{"as_of":"2026-08-23T04:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d314bbc1ddc1ab7ef7efbcf3cd89d58f7eaeac11f8c91e5a279140e08fa038c0","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":18,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":18,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":18,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":18,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:07:01.972960Z","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":"2026-07-02T14:57:04.954990Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-11T23:23:23.429506Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02740","last_updated":"2024-12-26T13:10:17Z","snapshot_observed_at":"2026-08-20T08:05:13.099504Z","submitted_at":"2024-12-03T19:00:00Z","title":"Regular black holes from thin-shell collapse","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T23:23:23.429506Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2412.02740"},"observation_digest":"sha256:bc7af33c4e82262e3a4bc973561b0ba4c5aab3156fc58fe82f494b20d9ce6eee","observation_id":"87aafb40-f1e9-4f01-b3fe-1147be954f49","resolution":{"observed_at":"2026-08-11T23:23:23.429506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-11T23:13:50.148765Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02742","last_updated":"2024-12-26T13:14:58Z","snapshot_observed_at":"2026-08-20T09:56:09.183175Z","submitted_at":"2024-12-03T19:00:01Z","title":"Dynamical Formation of Regular Black Holes","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T23:13:50.148765Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2412.02742"},"observation_digest":"sha256:6146319d6afdd7498e8eb64a61186705244a08af2f02b48ddfb6a205b3752fb3","observation_id":"917b55a7-57e2-42a0-99fb-df08495eb7a9","resolution":{"observed_at":"2026-08-11T23:13:50.148765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-11T22:19:34.613439Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.04513","last_updated":"2024-12-04T19:43:42Z","snapshot_observed_at":"2026-08-18T22:31:19.274911Z","submitted_at":"2024-12-04T19:43:42Z","title":"Quasinormal Modes and GUP-Corrected Hawking Radiation of BTZ Black Holes within Modified Gravity Frameworks","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T22:19:34.613439Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2412.04513"},"observation_digest":"sha256:9fbe359cada8ff21d29668afbc03f1b3e88d5dcfdf67ca7669d8e63deb254401","observation_id":"d1880d72-0f2c-472c-bc3d-d741cde4b0d4","resolution":{"observed_at":"2026-08-11T22:19:34.613439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-16T05:07:01.972960Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.21460","last_updated":"2025-04-30T09:28:08Z","snapshot_observed_at":"2026-08-19T07:37:04.903731Z","submitted_at":"2025-04-30T09:28:08Z","title":"Scalar quasinormal modes, Lyapunov exponents and radii of null geodesics of rotating regular black holes","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-16T05:07:01.972960Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2504.21460"},"observation_digest":"sha256:310bf778533a354b7ae7d670fff008f71b8ed98a6f44459faa591049c5a7284d","observation_id":"b1770648-885a-41de-a629-cd1e0489f6ee","resolution":{"observed_at":"2026-08-16T05:07:01.972960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-15T23:36:25.475934Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.04427","last_updated":"2025-07-09T11:45:45Z","snapshot_observed_at":"2026-08-18T04:02:25.773956Z","submitted_at":"2025-05-07T13:58:30Z","title":"Topological regular black holes without Cauchy horizon","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T23:36:25.475934Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2505.04427"},"observation_digest":"sha256:dcd9f2f27c19a1f104d6e6f53e9f83c3c371d25c9c5aefe1bf0da03943689288","observation_id":"00fdc768-cc35-4051-b989-8bce4f0b3d60","resolution":{"observed_at":"2026-08-15T23:36:25.475934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-15T21:44:35.574123Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.09680","last_updated":"2025-05-14T18:00:01Z","snapshot_observed_at":"2026-08-22T08:51:43.849292Z","submitted_at":"2025-05-14T18:00:01Z","title":"Regular black holes from Oppenheimer-Snyder collapse","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T21:44:35.574123Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2505.09680"},"observation_digest":"sha256:45673bf78f906fc6063bf7cae237001b791eb292c3b0f9a6ec87a2f6b426cff9","observation_id":"4af9f265-17b8-4118-8508-2e488dae6ce5","resolution":{"observed_at":"2026-08-15T21:44:35.574123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2507.09563","last_updated":"2026-05-16T07:57:18Z","snapshot_observed_at":"2026-07-06T21:56:19.049474Z","submitted_at":"2025-07-13T10:11:01Z","title":"Light Rings, Accretion Disks and Shadows of Hayward Boson Stars","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-21T23:42:13.280581Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2507.09563"},"observation_digest":"sha256:fa6da3617323f7bb6fbd98e03308a2e66980bb6d48f3a161a8810c231f2f61fe","observation_id":"d76ed025-dba8-49f0-8ff8-0802296e975c","resolution":{"observed_at":"2026-05-21T23:44:26.693627Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-08-20T21:51:54.591455Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:b7252b10b80e35ddce38bbdd32ce99a3a29e2fc254974f5caeb38b98417d7a00","observation_id":"6e8a4512-882c-4974-971f-86b7d879e4d9","resolution":{"observed_at":"2026-05-16T14:41:02.413851Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2601.10806","last_updated":"2026-05-01T06:09:01Z","snapshot_observed_at":"2026-08-11T07:16:11.663114Z","submitted_at":"2026-01-15T19:15:58Z","title":"Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-16T13:33:18.133767Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2601.10806"},"observation_digest":"sha256:6a358c41b3dc3d96f8e02294ba3ead926533c3128862ae102723501b9f39fca7","observation_id":"43630147-34cf-44f0-ab5f-ca80924f9dec","resolution":{"observed_at":"2026-05-16T13:37:57.182794Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-08-17T14:14:00.331787Z","submitted_at":"2026-01-29T21:33:15Z","title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-21T14:22:03.468102Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:ec1b1883b5d6ddd51f3f48a5d47845fd14191ec20f7f0f1e975cf13fc2173978","observation_id":"402ad882-c740-4e3f-95f8-33a53b29db08","resolution":{"observed_at":"2026-05-21T14:24:13.215893Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-08-17T14:14:00.331787Z","submitted_at":"2026-01-29T21:33:15Z","title":"Grey-body