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Paper Citation Record · LEDGER

Cosmological simulations of the generation of cluster-scale radio emission from turbulent re-acceleration

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2406.09859.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2406.09859 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:26:52.297156Z

measured 0 of 1 external citation measurements

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 1d08352e-b82f-4620-8262-ee41059417d2 · inbound

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Cosmological simulations of the generation of cluster-scale radio emission from turbulent re-acceleration

Reference 188

Resolution
unresolved
no resolver link, observed 2026-08-02T02:26:52.297156Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:26:52.297156Z digest=sha256:94141bb89e086e8e04cffa2b44db201efa7066f86bd81b9d937b24e79d630829

Observation 07eab0f9-2cf0-4d5a-a6de-ba30bfb7019e · inbound

Two-component large-scale radio emission in Abell 2244 cites this paper.

Two-component large-scale radio emission in Abell 2244 Cosmological simulations of the generation of cluster-scale radio emission from turbulent re-acceleration

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-01T23:28:42.923404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:28:42.923404Z digest=sha256:d9796ae2337f3ab1ca5c2ba01b9cb8ca4ee7b90ba6d616fb71f8303429b7468c