Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_\odot$ at a metallicity Z = 0.006
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2201.12262.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T17:49:20.102891Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 b9fbdc50-be5c-4d3f-a4f6-b9f80378e23e · inbound
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_\odot$ at a metallicity Z = 0.006
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:48.887601Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6104123d-3414-40d8-ba64-6d8d2984fcb7 · inbound
Discovery of the $\lambda$ Bootis phenomenon in an early B-type star cites this paper.
Discovery of the $\lambda$ Bootis phenomenon in an early B-type star Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_\odot$ at a metallicity Z = 0.006
Reference 247
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T17:49:20.102891Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.