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Paper Citation Record · LEDGER

On the population III binary black hole mergers beyond the pair-instability mass gap

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2104.13384.

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

pith.paper-citation-record.v1
2104.13384 v2

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 2026-08-10T13:27:10.675033Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T22:56:53.680192Z

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 e0bc0133-1cb7-49b2-b8a0-d00fcd9586ed · 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 On the population III binary black hole mergers beyond the pair-instability mass gap

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-10T13:27:10.675033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T13:27:10.675033Z digest=sha256:9487d2a6a3a5f64c29d049cb864f5ca785b63d860922905883b4c988cc1d3ab2

Observation e4774e64-f65f-4feb-b65a-000838ef83a7 · inbound

GW231123: A Possible Primordial Black Hole Origin cites this paper.

GW231123: A Possible Primordial Black Hole Origin On the population III binary black hole mergers beyond the pair-instability mass gap

Reference 127

Resolution
verified exact
arxiv_id, observed 2026-05-18T22:56:53.682038Z

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=2026-05-18T22:52:55.899162Z digest=sha256:f0786bd2ad84ae024789d754228d2559d6955f9b377105b2a3cd266d8d2e3c37

Observation 93a36c38-5fd2-4f1d-bdc2-1cd030111572 · inbound

January Food Benchmark (JFB): A Public Benchmark Dataset and Evaluation Suite for Multimodal Food Analysis cites this paper.

January Food Benchmark (JFB): A Public Benchmark Dataset and Evaluation Suite for Multimodal Food Analysis On the population III binary black hole mergers beyond the pair-instability mass gap

Reference 129

Resolution
unresolved
no resolver link, observed 2026-08-05T20:46:11.238458Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T20:46:11.238458Z digest=sha256:9a9e69d3b04ea4acafee6e0aff1ee62fef680b73e84916d56b8618f1d1902ba2