Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups
As of 2 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1108.3868.
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 2026-08-02T06:30:47.504484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T02:59:10.770850Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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- 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 5c1dcc44-6e3b-4ca4-89e3-96610d3c14d3 · inbound
The complex stellar system M 22: confirming abundance variations with high precision differential measurements cites this paper.
The complex stellar system M 22: confirming abundance variations with high precision differential measurements Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:58:15.842761Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fc4614e0-3f81-4f54-945f-121fcfcb9942 · inbound
The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios cites this paper.
The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios Characterizing the Heavy Elements in Globular Cluster M22 and an Empirical s-process Abundance Distribution Derived from the Two Stellar Groups
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:59:10.770850Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.