{"as_of":"2026-08-08T03:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6a103607105902bb8780f523b53c1f1b229610abfa4dea4bd1077d662afebb13","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":23,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":23,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":23,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":23,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:46:17.779922Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T14:47:14.283401Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-07T04:46:17.779922Z","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":80,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.779922Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:99dfd4101929099aa8b798a3fe2438ca1914b65c5ff943633983f16e291195d9","observation_id":"caced46a-a075-490f-9f97-a438771614d0","resolution":{"observed_at":"2026-08-07T04:46:17.779922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-05T19:07:37.824315Z","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":81,"source":"pdf_text","source_observed_at":"2026-08-05T19:07:37.824315Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2508.13366"},"observation_digest":"sha256:99aac4604c2194ea088365b3fb3c056c158a3d6afd673af0af844a76b5e75ab9","observation_id":"4e48a62e-602b-40eb-aec0-10a9baf520f9","resolution":{"observed_at":"2026-08-05T19:07:37.824315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-04T11:09:54.996908Z","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":96,"source":"pdf_text","source_observed_at":"2026-08-04T11:09:54.996908Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2510.06689"},"observation_digest":"sha256:d79882945fabe09bc9e5fb087cfe96c9c3231ef9ed58ff58a6d840c5aa29349e","observation_id":"e98f2916-540b-4d0b-9746-f988529a2ea6","resolution":{"observed_at":"2026-08-04T11:09:54.996908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-03T22:11:08.080439Z","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":68,"source":"pdf_text","source_observed_at":"2026-08-03T22:11:08.080439Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2511.12335"},"observation_digest":"sha256:bb07be501e5386c010ad4fbef575f0a8ac4591e3ad725fac62ed3c2e5d8d186e","observation_id":"32dca6a8-a7a8-425e-8a0d-2e9e73135350","resolution":{"observed_at":"2026-08-03T22:11:08.080439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":149,"source":"pdf_text","source_observed_at":"2026-05-16T11:06:54.209646Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2601.17906"},"observation_digest":"sha256:3a8de4835a3d9801b2f194730dd3825333cf27c2389c4c5ad7ccd798d3ebdd06","observation_id":"88330aab-a63a-47e2-89f6-6ae527808d8c","resolution":{"observed_at":"2026-05-16T11:07:47.286384Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":102,"source":"pdf_text","source_observed_at":"2026-05-16T02:41:01.645151Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2602.11001"},"observation_digest":"sha256:a0cb6dd1c20d08382fe2b00bb5d19eff0dd685ca2acef965ac4649bb1211d260","observation_id":"351c06a6-9290-41a8-85d8-e044f7c7361e","resolution":{"observed_at":"2026-05-16T02:42:10.947927Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":195,"source":"pdf_text","source_observed_at":"2026-05-15T13:15:54.975020Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2603.10844"},"observation_digest":"sha256:d4431d360ce7e471a5fbd339350fefb34b39cc71cc1ef145bbedcaae21f32814","observation_id":"250a0a44-330c-48d5-9036-598d6e11c26b","resolution":{"observed_at":"2026-05-15T13:20:02.688472Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-04T05:43:13.529895Z","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":"2026-08-07T15:27:22.728093Z","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":106,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:13.529895Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2603.28415"},"observation_digest":"sha256:a1a7849545d1e896b8c79247bdb70373bfd04b71bedf3394e29bc129efa43439","observation_id":"23a30814-dfa7-40ff-bf3f-add6e4922453","resolution":{"observed_at":"2026-08-04T05:43:13.529895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":66,"source":"pdf_text","source_observed_at":"2026-05-10T15:10:05.638518Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2604.11845"},"observation_digest":"sha256:452c7c586711d1f07b551425be4ca846708fafcc1e9764af9f5e91efb5dd8a5b","observation_id":"f14906c8-ca6a-4be3-a31d-b853e49ec233","resolution":{"observed_at":"2026-05-11T11:06:03.007417Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":64,"source":"pdf_text","source_observed_at":"2026-05-08T02:18:25.796367Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:7c5e15935482d3dd89b3cb2f6b00890f4bc1dfbd1cdea52ed638cbbbdf1b59f4","observation_id":"d92b5a3d-a801-49f0-86c9-f8b0015f9c98","resolution":{"observed_at":"2026-05-11T22:51:23.824215Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":64,"source":"pdf_text","source_observed_at":"2026-05-14T22:18:47.797399Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:a02af330101a5ec39103b0876ed730f29c06b369ea6bf0c987bd0cb3ddf6baa3","observation_id":"89e0f004-5aee-40d8-804b-b81c3a035e34","resolution":{"observed_at":"2026-05-14T22:19:31.505355Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":153,"source":"pdf_text","source_observed_at":"2026-05-07T15:29:43.270538Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2604.25471"},"observation_digest":"sha256:7c3a40a54a7dfb8605b708664c8d677a0ca661c3fcc6bc4f4096a3cb7a2434f2","observation_id":"b427a76d-2a13-4429-af3c-374f25d8c6bd","resolution":{"observed_at":"2026-05-12T00:21:19.188525Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