{"as_of":"2026-08-01T22:09:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c1a89b26affc2e1229de118ffb5b80793b81673597be8b6f1fa44e957603f353","coverage":[{"denominator":97,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":97,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-16T14:40:32.437670Z","state":"measured"},{"denominator":99,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":99,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-01T06:32:01.292127+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T02:56:25.868581Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.09607","snapshot_observed_at":"2026-08-01T02:56:25.868581Z","title":"De Simone, S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.25311","last_updated":"2026-07-28T05:48:30Z","snapshot_observed_at":"2026-08-01T02:56:15.147241Z","submitted_at":"2026-07-28T05:48:30Z","title":"Parametrized beyond-Teukolsky framework in the time domain","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-01T02:56:25.868581Z"},"links":{"cited_paper":"/paper/2601.09607","citing_paper":"/paper/2607.25311"},"observation_digest":"sha256:17d1f5607789a4d5eac7a6b04a2d47d187b5049bbce9dfe4fc48a16436224527","observation_id":"e01edd86-b597-4e28-aa7d-9cc50844bdc3","resolution":{"observed_at":"2026-08-01T02:56:25.868581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.09607","snapshot_observed_at":"2026-07-30T12:35:24.745339Z","title":"De Simone, S","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.27053","last_updated":"2026-07-29T15:44:42Z","snapshot_observed_at":"2026-08-01T21:48:47.569811Z","submitted_at":"2026-07-29T15:44:42Z","title":"Discrete symmetries of modified Teukolsky equations","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-30T12:35:24.745339Z"},"links":{"cited_paper":"/paper/2601.09607","citing_paper":"/paper/2607.27053"},"observation_digest":"sha256:f0fd1770f32d2109f9dccf5ff7af0cba120aaafd0185b84e725bb208bfb3b985","observation_id":"003264ba-3081-4fe0-b218-7edea91ecaae","resolution":{"observed_at":"2026-07-30T12:35:24.745339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2601.09607/citation-record","integrity":"/paper/2601.09607/integrity","json":"/paper/2601.09607/citation-record.json","paper":"/paper/2601.09607"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":"1602.03837","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-07-11T00:07:39.821374Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","venue":"gr-qc","work_id":"ab878228-151c-4a29-8026-a4308b076d30","year":2016},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:fe063c9ee138fc285168b3b3ccb555ae1d82af4006dfca68bc383a1b0df6411d","observation_id":"b31460a6-bd10-46ee-94e7-bf067823a17e","resolution":{"observed_at":"2026-05-16T14:41:02.539560Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":"1811.12907","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-07-09T20:06:29.259645Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","venue":"astro-ph.HE","work_id":"ed2ab6af-3b84-426b-a8d5-c1f2cb6b0af7","year":2018},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:5204900c898e6decc8488636c4c5c2dcc5c76bba4880c8456c59f2a35742e164","observation_id":"647a5b7a-0e96-4563-84e9-79500376506f","resolution":{"observed_at":"2026-05-16T14:41:02.542582Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14527","last_updated":"2021-03-08T18:36:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:31Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":3},"cited_work":{"arxiv_id":"2010.14527","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.14527","snapshot_observed_at":"2026-07-10T13:17:05.780253Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","venue":"gr-qc","work_id":"7410f8dd-43ce-418e-a2fe-baea0cf36999","year":2020},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2010.14527","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:01afb1b9be64f2bb6115901e70918d563361e36f3adf1f43acde455261b67640","observation_id":"e0cbc7c1-1f8e-4d8d-96ed-ccd61c413cd3","resolution":{"observed_at":"2026-05-16T14:41:02.559839Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01045","last_updated":"2022-05-10T14:16:51Z","snapshot_observed_at":"2026-07-29T23:10:57.700271Z","submitted_at":"2021-08-02T17:09:29Z","title":"GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":2},"cited_work":{"arxiv_id":"2108.01045","doi":"10.48550/arxiv.2108.01045","metadata_source":"pith","pith_arxiv_id":"2108.01045","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","venue":"gr-qc","work_id":"38dc3e43-0988-49cb-9c1d-d4ee3fffc8bb","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2108.01045","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:7e9a71a8d106421508f8f8b4ac2988acfa1b5a9d473ce968333256176cb91390","observation_id":"3271790c-9449-4c20-8805-3df8f10c335c","resolution":{"observed_at":"2026-05-16T14:41:02.545860Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03606","last_updated":"2023-10-23T13:37:50Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-11-05T16:43:17Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","version":3},"cited_work":{"arxiv_id":"2111.03606","doi":"10.48550/arxiv.2111.03606","metadata_source":"pith","pith_arxiv_id":"2111.03606","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","venue":"gr-qc","work_id":"da52a8d9-11a6-46c6-a2f5-89dab8381497","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2111.03606","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:9496b653473310271943f041718dc72321e2b501cd0a80431023e855d4c22fa4","observation_id":"7c29d392-ea5a-4c34-bdd5-18d8d95de3b7","resolution":{"observed_at":"2026-05-16T14:41:02.552055Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-05-25T07:54:10.687378+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-25T07:54:10.687378+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2508.18082","last_updated":"2026-06-26T11:38:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-08-25T14:46:09Z","title":"GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run","version":3},"cited_work":{"arxiv_id":"2508.18082","doi":"10.1103/physrevd.70.082001","metadata_source":"pith","pith_arxiv_id":"2508.18082","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run","venue":"gr-qc","work_id":"373a2c61-2309-4528-87c8-9053657b5ebd","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2508.18082","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:1da2d9aa17de4d93c6214677d6a4e6f6929642732c56e768d16c5c74fe73e004","observation_id":"aaba6276-6035-47d3-bb14-3bdff9fc63a4","resolution":{"observed_at":"2026-05-16T14:41:02.576854Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.08099","last_updated":"2025-09-09T19:17:32Z","snapshot_observed_at":"2026-07-06T22:27:20.170280Z","submitted_at":"2025-09-09T19:17:32Z","title":"Black Hole Spectroscopy and Tests of General Relativity with GW250114","version":1},"cited_work":{"arxiv_id":"2509.08099","doi":"10.48550/arxiv.2509.08099","metadata_source":"pith","pith_arxiv_id":"2509.08099","snapshot_observed_at":"2026-07-10T23:37:41.337655Z","title":"Black Hole Spectroscopy and Tests of General Relativity with GW250114","venue":"gr-qc","work_id":"dc4b2f4a-8133-4076-a219-13310060c8bd","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2509.08099","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:9aef9ee1a32809c7034a907953b7d095b69217a56d91bdacc05cc14ee892d577","observation_id":"93d0e003-223e-43e8-8403-ffac214f8276","resolution":{"observed_at":"2026-05-16T14:41:02.555889Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-05-24T02:23:07.710015+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T02:23:07.710015+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.23895","last_updated":"2025-08-24T14:24:16Z","snapshot_observed_at":"2026-08-01T14:00:16.213665Z","submitted_at":"2025-05-29T18:00:01Z","title":"Black hole spectroscopy: from theory to experiment","version":2},"cited_work":{"arxiv_id":"2505.23895","doi":"10.1088/1361-6382/ae59e2","metadata_source":"pith","pith_arxiv_id":"2505.23895","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Black hole spectroscopy: from theory to experiment","venue":"gr-qc","work_id":"d5c07d13-a0ab-4c80-9fcd-dbbfcd03378c","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2505.23895","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3c4b1eb2ef81c777132540899eb0215b681a8dfbcdf40483bd3bf59e7d6526a7","observation_id":"36064646-c73d-4ba0-a9f4-68d1b442d63c","resolution":{"observed_at":"2026-05-16T14:41:02.579467Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-07-17T23:51:39.358198+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-17T23:51:39.358198+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9909058","last_updated":"1999-09-20T14:43:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1999-09-20T14:43:09Z","title":"Quasi-Normal Modes of Stars and Black Holes","version":1},"cited_work":{"arxiv_id":"gr-qc/9909058","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9909058","snapshot_observed_at":"2026-07-10T14:47:14.213271Z","title":"Quasi-Normal Modes of Stars and Black