sha256:0d5081536dc283c6f0058841940a92e118034905452780db52d28cfe26f2061a","observation_id":"a54ea0b9-0e34-41d9-be30-778350d23cf7","resolution":{"observed_at":"2026-08-02T12:12:04.979800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2405.06390/citation-record","integrity":"/paper/2405.06390/integrity","json":"/paper/2405.06390/citation-record.json","paper":"/paper/2405.06390"},"outbound":[],"paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-08T23:56:28.028367Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of 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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 24 inbound Pith citation observations for arXiv:2405.06390."}