{"as_of":"2026-08-07T19:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:acd0ddba1367f3a62b52304369f3cef029ab88a11f1facd9349c24514e332f50","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":22,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":22,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":22,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":22,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T13:41:48.904687Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-19T17:47:41.806126Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-07T13:41:48.904687Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.21303","last_updated":"2025-07-03T13:24:54Z","snapshot_observed_at":"2026-08-07T13:28:11.475614Z","submitted_at":"2025-05-27T15:05:21Z","title":"Spectrum instability and greybody factor stability for parabolic approximation of Regge-Wheeler potential","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T13:41:48.904687Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2505.21303"},"observation_digest":"sha256:79006900c993db9583f044722d936b251057a0acff34139e43dec444562e5736","observation_id":"acbd9104-079a-4188-9779-d67a082390eb","resolution":{"observed_at":"2026-08-07T13:41:48.904687Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-07T04:46:12.394638Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.394638Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:396507c225e2713e80d9bd5f77ad63217ea187eb48c3c27881d8e3607f1bd381","observation_id":"e6af6506-71d5-4d41-bf28-929fd5589865","resolution":{"observed_at":"2026-08-07T04:46:12.394638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-06T19:10:27.070151Z","title":"Review of analytic results on quasinormal modes of black holes","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.07196","last_updated":"2025-07-09T18:11:20Z","snapshot_observed_at":"2026-08-06T18:44:15.104893Z","submitted_at":"2025-07-09T18:11:20Z","title":"Gravitational Quasinormal Modes and Grey-Body Factors of Bonanno-Reuter Regular Black Holes","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T19:10:27.070151Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2507.07196"},"observation_digest":"sha256:c9eb1a17d15497fa7b36eaeb593642dd81cca4df3b78013365a2d199664ce9be","observation_id":"2f8b5e8a-573c-4a45-b4b1-3730db01c1f4","resolution":{"observed_at":"2026-08-06T19:10:27.070151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-05T19:07:26.479113Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.13366","last_updated":"2026-07-22T14:35:30Z","snapshot_observed_at":"2026-08-07T18:18:39.515438Z","submitted_at":"2025-08-18T21:17:11Z","title":"Where Do the Returns to Schooling Come From? Educational Transitions and Labor Market Payoffs","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-05T19:07:26.479113Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2508.13366"},"observation_digest":"sha256:7b4d1358c71f1f2672f22097d096da26f1e639102a3ca632f34e9975818dbaf9","observation_id":"59eaa81d-31ef-4b8c-9f80-939dd5707788","resolution":{"observed_at":"2026-08-05T19:07:26.479113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-04T11:09:44.673052Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06689","last_updated":"2026-05-28T09:50:09Z","snapshot_observed_at":"2026-08-04T11:09:41.169992Z","submitted_at":"2025-10-08T06:25:32Z","title":"Bonanno-Reuter regular black hole: quasi-resonances, grey-body factors and absorption cross-sections of a massive scalar field","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-04T11:09:44.673052Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2510.06689"},"observation_digest":"sha256:0092c7eca93c5c63ff8788cf958a2fa54bbf173f1c2d1d0cd543db566fb78c11","observation_id":"8ecdea78-2d55-4109-a84a-0cfa2f3d4303","resolution":{"observed_at":"2026-08-04T11:09:44.673052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-03T22:11:06.727891Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.12335","last_updated":"2026-05-28T09:58:14Z","snapshot_observed_at":"2026-08-03T22:11:04.419217Z","submitted_at":"2025-11-15T19:28:44Z","title":"Long-lived quasinormal modes and grey-body factors of supermassive black holes with a dark matter halo","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-03T22:11:06.727891Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2511.12335"},"observation_digest":"sha256:b9ba58243311c45f620662c54c3db30c68d3f04b97c7eaca8c8bcbbae6586321","observation_id":"58a86a03-7ddf-45a6-8c7f-c9e74f21e4b2","resolution":{"observed_at":"2026-08-03T22:11:06.727891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2512.01694","last_updated":"2026-05-06T12:34:49Z","snapshot_observed_at":"2026-07-06T22:37:26.652349Z","submitted_at":"2025-12-01T14:02:32Z","title":"Quasinormal