Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0804.4184.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T19:07:26.714717Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-19T07:52:09.665870Z
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 7a67e562-a05a-46bd-9654-826883c02ccb · inbound
Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves cites this paper.
Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T19:07:26.714717Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9a976ba4-926d-46c5-a3d9-9e3642c5cb25 · inbound
Binary black holes in the heat of merger cites this paper.
Binary black holes in the heat of merger High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T07:52:09.667855Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 510649ea-0d98-4dae-bb6f-a6f09b8ebf9e · inbound
Symplectic mechanics of relativistic spinning compact bodies. III. quadratic-in-spin integrability in Type-D Einstein spacetimes: persistence and breakdown cites this paper.
Symplectic mechanics of relativistic spinning compact bodies. III. quadratic-in-spin integrability in Type-D Einstein spacetimes: persistence and breakdown High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T11:30:36.174013Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.