{"as_of":"2026-08-10T11:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6771d107644d284bca14a014e1b7c40e7d61e46be2416ce410d1b64438079681","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T16:40:25.000701Z","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":"2026-07-03T02:57:35.426929Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-07T14:55:33.954655Z","title":null,"venue":null,"work_id":null,"year":2025},"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":52,"source":"pdf_text","source_observed_at":"2026-08-07T14:55:33.954655Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2505.17186"},"observation_digest":"sha256:11593823c2c5bf84d6e5cbd7aa57fab9d4e120a7b52a5111b85c95186dd2b097","observation_id":"f8e6a18d-f921-4059-a2ca-d9539a764c0b","resolution":{"observed_at":"2026-08-07T14:55:33.954655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-07T11:08:24.664945Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.03600","last_updated":"2025-07-08T14:44:56Z","snapshot_observed_at":"2026-08-09T16:02:14.508507Z","submitted_at":"2025-06-04T06:14:27Z","title":"Axial quasi-normal modes of slowly rotating black holes in dynamical Chern-Simons gravity to second-order in spin and coupling","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-07T11:08:24.664945Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2506.03600"},"observation_digest":"sha256:977fe751e2e981964b29ca5a7c2294cd1c4ee33169fa3362ffde5c2c42fda807","observation_id":"ed893ae5-024b-4d9a-bbfb-8daa207aa810","resolution":{"observed_at":"2026-08-07T11:08:24.664945Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-06T21:02:47.802674Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.02045","last_updated":"2025-07-07T04:17:36Z","snapshot_observed_at":"2026-08-08T14:53:25.848689Z","submitted_at":"2025-07-02T18:00:02Z","title":"Extreme mass-ratio inspiral within an ultralight scalar cloud I. Scalar radiation","version":2},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-08-06T21:02:47.802674Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2507.02045"},"observation_digest":"sha256:c7775af36291cc9f44887eafea3bf10d27d22e47ed356ca3eccff19c7f190c68","observation_id":"bec5adcb-565e-4ee7-b845-1ea4d379b6ba","resolution":{"observed_at":"2026-08-06T21:02:47.802674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-06T20:20:13.743559Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.03380","last_updated":"2026-06-26T06:16:22Z","snapshot_observed_at":"2026-08-09T20:30:52.423748Z","submitted_at":"2025-07-04T08:24:29Z","title":"Extreme mass-ratio inspirals and extra dimensions: Insights from modified Teukolsky framework","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T20:20:13.743559Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2507.03380"},"observation_digest":"sha256:4a56efe96253929a7e1843dcbb266c1cb6354f0b826e3a73ad4f078179377ff0","observation_id":"fda33ac1-0b75-44fb-9d12-c78ea8a0c8aa","resolution":{"observed_at":"2026-08-06T20:20:13.743559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":"2503.15606","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-07-03T02:57:35.426929Z","title":null,"venue":null,"work_id":"849308c2-a356-43d7-a7dd-69e5ab765190","year":2025},"citing_paper":{"arxiv_id":"2509.08054","last_updated":"2025-09-09T18:00:07Z","snapshot_observed_at":"2026-07-06T22:27:15.482704Z","submitted_at":"2025-09-09T18:00:07Z","title":"GW250114: testing Hawking's area law and the Kerr nature of black holes","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-13T21:29:44.416458Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2509.08054"},"observation_digest":"sha256:7ec50a8a4d46c9932eee89451fdfdd4a733ff63da013d3741868336e3bc2cc11","observation_id":"c8df8ad4-6fc6-45ac-badc-5ef45aeeb93e","resolution":{"observed_at":"2026-05-13T21:29:44.909153Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":"2503.15606","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-07-03T02:57:35.426929Z","title":null,"venue":null,"work_id":"849308c2-a356-43d7-a7dd-69e5ab765190","year":2025},"citing_paper":{"arxiv_id":"2510.11793","last_updated":"2026-05-13T10:10:18Z","snapshot_observed_at":"2026-08-01T10:09:57.706869Z","submitted_at":"2025-10-13T18:00:08Z","title":"Black hole mergers beyond general relativity: a self-force approach","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-18T07:14:28.658616Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2510.11793"},"observation_digest":"sha256:b6f6e7e3fbb0df5949c6e907b34273e4288efcb2173b84cd5561f9e7d4ab1617","observation_id":"16ac4678-5a37-47bd-b7fe-a555161994fe","resolution":{"observed_at":"2026-05-18T07:16:02.370584Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-03T16:10:09.576879Z","title":"Perturba- tions of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.14679","last_updated":"2026-06-02T20:05:19Z","snapshot_observed_at":"2026-08-06T20:17:09.405008Z","submitted_at":"2025-12-16T18:44:15Z","title":"Computing spectral shifts for Johannsen-Psaltis black