Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
An improved numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2111.08033.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T11:24:09.541315Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T20:05:02.935927Z
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 82b47567-5ad6-4e70-b35f-aac79e27acc4 · inbound
Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms cites this paper.
Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms An improved numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T11:24:09.541315Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d9d68d60-1a8e-49af-9720-fa1c798e565c · inbound
PRECESSION 2.1: black-hole binary spin precession on eccentric orbits cites this paper.
PRECESSION 2.1: black-hole binary spin precession on eccentric orbits An improved numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T20:26:51.047837Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 5e701cd9-25eb-4c81-a1bc-dc20385df3cc · inbound
Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era cites this paper.
Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era An improved numerical fit to the peak harmonic gravitational wave frequency emitted by an eccentric binary
Reference 73
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T20:05:02.937521Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.