Paper Citation Record · LEDGER

Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2012.11923.

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

pith.paper-citation-record.v1
2012.11923 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

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

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:33:29.238280Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T11:48:04.518049Z

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 70658eb1-f95d-4b2e-a8d4-c55f6cd755c0 · inbound

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes cites this paper.

Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 115

Resolution: metadata mismatch; arxiv_id, observed 2026-05-13T21:55:09.176603Z

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 21d371cd-fcea-4f6d-bb96-99e356100977 · 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 Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:43:38.827694Z

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 4e7f0c8d-72c7-4bb3-ad2c-81af9b493762 · inbound

Revisiting GW150914 with a non-planar, eccentric waveform model cites this paper.

Revisiting GW150914 with a non-planar, eccentric waveform model Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 182

Resolution: unresolved; no resolver link, observed 2026-08-07T13:33:29.238280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1607711a-f797-4d69-a329-ebcb0bfa17b7 · 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 Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 56

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 01edabb7-f733-4d6d-bf76-fffdb0d06d74 · 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 Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 33

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T00:35:51.862087Z

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 c452bbb9-3579-4b9f-9fb8-6ee6fa989932 · inbound

Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms cites this paper.

Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 127

Resolution: verified exact; arxiv_id, observed 2026-05-10T10:19:20.989126Z

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 863c4e49-b083-41bd-b424-1f1c376e7dcb · 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 Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 106

Resolution: metadata mismatch; arxiv_id, observed 2026-05-10T12:10:22.294668Z

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 6cb026fa-b72d-4216-ad07-ea97dd76a672 · inbound

Dynamical quasinormal mode excitation II: propagation and convergence in Schwarzschild cites this paper.

Dynamical quasinormal mode excitation II: propagation and convergence in Schwarzschild Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-20T16:28:38.512294Z

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 e66ab25d-f639-479e-9c24-2c95df37f035 · inbound

Shaping black hole resonances I. Black hole ringdown as a spectral filtering process cites this paper.

Shaping black hole resonances I. Black hole ringdown as a spectral filtering process Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 54

Resolution: verified exact; arxiv_id, observed 2026-06-30T13:14:41.139591Z

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 7f9cbc90-cb4a-4cdc-a26c-ade8f971caa0 · 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 Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 146

Resolution: verified exact; arxiv_id, observed 2026-07-03T11:48:04.519366Z

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 051c2141-795f-41ee-b731-02512fc2c703 · inbound

A stepping stone toward detecting gravitational wave memory: a cumulative analysis with the full $(\ell=2, m=0)$ spherical harmonic using events from GWTC-4.0 and GWTC-5.0 cites this paper.

A stepping stone toward detecting gravitational wave memory: a cumulative analysis with the full $(\ell=2, m=0)$ spherical harmonic using events from GWTC-4.0 and GWTC-5.0 Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences

Reference 42

Resolution: unresolved; no resolver link, observed 2026-07-11T11:36:39.369743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.