Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The importance of magnetic fields for the initial mass function of the first stars
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2002.11502.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T00:21:45.586302Z
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 9ab8f41b-dd05-4c1c-ae8c-fdb445b7d64b · 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 The importance of magnetic fields for the initial mass function of the first stars
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:54.546944Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 054b5c26-825d-48b1-87bd-a03e500cf635 · inbound
Searching for Population III stars with line intensity mapping cross-correlations cites this paper.
Searching for Population III stars with line intensity mapping cross-correlations The importance of magnetic fields for the initial mass function of the first stars
Reference 121
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T00:21:45.586302Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.