Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Success of the small mass ratio approximation during the final orbits of binary black hole simulations
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2207.04066.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-05-18T07:14:28.658616Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-18T07:16:02.339714Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 190a698c-fa09-427b-a8a1-24989e505851 · inbound
Black hole mergers beyond general relativity: a self-force approach cites this paper.
Black hole mergers beyond general relativity: a self-force approach Success of the small mass ratio approximation during the final orbits of binary black hole simulations
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T07:16:02.341366Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation 1227d203-0207-4d59-8f55-cfb66e27c625 · inbound
Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary cites this paper.
Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary Success of the small mass ratio approximation during the final orbits of binary black hole simulations
Reference 41
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T05:55:57.392390Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.