{"as_of":"2026-08-09T10:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9fa807073f0851f88e9111b785525dbf0c70f4cfb88a0d8d53883334b89d5bb6","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":37,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":37,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":37,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":37,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T18:28:50.614395Z","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":"2026-07-10T14:47:14.105906Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2501.16433","last_updated":"2026-05-13T15:28:20Z","snapshot_observed_at":"2026-08-02T14:23:16.098022Z","submitted_at":"2025-01-27T19:00:06Z","title":"Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects","version":3},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-05-23T04:43:04.006726Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2501.16433"},"observation_digest":"sha256:d602fc7fc37c60d7e5881cbb0a4e322e536d678daa6c7f1f4f96bef57b2a70ba","observation_id":"2d8f2aa8-6777-45e9-a122-5c25248299c7","resolution":{"observed_at":"2026-05-23T04:45:25.170674Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-08T18:28:50.614395Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.05689","last_updated":"2025-05-28T21:22:04Z","snapshot_observed_at":"2026-08-08T18:19:26.524368Z","submitted_at":"2025-02-08T20:44:31Z","title":"Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-08T18:28:50.614395Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2502.05689"},"observation_digest":"sha256:e08c81a876042a5ff2ab6e5e4991bcded15467aaa80b77fea2ec750fd0dd44d7","observation_id":"163ee136-049d-4367-a386-36f3566127e7","resolution":{"observed_at":"2026-08-08T18:28:50.614395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-07T13:41:54.146612Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.21303","last_updated":"2025-07-03T13:24:54Z","snapshot_observed_at":"2026-08-09T07:03:52.800027Z","submitted_at":"2025-05-27T15:05:21Z","title":"Spectrum instability and greybody factor stability for parabolic approximation of Regge-Wheeler potential","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T13:41:54.146612Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2505.21303"},"observation_digest":"sha256:5102fd2f8b668a40faef8f3c55955bf4ef25f3b72488ae2ee233bd2cfc31ce4e","observation_id":"455930bf-e705-4bb3-a07a-ee43c9f0378a","resolution":{"observed_at":"2026-08-07T13:41:54.146612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2506.16217","last_updated":"2026-04-06T09:35:14Z","snapshot_observed_at":"2026-07-06T21:44:42.748650Z","submitted_at":"2025-06-19T11:09:00Z","title":"Quasinormal modes and grey-body factors of axial gravitational perturbations of regular black holes in asymptotically safe gravity","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-19T09:05:31.241151Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2506.16217"},"observation_digest":"sha256:ec590d4809fb5001247cfe8e6f5294aa455bac902a43fd4e392dfb7aec425598","observation_id":"524b7423-4a54-4a1d-9134-468918d4064d","resolution":{"observed_at":"2026-05-19T09:07:14.364717Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-04T08:24:54.944659Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.21256","last_updated":"2026-07-02T11:53:26Z","snapshot_observed_at":"2026-08-07T14:03:10.430414Z","submitted_at":"2025-10-24T08:41:53Z","title":"Exact Regions of Superradiant Instability of Kerr-Newman Black Holes and Massive Scalar Fields","version":4},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-04T08:24:54.944659Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2510.21256"},"observation_digest":"sha256:538837ba9d6b792f1953ddd0461c1fe65b0b4005a75aa8a1e4aa7f8c15039474","observation_id":"5fd4637a-4a99-467e-a2b9-a3df931a212a","resolution":{"observed_at":"2026-08-04T08:24:54.944659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-03T18:08:26.291697Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.07291","last_updated":"2026-07-24T05:07:32Z","snapshot_observed_at":"2026-08-04T03:47:00.493724Z","submitted_at":"2025-12-08T08:31:25Z","title":"Revisiting PBH accretion, evaporation and their