Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2501.12734.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T13:44:46.515467Z
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
0
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 30c0421c-4804-4ba5-bd5c-1c30a96fedb4 · inbound
Effect of Magnetic Field on the Accretion Phase of Population III Star Formation cites this paper.
Effect of Magnetic Field on the Accretion Phase of Population III Star Formation Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
Reference 58
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-07T13:44:47.985467Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 20e82e14-425a-4ae9-915b-a0498b69794d · 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 Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T00:21:45.241141Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.