Paper Citation Record · LEDGER

From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2006.04810.

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

pith.paper-citation-record.v1
2006.04810 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T16:53:02.699821Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T10:21:14.818216Z

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 16af1d20-2c33-41db-bc0e-64b3f5aed87f · inbound

Constraining inflation with nonminimal derivative coupling with the Parkes Pulsar Timing Array third data release cites this paper.

Constraining inflation with nonminimal derivative coupling with the Parkes Pulsar Timing Array third data release From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-11T16:53:02.699821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9491bd13-840e-4da3-b59c-3803faf15044 · 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? From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-06T12:54:26.888718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c69676f8-e086-4d56-9933-5cdcfc16d8df · inbound

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

Cosmic Variance in Anisotropy Searches at Pulsar Timing Arrays From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-05T14:45:51.234584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2d6ea59-b7bc-4aab-b846-bbc04606fd07 · 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 From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T22:54:55.831525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2fba4470-c88d-4cbd-8bf7-28e0f6fff7f8 · 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 From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:21:14.820723Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a9524248-2961-4a8d-b933-f737710629f3 · 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 From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:16:13.664569Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 94fbe407-1a74-4027-a76b-07f6d5eca887 · inbound

Bias from small-scale leakage in Pulsar Timing Array maps cites this paper.

Bias from small-scale leakage in Pulsar Timing Array maps From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-04T07:43:36.162236Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db0b9943-8276-40c3-a4ce-625047f11a3b · inbound

Reaching diffraction-limited localization with coherent PTAs cites this paper.

Reaching diffraction-limited localization with coherent PTAs From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-16T22:48:37.776521Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation cf8a384e-bd42-4aa3-beb1-04ba5af87a6b · 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 From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-11T07:56:00.083240Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 488dbe67-f849-4d98-8b2d-ca6b14c8f327 · 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 From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 83

Resolution: verified exact; arxiv_id, observed 2026-05-09T05:50:27.321333Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 762b8dde-ca58-4fee-b162-32bd4ee6ba52 · inbound

Realization Variance of Gravitational Wave Background Anisotropies from Shot Noise for Pulsar Timing Arrays cites this paper.

Realization Variance of Gravitational Wave Background Anisotropies from Shot Noise for Pulsar Timing Arrays From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T04:19:24.683645Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.