Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Very-high-energy $\gamma$-ray emission from young massive star clusters in the Large Magellanic Cloud
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.16219.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T22:21:57.280165Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-01T20:06:11.959816Z
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 6073c507-82ad-4391-8d65-51e14720271a · inbound
Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays cites this paper.
Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays Very-high-energy $\gamma$-ray emission from young massive star clusters in the Large Magellanic Cloud
Reference 53
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T20:06:11.960998Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 3a2d5e78-438f-4316-ac2e-4bf1c6bf612f · inbound
A cosmic-ray loaded nascent outflow driven by a massive star cluster cites this paper.
A cosmic-ray loaded nascent outflow driven by a massive star cluster Very-high-energy $\gamma$-ray emission from young massive star clusters in the Large Magellanic Cloud
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T22:21:57.280165Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.