Holes","venue":"gr-qc","work_id":"5f6526a3-3308-428c-ae22-7187b9a18231","year":1999},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/gr-qc/9909058","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:cec5ae3689a198cbe3fb433ea89715396874226aa498a1cc1a527b59a57ad5fb","observation_id":"d3367f8e-3735-46a0-8f15-0a4ebb22bfc8","resolution":{"observed_at":"2026-05-16T14:41:02.563235Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Nollert, TOPICAL REVIEW: Quasinormal modes: the characteristic ‘sound’ of black holes and neutron stars, Class","venue":null,"work_id":"0be83c3b-35dc-43be-82d0-b30fa2fd5bdd","year":1999},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:e3685c63e79cbe34199cc1998d72195df4c07a80bf3e8bdc12b4e5481a594f97","observation_id":"2530031e-d6c8-4a20-b05f-ebd65a5584b4","resolution":{"observed_at":"2026-05-16T14:41:02.893760Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0905.2975","last_updated":"2009-07-29T07:41:21Z","snapshot_observed_at":"2026-07-06T01:54:40.501878Z","submitted_at":"2009-05-19T05:15:43Z","title":"Quasinormal modes of black holes and black branes","version":2},"cited_work":{"arxiv_id":"0905.2975","doi":"10.1088/0264-9381/26/16/163001.arxiv:0905.2975","metadata_source":"pith","pith_arxiv_id":"0905.2975","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Quasinormal modes of black holes and black branes","venue":"gr-qc","work_id":"51775bcb-14dc-4eec-8c8c-179fd9588810","year":2009},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/0905.2975","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:a228d563a5561a9d6c1365f3eefe43b5f244a26bc33cc2a4c0042250dc871a11","observation_id":"1aa05c61-2231-4e0f-9f1c-9a756f248ee3","resolution":{"observed_at":"2026-05-16T14:41:02.536791Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1102.4014","last_updated":"2011-06-15T11:51:40Z","snapshot_observed_at":"2026-07-06T02:23:46.264528Z","submitted_at":"2011-02-19T18:38:22Z","title":"Quasinormal modes of black holes: from astrophysics to string theory","version":2},"cited_work":{"arxiv_id":"1102.4014","doi":null,"metadata_source":"pith","pith_arxiv_id":"1102.4014","snapshot_observed_at":"2026-07-10T14:47:14.296140Z","title":"Quasinormal modes of black holes: from astrophysics to string theory","venue":"gr-qc","work_id":"e47c6253-8456-4fd4-b1a1-4c37b6613e6e","year":2011},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1102.4014","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:052d32a8f95ae04d55bd9c056717913dd322ac9c92b8caafed9ea187d4186ea0","observation_id":"c2841a0d-6d3c-4a41-8407-0e03b1be3a26","resolution":{"observed_at":"2026-05-16T14:41:02.570547Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01696","last_updated":"2023-05-02T18:04:26Z","snapshot_observed_at":"2026-07-06T15:22:28.700249Z","submitted_at":"2023-05-02T18:04:26Z","title":"Testing General Relativity with Black Hole Quasi-Normal Modes","version":1},"cited_work":{"arxiv_id":"2305.01696","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2305.01696","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Franchini and S","venue":null,"work_id":"6f5f8772-5acb-417c-96e1-cfcc674b3612","year":2023},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2305.01696","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4eef7da6456a984d9881ef939b35a0e69e52296074bf4f9ac263e8be67bc579e","observation_id":"04eea347-6e9f-4bc8-9a00-4309f45c3d93","resolution":{"observed_at":"2026-05-16T14:41:02.566796Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"4c86070b-e3aa-4fc8-a456-2a86e0ecdad8","year":1963},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:cd353ecfa459a99ce8719a331f58e2b6e6e7efcf7cc272958d5eec08e56fc042","observation_id":"8f712d88-098e-4b6e-8d75-442bb9d7f3ee","resolution":{"observed_at":"2026-05-16T14:41:02.895530Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.12263","last_updated":"2025-08-29T11:52:35Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-15T21:04:14Z","title":"The Science of the Einstein Telescope","version":2},"cited_work":{"arxiv_id":"2503.12263","doi":"10.48550/arxiv.2503.12263","metadata_source":"pith","pith_arxiv_id":"2503.12263","snapshot_observed_at":"2026-07-10T23:57:41.329696Z","title":"The Science of the Einstein Telescope","venue":"gr-qc","work_id":"efdd99b4-9e0f-42be-b538-1f14391dd6f3","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2503.12263","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:182175992318643361dca455698597c9c541463e950503a7e75f4f086416ab9f","observation_id":"ae870c2d-3bff-4b65-9408-bb11a001004f","resolution":{"observed_at":"2026-05-16T14:41:02.573654Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-07-13T21:50:53.380149+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T21:50:53.380149+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07571","last_updated":"2024-02-12T11:06:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-02-12T11:06:12Z","title":"LISA Definition Study Report","version":1},"cited_work":{"arxiv_id":"2402.07571","doi":"10.1086/511063","metadata_source":"pith","pith_arxiv_id":"2402.07571","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"LISA Definition Study Report","venue":"astro-ph.CO","work_id":"0417ec60-d1d3-40b8-8dd8-853e19bc7adf","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2402.07571","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:52a3298b955b37e59ba1bdda30efe689f6bc0b1080ff32d7fbc27315903aa319","observation_id":"b3071fb1-3d2f-4437-bfb0-c38dffb5630d","resolution":{"observed_at":"2026-05-16T14:41:02.548624Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-07-13T22:21:41.501094+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T22:21:41.501094+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.07274","last_updated":"2015-12-02T03:09:26Z","snapshot_observed_at":"2026-07-06T04:07:31.249848Z","submitted_at":"2015-01-28T21:00:11Z","title":"Testing General Relativity with Present and Future Astrophysical Observations","version":4},"cited_work":{"arxiv_id":"1501.07274","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.07274","snapshot_observed_at":"2026-07-09T20:56:34.451143Z","title":"Testing General Relativity with Present and Future Astrophysical Observations","venue":"gr-qc","work_id":"219087d7-5726-4967-bc19-af2ca31335c7","year":2015},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1501.07274","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:c9dfb6e6d3ada8c48621de25678cd039dca0be5c77868b85b11f493c5ed11fc2","observation_id":"dfce6b98-4215-47d3-9679-da791843c14c","resolution":{"observed_at":"2026-05-16T14:41:02.483137Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.09793","last_updated":"2020-04-27T10:03:32Z","snapshot_observed_at":"2026-07-06T08:52:57.511608Z","submitted_at":"2020-01-27T14:00:40Z","title":"Prospects for Fundamental Physics with LISA","version":3},"cited_work":{"arxiv_id":"2001.09793","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2001.09793","snapshot_observed_at":"2026-07-03T07:07:44.428087Z","title":"Barausse et al., Prospects for Fundamental Physics with LISA, Gen","venue":null,"work_id":"a783e3fa-be49-4708-a6fc-0e4eff180af6","year":2020},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2001.09793","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:68ce5fdbab9982aedce4e901131fdd58752603441302128e6554d2996caa9874","observation_id":"d1998808-bc33-4b7c-b557-fd3df8d0965a","resolution":{"observed_at":"2026-05-16T14:41:02.430022Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-07T11:33:45.357263Z","title":"Regge and J","venue":null,"work_id":"36a917e8-9c13-4be4-9302-0d03390319ea","year":1957},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:5b534a1093e5d2e3fa63f817cd479f04f763195b77da690b24dbbe6d0609fc96","observation_id":"9b960141-58cb-4126-8416-8d6d67093fc0","resolution":{"observed_at":"2026-05-16T14:41:02.867366Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"5e2c6e96-c763-42ad-9401-9bf0d067bd13","year":1970},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:2e1162311e0452cf08f022abea43e7d85b75f38c6bda0217f579b26e36386c63","observation_id":"196d4557-f811-42a4-a21c-db6d531fa3b8","resolution":{"observed_at":"2026-05-16T14:41:02.891805Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"550a4d79-b03b-4b0c-a282-7056fc8ff1e5","year":1972},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:c332da43b8ae755f965d79cbd0384a358f9e0c9d95d43ae40844caed037ed702","observation_id":"f94ddeb6-7f7b-4ade-b448-461bdd82a1d6","resolution":{"observed_at":"2026-05-16T14:41:02.874252Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2103.09870","last_updated":"2021-03-23T17:58:28Z","snapshot_observed_at":"2026-07-06T10:50:54.559108Z","submitted_at":"2021-03-17T19:15:06Z","title":"Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the first order in rotation","version":2},"cited_work":{"arxiv_id":"2103.09870","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2103.09870","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Pierini and