Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the approximate relation between black-hole perturbation theory and numerical relativity
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2307.03155.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:08:46.780332Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T00:42:49.292167Z
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 6c204a61-90d8-4977-a050-9db423f48968 · inbound
Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA cites this paper.
Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA On the approximate relation between black-hole perturbation theory and numerical relativity
Reference 119
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:08:46.780332Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2cf9d33-3423-48e1-a2a5-8b0d10dab33e · 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 On the approximate relation between black-hole perturbation theory and numerical relativity
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T13:28:18.903546Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation db9d9fb5-5d71-447b-b7b1-0c40df692909 · inbound
Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications cites this paper.
Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications On the approximate relation between black-hole perturbation theory and numerical relativity
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T22:13:55.902335Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc003af8-77c5-4134-a575-09c7fd797620 · inbound
Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers cites this paper.
Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers On the approximate relation between black-hole perturbation theory and numerical relativity
Reference 86
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T00:42:49.352878Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.