Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0608078.
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 2026-08-08T16:32:31.753868Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T13:02:10.934470Z
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 3e997ba0-3708-41ba-b5f1-379d6f4703f8 · inbound
Giants, Supergiants and Hypergiants cites this paper.
Giants, Supergiants and Hypergiants The Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:54:17.885551Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1059cc19-bd44-40a6-a6f1-08613eb88165 · inbound
Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.
Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models The Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
Reference 191
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T02:13:55.760807Z
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 50798d78-c6df-4693-ae06-9c570fc0d8af · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? The Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
Reference 139
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.935876Z
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 4c0d4da7-72f4-4b05-abd0-4143192b2c97 · inbound
A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind cites this paper.
A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind The Galactic WN stars: Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T16:32:31.753868Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.