Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Inefficient star formation in high Mach number environments I. The turbulent support analytical model
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2404.17368.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-13T06:20:04.707661Z
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 c92ae9af-0a5d-41e8-9a4e-fe84f1c4ebe5 · inbound
mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.
mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Inefficient star formation in high Mach number environments I. The turbulent support analytical model
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T06:20:04.707661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.