Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Angular Momentum Transport by Internal Gravity Waves. I - Pop I Main Sequence Stars
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:astro-ph/0305151.
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 2026-08-08T13:33:06.565688Z
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 60a085ff-d8e1-4e0e-83c2-931d5e98314b · inbound
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars Angular Momentum Transport by Internal Gravity Waves. I - Pop I Main Sequence Stars
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T13:33:06.565688Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.