cosmological consequences","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T18:08:26.291697Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2512.07291"},"observation_digest":"sha256:fd7bf7013621d0f5dac7828a3805639dd14f78f3f591645b3f603e3ec7f41af4","observation_id":"43171b4e-9606-4e8a-8f1e-76ac9e6f9cd7","resolution":{"observed_at":"2026-08-03T18:08:26.291697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2512.23510","last_updated":"2026-04-08T06:40:48Z","snapshot_observed_at":"2026-07-06T22:40:17.725041Z","submitted_at":"2025-12-29T14:47:19Z","title":"Quasinormal mode/grey-body factor correspondence for Kerr black holes","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-16T19:26:13.414782Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2512.23510"},"observation_digest":"sha256:f72c2e72c3a8d21cfa7295829e9caa808213700d3df682fa14ab5c2e5d0c5c65","observation_id":"4bf49f7f-85e0-41a1-a23a-7fc05de57777","resolution":{"observed_at":"2026-05-16T19:28:20.204790Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2601.18613","last_updated":"2026-01-26T15:53:33Z","snapshot_observed_at":"2026-07-06T22:43:02.453697Z","submitted_at":"2026-01-26T15:53:33Z","title":"Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-16T10:39:53.182650Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2601.18613"},"observation_digest":"sha256:501262ce506fa67df86610601bfb146c77e4b0cf9482dc22cc9e73422835baa1","observation_id":"cff5ad2b-954c-4471-aac9-7077600e716b","resolution":{"observed_at":"2026-05-16T10:40:50.968077Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-07-06T22:43:35.226546Z","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":108,"source":"pdf_text","source_observed_at":"2026-05-21T14:22:03.468102Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:0df3419fdfd87cd409d98a7b786c0e9688fe473d0f58ca76ebc6f9bfbbdca61a","observation_id":"4e9c4e7b-7a4b-4f35-8231-a81cda721673","resolution":{"observed_at":"2026-05-21T14:24:13.439766Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2601.22340","last_updated":"2026-05-22T03:16:49Z","snapshot_observed_at":"2026-07-06T22:43:35.226546Z","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":108,"source":"pdf_text","source_observed_at":"2026-05-25T07:20:50.943166Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2601.22340"},"observation_digest":"sha256:857bd7f71ba9db0b78c9b793d936ac099d9bf7e3316cb7f0733c9c751b90a367","observation_id":"81a7ed07-5eb8-470c-9034-e7cf3bc8e197","resolution":{"observed_at":"2026-05-25T07:25:29.691378Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":222,"source":"pdf_text","source_observed_at":"2026-05-15T13:15:54.975020Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2603.10844"},"observation_digest":"sha256:9beb9d1bc74a324c175df3dafeb0010cc2169ae1d4e4e00a7c8aa6616a055f72","observation_id":"cdd4de9c-6dc0-4358-8877-5a2ac61e9e68","resolution":{"observed_at":"2026-05-15T13:20:02.742157Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-04T05:43:13.598016Z","title":null,"venue":null,"work_id":null,"year":2025},"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":130,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:13.598016Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2603.28415"},"observation_digest":"sha256:b6f3f21c8e89d34a719e8cc29e5e529eda6febb0231bcb4561d89f86321aa663","observation_id":"0faec741-2a8f-402d-9a2e-af0e3b7f5682","resolution":{"observed_at":"2026-08-04T05:43:13.598016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2604.05084","last_updated":"2026-04-06T18:37:06Z","snapshot_observed_at":"2026-07-06T22:53:55.926521Z","submitted_at":"2026-04-06T18:37:06Z","title":"Parametrized quasinormal modes, greybody factors and their