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Paper Citation Record · LEDGER

How to Detect an Astrophysical Nanohertz Gravitational-Wave Background

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2309.04443.

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

pith.paper-citation-record.v1
2309.04443 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-30T23:14:56.700710Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T23:15:07.672133Z

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 01e750c4-677d-4cf2-9955-561c91bfcfa4 · inbound

Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization cites this paper.

Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization How to Detect an Astrophysical Nanohertz Gravitational-Wave Background

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-05-18T10:21:14.811944Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation af15ff62-f2a6-41fc-beb5-8816f01da834 · inbound

Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy cites this paper.

Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy How to Detect an Astrophysical Nanohertz Gravitational-Wave Background

Reference 85

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verified exact
arxiv_id, observed 2026-05-18T10:16:13.972236Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-18T10:15:12.128371Z digest=sha256:6bad5f0261b06edf0b39d64ca1a0f90053969c08712f0900d20e1efb91b66e5d

Observation 3b7fe5f6-bce7-426b-826c-b441065b3f94 · inbound

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

Are PTA measurements sensitive to gravitational wave non-Gaussianities? How to Detect an Astrophysical Nanohertz Gravitational-Wave Background

Reference 26

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verified exact
arxiv_id, observed 2026-05-11T18:06:08.925341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-08T16:37:40.249295Z digest=sha256:a4f6abecf83abd9fa7511958eae8261b9ed1d9f644602ce362e76fcfb9bc9181

Observation 5cde69e1-7fbe-4a03-ac51-291a8650c981 · inbound

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

Are PTA measurements sensitive to gravitational wave non-Gaussianities? How to Detect an Astrophysical Nanohertz Gravitational-Wave Background

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-06-30T23:15:07.673663Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-06-30T23:14:56.700710Z digest=sha256:cba6ad45f56a3f52f0bc234558da1b82a499c0b66825f69ccbfe8dc490c4e13f