Paper Citation Record · LEDGER

Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2208.02055.

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

pith.paper-citation-record.v1
2208.02055 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T03:14:27.551755Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T11:48:04.640913Z

Reference resolution

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External citation measurements

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Outbound references

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Pith citing papers

Observation 6c4fbe9f-9d52-4287-ba0e-20aa3116fd9d · 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 Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

Reference 155

Resolution: verified exact; arxiv_id, observed 2026-05-18T05:55:57.351567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 18587259-ad48-415a-9f62-722cbe26d15d · inbound

From the confluent Heun equation to a new factorized and resummed gravitational waveform for circularized, nonspinning, compact binaries cites this paper.

From the confluent Heun equation to a new factorized and resummed gravitational waveform for circularized, nonspinning, compact binaries Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-03T03:14:27.551755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3074c260-ec61-4aaa-b7f6-76bb77cdde28 · inbound

Advancing the Effective-One-Body Framework in the Test-Mass Limit cites this paper.

Advancing the Effective-One-Body Framework in the Test-Mass Limit Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

Reference 110

Resolution: unresolved; no resolver link, observed 2026-07-15T14:26:35.666160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7eb8e092-6072-423b-b3c3-618255c0a5b0 · inbound

Secular evolution of orbital parameters for general bound orbits in Kerr spacetime cites this paper.

Secular evolution of orbital parameters for general bound orbits in Kerr spacetime Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-03T02:30:56.251453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0e46f89-8f73-42b2-a010-0b68c5ff7f94 · inbound

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis cites this paper.

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-07-03T11:48:04.642262Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 28e76be2-dcd9-4316-96a2-b4e371d2297c · inbound

Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations cites this paper.

Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case

Reference 160

Resolution: verified exact; arxiv_id, observed 2026-06-30T16:25:03.273189Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.