correspondence","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-10T18:56:32.433489Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.05084"},"observation_digest":"sha256:f7bcdeb0eb7f99aa4a2208d9ee1b7b2aad3f5d23e59f9d9ee3722fa0905683dc","observation_id":"643f177e-0443-4cae-a3b8-8aa2609acfe6","resolution":{"observed_at":"2026-05-10T23:40:52.823871Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":97,"source":"pdf_text","source_observed_at":"2026-05-10T15:10:05.638518Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.11845"},"observation_digest":"sha256:4d16e66b8919dd7b89861e03ba5fd7ec9a67459221913a09797fe971c66ef918","observation_id":"d7477cf2-e3d4-42a7-9920-77734567ca52","resolution":{"observed_at":"2026-05-11T11:06:03.392090Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2604.14999","last_updated":"2026-05-09T20:33:29Z","snapshot_observed_at":"2026-07-06T23:02:40.364114Z","submitted_at":"2026-04-16T13:25:15Z","title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","version":1},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-05-10T10:46:09.790506Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.14999"},"observation_digest":"sha256:4461749bac7cfccb972841864bfdbdb09dbde684c80eacaeb214ef8bf2549353","observation_id":"148e9065-424c-45a2-b7a6-6056a31e7846","resolution":{"observed_at":"2026-05-10T10:49:56.519579Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2604.14999","last_updated":"2026-05-09T20:33:29Z","snapshot_observed_at":"2026-07-06T23:02:40.364114Z","submitted_at":"2026-04-16T13:25:15Z","title":"A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric","version":2},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-05-12T01:50:35.608231Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.14999"},"observation_digest":"sha256:8580a92899c40e4f9546ad24aa8e7ae330ed91bb8cc2557405690c82e871c241","observation_id":"0a7298cc-a395-4817-98c7-41009c1f1ec2","resolution":{"observed_at":"2026-05-12T01:51:14.592534Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2604.20066","last_updated":"2026-07-06T16:43:24Z","snapshot_observed_at":"2026-07-16T23:18:42.504670Z","submitted_at":"2026-04-22T00:12:23Z","title":"Regular Black Holes in General Relativity from Nonlinear Electrodynamics with de Sitter Cores","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-10T00:41:07.975731Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.20066"},"observation_digest":"sha256:81b59951dfbd3fb456e8e1c85fdd74a96ae11badcc1d26e16e8c675850860368","observation_id":"51e60233-2942-4e0c-858d-9953520f812c","resolution":{"observed_at":"2026-05-11T13:41:10.646717Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-12T18:47:29.314206Z","title":"Correspondence be- tween grey-body factors and quasinormal frequencies for rotating black holes,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2604.20066","last_updated":"2026-07-06T16:43:24Z","snapshot_observed_at":"2026-07-16T23:18:42.504670Z","submitted_at":"2026-04-22T00:12:23Z","title":"Regular Black Holes in General Relativity from Nonlinear Electrodynamics with de Sitter Cores","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-12T18:47:29.314206Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.20066"},"observation_digest":"sha256:45f7fabd02a8e7b8ca5e021ede0f527194500137a6c9a6a58aa2c539ae70c5d9","observation_id":"66b52647-3b3f-45bd-bfd3-09ad55135ce1","resolution":{"observed_at":"2026-07-12T18:47:29.314206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":105,"source":"pdf_text","source_observed_at":"2026-05-08T02:18:25.796367Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:6021d2ccfd4c55956127ed83583f816d696052c48fb01a9714b2a7d3afcc2aac","observation_id":"b6935a90-eb81-4fc1-a716-a7e98ecc13fc","resolution":{"observed_at":"2026-05-11T22:51:27.790514Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":105,"source":"pdf_text","source_observed_at":"2026-05-14T22:18:47.797399Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:0ec2c21e0ce5b44ccab24de1e636184a22752eb8b79b47e8eb75476577c3eeda","observation_id":"896bbc30-7f52-4f78-aaa9-807607535f2f","resolution":{"observed_at":"2026-05-14T22:19:31.355680Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":162,"source":"pdf_text","source_observed_at":"2026-05-07T15:29:43.270538Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.25471"},"observation_digest":"sha256:d2e60b880659b4246633340b0456879d51745d26a2590bfd3d8f19ae0b2f4549","observation_id":"13166c74-89d9-417f-bdc3-18f89afb4e0c","resolution":{"observed_at":"2026-05-12T00:21:20.476962Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2604.26166","last_updated":"2026-04-28T23:17:26Z","snapshot_observed_at":"2026-07-06T23:11:52.954360Z","submitted_at":"2026-04-28T23:17:26Z","title":"Scattering