Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Asteroseismology of the fast-rotating high-amplitude $\delta$ Scuti star V2367 Cygni
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2406.11060.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T14:45:20.125025Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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External citation measurements
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Outbound references
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Pith citing papers
Observation 6ffe18c8-59eb-4a2d-990f-d967a054ffda · inbound
Re-examining Super-Nyquist Frequencies of 68 $\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry cites this paper.
Re-examining Super-Nyquist Frequencies of 68 $\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry Asteroseismology of the fast-rotating high-amplitude $\delta$ Scuti star V2367 Cygni
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T14:45:20.125025Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.