Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational fragmentation in turbulent primordial gas and the initial mass function of Population III stars
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1006.1508.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T10:19:04.105934Z
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 7151ea1b-4252-4cca-9270-7fc10ae18760 · inbound
Constraining Population III stellar demographics with next-generation gravitational-wave observatories cites this paper.
Constraining Population III stellar demographics with next-generation gravitational-wave observatories Gravitational fragmentation in turbulent primordial gas and the initial mass function of Population III stars
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T10:19:04.105934Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4cd50040-3ec0-4794-b720-4069ff90f711 · inbound
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Gravitational fragmentation in turbulent primordial gas and the initial mass function of Population III stars
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:48.806496Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.