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Paper Citation Record · LEDGER

Pulsar timing array sensitivity to anisotropies in the gravitational wave background

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2407.14460.

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

pith.paper-citation-record.v1
2407.14460 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

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

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T21:12:53.427453Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T18:10:02.218845Z

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 88fab72f-dc52-4e93-803f-f95a07bbd7e0 · inbound

Pulsar timing and polarimetry: results and perspectives cites this paper.

Pulsar timing and polarimetry: results and perspectives Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 147

Resolution
unresolved
no resolver link, observed 2026-08-09T21:12:53.427453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 0c422e41-9bef-4b07-b46f-1aea4ac0ab20 · inbound

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis cites this paper.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-07T00:33:36.426292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:33:36.426292Z digest=sha256:087be2eeaccb44d5e900d10526e90087c7a249003c0ab47ea9561b4f3ed362d6

Observation e2945bb1-03e5-414e-9296-9527969cc981 · inbound

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data cites this paper.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-06T21:42:13.290386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:42:13.290386Z digest=sha256:5577743f2676cb3efaebfaa6553c910323269ec8f45567fccbd374033500d04d

Observation d94c35cc-7324-4e24-8083-a4129b309dd0 · inbound

Do Pulsar Timing Datasets Favor Massive Gravity? cites this paper.

Do Pulsar Timing Datasets Favor Massive Gravity? Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-06T20:45:32.116220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:45:32.116220Z digest=sha256:c168901df74282b7523543eaeafadd3c5f2b498ecea2a96b3daa0fb021b122a0

Observation cc995d9c-5d4c-4c1c-8e29-274d64ff171d · 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 Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-06T15:30:10.071755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:30:10.071755Z digest=sha256:699190c858d3b1575074b94a6862376b3cc0f86d7251cfb61c559af8bc8efc5a

Observation 865312d6-a92c-43a8-b170-b865d72b7a9f · inbound

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

Cosmic Variance in Anisotropy Searches at Pulsar Timing Arrays Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-05T14:45:51.256876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:45:51.256876Z digest=sha256:a6bd55eb68ea87ecea69bdf5aa3d39e77ecf1962a8849e67f36dd7f85ab71036

Observation 033ed1d6-54aa-49f0-a7bf-182b4920689f · inbound

Are PTA measurements sensitive to gravitational wave non-Gaussianities? cites this paper.

Are PTA measurements sensitive to gravitational wave non-Gaussianities? Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:06:08.786428Z

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.

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Observation e7009c8a-0dab-4270-bd97-9878b624e8d8 · inbound

Are PTA measurements sensitive to gravitational wave non-Gaussianities? cites this paper.

Are PTA measurements sensitive to gravitational wave non-Gaussianities? Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-06-30T23:15:07.682018Z

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.

source=pdf_text observed=2026-06-30T23:14:56.700710Z digest=sha256:2ee72b669ac6959b06f1d2b4ce8a0a7705ec28c8183f69d6bb011665fa4ebe56

Observation 22fdc0b2-066b-46ef-8bc1-1dbf1da921c4 · inbound

Detecting Gravitational-Wave Anisotropies with Simulation-Based Inference cites this paper.

Detecting Gravitational-Wave Anisotropies with Simulation-Based Inference Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 17

Resolution
verified exact
arxiv_id, observed 2026-06-30T14:44:45.462658Z

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.

source=pdf_text observed=2026-06-30T14:35:45.210384Z digest=sha256:3e73503beb5d21d6be851ee12995328eecdc3326a4e9c48ceda34f7283769507

Observation 350c4d9d-ae62-424c-9424-773b63866c5d · inbound

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO cites this paper.

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 110

Resolution
verified exact
arxiv_id, observed 2026-07-04T18:10:02.220892Z

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.

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