Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Towards a universal analytical model for Population III star formation: interplay between feedback and fragmentation
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.14294.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T12:42:56.189770Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
3
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 39c5e8fa-167b-461a-8eab-df1c06b39a3c · inbound
Simulating High-redshift Galaxies: Enhancing UV Luminosity with Star Formation Efficiency and a Top-heavy IMF cites this paper.
Simulating High-redshift Galaxies: Enhancing UV Luminosity with Star Formation Efficiency and a Top-heavy IMF Towards a universal analytical model for Population III star formation: interplay between feedback and fragmentation
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T12:42:56.189770Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 57e7933b-c7c8-439a-a2c0-fc3b47d41e0b · inbound
Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum cites this paper.
Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Towards a universal analytical model for Population III star formation: interplay between feedback and fragmentation
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T23:09:27.418642Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.