Paper Citation Record · LEDGER

A Rosetta Stone for eccentric gravitational waveform models

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2207.14346.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2207.14346 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:40:19.826868Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-06-29T01:02:56.048916Z

Reference resolution

0 of 0 outbound references displayed

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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 71eb1665-efbc-4c1e-bf9e-48d80c75adaf · inbound

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM cites this paper.

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM A Rosetta Stone for eccentric gravitational waveform models

Reference 275

Resolution: unresolved; no resolver link, observed 2026-08-11T13:49:13.791216Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75c39afe-68d6-432a-8fa3-6ecf1aa5a796 · 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 A Rosetta Stone for eccentric gravitational waveform models

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-09T11:24:09.590789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2f2ac3da-9143-4ed0-99d3-d9551f0d4388 · 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 A Rosetta Stone for eccentric gravitational waveform models

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-16T12:37:52.099630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29c0f6e1-1557-466c-8500-c0281fae972d · 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 A Rosetta Stone for eccentric gravitational waveform models

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-16T12:40:19.826868Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fdc23dee-4917-4069-b4f3-9b95fb617270 · inbound

First ICCUB Numerical Relativity Waveform Catalog of Eccentric Black Hole Binaries cites this paper.

First ICCUB Numerical Relativity Waveform Catalog of Eccentric Black Hole Binaries A Rosetta Stone for eccentric gravitational waveform models

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-15T16:30:11.492074Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0edee28b-bd37-4dab-83ef-6603b5f3e6ad · inbound

Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms cites this paper.

Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms A Rosetta Stone for eccentric gravitational waveform models

Reference 152

Resolution: verified exact; arxiv_id, observed 2026-05-10T10:19:21.270934Z

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 6155cce7-ad6e-4bc8-80b9-3a9e42322467 · inbound

A universal framework to identify eccentric binary mergers: GW200105 case study cites this paper.

A universal framework to identify eccentric binary mergers: GW200105 case study A Rosetta Stone for eccentric gravitational waveform models

Reference 68

Resolution: verified exact; arxiv_id, observed 2026-05-20T08:53:09.881519Z

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 21c86470-df4a-4fb3-ac28-5db1d5b37204 · inbound

Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework cites this paper.

Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework A Rosetta Stone for eccentric gravitational waveform models

Reference 119

Resolution: verified exact; arxiv_id, observed 2026-06-29T01:02:56.050414Z

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.