Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Improvements to stellar structure models, based on a grid of 3D convection simulations. II. Calibrating the mixing-length formulation
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1410.1559.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T13:35:03.085584Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T13:35:04.230514Z
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 304cfc35-8642-4c3d-91ce-f8622f2ff7e2 · inbound
Evolution and final fates of low- and intermediate-mass stars cites this paper.
Evolution and final fates of low- and intermediate-mass stars Improvements to stellar structure models, based on a grid of 3D convection simulations. II. Calibrating the mixing-length formulation
Reference 93
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T13:35:04.234778Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 43be2278-786e-494b-84a1-75a421f0879c · inbound
Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones cites this paper.
Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones Improvements to stellar structure models, based on a grid of 3D convection simulations. II. Calibrating the mixing-length formulation
Reference 101
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:39:52.863855Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.