Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Demonstration of a novel method for measuring mass-loss rates for massive stars
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1803.02794.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-31T12:04:42.954785Z
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
21
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 86d68bd7-98d1-4893-91c3-f91478971a7b · inbound
Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.
Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Demonstration of a novel method for measuring mass-loss rates for massive stars
Reference 288
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T18:09:41.369846Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation eeead24c-9258-4d1c-a9c5-d560469c704b · inbound
An Halpha survey of infrared bow-shocks around OB-type stars cites this paper.
An Halpha survey of infrared bow-shocks around OB-type stars Demonstration of a novel method for measuring mass-loss rates for massive stars
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:42.954785Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.