":92,"source":"pdf_text","source_observed_at":"2026-05-07T14:06:56.581854Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.03659"},"observation_digest":"sha256:de564504770b926354994b1b97847f661f8bff95f4f77af6e3a9e03d2cd4451d","observation_id":"e60d300c-2427-43a5-b878-99582a935047","resolution":{"observed_at":"2026-05-12T00:46:14.260513Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":148,"source":"pdf_text","source_observed_at":"2026-05-13T01:58:50.185004Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.11013"},"observation_digest":"sha256:21dae0ec78ebede8766a12c02a28a57dfa04b217e3263923906335e71092c637","observation_id":"cda49ca1-4815-4b02-80bd-7c25219833e4","resolution":{"observed_at":"2026-05-13T02:02:06.667191Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":109,"source":"pdf_text","source_observed_at":"2026-05-13T02:39:27.974688Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.11364"},"observation_digest":"sha256:2152ceaaffd95b3480f80173d0117f39b4b2b1d7cea89659f2829516f5f418a3","observation_id":"bd74df0a-1f7f-4d9b-b8f7-be9ae8880255","resolution":{"observed_at":"2026-05-13T02:42:09.050774Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":90,"source":"pdf_text","source_observed_at":"2026-05-13T04:51:34.508568Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.12113"},"observation_digest":"sha256:e197baa99377b922e87d640b9d53cc8a8babdc63cda8afc8946945754c7de693","observation_id":"0557950a-103a-4bd6-863d-313e76f542d2","resolution":{"observed_at":"2026-05-13T04:52:16.410743Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":112,"source":"pdf_text","source_observed_at":"2026-05-22T00:57:40.683341Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.21533"},"observation_digest":"sha256:e5f0dc5c7bdceb3f4d21abe4fb681d4510446f64f679f167c44067a44cd2e0bc","observation_id":"fd787f4c-a764-4435-a6c4-894ceb21bf67","resolution":{"observed_at":"2026-05-22T01:00:51.646921Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":6,"source":"pdf_text","source_observed_at":"2026-06-29T23:58:23.049086Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.25076"},"observation_digest":"sha256:5b87339169b831e7ec57c260dc9b6f115807beb3d34f07c27001e3fb9f398b6c","observation_id":"fba60f8d-cc8b-41f6-bff4-a88315006974","resolution":{"observed_at":"2026-06-30T00:04:06.237770Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"citing_paper":{"arxiv_id":"2605.28917","last_updated":"2026-05-27T17:57:30Z","snapshot_observed_at":"2026-07-06T23:38:27.990823Z","submitted_at":"2026-05-27T17:57:30Z","title":"Greybody Factors, Absorption Cross Sections and Hawking Radiation of Holonomy-Corrected Schwarzschild Black Holes","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-06-29T10:32:37.980036Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2605.28917"},"observation_digest":"sha256:1807fc32b83277ea982f6eb85d316ea27839fda5676329b91f8060b1e348a265","observation_id":"75459cd1-0572-447a-968d-480bf708a155","resolution":{"observed_at":"2026-06-29T10:33:18.643474Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":20,"source":"pdf_text","source_observed_at":"2026-06-28T08:52:29.167858Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2606.03842"},"observation_digest":"sha256:f4a9aca32820fbad161aa30b81ae3227b746161b74f0369e145574437a57afa0","observation_id":"192e00c0-4dca-4642-835b-54d4991d9656","resolution":{"observed_at":"2026-07-02T04:46:38.220480Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"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":68,"source":"pdf_text","source_observed_at":"2026-06-27T19:13:05.039350Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2606.08351"},"observation_digest":"sha256:337c18e1b9a63e01e4ef34c8cb1b7e209c622b9c613bcc9746d73a82feb921cc","observation_id":"2ff483d4-4cc3-4db8-9482-9d49e58227c4","resolution":{"observed_at":"2026-07-02T22:07:26.285498Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-02T12:12:04.780353Z","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":29,"source":"pdf_text","source_observed_at":"2026-08-02T12:12:04.780353Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2606.08351"},"observation_digest":"sha256:227b3c46cbb4b319f85fb81a2f8e0a488f45adab2c75c2106039a7b5a38c1372","observation_id":"129dc1f6-5564-44a8-86c5-e3f1e28675fb","resolution":{"observed_at":"2026-08-02T12:12:04.780353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":"2311.11650","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-07-10T14:47:14.283401Z","title":"Skvortsova, Fortsch","venue":"gr-qc","work_id":"2dd91879-91dc-466c-ba6b-d5ee3127c545","year":2023},"citing_paper":{"arxiv_id":"2607.07955","last_updated":"2026-07-08T22:22:08Z","snapshot_observed_at":"2026-08-02T01:08:18.902253Z","submitted_at":"2026-07-08T22:22:08Z","title":"Wave and particle probes of a regular T-duality-inspired black hole with gravitational self-energy","version":1},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-07-10T14:46:36.212660Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2607.07955"},"observation_digest":"sha256:01b6fd7ae19d0ee9a6de364d06a55ae51885056dee8039886f0de409882c4250","observation_id":"b03723c0-422b-4851-b742-9298b28d3076","resolution":{"observed_at":"2026-07-10T14:47:14.284752Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2311.11650/citation-record","integrity":"/paper/2311.11650/integrity","json":"/paper/2311.11650/citation-record.json","paper":"/paper/2311.11650"},"outbound":[],"paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS 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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 inbound Pith citation observations for arXiv:2311.11650."}