of electromagnetic field in quasi-topological gravity","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-07T14:54:38.809214Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2604.26166"},"observation_digest":"sha256:9c4d4ee27f4a1d3af9f015be0197da2e4f576f70c7ccf53944f054c1e64d685a","observation_id":"6890e3bd-b594-4feb-bea2-564581187b1f","resolution":{"observed_at":"2026-05-12T00:36:16.960235Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2605.03137","last_updated":"2026-05-04T20:22:29Z","snapshot_observed_at":"2026-07-06T23:16:05.372336Z","submitted_at":"2026-05-04T20:22:29Z","title":"Scattering of scalar, electromagnetic, and Dirac fields in an asymptotically flat regular black hole supported by primordial dark matter","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-07T02:21:14.281286Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.03137"},"observation_digest":"sha256:80eda79c1660d713bd23a6ffb70cc71fc52191bec45e8c1838c7c2099fefd6f1","observation_id":"9e86567f-7fd6-4ce3-b524-a0ccc5b04692","resolution":{"observed_at":"2026-05-12T10:46:30.341074Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":114,"source":"pdf_text","source_observed_at":"2026-05-07T14:06:56.581854Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.03659"},"observation_digest":"sha256:7e71728f6964a3c68b98faceac5152dd10bb80f0382de3bcb0bee9bf3bf650da","observation_id":"9e9362cf-fde7-4c09-bd4a-938ed087435c","resolution":{"observed_at":"2026-05-12T00:46:14.166188Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":158,"source":"pdf_text","source_observed_at":"2026-05-13T01:58:50.185004Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.11013"},"observation_digest":"sha256:9f21d4b5e649124f0abc5b349f82b6c74417787eecec31bb6ac6016619b2bc06","observation_id":"51d01d35-c7d6-44c1-b856-6b3037549358","resolution":{"observed_at":"2026-05-13T02:02:06.536434Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":126,"source":"pdf_text","source_observed_at":"2026-05-13T02:39:27.974688Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.11364"},"observation_digest":"sha256:77351f101720c11fec1c5514dd392f549602921c0e747c66ee44b6fd1bfcff49","observation_id":"e049a3a9-d983-4a46-a047-c22be6718dcb","resolution":{"observed_at":"2026-05-13T02:47:08.381110Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":94,"source":"pdf_text","source_observed_at":"2026-05-13T04:51:34.508568Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.12113"},"observation_digest":"sha256:d5c5cfc455597209e7da6e91289afca110f0180ceb12bc683141be8e26acfa75","observation_id":"3e1a2413-4784-4015-b4a0-c1bf39b4b1e0","resolution":{"observed_at":"2026-05-13T04:52:16.379612Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":123,"source":"pdf_text","source_observed_at":"2026-05-22T00:57:40.683341Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.21533"},"observation_digest":"sha256:e76a60bb7ba0fec57a9497be8dbd0fb7ed9fbc0f2f37cd622593e52608a0f8ce","observation_id":"d050d74f-399f-4103-a96b-06b6ba619a02","resolution":{"observed_at":"2026-05-22T01:00:51.938367Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":44,"source":"pdf_text","source_observed_at":"2026-06-29T23:58:23.049086Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.25076"},"observation_digest":"sha256:066d75007a2da8da49843f45afc41bafe1b0fd3777d0550565e543c62839d5ed","observation_id":"e478ea50-541f-4838-9cef-17835b01c9d7","resolution":{"observed_at":"2026-06-30T00:04:06.064684Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"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":8,"source":"pdf_text","source_observed_at":"2026-06-29T10:32:37.980036Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2605.28917"},"observation_digest":"sha256:bece556388c4ecff3af19f3b72fedf606420aa35e5ba97e2f9a339ef4f94823b","observation_id":"cf53b484-5cdf-4079-ac46-7863af1af0c1","resolution":{"observed_at":"2026-06-29T10:33:18.645096Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":81,"source":"pdf_text","source_observed_at":"2026-06-28T08:52:29.167858Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2606.03842"},"observation_digest":"sha256:fd4da01f512513bb80315541e4838200467760202d4659e11