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Paper Citation Record · LEDGER

Pulsar timing array source ensembles

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2401.14329.

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

pith.paper-citation-record.v1
2401.14329 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T14:26:32.077113Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T07:55:59.761748Z

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 cc07ad48-3288-4c09-a0ad-90d594df4822 · 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 timing array source ensembles

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-11T14:26:32.077113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:26:32.077113Z digest=sha256:18f85e742e3ad71cb728fbddf39e53614f0356ce3414e1dcf460c964211a3b5e

Observation d3bb421e-ce63-47b6-83f3-1b907c30bf8c · 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 Pulsar timing array source ensembles

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-05-11T07:55:59.763987Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-10T16:54:03.779202Z digest=sha256:5191b51d6c80af815e2354138840e26ab6b1ef1fa59f27ba42328da22c09186e