Paper Citation Record · LEDGER

N-body simulations of globular cluster tides

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9910148.

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

pith.paper-citation-record.v1
astro-ph/9910148 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:24:19.402172Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d93b3e0d-6aa3-48e5-8ecc-5193bc075dbe · inbound

The ejection and detectability of high- and hyper-velocity stars by compact object binaries in globular clusters cites this paper.

The ejection and detectability of high- and hyper-velocity stars by compact object binaries in globular clusters N-body simulations of globular cluster tides

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T00:24:19.402172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4dccf4ba-664d-4bd7-bf4b-a5fa1efba904 · inbound

Dynamical evolution of Milky Way globular clusters on the cosmological timescale II. Terzan 2, 4, and 5 mass loss and collision tracking cites this paper.

Dynamical evolution of Milky Way globular clusters on the cosmological timescale II. Terzan 2, 4, and 5 mass loss and collision tracking N-body simulations of globular cluster tides

Reference 156

Resolution: verified exact; arxiv_id, observed 2026-07-04T17:22:36.607155Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.