Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2211.04485.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T04:25:28.521958Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 0df3fc85-87a6-478c-b77a-2de8c0d8f3c2 · inbound
The role of filaments in the large-scale conformity signal cites this paper.
The role of filaments in the large-scale conformity signal The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T04:25:28.521958Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bf26bf6b-a0f4-45cc-80ee-38ff31ee3ba5 · inbound
Identifying backsplash galaxies using machine learning cites this paper.
Identifying backsplash galaxies using machine learning The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:44:56.709894Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.