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Paper Citation Record · LEDGER

Hellings and Downs correlation of an arbitrary set of pulsars

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2208.07230.

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

pith.paper-citation-record.v1
2208.07230 v6

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 2026-08-18T06:34:40.430872+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T14:26:32.048742Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T16:15:49.937950Z

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 83e10778-620e-494b-951f-cacd5e3bf0b4 · inbound

The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals cites this paper.

The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals Hellings and Downs correlation of an arbitrary set of pulsars

Reference 2

Resolution
verified exact
arxiv_id, observed 2026-05-16T08:20:32.518416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-16T08:20:32.468142Z digest=sha256:b19889d48b88df61f7c969ad944e033e0df5095d4fda76772e0b827681ff55e3

Observation b0bd0afd-6612-401c-aa00-5b7d341bb16c · inbound

Mitigating cosmic variance in the Hellings-Downs curve: a Cosmic Microwave Background analogy cites this paper.

Mitigating cosmic variance in the Hellings-Downs curve: a Cosmic Microwave Background analogy Hellings and Downs correlation of an arbitrary set of pulsars

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-11T14:26:32.048742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:26:32.048742Z digest=sha256:53293c61364920023fb9e970c313e3a344e16d0e7ae497129974cc1b13cc1775

Observation a2a04091-d9fc-4ded-a727-4a78049970f2 · inbound

Do Pulsar Timing Datasets Favor Massive Gravity? cites this paper.

Do Pulsar Timing Datasets Favor Massive Gravity? Hellings and Downs correlation of an arbitrary set of pulsars

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-06T20:45:32.113323Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:45:32.113323Z digest=sha256:e33645ce940815c84c821874045b0bab8e324283fde98eecfb82a7d5c2c72e47

Observation 7db87289-1212-4715-95da-c2cd1a4a4b71 · 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 Hellings and Downs correlation of an arbitrary set of pulsars

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-04T22:54:55.852726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:54:55.852726Z digest=sha256:dc2988b2455416bc1d3942559ecc6a5dc4996b9da06167b9b8e5d30e7bd57962

Observation 414461b1-4102-4311-aa4b-9cc201273484 · inbound

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background cites this paper.

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background Hellings and Downs correlation of an arbitrary set of pulsars

Reference 54

Resolution
verified exact
arxiv_id, observed 2026-05-21T19:04:19.028438Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-21T19:03:22.579341Z digest=sha256:c53f4a33441a2ab36e13fe2a621335872aa3aeedd279fded162260ea652010a7

Observation b2ceaef6-1c24-439f-8238-98406679e303 · inbound

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background cites this paper.

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background Hellings and Downs correlation of an arbitrary set of pulsars

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-03T22:40:19.212241Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T22:40:19.212241Z digest=sha256:e5d5cf33c207c88ac036d1dd0d7a7aff02bdde3204971d5179ece96ea4c48e2d

Observation 4e916e1c-0aea-4c8b-b6ac-d1e49cfa59df · inbound

Stochastic gravitational-wave background search using data from five pulsar timing arrays cites this paper.

Stochastic gravitational-wave background search using data from five pulsar timing arrays Hellings and Downs correlation of an arbitrary set of pulsars

Reference 59

Resolution
verified exact
arxiv_id, observed 2026-05-17T00:08:43.392203Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-17T00:05:42.521526Z digest=sha256:02c871f17de4f4fda281292d681a3e6af7a1be49b018969aa952ad33e8d361bb

Observation db6a31b0-1627-4911-803d-a4378707f47f · inbound

Forecasting graviton-mass constraints from the full covariance of PTA-astrometry ORF estimators cites this paper.

Forecasting graviton-mass constraints from the full covariance of PTA-astrometry ORF estimators Hellings and Downs correlation of an arbitrary set of pulsars

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-05-11T20:56:10.024000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-08T07:42:15.997427Z digest=sha256:16caf839b4b527d7bdc017146deb5b6684e86698e67b61129fc1a31d8e08028f

Observation 8da2da4c-959a-451b-856d-59b8157d7fb1 · inbound

The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses cites this paper.

The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses Hellings and Downs correlation of an arbitrary set of pulsars

Reference 124

Resolution
verified exact
arxiv_id, observed 2026-07-01T16:15:49.939413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-06-30T00:43:09.947073Z digest=sha256:8d8c51f00e7010e304322e5d4b160629728942f9fbf19b0330ced6770735b6ac

Observation dea27793-a25c-4ffb-8d65-c1fe53060f06 · inbound

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models cites this paper.

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models Hellings and Downs correlation of an arbitrary set of pulsars

Reference 134

Resolution
verified exact
arxiv_id, observed 2026-07-01T15:35:48.448937Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-06-30T01:20:21.581469Z digest=sha256:351afa8d36d85945ef3c57959de93c5f14c077399585dc6d8413db247e94f3fa

Observation 370320af-ba7e-4bd8-acbb-9ba3188a3635 · inbound

Gravitational-Wave Sky Mapping with Pulsar Timing Arrays: The Full Earth-Pulsar Response and Fundamental Resolution Limits cites this paper.

Gravitational-Wave Sky Mapping with Pulsar Timing Arrays: The Full Earth-Pulsar Response and Fundamental Resolution Limits Hellings and Downs correlation of an arbitrary set of pulsars

Reference 162

Resolution
unresolved
no resolver link, observed 2026-08-01T12:52:24.341297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:52:24.341297Z digest=sha256:17d33ca5352b39b3b61db5beed42109c6c8da3572f1195283207b3c93eeb13fe