Paper Citation Record · LEDGER

The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2306.16229.

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

pith.paper-citation-record.v1
2306.16229 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:42:21.399578Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T00:16:24.427600Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 6eac12f8-2b16-4bdc-9b94-98826a806d30 · inbound

Unlocking the hidden potential of pulsar astronomy cites this paper.

Unlocking the hidden potential of pulsar astronomy The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-07T05:42:21.399578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d637f59-1241-4a1e-b234-fada838be86b · inbound

Observable Gravitational Wave Strain at Second Order cites this paper.

Observable Gravitational Wave Strain at Second Order The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-03T15:50:30.180501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad9baa8c-d56d-4e19-9225-62a838c89576 · inbound

Probing non-Gaussianity during reheating with SIGW in the LISA band cites this paper.

Probing non-Gaussianity during reheating with SIGW in the LISA band The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-11T07:45:56.976632Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 8fac7539-b18d-4ed3-9bbc-bd12ffaffac7 · inbound

Gravitational-wave lensing beyond rays: a disordered-system approach cites this paper.

Gravitational-wave lensing beyond rays: a disordered-system approach The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 3

Resolution: verified exact; arxiv_id, observed 2026-05-10T09:43:48.539029Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation e0dfae89-4c0d-4e92-89f3-9b8e790a63c7 · inbound

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-10T00:59:49.860833Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 4b5cb4c5-6fa0-4305-b0b9-7efe07b2bf96 · inbound

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-02T15:56:56.997795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f86a8ff5-94b8-4322-9deb-4d2f80861f6e · inbound

Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2 cites this paper.

Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2 The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-05-09T05:50:27.442113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation df33d220-d877-41f2-b357-2581fd276a0a · inbound

Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias cites this paper.

Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-09T06:40:42.873617Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 26cec7a8-81e1-4eb3-896a-3a3e7a05d15e · inbound

Thermal Metastable Strings in One-Scale Models and Gravitational Waves cites this paper.

Thermal Metastable Strings in One-Scale Models and Gravitational Waves The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 2

Resolution: verified exact; arxiv_id, observed 2026-07-02T00:16:24.430365Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation d0500d21-38c0-4f3f-9e06-b5ad0ffbcdc0 · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 204

Resolution: unresolved; no resolver link, observed 2026-07-12T05:10:13.912506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e6450444-4cf8-4e9e-b4b3-9a2fd3cddbf4 · inbound

Exploring the Galactic plasma with pulsars in the SKA Era cites this paper.

Exploring the Galactic plasma with pulsars in the SKA Era The gravitational-wave background null hypothesis: Characterizing noise in millisecond pulsar arrival times with the Parkes Pulsar Timing Array

Reference 10

Resolution: unresolved; no resolver link, observed 2026-07-12T08:30:18.472851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9ab26bdf-fa88-41ed-aeb0-85c685dfaca8 · inbound

Exploring the Galactic plasma with pulsars in the SKA Era cites this paper.

Reference 10

Resolution: unresolved; no resolver link, observed 2026-07-14T16:43:10.179035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.