Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Matrix Method for Quasinormal Modes: Kerr and Kerr-Sen Black Holes
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1703.06439.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T21:39:59.841089Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T01:26:24.433935Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 d40eb39a-5393-4660-acb1-f932b2038277 · inbound
Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant cites this paper.
Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant A Matrix Method for Quasinormal Modes: Kerr and Kerr-Sen Black Holes
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T21:39:59.841089Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2d3c065-6b15-4228-80cb-cccb8b216224 · inbound
Late-Time Cosmology and Structure Formation in Quadratic $f(Q)$ Gravity cites this paper.
Late-Time Cosmology and Structure Formation in Quadratic $f(Q)$ Gravity A Matrix Method for Quasinormal Modes: Kerr and Kerr-Sen Black Holes
Reference 94
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T01:26:24.435227Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.