Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1402.5694.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T04:22:56.138065Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T23:07:42.733357Z
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 8142a8c2-82eb-4ea7-a946-44f39b433e5f · inbound
From stellar light to astrophysical insight: automating variable star research with machine learning cites this paper.
From stellar light to astrophysical insight: automating variable star research with machine learning Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample
Reference 124
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:22:34.998805Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 72f960d6-1840-4892-b230-e7b509672ed6 · 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 Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample
Reference 133
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T04:19:29.170180Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5e093bec-2877-44b2-865e-bb9b007a274f · inbound
Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star cites this paper.
Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample
Reference 207
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T23:07:42.747619Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation c4c6edb8-8605-4d63-a946-cae031da6022 · inbound
The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper cites this paper.
The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample
Reference 276
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:41:50.108493Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e300719c-977b-4de9-a834-9eebcf6aac6a · inbound
The Maunder Model and Catalog: Stellar Rotation, Bimodal Activity, and Magnetic Braking in Kepler Main-Sequence Stars cites this paper.
The Maunder Model and Catalog: Stellar Rotation, Bimodal Activity, and Magnetic Braking in Kepler Main-Sequence Stars Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T04:22:56.138065Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.