L","venue":null,"work_id":"cba1d683-73ec-4d69-83b1-ddd67b3db467","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2103.09870","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4e0ec4c06caea648050803671723f082dfaedbfeaf8ef50d418e49e6d752288a","observation_id":"17d56270-121b-41ac-af9f-b6d1edf11529","resolution":{"observed_at":"2026-05-16T14:41:02.396267Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2103.09913","last_updated":"2022-06-14T21:23:57Z","snapshot_observed_at":"2026-07-06T10:50:54.559108Z","submitted_at":"2021-03-17T21:17:24Z","title":"Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity","version":3},"cited_work":{"arxiv_id":"2103.09913","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2103.09913","snapshot_observed_at":"2026-07-03T02:57:35.437595Z","title":"Wagle, N","venue":null,"work_id":"32f875df-68bf-4f3d-9e09-0588bbe6dc87","year":2022},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2103.09913","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4fd35d555cb134bd2184053df1a6a542b54f98c1faaea5554a3ff5646c77cd2e","observation_id":"cbf4cac5-5153-4ead-80c9-7d5cbfd9b087","resolution":{"observed_at":"2026-05-16T14:41:02.471128Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2106.06209","last_updated":"2021-08-09T16:33:07Z","snapshot_observed_at":"2026-07-06T11:18:16.145357Z","submitted_at":"2021-06-11T07:28:26Z","title":"Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity","version":2},"cited_work":{"arxiv_id":"2106.06209","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2106.06209","snapshot_observed_at":"2026-07-03T02:57:35.421956Z","title":"Srivastava, Y","venue":null,"work_id":"8e82e75b-4a2c-4144-9070-265e0104503f","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2106.06209","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:a13c012fc60fa06926b07525e89168a4832044f05f56ece2d0f95a8a514729e7","observation_id":"abd44054-9d18-4597-86b9-c8500db0ab73","resolution":{"observed_at":"2026-05-16T14:41:02.534088Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.11267","last_updated":"2022-11-14T20:31:31Z","snapshot_observed_at":"2026-07-06T13:34:22.280128Z","submitted_at":"2022-07-22T18:00:04Z","title":"Quasi-normal modes of rotating black holes in Einstein-dilaton Gauss-Bonnet gravity: the second order in rotation","version":2},"cited_work":{"arxiv_id":"2207.11267","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.11267","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Pierini and L","venue":null,"work_id":"ad465c09-b2bf-4957-ba82-d3de506b750b","year":2022},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2207.11267","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3e486f12b08ddf46854d47f05dd6835a522200e56e96c4e698f6bcb67547198b","observation_id":"8a9ec034-fa35-4e06-b695-0b0882e87300","resolution":{"observed_at":"2026-05-16T14:41:02.427311Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.02663","last_updated":"2023-07-23T09:23:22Z","snapshot_observed_at":"2026-07-06T15:12:41.675871Z","submitted_at":"2023-04-05T18:00:02Z","title":"The universal Teukolsky equations and black hole perturbations in higher-derivative gravity","version":3},"cited_work":{"arxiv_id":"2304.02663","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.02663","snapshot_observed_at":"2026-07-03T02:57:35.573799Z","title":"Universal Teukolsky equations and black hole perturbations in higher-derivative gravity","venue":null,"work_id":"fa43fec3-4c42-4181-b0a6-11de0829bdb0","year":2023},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2304.02663","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:6fec0496953e67c03899cf6c9f4d6b13d40cde91575d293e04351ba79dd9cdd5","observation_id":"f4b8c653-a2c7-433b-b57b-dca459db155d","resolution":{"observed_at":"2026-05-16T14:41:02.531193Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07706","last_updated":"2023-11-13T19:45:22Z","snapshot_observed_at":"2026-07-06T16:47:01.374736Z","submitted_at":"2023-11-13T19:45:22Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity I. Slow rotation equations","version":1},"cited_work":{"arxiv_id":"2311.07706","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.07706","snapshot_observed_at":"2026-07-04T18:20:04.735330Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation equations","venue":null,"work_id":"6de27e1f-55d3-42dc-8e98-c3bf30c100f5","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2311.07706","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:99af13f49f6ca3fcbeb0f9f9504a4b8998b72e7cf7915da8854b62e28a1d044f","observation_id":"50db0354-0385-4c48-8ae5-139533df975a","resolution":{"observed_at":"2026-05-16T14:41:02.313169Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02017","last_updated":"2024-09-23T17:36:16Z","snapshot_observed_at":"2026-07-06T18:40:05.778984Z","submitted_at":"2024-07-02T07:39:08Z","title":"Teukolsky equation for near-extremal black holes beyond general relativity: near-horizon analysis","version":3},"cited_work":{"arxiv_id":"2407.02017","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.02017","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"fc04bf7f-b917-43b3-b537-ca42d029e025","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2407.02017","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:fbb36960bd9bb81268dfbd90fb8945a2f73fd0caa5ec0006febf856a96024af8","observation_id":"c20fe1dd-022e-4153-82cd-55674f39948d","resolution":{"observed_at":"2026-05-16T14:41:02.452842Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04517","last_updated":"2024-09-16T07:45:46Z","snapshot_observed_at":"2026-07-06T19:11:44.961846Z","submitted_at":"2024-09-06T18:00:00Z","title":"Higher-derivative corrections to the Kerr quasinormal mode spectrum","version":2},"cited_work":{"arxiv_id":"2409.04517","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.04517","snapshot_observed_at":"2026-07-04T18:20:04.729325Z","title":null,"venue":null,"work_id":"72392ea9-bf08-474b-a6e1-e961e886d405","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2409.04517","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:b033495233ea83f6518fbe831147269e60f5d55023f5a2ddeaa53117ef618a7d","observation_id":"66448a8f-833a-41ad-b8a8-5917a532ef66","resolution":{"observed_at":"2026-05-16T14:41:02.354441Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.11986","last_updated":"2024-09-07T09:58:49Z","snapshot_observed_at":"2026-07-06T18:32:32.228906Z","submitted_at":"2024-06-17T18:04:12Z","title":"Quasi-normal mode frequencies and gravitational perturbations of black holes with any subextremal spin in modified gravity through METRICS: the scalar-Gauss-Bonnet gravity case","version":2},"cited_work":{"arxiv_id":"2406.11986","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.11986","snapshot_observed_at":"2026-07-03T02:57:35.530577Z","title":null,"venue":null,"work_id":"0ca1bcb7-e1bd-4211-a917-dfd29fe7e65b","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2406.11986","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:acb1ec0fb8db4b9b4bf372e03ee51eb92388b89dfa1f793de5536c596c9e979c","observation_id":"e61850d4-8c1a-498a-bfbc-a3f552ea4875","resolution":{"observed_at":"2026-05-16T14:41:02.518980Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12280","last_updated":"2024-11-01T19:06:17Z","snapshot_observed_at":"2026-07-06T18:16:55.387253Z","submitted_at":"2024-05-20T18:00:01Z","title":"Ringing out General Relativity: Quasi-normal mode frequencies for black holes of any spin in modified gravity","version":3},"cited_work":{"arxiv_id":"2405.12280","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12280","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ringing Out General Relativity: Quasinormal Mode Frequencies for Black Holes of Any Spin in Modified Gravity","venue":null,"work_id":"b65428db-7086-4087-adf1-2419a38c2191","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2405.12280","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:9f3ad49800ccb0e3386a3d689cf36c535e15b3cebe2c3f2bbb5fbf58d366089b","observation_id":"f25b1b24-a044-4118-926d-9555c09f42c2","resolution":{"observed_at":"2026-05-16T14:41:02.445163Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.20760","last_updated":"2025-01-21T16:52:17Z","snapshot_observed_at":"2026-07-06T18:53:53.776421Z","submitted_at":"2024-07-30T12:02:23Z","title":"Quasinormal modes of rapidly rotating Einstein-Gauss-Bonnet-dilaton black holes","version":3},"cited_work":{"arxiv_id":"2407.20760","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.20760","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"8df254a5-fc14-43c6-afa6-759ca8fe37bd","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2407.20760","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:f941d9a35c626133362b99724903847aa7e11de1df072e99417678397777c97b","observation_id":"c671b2db-deea-46d0-add9-a6c63a7bc288","resolution":{"observed_at":"2026-05-16T14:41:02.335883Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2412.09377","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"ab8ecd15-90fb-41e9-8982-e8db5c9f4bc2","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:d3517d9716a9c9455beb889ded9c43b7209332a6ff743f717d7dfa106988ef06","observation_id":"a9c4b15a-0552-4568-b6d8-9bb48b265c8b","resolution":{"observed_at":"2026-05-16T14:41:02.414167Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10652","last_updated":"2023-05-25T15:16:59Z","snapshot_observed_at":"2026-07-06T13:23:15.117710Z","submitted_at":"2022-06-21T18:04:48Z","title":"Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation","version":2},"cited_work":{"arxiv_id":"2206.10652","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.10652","snapshot_observed_at":"2026-07-03T02:57:35.511777Z","title":"Perturbations of Spinning Black Holes beyond General