modes of Reissner-Nordstr\\\"om-AdS black holes under physical field-vanishing boundary conditions","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-17T03:13:17.833343Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2512.01694"},"observation_digest":"sha256:5c2c78315ae0960c01cece2421d63043f605618e06d17f9a184d95342d29fbb8","observation_id":"dc328e0e-8c4f-495f-b3d8-49f8a8224c80","resolution":{"observed_at":"2026-05-17T03:13:56.349892Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2601.17906","last_updated":"2026-04-02T18:11:47Z","snapshot_observed_at":"2026-07-06T22:42:57.796038Z","submitted_at":"2026-01-25T16:54:41Z","title":"Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-16T11:06:54.209646Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2601.17906"},"observation_digest":"sha256:758d03fa9ab0658255398e0ebb95b1fce2b98a6bbb492a24a80e36ff5e061198","observation_id":"7f12a466-d703-4e36-b34d-c4e0da18f836","resolution":{"observed_at":"2026-05-16T11:07:47.557855Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2602.11001","last_updated":"2026-04-17T10:43:09Z","snapshot_observed_at":"2026-07-06T22:45:29.609382Z","submitted_at":"2026-02-11T16:23:23Z","title":"Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-16T02:41:01.645151Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2602.11001"},"observation_digest":"sha256:9c1cd7ea75296fe44c1912cd2febd8480400c818bec1bac9765ae84a5930f6e9","observation_id":"addef51d-c761-4f03-b2a6-3f8a815e9f85","resolution":{"observed_at":"2026-05-16T02:42:11.078527Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2603.10844","last_updated":"2026-04-16T17:09:38Z","snapshot_observed_at":"2026-07-06T22:48:39.649787Z","submitted_at":"2026-03-11T14:52:37Z","title":"Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity","version":2},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-05-15T13:15:54.975020Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2603.10844"},"observation_digest":"sha256:3cb878c30413fa1892421241179dbb3d9a8c8216ebd39c6923fc6b7eb9a76672","observation_id":"96d6139b-f0a1-4e34-a66e-0cde2a83f77f","resolution":{"observed_at":"2026-05-15T13:20:02.613603Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-04T05:43:13.377002Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.28415","last_updated":"2026-08-03T09:20:37Z","snapshot_observed_at":"2026-08-07T15:27:22.728093Z","submitted_at":"2026-03-30T13:27:04Z","title":"Long-lived quasinormal frequencies for regular black hole supported by the Einasto profile in the presence of the magnetic field","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:13.377002Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2603.28415"},"observation_digest":"sha256:7aabb2b3ceec27b39d2815d4a1f8ee2ec3ff87bdcb0b4fd52fa1513ecbafa47b","observation_id":"078f83c9-e10b-4536-a90a-fc02683e345b","resolution":{"observed_at":"2026-08-04T05:43:13.377002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.05988","last_updated":"2026-04-14T01:19:58Z","snapshot_observed_at":"2026-07-06T22:54:34.877944Z","submitted_at":"2026-04-07T15:15:39Z","title":"Quasinormal modes of coupled metric-dilaton perturbations in two-dimensional stringy black holes","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-10T19:27:42.210539Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.05988"},"observation_digest":"sha256:47ec91b81bf2b14bf49973fe8b0122662ca1ff3371cbcbe17a4e993892754160","observation_id":"66fc7e31-8c8d-48f7-88b3-779299f529cb","resolution":{"observed_at":"2026-05-10T22:55:51.485594Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.14011","last_updated":"2026-05-15T14:49:14Z","snapshot_observed_at":"2026-07-06T23:01:55.698452Z","submitted_at":"2026-04-15T15:56:46Z","title":"Properties of black holes in non-linear electrodynamics","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-10T13:14:49.840034Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.14011"},"observation_digest":"sha256:00a7a48a8cf74e8469a385f2cdf2b63c669b5d0a52b4304a71e56eb6089fc1f4","observation_id":"7ef19517-5162-4e87-975f-f8abc7786ba1","resolution":{"observed_at":"2026-05-10T13:15:26.035080Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.14011","last_updated":"2026-05-15T14:49:14Z","snapshot_observed_at":"2026-07-06T23:01:55.698452Z","submitted_at":"2026-04-15T15:56:46Z","title":"Properties of black holes in non-linear