{"as_of":"2026-08-08T18:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fdf4654702f61468e1343e3feb90cf7d175a721f7e37fae089ada0d0cbbccbcd","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":14,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":14,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:55:31.660650Z","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":"2026-06-29T20:43:58.785376Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"1907.06463","last_updated":"2019-07-23T16:45:37Z","snapshot_observed_at":"2026-08-03T18:17:01.815766Z","submitted_at":"2019-07-15T12:20:44Z","title":"Perturbing microscopic black holes inspired by noncommutativity","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-24T21:26:05.683547Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/1907.06463"},"observation_digest":"sha256:1923ffa2cdec4e45b45d38bb9f963722f556734844b8575c0b46b0464511e720","observation_id":"292db740-ac34-422c-aff7-fa974b85f789","resolution":{"observed_at":"2026-05-24T21:26:22.759140Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-08-07T14:55:31.660650Z","title":"Hatsuda, Quasinormal modes of black holes and Borel summation, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.17186","last_updated":"2025-06-26T08:22:36Z","snapshot_observed_at":"2026-08-08T12:28:05.504844Z","submitted_at":"2025-05-22T18:00:03Z","title":"Bound States of the Schwarzschild Black Hole","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T14:55:31.660650Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2505.17186"},"observation_digest":"sha256:c47548c1c3ed91d18beefcbe774268ba48325919bdbc1a013396d9f87e74cf96","observation_id":"b810e4ca-b654-440a-9015-6fdffb0a0dd6","resolution":{"observed_at":"2026-08-07T14:55:31.660650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-08-07T14:46:39.360988Z","title":"Quasinormal modes of black holes and Borel summation,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.17947","last_updated":"2025-05-23T14:24:05Z","snapshot_observed_at":"2026-08-07T14:35:26.578610Z","submitted_at":"2025-05-23T14:24:05Z","title":"Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-07T14:46:39.360988Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2505.17947"},"observation_digest":"sha256:0450ecdb55d8f42ab3b6d94e1da5b7e53e1da7c6cd6e6ec9ce4f17097ec96279","observation_id":"2d159e2f-0748-4b06-8b51-3a1c2c9c2dff","resolution":{"observed_at":"2026-08-07T14:46:39.360988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"2510.11766","last_updated":"2026-03-30T15:33:50Z","snapshot_observed_at":"2026-07-31T11:31:52.166326Z","submitted_at":"2025-10-13T14:34:27Z","title":"Exact WKB method for radial Schr\\\"odinger equation","version":4},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-18T07:46:22.313894Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2510.11766"},"observation_digest":"sha256:f4574883c3190d5925a2703cc7d2bc4894adc4166500c40ba50cd87a18fbc6d0","observation_id":"462edf1f-9026-4345-8441-b8c33b28baa3","resolution":{"observed_at":"2026-05-18T07:51:03.962497Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-08-03T21:34:56.864031Z","title":"Hatsuda, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.15140","last_updated":"2026-06-01T14:01:36Z","snapshot_observed_at":"2026-08-07T15:12:11.685935Z","submitted_at":"2025-11-19T05:38:36Z","title":"Gravitational Bound State Perturbations Inside Black Holes and Isospectrality","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T21:34:56.864031Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2511.15140"},"observation_digest":"sha256:9115005a035aceb9d54da93e0a2561a30fc4779fcf4c869ff314d93f9add6b0e","observation_id":"1443b892-8465-4606-a904-cf3416ee7a43","resolution":{"observed_at":"2026-08-03T21:34:56.864031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"2602.16972","last_updated":"2026-04-17T12:34:00Z","snapshot_observed_at":"2026-07-06T22:46:21.571641Z","submitted_at":"2026-02-19T00:24:12Z","title":"Anomalous Decay Rate and Greybody Factors for Regular Black Holes with Scalar Hair","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-15T21:46:56.981507Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2602.16972"},"observation_digest":"sha256:a13c19dd1dcb30af258b97e44d9f3cbd938223c7e40cbe67a5d74f43e4d09bae","observation_id":"618d658f-5061-4c30-8eea-bfd454b63c43","resolution":{"observed_at":"2026-05-15T21:50:21.044431Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"2603.19168","last_updated":"2026-07-16T16:18:10Z","snapshot_observed_at":"2026-08-02T17:54:52.841712Z","submitted_at":"2026-03-19T17:24:47Z","title":"Quasinormal Modes of Extremal Reissner-Nordstrom Black Holes via Seiberg-Witten Quantization","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-21T10:54:19.470781Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2603.19168"},"observation_digest":"sha256:11845332d9b3b4b40a98c2f813b212c710ea1f6692e754ed6d6681a8c37cad2b","observation_id":"02ae83e4-157a-4210-8076-a76228d46213","resolution":{"observed_at":"2026-05-21T10:55:01.185442Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-08-02T17:54:56.293926Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.19168","last_updated":"2026-07-16T16:18:10Z","snapshot_observed_at":"2026-08-02T17:54:52.841712Z","submitted_at":"2026-03-19T17:24:47Z","title":"Quasinormal