Relativity: Modified Teukolsky Equation","venue":null,"work_id":"083d8dbe-6632-4997-b8be-5ee6188ded6d","year":2023},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2206.10652","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3450ccc4283938b2d702fb24218743fa776ecf404c7b3a978303eab7665d827f","observation_id":"010f88bf-5ec1-481a-b1f3-068a95993ae8","resolution":{"observed_at":"2026-05-16T14:41:02.474007Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10653","last_updated":"2022-06-21T18:06:02Z","snapshot_observed_at":"2026-07-06T13:23:15.117710Z","submitted_at":"2022-06-21T18:06:02Z","title":"An approach to computing spectral shifts for black holes beyond Kerr","version":1},"cited_work":{"arxiv_id":"2206.10653","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.10653","snapshot_observed_at":"2026-07-04T18:20:04.718307Z","title":"Hussain and A","venue":null,"work_id":"2a7e9857-0464-4862-be65-1453ae6b9cbb","year":2022},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2206.10653","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:2de965aa3d6fdb6f3bbd9d903fd884c2864e2f6868df1d3eebe347b96ecf4a89","observation_id":"a8369d41-7851-46d4-9f9b-9000d439b5dd","resolution":{"observed_at":"2026-05-16T14:41:02.409344Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15947","last_updated":"2024-10-30T11:15:37Z","snapshot_observed_at":"2026-07-06T18:50:17.892140Z","submitted_at":"2024-07-22T18:01:30Z","title":"Parametrized quasi-normal mode framework for modified Teukolsky equations","version":3},"cited_work":{"arxiv_id":"2407.15947","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.15947","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Parametrized quasinormal mode framework for modified Teukolsky equations","venue":null,"work_id":"c55e375a-657e-416f-a5f8-7c539cf114ef","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2407.15947","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4ed95c77a9b2cb43fa906137320b2cb84f0aa2a8d3e01f741f0b31d3a4b08484","observation_id":"0016f5d4-422b-46d4-9051-ccf7fc31654f","resolution":{"observed_at":"2026-05-16T14:41:02.387469Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"a73996ca-8706-48b1-a8f4-bd45151c0d02","year":1985},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:230a1467bff01620c8b7130b9642b14b962de2237ac3ec2eb4d76d5ffa1c2027","observation_id":"5be370f9-98bc-497f-a75b-8e6bc71d1469","resolution":{"observed_at":"2026-05-16T14:41:02.885291Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"65248413-a944-4988-b7ab-84d249df4943","year":1985},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:2cd2812eb503f48162569153d3d8dd3e406b1f4922e9d819da774c9c52e117b8","observation_id":"af1d84cc-7178-48e2-a35e-2d8e322471d6","resolution":{"observed_at":"2026-05-16T14:41:02.877996Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"3f774c67-224d-4189-b8c0-db6eeb2fda64","year":1970},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:77a2750f6c5e1cef58dd10da321c865611f954ae6ac857a201fe0f273a39421e","observation_id":"a0e5db22-10c3-43ca-82e0-663668213898","resolution":{"observed_at":"2026-05-16T14:41:02.865481Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"516304db-3364-4c43-a95a-029f803ef8b2","year":1972},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:b6b6cf320be64bf54b402b5b352a38306de8ec712cc7e4dca4c94c240286bfb9","observation_id":"3abc51a5-c177-486f-9e3b-60e65dceff7d","resolution":{"observed_at":"2026-05-16T14:41:02.879860Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.07391","last_updated":"2020-08-17T15:02:57Z","snapshot_observed_at":"2026-07-06T09:47:48.007337Z","submitted_at":"2020-08-17T15:02:57Z","title":"Black hole scalarization induced by the spin -- 2+1 time evolution","version":1},"cited_work":{"arxiv_id":"2008.07391","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2008.07391","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Black hole scalarization induced by the spin: 2+1 time evolution","venue":null,"work_id":"d144047f-52f0-4ac2-a12c-e42a7434ce4c","year":2020},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2008.07391","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:5f3abb944cc2019c9a84720315b3bac06c650941c66722a1f0d0f04ee3c854f9","observation_id":"8602b14c-778e-4455-9c28-605a030568dd","resolution":{"observed_at":"2026-05-16T14:41:02.476731Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"vibrations","venue":null,"work_id":"fd485c7d-130c-4cad-b5d2-c94e3f1172b5","year":1972},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:efba97001b112b3b9b720860127316cd17228b2f1ae961ca92a30682e21dd1f7","observation_id":"766b5633-e6bf-433f-91b0-0b427f6bdff2","resolution":{"observed_at":"2026-05-16T14:41:02.883669Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ferrari and B","venue":null,"work_id":"40acbeb5-a8f2-4409-a1cf-55d3137a1cb5","year":1984},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:2f3edcc4377605cee0cf9874af3847f07fe56179023001d7b77f05ebcfc3e5b7","observation_id":"ff2a570b-c723-4be4-bec4-dab36d07a0f3","resolution":{"observed_at":"2026-05-16T14:41:02.881780Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1706.07658","last_updated":"2017-06-23T12:17:31Z","snapshot_observed_at":"2026-08-01T14:54:14.659181Z","submitted_at":"2017-06-23T12:17:31Z","title":"Post-Kerr black hole spectroscopy","version":1},"cited_work":{"arxiv_id":"1706.07658","doi":null,"metadata_source":"pith","pith_arxiv_id":"1706.07658","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Post-Kerr black hole spectroscopy","venue":"gr-qc","work_id":"48e7c165-a865-449c-a829-cdb9d6c1e4d1","year":2017},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1706.07658","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3c6c7898c05b439b5f9021b8711b2f673de2bd9ad70ba93743e35a783738bc7d","observation_id":"70959b9f-2a7e-459e-af2f-8ce59c7fe6dd","resolution":{"observed_at":"2026-05-16T14:41:02.513247Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.07195","last_updated":"2018-04-16T23:59:07Z","snapshot_observed_at":"2026-07-06T06:19:41.641820Z","submitted_at":"2018-01-22T17:05:34Z","title":"Axisymmetric black holes allowing for separation of variables in the Klein-Gordon and Hamilton-Jacobi equation","version":3},"cited_work":{"arxiv_id":"1801.07195","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.07195","snapshot_observed_at":"2026-07-10T14:47:14.253383Z","title":"Axisymmetric black holes allowing for separation of variables in the Klein-Gordon and Hamilton-Jacobi equation","venue":"gr-qc","work_id":"073bacd5-bb25-4c0d-b6ca-7fa90a953ba9","year":2018},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1801.07195","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:c5a2bf749e2a219027096a85f438736fdce2954317f8ed65cef109853a70893d","observation_id":"1a59290c-e538-4d70-a861-fb91f449cc4c","resolution":{"observed_at":"2026-05-16T14:41:02.527878Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Pedrotti,Studies on Quasi-Normal Modes and Shad- ows of Black Holes, Master’s thesis, Trento U","venue":null,"work_id":"ddfae11a-8232-42ea-86b7-13064cc8409b","year":2023},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:98ceceb9ccb9d060dfa73710b6a4fbb72cbd20f9866e447b9efdf99b735ae0ab","observation_id":"f18f0a10-6be8-478a-afec-df0651a754f2","resolution":{"observed_at":"2026-05-16T14:41:02.887836Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07589","last_updated":"2024-10-28T15:51:15Z","snapshot_observed_at":"2026-07-06T17:58:43.506575Z","submitted_at":"2024-04-11T09:19:32Z","title":"Quasinormal modes-shadow correspondence for rotating regular black holes","version":3},"cited_work":{"arxiv_id":"2404.07589","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.07589","snapshot_observed_at":"2026-07-02T14:57:04.954990Z","title":"Pedrotti and S","venue":null,"work_id":"3d590aac-9cef-4052-8023-0f5f936c2566","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2404.07589","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:2797948994ce8582116c08be90bcdf8b14a19bf76467414073f4d16a999269a3","observation_id":"6e8a4512-882c-4974-971f-86b7d879e4d9","resolution":{"observed_at":"2026-05-16T14:41:02.413851Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"qc/0701086","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Berti, V","venue":null,"work_id":"4419262d-b610-4ca8-9b45-57ba8eadf46e","year":2007},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:2292cd1d4c3e715c415a1d1dbc5e033990217e9db1cb28b89e5b1908c8ca3811","observation_id":"aff8c10b-5bb7-4b95-9a61-f5fcbb8c6a67","resolution":{"observed_at":"2026-05-16T14:41:02.483149Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1007.5097","last_updated":"2010-07-29T00:52:32Z","snapshot_observed_at":"2026-07-06T02:13:39.237830Z","submitted_at":"2010-07-29T00:52:32Z","title":"The Quasinormal Mode Spectrum of a Kerr Black Hole in the Eikonal Limit","version":1},"cited_work":{"arxiv_id":"1007.5097","doi":null,"metadata_source":"pith","pith_arxiv_id":"1007.5097","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The Quasinormal Mode Spectrum of a Kerr Black Hole in the Eikonal