Paper Citation Record · LEDGER

IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:2004.08302.

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pith.paper-citation-record.v1
2004.08302 v2

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measured 15 of 15 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:16:49.228310Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-23T23:43:38.701096Z

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Pith citing papers

Observation 84b22194-9c04-4afe-a1f5-b56991e09365 · 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 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 55

Resolution: metadata mismatch; arxiv_id, observed 2026-05-13T21:55:09.230391Z

Source-reported events for the cited work

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Observation e7f5fe97-0a7b-4831-9fc3-7fad1a0f0efd · 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 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:43:38.708410Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 9e957a18-0f62-4879-9630-7b9e0faf90d6 · inbound

AthenaK simulations of the binary black hole merger GW150914 cites this paper.

AthenaK simulations of the binary black hole merger GW150914 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T05:57:54.253232Z

Source-reported events for the cited work

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Observation 73d5ff06-31fb-415d-ac9a-5df11be15352 · inbound

TDI on the fly cites this paper.

TDI on the fly IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T05:26:16.151981Z

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Observation bc47b0a2-c77a-4652-9d58-1fbca24554af · 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 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-04T13:28:20.595390Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 98b7054c-c803-4ba9-9295-d4350113093c · inbound

Biased parameter inference of eccentric, spin-precessing binary black holes cites this paper.

Biased parameter inference of eccentric, spin-precessing binary black holes IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 68

Resolution: verified exact; arxiv_id, observed 2026-05-18T09:51:13.016748Z

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 22ae3ff4-70a9-4048-9588-b26f35e87f09 · 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 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 57

Resolution: unresolved; no resolver link, observed 2026-07-15T14:26:35.666160Z

Source-reported events for the cited work

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Observation f0ea0113-24ce-4cf1-aecb-f35d86bc0159 · 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 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 126

Resolution: verified exact; arxiv_id, observed 2026-05-10T10:19:20.887236Z

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 d8d3c788-729b-40a8-9d11-deb1b08cc172 · inbound

Properties of natural polynomials for Schwarzschild and Kerr black holes cites this paper.

Properties of natural polynomials for Schwarzschild and Kerr black holes IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-15T01:58:29.109102Z

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 e84226fb-e9fc-4d9f-9661-dcc1a8e59fa1 · inbound

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

Dynamical quasinormal mode excitation II: propagation and convergence in Schwarzschild IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 21

Resolution: verified exact; arxiv_id, observed 2026-05-20T16:28:38.572936Z

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 c24f60c8-37a2-4892-bbc1-947977ff8868 · inbound

Measurability of Quadrupole Deviations from Kerr in Binary black hole Mergers cites this paper.

Measurability of Quadrupole Deviations from Kerr in Binary black hole Mergers IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 52

Resolution: unresolved; no resolver link, observed 2026-07-11T13:55:39.032057Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 58bc7d03-ccc1-44ce-8832-f5eee889e323 · 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 IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 41

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 7b268c64-c04b-4dbf-b9af-f3873cc7b088 · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-04T21:28:07.558978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f8ec66c-93a5-4367-8c5c-d169a999d191 · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T00:15:14.238187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 295a366d-618a-4a75-8a6d-58a05fff3e71 · inbound

Ensemble-Based Residual Tests of GW231123 across Waveform Models cites this paper.

Ensemble-Based Residual Tests of GW231123 across Waveform Models IMRPhenomTP: A phenomenological time domain model for dominant quadrupole gravitational wave signal of coalescing binary black holes

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T04:16:49.228310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.