Paper Citation Record · LEDGER

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

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 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 9 of 9 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 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T12:54:26.888718Z

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 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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+00:00.