Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
How stellar rotation shapes the colour magnitude diagram of the massive intermediate-age star cluster NGC 1846
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2001.01731.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T14:44:02.812922Z
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 7414daa3-8e75-494b-a0db-951e8aad756e · inbound
Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations cites this paper.
Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations How stellar rotation shapes the colour magnitude diagram of the massive intermediate-age star cluster NGC 1846
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:44:02.812922Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.