Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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 12 inbound Pith citation observations for arXiv:2012.11923.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T04:16:49.232218Z
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
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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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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.
Observation 94600cb7-4b22-43c2-a943-8b00efcd03a4 · inbound
Ensemble-Based Residual Tests of GW231123 across Waveform Models cites this paper.
Ensemble-Based Residual Tests of GW231123 across Waveform Models Time domain phenomenological model of gravitational wave subdominant harmonics for quasi-circular non-precessing binary black hole coalescences
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T04:16:49.232218Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.