Paper Citation Record · LEDGER

Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2410.03832.

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

pith.paper-citation-record.v1
2410.03832 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T19:07:34.938630Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T04:26:36.086271Z

Reference resolution

0 of 0 outbound references displayed

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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 207fea8d-2294-4eb3-b9c6-8092d1048373 · inbound

Simulation of Binary-Single Interactions in AGN Disk I: Gas-Enhanced Binary Orbital Hardening cites this paper.

Simulation of Binary-Single Interactions in AGN Disk I: Gas-Enhanced Binary Orbital Hardening Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T19:07:34.938630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 404c2a3b-e671-4ddf-bc9a-32f6e7b4f31e · inbound

A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters cites this paper.

A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T13:41:03.146026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83430bea-08b2-47fc-9d69-4499a4cbdeb7 · inbound

Stellar-mass black holes in young massive and open stellar clusters -- VI. Role of external galactic field cites this paper.

Stellar-mass black holes in young massive and open stellar clusters -- VI. Role of external galactic field Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-07T14:45:49.781106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7385c12f-7bd5-4697-9ace-5e2d9e38ab60 · inbound

Seeds to success: growing heavy black holes in dense star clusters cites this paper.

Seeds to success: growing heavy black holes in dense star clusters Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-18T02:05:39.172397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation bed712d1-a441-45ef-923a-882f2fcbae47 · 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 Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.787381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation d3a50eb0-6b18-452f-959e-023639adb6b7 · inbound

Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.

Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors Formation and evolution of binary black holes in $N$-body simulations of star clusters with up to two million stars

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-07-02T04:26:36.087670Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.