Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Calculation of gravitational wave forms from black hole collisions and disk collapse: Applying perturbation theory to numerical spacetimes
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/9408036.
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 2026-08-12T18:22:50.433456Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-13T02:26:20.238803Z
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 20b65cf7-e275-4369-b72d-39b589578229 · inbound
Perturbations of Black Holes Surrounded by Anisotropic Matter Field cites this paper.
Perturbations of Black Holes Surrounded by Anisotropic Matter Field Calculation of gravitational wave forms from black hole collisions and disk collapse: Applying perturbation theory to numerical spacetimes
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T18:22:50.433456Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6df1edc8-3b67-433a-ac62-5cc2f043bbd1 · inbound
Quasi-Normal Modes of Stars and Black Holes cites this paper.
Quasi-Normal Modes of Stars and Black Holes Calculation of gravitational wave forms from black hole collisions and disk collapse: Applying perturbation theory to numerical spacetimes
Reference 3
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T15:56:55.392051Z
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.