Paper Citation Record · LEDGER

The runaway growth of intermediate-mass black holes in dense star clusters

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:astro-ph/0201055.

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

pith.paper-citation-record.v1
astro-ph/0201055 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:08:39.310899Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T17:57:14.610759Z

Reference resolution

0 of 0 outbound references displayed

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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 45e644e2-b826-40be-b381-e9128772c809 · inbound

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA cites this paper.

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA The runaway growth of intermediate-mass black holes in dense star clusters

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T21:08:39.310899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 19aa0424-ed63-4044-ab9b-98d8274a04b3 · inbound

The origin of the most recently ejected OB runaway star from the R136 cluster cites this paper.

The origin of the most recently ejected OB runaway star from the R136 cluster The runaway growth of intermediate-mass black holes in dense star clusters

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-06T17:10:49.002651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6b7ecd86-c2ae-4a1b-970b-cb0a45e87457 · inbound

Formation and Redshift Evolution of Dark Matter Spikes cites this paper.

Formation and Redshift Evolution of Dark Matter Spikes The runaway growth of intermediate-mass black holes in dense star clusters

Reference 61

Resolution: verified exact; arxiv_id, observed 2026-05-11T16:16:08.249092Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f9bf2587-b66e-447f-85bb-b30729c0c844 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning The runaway growth of intermediate-mass black holes in dense star clusters

Reference 118

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:21:20.786571Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 887264dd-9346-42e5-a1ad-a8bcc519d911 · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? The runaway growth of intermediate-mass black holes in dense star clusters

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.477278Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 7ae703ea-cfdd-4a2e-a622-2068907c4d48 · inbound

Too shy to spin? Cosmic wallflowers as proto-globular clusters cites this paper.

Too shy to spin? Cosmic wallflowers as proto-globular clusters The runaway growth of intermediate-mass black holes in dense star clusters

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-06-29T02:13:00.105050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 6865b778-55e2-4f3a-98ee-5e75944c1ded · 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 The runaway growth of intermediate-mass black holes in dense star clusters

Reference 2

Resolution: verified exact; local_arxiv, observed 2026-07-02T17:57:14.612355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f7b7db8b-f114-4a5b-b8d1-6938f1a511f7 · 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 The runaway growth of intermediate-mass black holes in dense star clusters

Reference 78

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f879d0a-5a41-4cc4-adf1-a783481d9082 · inbound

The gravitational-wave fingerprint of dynamically assembled primordial black hole cluster seeds in JWST's Little Red Dots cites this paper.

The gravitational-wave fingerprint of dynamically assembled primordial black hole cluster seeds in JWST's Little Red Dots The runaway growth of intermediate-mass black holes in dense star clusters

Reference 33

Resolution: unresolved; no resolver link, observed 2026-07-13T04:45:18.545506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6499ec1-753e-4685-82ee-18c7ed979840 · 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 The runaway growth of intermediate-mass black holes in dense star clusters

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:34.661338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.