Paper Citation Record · LEDGER

Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2210.10055.

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

pith.paper-citation-record.v1
2210.10055 v3

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 7 of 7 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 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T13:27:10.478511Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T09:21:20.829081Z

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Outbound references

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Pith citing papers

Observation e9653991-0141-4798-a7c4-a85800ba5092 · 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 Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.478511Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 61aa8e0d-8bef-4ee8-8228-633e05958cac · inbound

Population Synthesis of Gravitational Wave Sources cites this paper.

Population Synthesis of Gravitational Wave Sources Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 125

Resolution: unresolved; no resolver link, observed 2026-08-09T04:41:35.694050Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89862768-0035-4d5c-a022-3ddc2c53e61c · inbound

Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation cites this paper.

Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-06T18:29:55.844592Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab3bf59c-aeb3-4b4a-ae40-535fe8f8e8db · inbound

PRECESSION 2.1: black-hole binary spin precession on eccentric orbits cites this paper.

PRECESSION 2.1: black-hole binary spin precession on eccentric orbits Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 9

Resolution: verified exact; arxiv_id, observed 2026-05-18T20:26:51.020721Z

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.

Observation a443d323-51cc-41ac-8b40-c61c12cf2ee9 · inbound

Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications cites this paper.

Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-03T22:13:56.759034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aea46258-e4ad-45c3-8388-0fe6fd3643c6 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 71

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:21:20.831880Z

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.

Observation ad570f17-5fa3-429d-a312-09230660c31e · inbound

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 140

Resolution: unresolved; no resolver link, observed 2026-08-01T09:38:58.407576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.