Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Quasinormal frequencies of D-dimensional Schwarzschild black holes: evaluation via continued fraction method
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:gr-qc/0606110.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-29T20:43:00.569439Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-29T21:03:59.158668Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
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- parse uncertain0
- malformed identifier0
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External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation dca050e3-1eca-4633-8a2f-d022511bdd7d · inbound
Quasinormal modes of black holes and black branes cites this paper.
Quasinormal modes of black holes and black branes Quasinormal frequencies of D-dimensional Schwarzschild black holes: evaluation via continued fraction method
Reference 274
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-12T00:59:53.418574Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 4f096c17-5efa-4e7f-bef3-ea205b8f8eae · inbound
Quasinormal modes of black holes: from astrophysics to string theory cites this paper.
Quasinormal modes of black holes: from astrophysics to string theory Quasinormal frequencies of D-dimensional Schwarzschild black holes: evaluation via continued fraction method
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T02:19:40.799009Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation b4949db3-2323-4205-80a4-ff1e630caf1b · inbound
Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes cites this paper.
Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes Quasinormal frequencies of D-dimensional Schwarzschild black holes: evaluation via continued fraction method
Reference 93
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T10:40:51.115386Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 64875ddf-8446-4e9d-97b9-632630690a99 · inbound
Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes cites this paper.
Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes Quasinormal frequencies of D-dimensional Schwarzschild black holes: evaluation via continued fraction method
Reference 120
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-16T02:42:10.663986Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 5b04dbb1-42b1-4cf2-af83-8c7a6cf1e4bc · inbound
Ces\`aro convergence of the high-order WKB method and its applications to black-hole overtones and long-lived modes cites this paper.
Ces\`aro convergence of the high-order WKB method and its applications to black-hole overtones and long-lived modes Quasinormal frequencies of D-dimensional Schwarzschild black holes: evaluation via continued fraction method
Reference 60
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-29T21:03:59.160258Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.