Paper Citation Record · LEDGER

Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2106.02643.

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

pith.paper-citation-record.v1
2106.02643 v3

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:25:35.087633Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T09:21:21.208249Z

Reference resolution

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b147ceef-410a-4f85-9d99-949500ccd778 · inbound

Population Synthesis of Gravitational Wave Sources cites this paper.

Population Synthesis of Gravitational Wave Sources Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 204

Resolution: unresolved; no resolver link, observed 2026-08-09T04:41:35.954855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97ff898e-5a5b-48c5-93a4-6f490c2a2644 · inbound

Evolution of a black hole cluster in full general relativity cites this paper.

Evolution of a black hole cluster in full general relativity Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 130

Resolution: unresolved; no resolver link, observed 2026-08-16T04:25:35.087633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01e198a0-7060-424a-bb37-198dc2e8af94 · inbound

The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets cites this paper.

The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T15:36:21.519994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc52b59e-dd2b-49ab-abf8-2408e636dd40 · inbound

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset cites this paper.

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-05-09T02:57:52.357708Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 3d2c3a29-6d5a-434a-8ba0-f5b8f5ac81d7 · inbound

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset cites this paper.

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-03T11:02:35.494919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5bf33a73-4137-46a7-bf3d-40e68db7bd6e · inbound

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters cites this paper.

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.813060Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 39719196-dc1c-407c-a3e9-5ab1e201c44c · 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 Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 56

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:21:21.210868Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e0d057bb-ca1b-432d-8b4a-d8fe1fe346e5 · 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 Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Reference 227

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.