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Paper Citation Record · LEDGER

IMBH Progenitors from Stellar Collisions in Dense Star Clusters

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2404.11646.

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

pith.paper-citation-record.v1
2404.11646 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T13:27:10.704248Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T18:00:00.323451Z

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 2bfcf7eb-72e2-422b-a85a-a39e65289af7 · inbound

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers cites this paper.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers IMBH Progenitors from Stellar Collisions in Dense Star Clusters

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-10T13:27:10.704248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T13:27:10.704248Z digest=sha256:c0692c1722fb7ea4070f8c80d5335c6eaf6313f00afc9da056eedccdb81c3cb1

Observation db70c516-575d-4649-b67d-667a3acfc708 · inbound

Solving Inverse Problems of Chaotic Systems with Bidirectional Conditional Flow Matching cites this paper.

Solving Inverse Problems of Chaotic Systems with Bidirectional Conditional Flow Matching IMBH Progenitors from Stellar Collisions in Dense Star Clusters

Reference 115

Resolution
malformed identifier
arxiv_id, observed 2026-07-04T18:00:00.324950Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-06-25T23:18:24.145654Z digest=sha256:9cb81da810b41722b659edd1c8a5e7934e8c58f381e7c34e2963a1e23ead98b3

Observation f839bcc6-e2fe-40b1-a41f-19ca1809d12e · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins IMBH Progenitors from Stellar Collisions in Dense Star Clusters

Reference 82

Resolution
unresolved
no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:c4a57d37ad63c1107e1887dcf3a1a3959660c8f3e2fa563a7c182607ed25c738