Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1911.08988.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T14:56:13.130680Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T20:16:09.815371Z
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 cb3ab4a0-2815-45f9-956a-bbbd3f76b623 · inbound
Evolution and final fates of massive stars cites this paper.
Evolution and final fates of massive stars The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T14:56:13.130680Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb6fe374-1a5b-4d58-9ab0-2c3a7f8c330a · inbound
The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants cites this paper.
The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T20:16:09.817477Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.