Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Wind Momentum - Luminosity Relationship of Galactic A- and B- Supergiants
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9910449.
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 2026-08-06T18:25:19.720435Z
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
9
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 80b1c80b-0299-4a59-a2dc-694d980cf24f · inbound
On the origin of variability in $\alpha$ Cygni variable $\epsilon$ Ori (HD 37128) using TESS observations and modelling cites this paper.
On the origin of variability in $\alpha$ Cygni variable $\epsilon$ Ori (HD 37128) using TESS observations and modelling The Wind Momentum - Luminosity Relationship of Galactic A- and B- Supergiants
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T17:56:50.277117Z
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 51750e37-60ab-45ed-8b0a-6ee59559205e · 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 Wind Momentum - Luminosity Relationship of Galactic A- and B- Supergiants
Reference 230
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.774503Z
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 9406e3c9-b148-45db-8c70-1ed1b16c270f · inbound
Characterization of the variability of the blue supergiant HD 14134 cites this paper.
Characterization of the variability of the blue supergiant HD 14134 The Wind Momentum - Luminosity Relationship of Galactic A- and B- Supergiants
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:25:19.720435Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.