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Paper Citation Record · LEDGER

Initial Populations of Black Holes in Star Clusters

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0508005.

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

pith.paper-citation-record.v1
astro-ph/0508005 v3

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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:25:34.651422Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

38
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 003f417c-1001-4009-beda-5ec987366997 · inbound

Evolution of a black hole cluster in full general relativity cites this paper.

Evolution of a black hole cluster in full general relativity Initial Populations of Black Holes in Star Clusters

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-16T04:25:34.651422Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:25:34.651422Z digest=sha256:df24ad31b83e4aa77b9eeac863f17744bbc04f94b33fd756f94ef5dfd676343d

Observation 5fbd0c5e-dc05-48df-ba61-97ce5556ea42 · inbound

A possible high-redshift origin for the short GRB 061201: implications of a compact binary merger beyond cosmic noon cites this paper.

A possible high-redshift origin for the short GRB 061201: implications of a compact binary merger beyond cosmic noon Initial Populations of Black Holes in Star Clusters

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-07-03T19:48:53.384596Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c1121b1f5180d51800984e95fac6fe30d3b8dca8bd31eaa38456d89ebf423c9c