Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2402.14954.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T00:33:17.275137Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-04T23:33:10.175080Z
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 d56faa41-690a-4cee-bbaf-da052ba47f99 · inbound
Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF cites this paper.
Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T21:15:43.368350Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 466e11e1-9d0c-4787-9366-88010ec46b99 · 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 Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:22:28.265800Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 401959f8-0e64-46e3-b42f-e8ebe61ac90a · inbound
Selected Results on Variable Stars Observed by TESS cites this paper.
Selected Results on Variable Stars Observed by TESS Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-08-04T23:33:10.180128Z
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.
Observation 87f529f8-c97f-4667-9a05-2b28523165cf · 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 Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission
Reference 278
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:41:50.113777Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cb88ba7a-a67d-4958-b9ac-14d34369f598 · inbound
Three new exoplanet systems from the Dispersed Matter Planet Project cites this paper.
Three new exoplanet systems from the Dispersed Matter Planet Project Methods for the detection of stellar rotation periods in individual TESS sectors and results from the Prime mission
Reference 139
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:33:17.275137Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.