Limit","venue":"gr-qc","work_id":"551c1c81-d981-4694-99d9-64494d9adda7","year":2010},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1007.5097","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:ebb6a73d1d0c47475ffc02eea99390e7385755d8492ccab91e0e0f2a6452d2f1","observation_id":"b4dc0765-3fd5-4e09-8807-97bc1a4ea71c","resolution":{"observed_at":"2026-05-16T14:41:02.455281Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.05455","last_updated":"2019-08-26T19:40:41Z","snapshot_observed_at":"2026-07-06T08:00:00.020917Z","submitted_at":"2019-06-13T02:10:59Z","title":"Eikonal quasinormal modes of black holes beyond General Relativity","version":2},"cited_work":{"arxiv_id":"1906.05455","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.05455","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Glampedakis and H","venue":null,"work_id":"9c6dd08a-edf3-4ec3-b08c-dce996493d68","year":2019},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1906.05455","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:5272e0a2590869f5fcc06fd7061bfc012252f684914a756fd22c22cfd001b3d3","observation_id":"eb4f5cbf-fcf4-4385-918e-5f2bab03152f","resolution":{"observed_at":"2026-05-16T14:41:02.373707Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"9e74772e-5700-4653-8f51-5c4f09f08285","year":1972},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:29df93a47f78773df407c2ee883b77f9f5bddbe7ad5c58ca7a232e614940f26e","observation_id":"cdc2fa77-f6f2-4b6c-93d3-7982f0900616","resolution":{"observed_at":"2026-05-16T14:41:02.876134Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13673","last_updated":"2024-12-18T09:57:17Z","snapshot_observed_at":"2026-07-06T20:09:05.798010Z","submitted_at":"2024-12-18T09:57:17Z","title":"Black Hole Shadow and other Observables away from the Horizon: Extending the Effective Metric Descriptions","version":1},"cited_work":{"arxiv_id":"2412.13673","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13673","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Del Piano, S","venue":null,"work_id":"5d7f1ae6-3e04-460b-b349-a62139b89cbf","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2412.13673","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:33fa4e39202905c8758b56e8ee75d3c17211fd69adf362d59d18e7a8992e2acb","observation_id":"280cf415-26a2-46e7-b3b2-93e35b90d092","resolution":{"observed_at":"2026-05-16T14:41:02.442132Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.14707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-04T18:20:04.688672Z","title":"Del Piano, C","venue":null,"work_id":"768b7c38-8b82-4f68-adbb-f0428c3ae6df","year":2026},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:c184fc8482314c9717b96d426ce8954bdb758da6e2f23111e93bffd93e9a6299","observation_id":"b781c69c-60e1-4855-a03a-008e4d727659","resolution":{"observed_at":"2026-05-16T14:41:02.419450Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.02814","last_updated":"2015-01-12T21:01:21Z","snapshot_observed_at":"2026-07-06T04:06:00.000587Z","submitted_at":"2015-01-12T21:01:21Z","title":"Photon Rings around Kerr and Kerr-like Black Holes","version":1},"cited_work":{"arxiv_id":"1501.02814","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.02814","snapshot_observed_at":"2026-06-29T11:13:21.041577Z","title":"Photon Rings around Kerr and Kerr-like Black Holes","venue":"astro-ph.HE","work_id":"ad263e15-6e35-48c9-ab28-dc614310d518","year":2015},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1501.02814","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:f1ac14796969b2dbf3d6317184385360adf4dd0975705ea4433ca22b64028775","observation_id":"b0f7753b-81a4-44c2-b1f6-d8810a882694","resolution":{"observed_at":"2026-05-16T14:41:02.461454Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.3191","last_updated":"2011-05-20T23:40:40Z","snapshot_observed_at":"2026-07-06T02:27:49.258804Z","submitted_at":"2011-05-16T20:00:02Z","title":"A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem","version":2},"cited_work":{"arxiv_id":"1105.3191","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.3191","snapshot_observed_at":"2026-07-04T18:20:04.683129Z","title":"A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem","venue":"gr-qc","work_id":"056b4dbe-d7c7-444a-b14f-b80b072bafb5","year":2011},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1105.3191","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:e50b32089714d407bf77fed4a391be766b13ea2becca197b52d62d5befe492de","observation_id":"9057d25d-d648-4b1b-81e4-1443ea3082c0","resolution":{"observed_at":"2026-05-16T14:41:02.347483Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.02378","last_updated":"2016-02-07T14:56:50Z","snapshot_observed_at":"2026-07-06T04:45:22.256718Z","submitted_at":"2016-02-07T14:56:50Z","title":"General parametrization of axisymmetric black holes in metric theories of gravity","version":1},"cited_work":{"arxiv_id":"1602.02378","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.02378","snapshot_observed_at":"2026-06-30T00:24:04.866816Z","title":"General parametrization of axisymmetric black holes in metric theories of gravity","venue":"gr-qc","work_id":"5ad687cd-fb82-49d9-82f8-7f656b967641","year":2016},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1602.02378","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:862189d4b43c3757bccb0ae601a6da00c9ae8018afc4f0946849f4ebb1f126cd","observation_id":"76a935f2-17e5-40d3-88ac-00109fede5b2","resolution":{"observed_at":"2026-05-16T14:41:02.379402Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04091","last_updated":"2019-04-12T13:00:10Z","snapshot_observed_at":"2026-07-06T06:44:11.115459Z","submitted_at":"2018-06-11T16:24:50Z","title":"On the connection of spacetime separability and spherical photon orbits","version":2},"cited_work":{"arxiv_id":"1806.04091","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.04091","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On the connection of spacetime separability and spherical photon orbits","venue":"gr-qc","work_id":"63b4a473-6a99-485f-96dd-745914e89840","year":2018},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1806.04091","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3fa286f60078d21a504c6734bb47bbbe164c30f0f8719ddff5b35071d7cc0a2b","observation_id":"a48028d6-9933-41c1-a91c-c77b66f9fd9b","resolution":{"observed_at":"2026-05-16T14:41:02.492698Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.04066","last_updated":"2021-06-07T15:03:53Z","snapshot_observed_at":"2026-07-06T10:39:22.798581Z","submitted_at":"2021-02-08T09:06:31Z","title":"Thermal behavior of a radially deformed black hole spacetime","version":2},"cited_work":{"arxiv_id":"2102.04066","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2102.04066","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Barman and S","venue":null,"work_id":"bd60f049-82e5-413d-8f08-c29b2248b9b8","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2102.04066","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:a27dd1e22eaf0518d23137b7d229093cd8716f5c310c7ef7bcf9a4e304709356","observation_id":"640f7f6e-bb48-430f-b9cc-7205dcc43cf4","resolution":{"observed_at":"2026-05-16T14:41:02.467530Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.03152","last_updated":"2021-04-16T12:01:23Z","snapshot_observed_at":"2026-07-06T10:38:46.169966Z","submitted_at":"2021-02-05T13:06:58Z","title":"Superradiance in Kerr-like black holes","version":2},"cited_work":{"arxiv_id":"2102.03152","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2102.03152","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Superradiance in Kerr-like black holes","venue":null,"work_id":"99216cdf-610f-4196-b4b5-86db29badb33","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2102.03152","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:cef249731b2298379fd3fc99a633e894db667a04235e15fbecd41b883b58fae6","observation_id":"22f8a0a9-e005-4050-a35b-30c69a7b40bf","resolution":{"observed_at":"2026-05-16T14:41:02.486380Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.08594","last_updated":"2018-07-23T13:25:27Z","snapshot_observed_at":"2026-07-06T06:51:45.783650Z","submitted_at":"2018-07-23T13:25:27Z","title":"Preserving Kerr symmetries in deformed spacetimes","version":1},"cited_work":{"arxiv_id":"1807.08594","doi":"10.1088/1361-6382/aad7f4","metadata_source":"pith","pith_arxiv_id":"1807.08594","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Preserving Kerr symmetries in deformed spacetimes","venue":"gr-qc","work_id":"6d154924-b04b-4548-b9da-c6ef53179e98","year":2018},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1807.08594","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:942666a4f24bf220316f3eba306e46a0f73eacac157c5b42b334e01c85dc3615","observation_id":"cab38c09-34b5-43f0-928b-4f90d1128866","resolution":{"observed_at":"2026-05-16T14:41:02.470480Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9606003","last_updated":"1996-06-04T13:12:35Z","snapshot_observed_at":"2026-07-07T03:26:28.487645Z","submitted_at":"1996-06-04T13:12:35Z","title":"Dynamics of Scalar Fields in the Background of Rotating Black Holes","version":1},"cited_work":{"arxiv_id":"gr-qc/9606003","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9606003","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Dynamics of Scalar Fields in the Background of Rotating Black