Paper Citation Record · LEDGER

Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2404.02864.

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

pith.paper-citation-record.v1
2404.02864 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 13 of 13 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 13 of 13 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:06:57.361430Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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External citation measurements

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 011902b6-bff8-4570-94f5-71d9768d2fa7 · inbound

Likelihoods for Stochastic Gravitational Wave Background Data Analysis cites this paper.

Likelihoods for Stochastic Gravitational Wave Background Data Analysis Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T12:22:43.916916Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 250bbd5d-d830-47c0-b830-bcf87d95d603 · inbound

Whispers from the Early Universe: The Ringdown of Primordial Black Holes cites this paper.

Whispers from the Early Universe: The Ringdown of Primordial Black Holes Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T18:42:54.942360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd24b4ae-b851-4be4-b537-31ee749fa36e · inbound

\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors cites this paper.

\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-06T15:30:12.582127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 831fd41e-b80f-459c-b7ff-7c60029365ad · inbound

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer cites this paper.

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T15:54:02.968799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 693ac7be-f74c-4de9-8fe7-521e77f161a6 · inbound

Cosmic Variance in Anisotropy Searches at Pulsar Timing Arrays cites this paper.

Cosmic Variance in Anisotropy Searches at Pulsar Timing Arrays Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-05T14:45:51.283417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f98dfec6-dfaa-4d7d-bbd2-d9c00a8ed8ba · inbound

Can Oscillatory and Persistent Nonlinearities Be Bridged in Black Hole Ringdown? cites this paper.

Can Oscillatory and Persistent Nonlinearities Be Bridged in Black Hole Ringdown? Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-15T15:40:09.064425Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation f82a9e1e-14a1-4988-94e5-72408e75247f · inbound

Can Oscillatory and Persistent Nonlinearities Be Bridged in Black Hole Ringdown? cites this paper.

Can Oscillatory and Persistent Nonlinearities Be Bridged in Black Hole Ringdown? Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-21T11:24:08.559179Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 83eab3c5-396d-47cf-93b0-a6cfa9e170d4 · inbound

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations cites this paper.

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 64

Resolution: verified exact; arxiv_id, observed 2026-05-11T17:21:07.159752Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation e316818f-7364-4954-841d-4630e8d1db31 · inbound

QCD axion from broken scale symmetry cites this paper.

QCD axion from broken scale symmetry Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 47

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T20:45:03.531280Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 789a058f-a130-4883-9ff8-8c17992cdd96 · inbound

The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses cites this paper.

The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 45

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T00:44:06.249469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 635d8166-70cc-4521-a0e4-6c7623bf553b · inbound

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models cites this paper.

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 59

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T01:24:08.865000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 92fa57fb-de62-4d68-a185-844d026735b0 · inbound

Probing Graviton Mass with MeerKAT PTA and SKA--PTA Forecasts cites this paper.

Probing Graviton Mass with MeerKAT PTA and SKA--PTA Forecasts Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-02T01:08:13.796102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f18e36b2-d37f-4079-9ff0-52f019518c0c · inbound

Pulsar Timing Array Sensitivity to Anisotropy: Empirical Sensitivity Curves, Scaling Relations, and the Multi-Resolution Pixel Basis cites this paper.

Pulsar Timing Array Sensitivity to Anisotropy: Empirical Sensitivity Curves, Scaling Relations, and the Multi-Resolution Pixel Basis Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T11:06:57.361430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.