Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:gr-qc/0607092.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T12:40:19.842736Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-24T01:35:55.914131Z
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 7df73455-5a34-4afd-ba41-fb958878827f · inbound
Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA cites this paper.
Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
Reference 222
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-24T01:35:55.916685Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 27a87830-4745-4e3b-9986-01ebe82dff44 · inbound
Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order cites this paper.
Spin effects in the phasing formula of eccentric compact binary inspirals up to the third post-Newtonian order Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T15:35:51.515896Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3dcbf117-1522-4c9e-a689-3008312094de · inbound
gwharmone: first data-driven surrogate for eccentric harmonics in binary black hole merger waveforms cites this paper.
gwharmone: first data-driven surrogate for eccentric harmonics in binary black hole merger waveforms Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T12:37:52.114484Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation af17e448-0299-4c10-9262-db2a19b14ade · inbound
Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms cites this paper.
Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T12:40:19.842736Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 64c27643-a904-476f-a6b5-bc3bb66bcea6 · inbound
Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework cites this paper.
Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework Phenomenology of amplitude-corrected post-Newtonian gravitational waveforms for compact binary inspiral. I. Signal-to-noise ratios
Reference 21
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-09T06:10:37.386336Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.