Holes","venue":"gr-qc","work_id":"a2e899ba-01e6-49bd-9980-67fd95602532","year":1996},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/gr-qc/9606003","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:a549fe1519439f3adbbcad9c605dba068001a52dcc562130ffb8b5f5d50bdad0","observation_id":"3e8ef1b4-bd29-4c6a-a868-5a9f52011d9e","resolution":{"observed_at":"2026-05-16T14:41:02.431203Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.02510","last_updated":"2020-12-21T11:17:22Z","snapshot_observed_at":"2026-07-06T09:44:58.164228Z","submitted_at":"2020-08-06T08:12:10Z","title":"A family of solutions to the inverse problem in gravitation: building a theory around a metric","version":2},"cited_work":{"arxiv_id":"2008.02510","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2008.02510","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"32a7cd05-27c2-4912-bc80-0894c40287ae","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2008.02510","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:46dcef4b50de73e07f13c5b12ad36681aa845883dc18ebe4af03603e2e6f0af6","observation_id":"9600a9ef-cc68-4468-8a39-910f6fed2984","resolution":{"observed_at":"2026-05-16T14:41:02.400129Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.09697","last_updated":"2021-02-09T11:58:35Z","snapshot_observed_at":"2026-07-06T10:35:03.891775Z","submitted_at":"2021-01-24T12:16:24Z","title":"Exact theory for the Rezzolla-Zhidenko metric and self-consistent calculation of quasinormal modes","version":2},"cited_work":{"arxiv_id":"2101.09697","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.09697","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"1a251298-a8ae-4325-b037-dea6271f7a16","year":2021},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2101.09697","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:428fcc655b891f58fcbd45da0065b3f466f9a6c91a549fe58a02f4ae340c7b0a","observation_id":"50fc3f11-9b95-48bd-a2a8-3241fb7db93c","resolution":{"observed_at":"2026-05-16T14:41:02.422479Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03133","last_updated":"2016-07-11T20:11:37Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:11:37Z","title":"Testing the black hole \"no-hair\" hypothesis","version":1},"cited_work":{"arxiv_id":"1607.03133","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.03133","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing the black hole \"no-hair\" hypothesis","venue":"gr-qc","work_id":"f20e7608-1c42-4712-9bd0-0da5fb9ace0a","year":2016},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1607.03133","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:c3620123703a22e2c126d0f15b442783442d52fe43ea3ef52b606779f3b0bea5","observation_id":"7377108b-8294-4cca-97bf-3722cd8780c4","resolution":{"observed_at":"2026-05-16T14:41:02.343389Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.06869","last_updated":"2017-06-01T17:30:30Z","snapshot_observed_at":"2026-07-06T05:34:27.624728Z","submitted_at":"2017-03-20T17:53:12Z","title":"Are LIGO's Black Holes Made From Smaller Black Holes?","version":3},"cited_work":{"arxiv_id":"1703.06869","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.06869","snapshot_observed_at":"2026-07-03T01:47:30.964576Z","title":"Are LIGO's Black Holes Made From Smaller Black Holes?","venue":"astro-ph.HE","work_id":"7e7cb2f9-b15b-4715-8b17-aa26dce859ea","year":2017},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1703.06869","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:bff4b3ef9ccd0258627c47c42e482a0871eda82d3cff8667ecb78eaeae1a2b6d","observation_id":"45d73f65-2d1e-434a-bae9-039a79a84009","resolution":{"observed_at":"2026-05-16T14:41:02.312464Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.00805","last_updated":"2024-01-01T16:25:11Z","snapshot_observed_at":"2026-08-01T04:10:13.267498Z","submitted_at":"2024-01-01T16:25:11Z","title":"Nonlinear Effects In Black Hole Ringdown From Scattering Experiments I: spin and initial data dependence of quadratic mode coupling","version":1},"cited_work":{"arxiv_id":"2401.00805","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.00805","snapshot_observed_at":"2026-07-10T23:37:42.111522Z","title":"Zhu et al","venue":"gr-qc","work_id":"8b326247-c663-4ab9-92e5-782d8e8c2849","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2401.00805","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:1c94cc1406e4afbff61d0ce1c7c3a7c0062d50c7a23dbfe4856feb9abf8bcdde","observation_id":"332b8394-4d15-4c8d-9726-031006aa304e","resolution":{"observed_at":"2026-05-16T14:41:02.450181Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2412.06887","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T23:37:42.019024Z","title":"De Amicis et al., (2024), arXiv:2412.06887 [gr-qc]","venue":null,"work_id":"c54c8cdc-54ff-4b3c-a0ac-6861b50d4d09","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:c1fc7ae98f0649a12ceb46eb13401a4d3da71b5d00d548714606545c37dd6fef","observation_id":"dab04f67-b47c-4497-af9d-dd4b0db8cd37","resolution":{"observed_at":"2026-05-16T14:41:02.496111Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1207.4253","last_updated":"2012-07-18T02:22:40Z","snapshot_observed_at":"2026-08-01T13:18:00.245687Z","submitted_at":"2012-07-18T02:22:40Z","title":"Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation","version":1},"cited_work":{"arxiv_id":"1207.4253","doi":null,"metadata_source":"pith","pith_arxiv_id":"1207.4253","snapshot_observed_at":"2026-07-04T09:29:44.383039Z","title":"Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation","venue":"gr-qc","work_id":"a627c5cf-758d-4161-9c41-9bc1f950fbc8","year":2012},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1207.4253","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:77b6ffc4a415d4b6a6fab055711c373688d02a91a3815ec58619ca1d1e73b41b","observation_id":"b4b17bb1-453b-4f90-a417-dfa9302fb18e","resolution":{"observed_at":"2026-05-16T14:41:02.468186Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0812.1806","last_updated":"2009-03-12T00:13:05Z","snapshot_observed_at":"2026-08-01T19:42:55.991469Z","submitted_at":"2008-12-09T21:38:26Z","title":"Geodesic stability, Lyapunov exponents and quasinormal modes","version":3},"cited_work":{"arxiv_id":"0812.1806","doi":null,"metadata_source":"pith","pith_arxiv_id":"0812.1806","snapshot_observed_at":"2026-07-10T14:47:14.221012Z","title":"Geodesic stability, Lyapunov exponents and quasinormal modes","venue":"hep-th","work_id":"deb8be82-19ff-40e9-85c4-1627a7c81b0f","year":2008},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/0812.1806","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:e4abd714942a89787f47aeef84ee209c98bb520c02762768b887e0b4806e5df9","observation_id":"a0872dbe-c87f-4a52-9426-896095a26cee","resolution":{"observed_at":"2026-05-16T14:41:02.504638Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05928","last_updated":"2017-06-01T22:35:22Z","snapshot_observed_at":"2026-07-06T05:42:58.053337Z","submitted_at":"2017-05-16T21:35:48Z","title":"Are eikonal quasinormal modes linked to the unstable circular null geodesics?","version":3},"cited_work":{"arxiv_id":"1705.05928","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.05928","snapshot_observed_at":"2026-07-09T09:36:09.264230Z","title":"Are eikonal quasinormal modes linked to the unstable circular null geodesics?","venue":"gr-qc","work_id":"70573a8a-b51e-4044-bd59-f19ecbd41b5e","year":2017},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1705.05928","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:64e8eab9e9007181127abaaa750544a52ac50b994d6546adac31c6ce6e0858ad","observation_id":"13279797-1537-4800-82d4-8b7bedb468d8","resolution":{"observed_at":"2026-05-16T14:41:02.320537Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Capozziello and V","venue":null,"work_id":"b27cd5a9-c896-461d-9453-62e518b1d4a8","year":2011},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:e01baa3d861936b9b383be6921cfde501ae0b3f1e8ef3a6d8454f161c79bf577","observation_id":"79b4ccd3-9eb7-47ab-8e3b-993318b9e7c9","resolution":{"observed_at":"2026-05-16T14:41:02.889975Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.03011","last_updated":"2022-12-03T10:08:33Z","snapshot_observed_at":"2026-07-06T13:38:59.709514Z","submitted_at":"2022-08-05T06:58:34Z","title":"Comparing Equivalent Gravities: common features and differences","version":2},"cited_work":{"arxiv_id":"2208.03011","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.03011","snapshot_observed_at":"2026-07-02T00:36:23.967558Z","title":"Capozziello, V","venue":null,"work_id":"9f72dab2-1149-43fd-a193-023e2d4cb0ce","year":2022},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2208.03011","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:6078453eea9de2cb73f74201e0d5a8e4fe2b6619340a6509c95311979e6a80e4","observation_id":"f4655816-9616-4395-9f19-3c239a52b238","resolution":{"observed_at":"2026-05-16T14:41:02.318923Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.09737","last_updated":"2024-06-20T06:52:32Z","snapshot_observed_at":"2026-07-06T17:17:11.535092Z","submitted_at":"2024-01-18T05:36:35Z","title":"The Equivalence Principle as a Noether Symmetry","version":3},"cited_work":{"arxiv_id":"2401.09737","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2401.09737","snapshot_observed_at":"2026-07-02T00:36:24.136072Z","title":"Capozziello and