electrodynamics","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-19T17:44:25.575644Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.14011"},"observation_digest":"sha256:1a930e4ba4f4dffbaf50595b35456c913ec2d681b96672d88ca48d3e19fd3bd9","observation_id":"9d53d110-c691-4f45-9675-f96696960324","resolution":{"observed_at":"2026-05-19T17:47:41.808283Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-07-06T23:10:24.992210Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-08T02:18:25.796367Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:fef6cfbfb225fe3fd93a0e1f042d2f5fa9e3f0ff3c03fa27237c5353c5ca5379","observation_id":"04734788-a883-4d27-a7c8-758eab847ee1","resolution":{"observed_at":"2026-05-11T22:51:24.290236Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-07-06T23:10:24.992210Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-14T22:18:47.797399Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:e48a90a08125ab094746148a2435297574563073b9736f61e30cd7a52bf5d65c","observation_id":"6a8435f4-3904-46ed-bcd3-2101bdf625e1","resolution":{"observed_at":"2026-05-14T22:19:31.416372Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.25471","last_updated":"2026-04-28T10:23:30Z","snapshot_observed_at":"2026-08-02T11:44:34.483229Z","submitted_at":"2026-04-28T10:23:30Z","title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-07T15:29:43.270538Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.25471"},"observation_digest":"sha256:386fd675c875ca14d0dfe33c331e596d556277fda0553fa38667785c4f9edf20","observation_id":"236a1764-2bdb-4e21-91f3-ea5d83bf0d7e","resolution":{"observed_at":"2026-05-12T00:21:19.070174Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.27377","last_updated":"2026-05-14T08:22:09Z","snapshot_observed_at":"2026-08-02T19:16:39.344546Z","submitted_at":"2026-04-30T03:40:14Z","title":"Bound-State Resonances of Schwarzschild-de Sitter Black Holes: Analytic Treatment","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-07T08:48:22.714715Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.27377"},"observation_digest":"sha256:d9d302b8a2e44de4d8980933d427087fc073757d40e19a9ebbfdd905564b799c","observation_id":"8e0713d8-6dc7-4fcc-96ec-7802b98d238a","resolution":{"observed_at":"2026-05-12T09:56:27.314816Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2604.27377","last_updated":"2026-05-14T08:22:09Z","snapshot_observed_at":"2026-08-02T19:16:39.344546Z","submitted_at":"2026-04-30T03:40:14Z","title":"Bound-State Resonances of Schwarzschild-de Sitter Black Holes: Analytic Treatment","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-15T06:54:18.351038Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2604.27377"},"observation_digest":"sha256:848f0df6486f44be492b4306f72f1d5e8909ffd83e36b6109e35e29898ac5d7c","observation_id":"864e8d59-2ee6-41ce-8f8b-2b981ef7fe5b","resolution":{"observed_at":"2026-05-15T06:55:10.247642Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2605.11364","last_updated":"2026-05-12T00:34:59Z","snapshot_observed_at":"2026-08-03T00:14:03.960316Z","submitted_at":"2026-05-12T00:34:59Z","title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-13T02:39:27.974688Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2605.11364"},"observation_digest":"sha256:dfe394a90a837ca8dbfb79b7ef7b4659c0d7483dd839d7084263adbe9d86cf36","observation_id":"bc4ac1fe-607a-4d11-a94a-56a1a209915b","resolution":{"observed_at":"2026-05-13T02:47:08.407300Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2605.12113","last_updated":"2026-05-12T13:29:10Z","snapshot_observed_at":"2026-08-04T03:37:25.006389Z","submitted_at":"2026-05-12T13:29:10Z","title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-13T04:51:34.508568Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2605.12113"},"observation_digest":"sha256:d9520c18a8628179e77cfac4930ebe9c30bf5cb8b155a813e8db5b68df4e1dd6","observation_id":"501d4425-ac71-4736-87f0-b8f1b64f496d","resolution":{"observed_at":"2026-05-13T04:52:16.350061Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":"2504.05014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bolokhov and M","venue":null,"work_id":"8f83628b-dc41-4d8d-991b-d34b674485d9","year":2025},"citing_paper":{"arxiv_id":"2605.13797","last_updated":"2026-05-13T17:19:24Z","snapshot_observed_at":"2026-08-05T23:10:41.768444Z","submitted_at":"2026-05-13T17:19:24Z","title":"Thin Accretion Disks around Rotating Charged Black Holes in an Effective Higher-Curvature Spacetime","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-14T17:44:03.513353Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2605.13797"},"observation_digest":"sha256:ae1d5f713d7868fb5fa24b265a2efbe6b4f237532295c4a27ce04cb42076ac95","observation_id":"4bb0ff6a-50c3-41af-9274-065952324fa7","resolution":{"observed_at":"2026-05-14T17:49:23.481994Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2504.05014/citation-record","integrity":"/paper/2504.05014/integrity","json":"/paper/2504.05014/citation-record.json","paper":"/paper/2504.05014"},"outbound":[],"paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2504.05014."}