holes","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T16:10:09.576879Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2512.14679"},"observation_digest":"sha256:88f0a8b2c37be7905b799ff44b2c51912d46cf761cabc2930a123428cb90259d","observation_id":"993bd6e3-f71a-486c-8077-a9980781093d","resolution":{"observed_at":"2026-08-03T16:10:09.576879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":"2503.15606","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-07-03T02:57:35.426929Z","title":null,"venue":null,"work_id":"849308c2-a356-43d7-a7dd-69e5ab765190","year":2025},"citing_paper":{"arxiv_id":"2604.18680","last_updated":"2026-04-20T18:00:01Z","snapshot_observed_at":"2026-07-06T23:05:30.879164Z","submitted_at":"2026-04-20T18:00:01Z","title":"Beyond Three Terms: Continued Fractions for Rotating Black Holes in Modified Gravity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-10T04:08:08.348850Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2604.18680"},"observation_digest":"sha256:dabb74acc56b76797fe16ddb8c10833f2fc25571e90c87c620eeace93100f4a2","observation_id":"cb93b356-bab6-4347-9478-0229ba4324b0","resolution":{"observed_at":"2026-05-11T12:11:03.612446Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":"2503.15606","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-07-03T02:57:35.426929Z","title":null,"venue":null,"work_id":"849308c2-a356-43d7-a7dd-69e5ab765190","year":2025},"citing_paper":{"arxiv_id":"2605.11080","last_updated":"2026-05-11T18:00:04Z","snapshot_observed_at":"2026-07-06T23:22:57.012338Z","submitted_at":"2026-05-11T18:00:04Z","title":"Metric Reconstruction for Generic Black-Hole Perturbations","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-13T03:23:04.483342Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2605.11080"},"observation_digest":"sha256:9aeb15a67db8f8a1c1b48b89abd5ce386870d57199358e01cf97800499baa0c5","observation_id":"8d79288c-021f-44eb-96c0-3857474975e1","resolution":{"observed_at":"2026-05-13T03:27:11.931418Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":"2503.15606","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-07-03T02:57:35.426929Z","title":null,"venue":null,"work_id":"849308c2-a356-43d7-a7dd-69e5ab765190","year":2025},"citing_paper":{"arxiv_id":"2606.09766","last_updated":"2026-06-08T17:29:05Z","snapshot_observed_at":"2026-07-06T23:49:03.237958Z","submitted_at":"2026-06-08T17:29:05Z","title":"Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-06-27T15:39:20.928032Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2606.09766"},"observation_digest":"sha256:e9035b732551ad11558ce8a9fd290f4c487f09b2925d0d99c80137da36fa1cc9","observation_id":"c0f370e9-1794-45a9-aafd-31bcefd37916","resolution":{"observed_at":"2026-07-03T02:57:35.428215Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-01T12:40:48.145641Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19492","last_updated":"2026-07-21T18:09:34Z","snapshot_observed_at":"2026-08-09T10:07:46.680871Z","submitted_at":"2026-07-21T18:09:34Z","title":"Schr\\\"odinger perturbation theory for black hole quasinormal modes","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-01T12:40:48.145641Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2607.19492"},"observation_digest":"sha256:57a0a012deede36b0e50248934ce087b8e6c537ecfd319f84bb2f40a1f93afba","observation_id":"05cdd2e4-abc7-40ea-be8b-9f469a37a6df","resolution":{"observed_at":"2026-08-01T12:40:48.145641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-01T02:56:25.105719Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.25311","last_updated":"2026-07-28T05:48:30Z","snapshot_observed_at":"2026-08-06T08:30:25.996678Z","submitted_at":"2026-07-28T05:48:30Z","title":"Parametrized beyond-Teukolsky framework in the time domain","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-01T02:56:25.105719Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2607.25311"},"observation_digest":"sha256:9dd1097ad5deaa48e9b6e27a8e98f4d8c1828baa022ec931f136e976ce4748c2","observation_id":"f96942f7-5436-444a-996a-a9d5093d053a","resolution":{"observed_at":"2026-08-01T02:56:25.105719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.15606","snapshot_observed_at":"2026-08-08T16:40:25.000701Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05268","last_updated":"2026-08-05T18:00:00Z","snapshot_observed_at":"2026-08-09T23:10:27.076184Z","submitted_at":"2026-08-05T18:00:00Z","title":"Living on the Edge of Effective Field Theory: Near-Extremal Black Holes in Quadratic Gravity","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-08T16:40:25.000701Z"},"links":{"cited_paper":"/paper/2503.15606","citing_paper":"/paper/2608.05268"},"observation_digest":"sha256:33d6b6994912d0879cc8fc358e8fa99fba84ed1da3aa81b4d0ec72d41c271b82","observation_id":"5185d797-f0ea-4645-bb76-d971f5643dbb","resolution":{"observed_at":"2026-08-08T16:40:25.000701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.15606/citation-record","integrity":"/paper/2503.15606/integrity","json":"/paper/2503.15606/citation-record.json","paper":"/paper/2503.15606"},"outbound":[],"paper":{"arxiv_id":"2503.15606","last_updated":"2025-03-19T18:00:02Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T16:50:56.726097Z","submitted_at":"2025-03-19T18:00:02Z","title":"Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2503.15606."}