C","venue":null,"work_id":"a2339f0e-a939-4518-b4fb-6ddad82cb97a","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2401.09737","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:e2cdafacede09b8026040d647f3aef0431dbea456879657b0efff463cff9bcff","observation_id":"3c34f754-2db1-4f19-a832-9e679a884d83","resolution":{"observed_at":"2026-05-16T14:41:02.479880Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.00083","last_updated":"2017-04-18T11:57:59Z","snapshot_observed_at":"2026-07-06T05:08:54.821151Z","submitted_at":"2016-09-01T01:39:55Z","title":"Black Hole Ringing, Quasinormal Modes, and Light Rings","version":3},"cited_work":{"arxiv_id":"1609.00083","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.00083","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Black Hole Ringing, Quasinormal Modes, and Light Rings","venue":"gr-qc","work_id":"3b81e5eb-6855-4bb3-8ad9-e75cffd9b922","year":2016},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1609.00083","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:afbf2a9c2bfd5a89b8bf8435459e702617d08d3ad749d80491039cc69f778fd7","observation_id":"1755f942-842c-4375-ad67-7165cadf59ad","resolution":{"observed_at":"2026-05-16T14:41:02.476722Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.08373","last_updated":"2022-10-20T12:55:34Z","snapshot_observed_at":"2026-07-06T14:06:05.716505Z","submitted_at":"2022-10-15T20:51:21Z","title":"Further clarification on quasinormal modes/circular null geodesics correspondence","version":2},"cited_work":{"arxiv_id":"2210.08373","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.08373","snapshot_observed_at":"2026-07-10T14:47:14.183115Z","title":"Further clarification on quasinormal modes/circular null geodesics correspondence","venue":"gr-qc","work_id":"556e03bf-831a-4210-8e53-554b7e49296b","year":2022},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2210.08373","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3552c7923045bfddc17c6b0984e4be88dc2665cde761d93b3d53674251371d5d","observation_id":"fb461f1b-9682-47d6-870d-3bb0c61152a4","resolution":{"observed_at":"2026-05-16T14:41:02.524649Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10377","last_updated":"2019-10-01T19:24:39Z","snapshot_observed_at":"2026-07-06T08:17:14.504195Z","submitted_at":"2019-08-27T18:00:03Z","title":"qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients","version":2},"cited_work":{"arxiv_id":"1908.10377","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.10377","snapshot_observed_at":"2026-07-04T09:29:44.428679Z","title":"Open Source Softw.4 1683 [arXiv:1908.10377]","venue":null,"work_id":"cd6b177f-e8d3-47e6-b03e-f3e1ce67edd0","year":2019},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/1908.10377","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:8f68d4ca8252399162341d49d05f7c612a094cacc6791644641c993f51485fd9","observation_id":"4edceb13-5fcc-4cb3-8ab5-ee2d3a677801","resolution":{"observed_at":"2026-05-16T14:41:02.327802Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.22122","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Quantifying Systematic Biases in Black Hole Spectroscopy","venue":null,"work_id":"72601547-0abb-4dbc-b3dd-28189c8219b4","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:667ff091ad8c9777076fbfc543f93bd7a90e59a0e2ab1aff5f1fa9df0031abbc","observation_id":"99c4a8e1-ddad-4f45-9f50-ee9827aaa112","resolution":{"observed_at":"2026-05-16T14:41:02.327948Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.10725","last_updated":"2023-08-07T08:57:18Z","snapshot_observed_at":"2026-07-06T14:33:16.914984Z","submitted_at":"2022-12-21T02:40:23Z","title":"Measuring deviations from the Kerr geometry with black hole ringdown","version":2},"cited_work":{"arxiv_id":"2212.10725","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.10725","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"a967022c-cc70-4eb0-b981-21b199b390d4","year":2023},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2212.10725","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:79df03258ae9d0f1f973176998454cbb1211646d75e89f9f4c0a63b401b1937d","observation_id":"b47224d1-d72e-4762-b440-2aca7fcb1311","resolution":{"observed_at":"2026-05-16T14:41:02.499019Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.11048","last_updated":"2024-11-12T08:16:06Z","snapshot_observed_at":"2026-07-06T12:40:29.970353Z","submitted_at":"2022-02-22T17:28:58Z","title":"Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors","version":3},"cited_work":{"arxiv_id":"2202.11048","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2202.11048","snapshot_observed_at":"2026-07-04T01:39:24.984710Z","title":"Borhanian and B","venue":null,"work_id":"39ca0c49-7857-4600-a905-23657b2f76a6","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2202.11048","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:619dabea7e24c5d00470a762e0b6f2d5ac43332f4647a0706f19dfd9f9927b3f","observation_id":"b47d3519-57e5-447b-bb7a-f7058bf1f29f","resolution":{"observed_at":"2026-05-16T14:41:02.521963Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9602032","last_updated":"1996-02-14T18:02:48Z","snapshot_observed_at":"2026-08-01T14:48:40.180648Z","submitted_at":"1996-02-14T18:02:48Z","title":"About the Significance of Quasinormal Modes of Black Holes","version":1},"cited_work":{"arxiv_id":"gr-qc/9602032","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9602032","snapshot_observed_at":"2026-07-01T10:55:41.643983Z","title":"About the Significance of Quasinormal Modes of Black Holes","venue":"gr-qc","work_id":"a800b10a-fcda-4361-a4ba-89e1adb32906","year":1996},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/gr-qc/9602032","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:3f6cc4a947043dd7f2ae185de60b2c81ca3cad6adb508f0ebfd12a3872abc101","observation_id":"b6d0ab04-cae1-4cc6-8159-12644cdf4e54","resolution":{"observed_at":"2026-05-16T14:41:02.516235Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.08547","last_updated":"2022-10-24T19:30:30Z","snapshot_observed_at":"2026-07-06T13:10:56.430851Z","submitted_at":"2022-05-17T18:00:01Z","title":"Stability of the fundamental quasinormal mode in time-domain observations against small perturbations","version":2},"cited_work":{"arxiv_id":"2205.08547","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2205.08547","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Berti, V","venue":null,"work_id":"6b1c0eeb-80fb-4220-ae5c-acc6aff6ddde","year":2022},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2205.08547","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:d55de98856f0849aa21ab17d96b0b34ee77dcc56fa3087b3eeb04ad3230e154f","observation_id":"e288b15f-9fe1-4a85-b2a2-676b4afe111d","resolution":{"observed_at":"2026-05-16T14:41:02.463801Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.14506","last_updated":"2023-04-13T12:47:03Z","snapshot_observed_at":"2026-07-06T14:10:32.433250Z","submitted_at":"2022-10-26T06:32:52Z","title":"Quasinormal modes in higher derivative gravity: testing the black hole parametrization and sensitivity of overtones","version":2},"cited_work":{"arxiv_id":"2210.14506","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.14506","snapshot_observed_at":"2026-06-29T20:43:58.743792Z","title":"Konoplya,Quasinormal modes in higher-derivative gravity: Testing the black hole parametrization and sensitivity of overtones,Phys","venue":null,"work_id":"9ce3e8b2-6c80-4089-bebc-b709c38edf88","year":2023},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2210.14506","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:8993c794a26c97e89d40935c7de159a065796b7fca3d383b7b9a5eeca1959057","observation_id":"688a70d9-639b-4559-a374-c9a874a5042f","resolution":{"observed_at":"2026-05-16T14:41:02.438558Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.22728","last_updated":"2026-05-14T14:37:19Z","snapshot_observed_at":"2026-07-06T22:40:12.666349Z","submitted_at":"2025-12-27T23:59:41Z","title":"Probing higher curvature gravity via ringdown with overtones","version":2},"cited_work":{"arxiv_id":"2512.22728","doi":null,"metadata_source":"pith","pith_arxiv_id":"2512.22728","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Probing higher curvature gravity via ringdown with overtones","venue":"gr-qc","work_id":"19f80237-8380-4ba7-b387-ef9716861692","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2512.22728","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:aa382994b683bfd2c8d8947698526952cf6cb633b7e99e4890460757f619e22a","observation_id":"15dba2d8-d187-42c9-9f64-8764688dea74","resolution":{"observed_at":"2026-05-16T14:41:02.448648Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2508.15534","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T09:26:51.314101Z","title":"Steppohn, S","venue":null,"work_id":"b8168600-41ad-44f3-adf1-1253c0f4afaf","year":2026},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:f7b9f3b6d14d5831221d16b76dee3ace67f1bd0cba0314b2a4cd7da3598de0ff","observation_id":"a94cbe55-7fa8-4edb-af2f-9d89c286a2f4","resolution":{"observed_at":"2026-05-16T14:41:02.473701Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.12080","last_updated":"2024-07-28T14:53:35Z","snapshot_observed_at":"2026-07-06T18:47:25.751118Z","submitted_at":"2024-07-16T18:00:00Z","title":"Isospectrality in Effective Field Theory Extensions of General