Modes of Extremal Reissner-Nordstrom Black Holes via Seiberg-Witten Quantization","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-02T17:54:56.293926Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2603.19168"},"observation_digest":"sha256:0062b62463c31f6def2aff998d0f1ccfe9d253acdb0cefe238f88ed9725f194a","observation_id":"3fb2387d-d7c7-4f3b-923e-cb5aa495d9ed","resolution":{"observed_at":"2026-08-02T17:54:56.293926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"2604.26166","last_updated":"2026-04-28T23:17:26Z","snapshot_observed_at":"2026-07-06T23:11:52.954360Z","submitted_at":"2026-04-28T23:17:26Z","title":"Scattering of electromagnetic field in quasi-topological gravity","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-07T14:54:38.809214Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2604.26166"},"observation_digest":"sha256:fd04a0e8d8ff3299820bf4e5e5b6204ce41a162b4129075acdf7abf79303e3a9","observation_id":"35586f8e-316b-4a8c-bbd7-fdb2d20dad12","resolution":{"observed_at":"2026-05-12T00:36:16.936569Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"2605.11013","last_updated":"2026-05-10T12:56:40Z","snapshot_observed_at":"2026-07-06T23:22:52.369277Z","submitted_at":"2026-05-10T12:56:40Z","title":"Massive Scalar Quasinormal Modes, Greybody Factors, and Absorption Cross Section of a Parity-Symmetric Beyond-Horndeski Black Hole","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-05-13T01:58:50.185004Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2605.11013"},"observation_digest":"sha256:c93597172a8090fb5529764d24eade1faf8648d183a30485779bb44427c4e165","observation_id":"4276e569-2c20-49f3-9c03-88b5c25920dc","resolution":{"observed_at":"2026-05-13T02:07:08.525877Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":"1906.07232","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-06-29T20:43:58.785376Z","title":"Hatsuda,Quasinormal modes of black holes and Borel summation,Phys","venue":null,"work_id":"d95c323a-fd55-4387-a35d-8e0cbe395bca","year":2020},"citing_paper":{"arxiv_id":"2605.25705","last_updated":"2026-05-25T11:03:23Z","snapshot_observed_at":"2026-07-06T23:35:36.158984Z","submitted_at":"2026-05-25T11:03:23Z","title":"Ces\\`aro convergence of the high-order WKB method and its applications to black-hole overtones and long-lived modes","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-06-29T20:43:00.569439Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2605.25705"},"observation_digest":"sha256:c8873d66a9c3b18adf2c0d4559ae037eba6adbee937379dce56c87ea3be66e90","observation_id":"7935d656-9b12-4d43-b5ab-4029e13f4eb3","resolution":{"observed_at":"2026-06-29T20:43:58.786775Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-07-12T01:38:05.217536Z","title":"Hatsuda, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-05T15:30:48.699158Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-12T01:38:05.217536Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:541d52100770f1d4dc65e4bec4df742640ebc90c6cc4e73a65e6346fb470aa82","observation_id":"16797cd6-39cd-4a88-9d24-75dd21339b1d","resolution":{"observed_at":"2026-07-12T01:38:05.217536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-08-02T08:53:13.406709Z","title":"Hatsuda, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-05T15:30:48.699158Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-02T08:53:13.406709Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:ad3a8ccea72bb150708c6b4723e26ce2100f69042a8850715a13889ec627c86f","observation_id":"f2fdf7de-0d50-44aa-83de-f66fc933ea10","resolution":{"observed_at":"2026-08-02T08:53:13.406709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.07232","snapshot_observed_at":"2026-07-30T12:53:50.371221Z","title":"Hatsuda, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.27043","last_updated":"2026-07-29T15:34:07Z","snapshot_observed_at":"2026-08-08T06:32:28.576733Z","submitted_at":"2026-07-29T15:34:07Z","title":"Resumming Kerr Quasinormal-Mode Frequencies: Accuracy and Breakdown Near Extremality","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-30T12:53:50.371221Z"},"links":{"cited_paper":"/paper/1906.07232","citing_paper":"/paper/2607.27043"},"observation_digest":"sha256:0a82b25c84dc2a0a00cf9c51e5eb13368fb1d9421c5c7d76249fbb1c37313c9e","observation_id":"b7f3203c-32fd-4dd2-b6f9-27b21455e622","resolution":{"observed_at":"2026-07-30T12:53:50.371221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1906.07232/citation-record","integrity":"/paper/1906.07232/integrity","json":"/paper/1906.07232/citation-record.json","paper":"/paper/1906.07232"},"outbound":[],"paper":{"arxiv_id":"1906.07232","last_updated":"2019-10-05T07:16:18Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-05T23:17:49.872445Z","submitted_at":"2019-06-17T19:34:17Z","title":"Quasinormal modes of black holes and Borel summation"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1906.07232."}