Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2312.06509.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T21:56:07.177614Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation ad3a6bcf-3a5f-4c54-965e-32da2e1681c1 · inbound
Cracking the relation between mass and 1P-star fraction of globular clusters: III. Initial distributions of in-situ and ex-situ clusters cites this paper.
Cracking the relation between mass and 1P-star fraction of globular clusters: III. Initial distributions of in-situ and ex-situ clusters Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T21:56:07.177614Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9ae590fa-7191-4bab-b316-a25c6e1c6b8e · inbound
Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn cites this paper.
Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
Reference 118
- Resolution
- verified exact
- arxiv_id, observed 2026-05-15T02:23:31.124218Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.