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Paper Citation Record · LEDGER

Simulations predict intermediate-mass black hole formation in globular clusters

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2406.06772.

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

pith.paper-citation-record.v1
2406.06772 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:25:40.943094Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T15:15:03.350901Z

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 270ffa44-c775-40bb-a964-203d6259de41 · inbound

Pulsars in Globular Clusters With the SKAO cites this paper.

Pulsars in Globular Clusters With the SKAO Simulations predict intermediate-mass black hole formation in globular clusters

Reference 89

Resolution
verified exact
local_arxiv, observed 2026-07-08T15:15:03.352494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:165f98549c30eb8d38c1168ead4dd0750904b0d120f650a9b6f1ba4530ddd9f0

Observation 7f9a631b-6b5e-43f8-858d-2996b1c0aa8f · inbound

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Simulations predict intermediate-mass black hole formation in globular clusters

Reference 135

Resolution
unresolved
no resolver link, observed 2026-08-01T00:25:40.943094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:25:40.943094Z digest=sha256:c09192ee6c02cc747d49301890bccf82856fab69fbd82b8286b2c46743fbe078