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Paper Citation Record · LEDGER

Particle acceleration in winds of star clusters

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:26:59.713570Z

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 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-28T21:39:08.628584Z digest=sha256:11c80799ac6bebf2fed4d9c9576d358ead790372affc60fc6f88fbc3c75f0b9e

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 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-27T15:39:48.644607Z digest=sha256:85344fd81491059d8c0902254e213ed9a07f7e2569c74c28a7bb539edec4577e

Observation 06fd8a04-6c91-49e7-b0fa-327d35106451 · inbound

Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region cites this paper.

Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region Particle acceleration in winds of star clusters

Reference 117

Resolution
unresolved
no resolver link, observed 2026-08-02T02:23:22.812518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:23:22.812518Z digest=sha256:2671fc45859a5d2f583a941e6ec44e477fd4a2b50b1284337c2ec01031895b98

Observation 0270a838-6172-4632-a9a8-73aed8e6dc77 · 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 Particle acceleration in winds of star clusters

Reference 253

Resolution
unresolved
no resolver link, observed 2026-08-02T02:26:59.713570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:26:59.713570Z digest=sha256:fd33b304836314732070d6671cae9d371e120aa9f9f71eedb36681eb432c7ea3

Observation 15e7bbcd-2f80-403e-8d84-3440690f3d3f · inbound

A cosmic-ray loaded nascent outflow driven by a massive star cluster cites this paper.

A cosmic-ray loaded nascent outflow driven by a massive star cluster Particle acceleration in winds of star clusters

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-01T22:21:55.566277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T22:21:55.566277Z digest=sha256:88ad88ac26e7a17d527e449c78b7605ea5bf3b6b6e63720ba2146201e4a62e97

Observation 51301dc6-9d43-4cc8-9191-fd5062aea137 · inbound

Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 cites this paper.

Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 Particle acceleration in winds of star clusters

Reference 106

Resolution
unresolved
no resolver link, observed 2026-08-01T21:55:38.450977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T21:55:38.450977Z digest=sha256:ff6628f53143792a703b335e2710d6a16baf18fbd1d597d04b419bfbb63c8e85