Relativity","version":2},"cited_work":{"arxiv_id":"2407.12080","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.12080","snapshot_observed_at":"2026-07-02T19:27:18.937837Z","title":"Cano and M","venue":null,"work_id":"658077db-c904-4f44-a516-31e4862ff305","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2407.12080","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4710817bcd31f3fe415a6765894f16aff7cf5911860b1459c06d1b1342e12a76","observation_id":"a9cd7ec3-a7a9-4f82-b5a1-b777829f942e","resolution":{"observed_at":"2026-05-16T14:41:02.382854Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2504.17848","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Thomopoulos, S","venue":null,"work_id":"670e42bc-60f7-4e26-92fe-f771cd656edb","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4b948cdc8d7a26caadc14af033f535be2b07bb3887b5fc030cb0b4c486836f82","observation_id":"8f71dd10-43e2-476b-8497-3aac9431a111","resolution":{"observed_at":"2026-05-16T14:41:02.507424Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Seidel and S","venue":null,"work_id":"4a66c234-ccd1-4d9e-b64c-a45f183055a4","year":1990},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:d3aaff8e471b039267bc24d22afaefae15af15ca53410674a4e519fbbf430596","observation_id":"6568f7e8-146c-49e4-941b-ad67310380ed","resolution":{"observed_at":"2026-05-16T14:41:02.872613Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"eb2d48be-a347-4545-85d0-6073b4519d67","year":1991},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:53ed9b17334e25ba066f4e0fc1fcf3bd24cadb2871b1c0cb48ea50dbbe3c2df6","observation_id":"7717367a-feab-4d48-a3f4-6de78e9f6ddb","resolution":{"observed_at":"2026-05-16T14:41:02.869340Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.17786","last_updated":"2026-05-04T11:04:58Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-12-19T16:57:57Z","title":"Quasinormal modes of rotating black holes beyond general relativity in the WKB approximation","version":2},"cited_work":{"arxiv_id":"2512.17786","doi":null,"metadata_source":"pith","pith_arxiv_id":"2512.17786","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Quasinormal modes of rotating black holes beyond general relativity in the WKB approximation","venue":"gr-qc","work_id":"ad91101e-89d4-41e6-8ebb-442814a0eba9","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2512.17786","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:81f6f13ac0ec5a884c79d435407268127d170665d4d35e9b0143cb9b60257502","observation_id":"41ad126f-1f86-484d-b033-70e321924e10","resolution":{"observed_at":"2026-05-16T14:41:02.489496Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2509.08664","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"892b8eea-fcaf-4c8e-8a19-eccb1032f548","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:01749934e7c4a10b6a18ad013be4efd40d0a9515f16fd86d57ac3661effe16ac","observation_id":"7ca6a90a-a17f-42d7-896e-fa0535fba52f","resolution":{"observed_at":"2026-05-16T14:41:02.510428Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.17962","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"341296e3-83dc-4156-84a9-6ca7aae5f02e","year":2025},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:b3c52e5131470bac05ccebbe44ec436c3e7ad294ade68e57e7fe68dcc99f4355","observation_id":"ded2b396-5ec5-4696-8587-5aa45fe51af4","resolution":{"observed_at":"2026-05-16T14:41:02.403671Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0408077","last_updated":"2004-08-23T15:13:23Z","snapshot_observed_at":"2026-07-07T03:19:53.552377Z","submitted_at":"2004-08-23T15:13:23Z","title":"Late time tails from momentarily stationary, compact initial data in Schwarzschild spacetimes","version":1},"cited_work":{"arxiv_id":"gr-qc/0408077","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0408077","snapshot_observed_at":"2026-07-02T00:26:23.716087Z","title":"Late time tails from momentarily stationary, compact initial data in Schwarzschild spacetimes","venue":"gr-qc","work_id":"4dbb90d2-746a-4f8d-ae48-ae53367525c7","year":2004},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/gr-qc/0408077","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:5f446ab7f1d84befdefd6962c24028586d9557644a279d7646d7552a0099d071","observation_id":"6da1eab7-697a-45b9-a928-c46ea049189e","resolution":{"observed_at":"2026-05-16T14:41:02.367036Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0705.3620","last_updated":"2007-08-20T15:03:36Z","snapshot_observed_at":"2026-07-06T01:27:33.591412Z","submitted_at":"2007-05-24T16:51:44Z","title":"Scalar-field perturbations from a particle orbiting a black hole using numerical evolution in 2+1 dimensions","version":2},"cited_work":{"arxiv_id":"0705.3620","doi":null,"metadata_source":"pith","pith_arxiv_id":"0705.3620","snapshot_observed_at":"2026-07-02T10:06:51.909377Z","title":"Scalar-field perturbations from a particle orbiting a black hole using numerical evolution in 2+1 dimensions","venue":"gr-qc","work_id":"a706e36e-42dd-4193-8213-efc995c9dd8b","year":2007},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/0705.3620","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:7ff38709426560e3233686d16c00bab236a8c67b9e647042139be0a6b05b4a56","observation_id":"925a71c3-0d37-4ce7-86c8-d9966626e6b2","resolution":{"observed_at":"2026-05-16T14:41:02.396634Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0409065","last_updated":"2004-09-17T00:09:25Z","snapshot_observed_at":"2026-07-07T03:19:58.621663Z","submitted_at":"2004-09-17T00:09:25Z","title":"Numerical integration of the Teukolsky Equation in the time domain","version":1},"cited_work":{"arxiv_id":"gr-qc/0409065","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0409065","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Numerical integration of the Teukolsky Equation in the time domain","venue":"gr-qc","work_id":"4b852440-c110-45d9-81b5-4c12c0be342a","year":2004},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/gr-qc/0409065","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:4771cdabb944b70c65ca9665b8e3f1a807e9dd6224fc8e32093a5d083d00c1ec","observation_id":"72743b22-abe6-423d-8e13-4cc0d180378f","resolution":{"observed_at":"2026-05-16T14:41:02.335219Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9902072","last_updated":"1999-12-29T07:48:05Z","snapshot_observed_at":"2026-07-07T03:30:05.486634Z","submitted_at":"1999-02-23T14:05:12Z","title":"Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field","version":4},"cited_work":{"arxiv_id":"gr-qc/9902072","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9902072","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Mode-Coupling in Rotating Gravitational Collapse of a Scalar Field","venue":"gr-qc","work_id":"efc4159e-99bf-4047-a390-96073e361a11","year":1999},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/gr-qc/9902072","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:d712c06fd16d1b8f50d1a7c0efc51ddf24c2981c03a3d3c5e055351490afc418","observation_id":"daa23a7c-c5f8-4e8f-8e0e-c4957455d390","resolution":{"observed_at":"2026-05-16T14:41:02.410381Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.10797","last_updated":"2024-02-22T10:58:50Z","snapshot_observed_at":"2026-07-06T17:31:13.010759Z","submitted_at":"2024-02-16T16:21:02Z","title":"BlackJAX: Composable Bayesian inference in JAX","version":2},"cited_work":{"arxiv_id":"2402.10797","doi":"10.48550/arxiv.2402.10797","metadata_source":"arxiv_reference","pith_arxiv_id":"2402.10797","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"BlackJAX: composable Bayesian inference in JAX","venue":null,"work_id":"c97ec9eb-af6a-459f-8338-c7119a28c640","year":2024},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"cited_paper":"/paper/2402.10797","citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:576e7595f3723668fbd1e7dfe7873f80ea67483be45b94e175bda327d74bb6a2","observation_id":"65eeea40-cf90-4f72-92ee-0114e98002c7","resolution":{"observed_at":"2026-05-16T14:41:02.502010Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bradbury, R","venue":null,"work_id":"e63123fd-c37e-431d-9dec-a2f8e26eea35","year":2018},"citing_paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-05-16T14:40:32.437670Z"},"links":{"citing_paper":"/paper/2601.09607"},"observation_digest":"sha256:086fd58cc96f3e7d8444a389e01364615eb57279234d7591e843396dedafb581","observation_id":"3a36b2ad-8757-4762-905b-131aada07442","resolution":{"observed_at":"2026-05-16T14:41:02.871042Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-01T06:32:01.292127+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2601.09607","last_updated":"2026-05-05T11:56:11Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T22:41:43.594456Z","submitted_at":"2026-01-14T16:30:02Z","title":"Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr"},"reference_resolution":{"displayed":97,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":9,"verified_exact":78,"verified_fuzzy":8},"total_outbound_references":97},"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":"2026-08-01T06:32:01.292127+00:00","source":"crossref"},{"observed_at":"2026-08-01T06:31:58.492377+00:00","source":"retraction_watch"}],"thesis":"As of 1 August 2026, this Paper Citation Record lists 97 of 97 outbound references and 2 inbound Pith citation observations for arXiv:2601.09607."}