Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2106.02643.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T11:02:35.494919Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T09:21:21.208249Z
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 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 2026-08-05T06:32:48.257954+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 2026-08-05T06:32:48.257954+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 2026-08-05T06:32:48.257954+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.