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Paper Citation Record · LEDGER

Particle acceleration in winds of star clusters

As of 31 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2102.09217.

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

pith.paper-citation-record.v1
2102.09217 v1

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 2026-07-31T06:34:12.847434+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-28T21:39:08.628584Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-03T02:57:35.367983Z

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 7db9b7d4-4ad4-4f1d-bc77-0311cbd48d8f · inbound

Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays cites this paper.

Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays Particle acceleration in winds of star clusters

Reference 21

Resolution
verified exact
arxiv_id, observed 2026-07-01T20:06:11.954676Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.

source=pdf_text observed=2026-06-28T21:39:08.628584Z digest=sha256:053cf47111f35bc9dccde17f073baa44464d1740bfea36dad9caae56dec7ad02

Observation 1a2e1938-1517-445c-af5c-36de07dbc4e3 · inbound

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays cites this paper.

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays Particle acceleration in winds of star clusters

Reference 8

Resolution
verified exact
arxiv_id, observed 2026-07-03T02:57:35.369468Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.

source=pdf_text observed=2026-06-27T15:39:48.644607Z digest=sha256:fa65eb3c22152656b277491cd5d7af0cc6793aa38d870c27a0d998eebae0bae3