Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Perturbative evolution of particle orbits around Kerr black holes: time domain calculation
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/0303054.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T15:21:11.751539Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T15:21:11.814778Z
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 2af4c8cf-9ef6-4107-a910-e048b8f8c5e5 · inbound
Gravitational-wave tails and memory effect for mergers in astrophysical environments cites this paper.
Gravitational-wave tails and memory effect for mergers in astrophysical environments Perturbative evolution of particle orbits around Kerr black holes: time domain calculation
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T15:21:11.817871Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 4b29f8df-9786-4ea6-b705-5f68b7c2af9a · inbound
Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries cites this paper.
Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries Perturbative evolution of particle orbits around Kerr black holes: time domain calculation
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:28:14.944749Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.