Paper Citation Record · LEDGER

Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1711.00075.

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

pith.paper-citation-record.v1
1711.00075 v1

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T15:56:34.457748Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T20:42:37.497180Z

Reference resolution

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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 c13b4e1a-35c9-475c-821f-a8495d856b88 · inbound

How many pixels are there in a polarized pulsar timing array map? cites this paper.

How many pixels are there in a polarized pulsar timing array map? Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-06T12:54:27.301262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9b315da-dfd6-4d8a-b165-874a4d0a3312 · inbound

Mapping the Gravitational-wave Background Across the Spectrum with a Next-Generation Anisotropic Per-frequency Optimal Statistic cites this paper.

Mapping the Gravitational-wave Background Across the Spectrum with a Next-Generation Anisotropic Per-frequency Optimal Statistic Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-04T22:54:55.943081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce82deeb-2da3-46b5-ad29-e914b1d16238 · 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 Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:21:14.553417Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 1b1cc3ae-0619-40a9-be08-eb6524bce4f4 · 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 Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:16:13.796137Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 87b7d9b9-c6ed-4a15-8f30-ddf74a35d32a · inbound

The Heavy Tailed Non-Gaussianity of the Supermassive Black Hole Gravitational Wave Background cites this paper.

The Heavy Tailed Non-Gaussianity of the Supermassive Black Hole Gravitational Wave Background Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-11T07:55:59.834564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 45a539fb-19b6-4e41-a72c-a79cb04ea44e · inbound

\texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series cites this paper.

\texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 144

Resolution: verified exact; local_arxiv, observed 2026-05-25T05:20:23.617612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation d7010639-c7f9-4c15-865e-032d266a9548 · inbound

Searching for a waveform-agnostic gravitational wave signal in pulsar timing arrays cites this paper.

Searching for a waveform-agnostic gravitational wave signal in pulsar timing arrays Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-06-28T20:42:37.498449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation f2d7571a-7644-4b50-8689-fe2a81b83fb3 · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 175

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 557dce00-42d2-4c43-bb8f-2a04fd2f4725 · inbound

Summary statistic for pulsar timing arrays cites this paper.

Summary statistic for pulsar timing arrays Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-08T15:56:34.457748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.