Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2104.10919.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:45.398131Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
93
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation aea1803b-ed9d-4873-863f-2e2f1094bb39 · inbound
Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet cites this paper.
Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs
Reference 95
- Resolution
- verified exact
- local_arxiv, observed 2026-07-11T04:27:48.329151Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 6a3cdb85-386c-47a2-8a7d-4f0ce34db6f1 · inbound
Something new under the Sun: A magnetically driven CH/CN anti-correlation cites this paper.
Something new under the Sun: A magnetically driven CH/CN anti-correlation Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs
Reference 263
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:15:45.398131Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.