Paper Citation Record · LEDGER

First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2310.16980.

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

pith.paper-citation-record.v1
2310.16980 v1

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:24:53.447464Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T22:28:59.862930Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f0a7076d-458e-4048-a77f-1634f6637127 · inbound

Fast frequency-domain gravitational waveforms for precessing binaries with a new twist cites this paper.

Fast frequency-domain gravitational waveforms for precessing binaries with a new twist First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-11T10:24:53.447464Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e6c9482-4169-4f77-9aa6-0a5386592117 · inbound

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries cites this paper.

Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 187

Resolution: unresolved; no resolver link, observed 2026-08-09T00:23:47.252095Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c75ca4c-482c-438a-ac7e-bbbcb2f0badc · inbound

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown cites this paper.

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-06T20:31:47.897891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76f0bfb1-198c-42da-90c2-8048139a775c · inbound

Challenges in the nonlinear evolution of unequal mass binaries in sGB gravity cites this paper.

Challenges in the nonlinear evolution of unequal mass binaries in sGB gravity First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-06T16:37:29.607830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75de97e1-af65-4edc-aa30-4aaa494bf115 · inbound

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects cites this paper.

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 169

Resolution: verified exact; arxiv_id, observed 2026-05-10T15:00:31.212382Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b184e5c3-0208-45c8-975a-483b189c078e · inbound

Compactness Inference in Gravitational-Wave Mergers with PhenomDECO: Catalog Benchmarks and Robustness Diagnostics cites this paper.

Compactness Inference in Gravitational-Wave Mergers with PhenomDECO: Catalog Benchmarks and Robustness Diagnostics First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:44.889189Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation cb8d2589-6993-4e67-a983-d46b98a199a0 · inbound

Compactness Inference in Gravitational-Wave Mergers with PhenomDECO: Catalog Benchmarks and Robustness Diagnostics cites this paper.

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-07-03T22:28:59.864382Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b41d79d9-c492-4e11-9cf7-d2528bb3c3c9 · inbound

Compactness Inference in Gravitational-Wave Mergers with PhenomDECO: Catalog Benchmarks and Robustness Diagnostics cites this paper.

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T09:27:41.086653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 900d52fc-d212-4006-b5e0-1b180b0bbdef · inbound

Ensemble-Based Residual Tests of GW231123 across Waveform Models cites this paper.

Ensemble-Based Residual Tests of GW231123 across Waveform Models First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-10T04:16:49.240131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.