Paper Citation Record · LEDGER

Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2203.10109.

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pith.paper-citation-record.v1
2203.10109 v2

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measured 10 of 10 standing notices

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

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:08:42.127629Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T23:43:38.441969Z

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Outbound references

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Pith citing papers

Observation d1f63413-0da2-4977-89c8-5887b651b84f · 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 Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:43:38.445437Z

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 3a5b0092-3ecf-46c1-a0e5-6dc57f1b25f4 · 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 Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T21:08:42.127629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 058b8a8b-3a3c-4d02-94cf-eebe6e1e54d1 · 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 Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-06T20:31:47.874718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84a054fa-f869-436f-a69c-650c084f5824 · inbound

Learning Post-Newtonian Corrections from Numerical Relativity cites this paper.

Learning Post-Newtonian Corrections from Numerical Relativity Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:35:25.178150Z

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 e787311d-9fea-4521-bfdf-fcd478bb3ec2 · 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 Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 33

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 7115b769-6ced-4aac-aa99-4420743519c3 · inbound

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T17:33:25.203838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4edddfc0-7518-4075-9206-cb4cab450855 · inbound

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge cites this paper.

Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-04T05:45:47.810978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc78a83f-b906-44d2-ad8d-d447da56e58f · 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 Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 28

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T00:35:51.382235Z

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 edbd4f59-8e0b-4de9-95e5-1a2b689d4470 · inbound

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries cites this paper.

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 26

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T15:01:09.235709Z

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 83d72b23-16a3-488f-9978-cdd514429c07 · inbound

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries cites this paper.

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Reference 26

Resolution: metadata mismatch; arxiv_id, observed 2026-05-22T10:41:25.666712Z

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.