ef90be5830f8d10","observation_id":"8c214eb2-669b-44fe-b756-b650ed4bbbfd","resolution":{"observed_at":"2026-07-02T04:46:38.333718Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","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":72,"source":"pdf_text","source_observed_at":"2026-06-27T19:13:05.039350Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2606.08351"},"observation_digest":"sha256:deb22b478c6438a78c50dd5de6ea6bb2a8e16a2927db64103fb93c0610da0396","observation_id":"6e9e4849-01de-4f37-981d-16053df9ea74","resolution":{"observed_at":"2026-07-02T22:07:26.366321Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-02T12:12:04.997570Z","title":null,"venue":null,"work_id":null,"year":2025},"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":78,"source":"pdf_text","source_observed_at":"2026-08-02T12:12:04.997570Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2606.08351"},"observation_digest":"sha256:e0e025a7afb690e0aaa852cb800f01660dac005c7cff8bcb6351736dd6d1a2fd","observation_id":"8e01ff9e-1304-40d6-b065-0800c10e0f78","resolution":{"observed_at":"2026-08-02T12:12:04.997570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"citing_paper":{"arxiv_id":"2606.08631","last_updated":"2026-06-07T13:50:43Z","snapshot_observed_at":"2026-08-05T07:55:09.060783Z","submitted_at":"2026-06-07T13:50:43Z","title":"Hawking Radiation from the Dymnikova Regular Black Hole","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-06-27T18:03:03.482642Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2606.08631"},"observation_digest":"sha256:7317b9a77a22b1319d5fe8d2b041db8a3e83fc300b02b3decd96e7c2bbbb2ae4","observation_id":"70808624-5237-444f-9262-9085ebab0bc8","resolution":{"observed_at":"2026-07-02T23:37:28.034710Z","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-12T01:38:05.217536Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-09T06:27:29.882199Z","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":117,"source":"pdf_text","source_observed_at":"2026-07-12T01:38:05.217536Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:0abadd8e881b13eb1acbf3f3d73dff3848853ed162f9080171b43ea566d79fe4","observation_id":"b2b17fd5-8a90-4273-b387-fbce380916ec","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":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-08-02T08:53:13.682601Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-09T06:27:29.882199Z","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":143,"source":"pdf_text","source_observed_at":"2026-08-02T08:53:13.682601Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:7758604e5acf3f2d6b7282157ea8a69d7dcf2de8f3f6dfd6ed0eb448a0739642","observation_id":"ba1c5c13-1681-4bf6-85df-10c12bd8d68f","resolution":{"observed_at":"2026-08-02T08:53:13.682601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating black holes","version":2},"cited_work":{"arxiv_id":"2408.11162","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.11162","snapshot_observed_at":"2026-07-10T14:47:14.105906Z","title":"Konoplya and A","venue":"gr-qc","work_id":"5998b363-5cfd-49d6-b471-07a2278473a4","year":2024},"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":123,"source":"pdf_text","source_observed_at":"2026-07-10T14:46:36.212660Z"},"links":{"cited_paper":"/paper/2408.11162","citing_paper":"/paper/2607.07955"},"observation_digest":"sha256:54ba90cf5616b6d6c9bb4d08b7c24ce7567ac195bf169341971f7c3d29e5dfc2","observation_id":"22249493-718f-4a02-b984-521e97bc974a","resolution":{"observed_at":"2026-07-10T14:47:14.107126Z","resolver_source":"local_arxiv","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"}}],"links":{"evidence":"/evidence","html":"/paper/2408.11162/citation-record","integrity":"/paper/2408.11162/integrity","json":"/paper/2408.11162/citation-record.json","paper":"/paper/2408.11162"},"outbound":[],"paper":{"arxiv_id":"2408.11162","last_updated":"2025-01-30T11:23:21Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-06T00:33:13.793021Z","submitted_at":"2024-08-20T19:38:32Z","title":"Correspondence between grey-body factors and quasinormal frequencies for rotating 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 37 inbound Pith citation observations for arXiv:2408.11162."}