Pith. sign in

Paper Citation Record · LEDGER

Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2209.14834.

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

pith.paper-citation-record.v1
2209.14834 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T04:42:52.375371Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T20:56:09.901506Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 f27a9a69-c7d9-455f-bb89-5615c8a07aed · inbound

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum cites this paper.

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-12T04:42:52.375371Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T04:42:52.375371Z digest=sha256:819ab30b8d7977e5aeff702aaf436fab46eeb2c713ebf5669ace1d46d7cda8ce

Observation f5d2e2e0-7d9a-4e5f-a234-18e3bc5e3a6f · 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 Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-11T14:26:32.001844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:26:32.001844Z digest=sha256:7be5d10f463c62887b8f25e33a79ea229ae993eec26c19e997b3ab193caa57b2

Observation dc5c544d-f1be-46ed-adc4-61ec0a98e4e5 · inbound

\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors cites this paper.

\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-06T15:30:12.266598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:30:12.266598Z digest=sha256:a5ffe96c1617ba762336c153bd99cbf4585b8449355b039ece00f040ad02acc2

Observation 10baf9e5-893a-44ed-b558-bc6c6427632f · inbound

Stochastic problems in pulsar timing cites this paper.

Stochastic problems in pulsar timing Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background

Reference 31

Resolution
verified exact
arxiv_id, observed 2026-05-11T05:21:02.161850Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-10T18:10:38.102559Z digest=sha256:7e58e9495a43e348b57a40764d0a13e7f0ef02cc08dc9c586460c327a6787025

Observation 232b6db2-b334-4769-91ac-50fe7cc86fae · 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 Pulsar and cosmic variances of pulsar timing-array correlation measurements of the stochastic gravitational wave background

Reference 36

Resolution
verified exact
arxiv_id, observed 2026-05-11T20:56:09.904492Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-08T07:42:15.997427Z digest=sha256:8ab06817f5c12682d24a19d3a42271b8d37ab20a5570dfea4186df77ac2f75ca