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Paper Citation Record · LEDGER

Monte Carlo Simulations of Globular Cluster Evolution. IV. Direct Integration of Strong Interactions

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0608261.

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

pith.paper-citation-record.v1
astro-ph/0608261 v3

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 2026-08-13T06:32:02.005865+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.200001Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T17:57:14.582056Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 8fc80058-63d6-4c4d-ac8f-dcd9d15fc61b · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Monte Carlo Simulations of Globular Cluster Evolution. IV. Direct Integration of Strong Interactions

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-06T22:52:12.200001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:52:12.200001Z digest=sha256:9add0fb14d0e9d0bac435ea217086697f1c1bb33b38ec94242f7eba535d61d10

Observation f4890896-bee8-4fda-965d-fba222c43bcd · inbound

The evolution of high-z proto-star clusters into local globular clusters cites this paper.

The evolution of high-z proto-star clusters into local globular clusters Monte Carlo Simulations of Globular Cluster Evolution. IV. Direct Integration of Strong Interactions

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-07-02T17:57:14.583589Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bf7290431835e2d0e88a675086ea2eabd5ed31deff5c628e7439b720175dbb97

Observation 8ada14bb-579c-4d8c-879c-d5e87b7074f4 · 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 Monte Carlo Simulations of Globular Cluster Evolution. IV. Direct Integration of Strong Interactions

Reference 57

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:72cfd9012cf8771d07080b0819020dd112a43a91b1812d49f44eb5277838c6ab