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Paper Citation Record · LEDGER

Too shy to spin? Cosmic wallflowers as proto-globular clusters

As of 6 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 0 inbound Pith citation observations for arXiv:2606.27426.

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

pith.paper-citation-record.v1
2606.27426 v2

Coverage vector

measured 2 of 2 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-02T10:03:03.324801Z

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

2 of 2 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved2
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 20014250-a760-42af-98ac-95219e5daf9a · outbound

This paper cites The Formation and Early Evolution of Young Massive Clusters.

Too shy to spin? Cosmic wallflowers as proto-globular clusters The Formation and Early Evolution of Young Massive Clusters

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-02T10:03:03.200776Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T10:03:03.200776Z digest=sha256:56b479630d38473e7c1c562af54ff2345736c65f27f7b2bc683d0068a88528b0

Observation 7d9a8e8f-c27f-44c7-8bcd-966f463d4daa · outbound

This paper cites All systems considered here satisfy these criteria and remain strongly baryon-dominated, with no evidence for associated dark matter subhaloes.

Too shy to spin? Cosmic wallflowers as proto-globular clusters All systems considered here satisfy these criteria and remain strongly baryon-dominated, with no evidence for associated dark matter subhaloes

Reference 2009

Resolution
unresolved
no resolver link, observed 2026-08-02T10:03:03.324801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T10:03:03.324801Z digest=sha256:87f63e54d9a411a3bbf3bba36198bd17721a6c2a7b3e5a22aefa5b66982ee679

Pith citing papers

No inbound Pith citation observations are available.