Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Evolution of massive population III stars with rotation and magnetic fields
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1201.2364.
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 2026-08-07T22:32:29.190660Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
226
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 7d0a6c04-c9de-4ca9-a800-783471874545 · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? Evolution of massive population III stars with rotation and magnetic fields
Reference 138
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.906771Z
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.
Observation bbccfe11-7e94-4ca4-99ed-e8db539af414 · inbound
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories cites this paper.
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Evolution of massive population III stars with rotation and magnetic fields
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T22:32:29.190660Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.