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Paper Citation Record · LEDGER

Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2012.04261.

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

pith.paper-citation-record.v1
2012.04261 v3

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 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:49:48.183522Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T19:47:19.905132Z

Reference resolution

0 of 0 outbound references displayed

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  • 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 2e0be7da-f51f-41ea-9938-5cff821d6f7b · inbound

Detection and parameter estimation of supermassive black hole ringdown signals using a pulsar timing array cites this paper.

Detection and parameter estimation of supermassive black hole ringdown signals using a pulsar timing array Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-11T18:49:48.183522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T18:49:48.183522Z digest=sha256:d0368aa77ad25cf42b75dcb99704c918a9cbf4bb6069ad2367aaf369ac585e6c

Observation 73cb512f-6f8f-4f7e-8726-62894bcb53bc · inbound

Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing array cites this paper.

Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing array Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations

Reference 21

Resolution
verified exact
arxiv_id, observed 2026-07-02T19:47:19.906518Z

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=2026-06-27T21:17:17.526820Z digest=sha256:699c8c314d4e568e256c6d7994b3b321f83311206c9bcff62334fab9612c09fe