Paper Citation Record · LEDGER

A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1910.10473.

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

pith.paper-citation-record.v1
1910.10473 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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 2026-08-22T06:32:14.747728+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:35:06.272947Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T02:57:35.545026Z

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 fb2ce2dd-afc0-4ac2-b667-f90664c0a52b · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:43:38.638427Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 9fac50c5-1fd0-4b3f-a467-911ade280a63 · inbound

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

Self-force framework for merger-ringdown waveforms A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:06.272947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 62489e1a-626c-4890-876a-c08ed3b58842 · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-06T21:08:42.436612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8151f90-43a6-49a6-a72c-86aa8d249b5e · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-06T18:34:53.183710Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97733fa0-cba8-4087-96d5-4d28573435c0 · inbound

Probing Direct Waves in Black Hole Ringdowns cites this paper.

Probing Direct Waves in Black Hole Ringdowns A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T19:41:19.147461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49e143c5-a0ab-464f-9508-075c69c4b71e · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-04T13:34:57.565404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9fbbe6d9-5695-4481-a064-1770f4093ed9 · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T13:28:16.633729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9c03643-340a-4406-9923-525c2b059c5e · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 30

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 e2d9c004-12b2-4989-b302-ff0afb6cb953 · 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 A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-07-03T02:57:35.546375Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.