Paper Citation Record · LEDGER

Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2204.01972.

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

pith.paper-citation-record.v1
2204.01972 v1

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measured 16 of 16 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:35:06.275142Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-10T06:15:00.866473Z

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Outbound references

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Pith citing papers

Observation 21f5b9f9-d8dd-44a3-96f5-b3ed05fd3a57 · inbound

Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity cites this paper.

Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:43:38.084465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 530087b8-feaa-405f-8af6-8ec9460a28c0 · inbound

Self-force framework for merger-ringdown waveforms cites this paper.

Self-force framework for merger-ringdown waveforms Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:06.275142Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ef34e0a-7ba8-4392-90e8-9df38f596aec · inbound

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA cites this paper.

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-06T21:08:42.035727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c7ed77d-9a6d-450d-940c-167062c9181a · inbound

Post-adiabatic dynamics and waveform generation in self-force theory: an invariant pseudo-Hamiltonian framework cites this paper.

Post-adiabatic dynamics and waveform generation in self-force theory: an invariant pseudo-Hamiltonian framework Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-06T18:34:53.187626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8bceb53-9107-4001-8191-ad01334dad7e · inbound

Probing Direct Waves in Black Hole Ringdowns cites this paper.

Probing Direct Waves in Black Hole Ringdowns Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-04T19:41:19.156818Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68309292-7139-4105-9227-f4dff524b051 · inbound

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates cites this paper.

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.568224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4996b2a6-8a83-40b4-9a7b-1ee4b0221878 · inbound

Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries cites this paper.

Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T13:28:16.584838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2513ef8b-3d2e-40ea-a9bf-137bbb3d874a · inbound

Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications cites this paper.

Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T22:13:55.037874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28670e84-87b6-4119-beee-4b3a6eb110ec · inbound

Analysis of late-time tails in spin-aligned eccentric binary black hole mergers cites this paper.

Analysis of late-time tails in spin-aligned eccentric binary black hole mergers Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-03T20:00:56.304580Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b567eabd-5a7a-4f90-a08d-03f7a9c78b8e · 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 Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 32

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 dcc49f24-b099-4792-8f44-e320da4fd0b0 · inbound

Shaving off soft hairs and the black hole image memory effect cites this paper.

Shaving off soft hairs and the black hole image memory effect Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-05-15T12:20:00.337171Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 71eb3ffc-2e0a-4420-8293-c18d0ec3de27 · inbound

GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog cites this paper.

GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-11T00:35:51.453892Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 5f30d990-7b13-4042-b604-dcea87cda1d8 · inbound

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions cites this paper.

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 95

Resolution: verified exact; arxiv_id, observed 2026-05-10T12:10:22.313008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation dacbb180-7c96-4475-8ea5-e742941f1630 · inbound

Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity cites this paper.

Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-07-03T02:57:35.557429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 73717f01-0b45-443f-83ef-ead28ca88874 · 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 Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-06-30T16:24:58.565729Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 2f920775-2d61-4169-8c47-febc92626cb4 · inbound

Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers cites this paper.

Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-06T00:42:37.041615Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.