Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2405.18265.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:56:27.365026Z
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
6
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation b2f8a887-0c98-4ffa-9643-dddca724671e · inbound
Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback cites this paper.
Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:56:27.365026Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c69d8418-b375-4d20-825f-4fcbebd3e8ee · 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 Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T13:44:46.424444Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 54874d2d-683e-400f-bc48-f27048d35509 · inbound
Turbulence in Primordial Dark Matter Halos and Its Impact on the First Star Formation cites this paper.
Turbulence in Primordial Dark Matter Halos and Its Impact on the First Star Formation Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T12:45:03.642977Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9287bdc0-382f-437e-bb7b-8141fcaf035f · inbound
Supersonic Turbulence in Primordial Halos: A Comparison With and Without The Stream Velocity cites this paper.
Supersonic Turbulence in Primordial Halos: A Comparison With and Without The Stream Velocity Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
Reference 81
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T16:39:51.289920Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 476b08af-5bd3-4b42-b7c1-3e4a8b34f40b · 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 Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T00:21:45.276472Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.