Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Modelling the alumina abundance of oxygen-rich evolved stars in the Large Magellanic Cloud
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1402.2485.
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 2026-08-11T15:58:18.796597Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 7931fbcd-81d9-449d-a3cd-3029e037d04e · inbound
JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822 cites this paper.
JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822 Modelling the alumina abundance of oxygen-rich evolved stars in the Large Magellanic Cloud
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T03:55:10.305506Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f4cee962-a037-4907-b725-4cc88da59fab · inbound
Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 cites this paper.
Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 Modelling the alumina abundance of oxygen-rich evolved stars in the Large Magellanic Cloud
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T15:58:18.796597Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.