factors of higher dimensional regular black holes in quasi-topological theories","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-25T07:20:50.943166Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:7ccbc0e8046ef0ab52d8d7cd548ac8512eba6ce930b2661baecbbbbc0f0232a3","observation_id":"4befbfce-96c7-4ecb-9ff6-c4c61b436d81","resolution":{"observed_at":"2026-05-25T07:25:29.744737Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2604.13613","last_updated":"2026-04-15T08:26:47Z","snapshot_observed_at":"2026-07-06T23:01:32.542040Z","submitted_at":"2026-04-15T08:26:47Z","title":"From Ringdown to Lensing: Analytic Eikonal Modes of Quasi-Topological Regular Black Holes","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:29.598674Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2604.13613"},"observation_digest":"sha256:1ef030265fc03d442793a2a5e8054ee5d4b1ab8bc9ee09652e2d00621f57cd37","observation_id":"90bbdd6d-7d5d-415d-8258-2197535720c0","resolution":{"observed_at":"2026-05-10T13:00:24.809960Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2606.06355","last_updated":"2026-06-22T12:59:38Z","snapshot_observed_at":"2026-07-06T23:46:10.612537Z","submitted_at":"2026-06-04T16:23:24Z","title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","version":2},"reference_index":300,"source":"pdf_text","source_observed_at":"2026-06-28T00:05:44.496054Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2606.06355"},"observation_digest":"sha256:d7e6231a31320a7607f5f00db96283f04c81caaf264abdfe1791a5bb0342aca8","observation_id":"461b016e-6d9c-43bf-8132-1836955dde8f","resolution":{"observed_at":"2026-07-02T14:57:04.956379Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-12T01:38:05.217536Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-20T21:29:40.209208Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-12T01:38:05.217536Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:bc50ad9ca001693679fca23167e520583b0bb358f8beb93ed9dd4cde3a9a29e1","observation_id":"47176017-a06d-49e4-812f-dec4a196e4dd","resolution":{"observed_at":"2026-07-12T01:38:05.217536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-02T08:53:13.190371Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-20T21:29:40.209208Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-02T08:53:13.190371Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:3d3fa80f98d70fb8c3ae133434de7b7e285d7e70ac8b838c5ae66f45a86b2ea8","observation_id":"011ce4bf-4bf8-45d4-9797-7b2298f0af62","resolution":{"observed_at":"2026-08-02T08:53:13.190371Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-02T03:36:02.625787Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.13857","last_updated":"2026-07-15T14:02:52Z","snapshot_observed_at":"2026-08-18T10:37:50.336246Z","submitted_at":"2026-07-15T14:02:52Z","title":"Evaporating cosmologically coupled black holes","version":1},"reference_index":154,"source":"pdf_text","source_observed_at":"2026-08-02T03:36:02.625787Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2607.13857"},"observation_digest":"sha256:ba322d540d4ae1f7d42f52d54c762532fdc833f965ded33f22507caaa31264a0","observation_id":"8c8f29fe-fe9d-47bf-a180-8e626a0e9dd5","resolution":{"observed_at":"2026-08-02T03:36:02.625787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-08-01T02:56:25.803156Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.25311","last_updated":"2026-07-28T05:48:30Z","snapshot_observed_at":"2026-08-15T12:46:47.639945Z","submitted_at":"2026-07-28T05:48:30Z","title":"Parametrized beyond-Teukolsky framework in the time domain","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-01T02:56:25.803156Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2607.25311"},"observation_digest":"sha256:04c5b0c4de347b354cebff5b51a3948659f5be5a59cfd89465b77646ebb7422f","observation_id":"0466261f-df58-4936-b0b9-d613101f4c80","resolution":{"observed_at":"2026-08-01T02:56:25.803156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-30T12:35:24.779697Z","title":"Pedrotti and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.27053","last_updated":"2026-07-29T15:44:42Z","snapshot_observed_at":"2026-08-18T23:08:57.828461Z","submitted_at":"2026-07-29T15:44:42Z","title":"Discrete symmetries of modified Teukolsky equations","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-30T12:35:24.779697Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2607.27053"},"observation_digest":"sha256:0bf22a0b22446fa65c3e379432d40c1cdda557b71daa24d561d34870ddc2a09c","observation_id":"70a79064-b0df-456f-91b4-847d9562899e","resolution":{"observed_at":"2026-07-30T12:35:24.779697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.07589/citation-record","integrity":"/paper/2404.07589/integrity","json":"/paper/2404.07589/citation-record.json","paper":"/paper/2404.07589"},"outbound":[],"paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-18T22:31:06.132815Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular 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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:2404.07589."}