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Paper Citation Record · LEDGER

The time-scale for core collapse in spherical star clusters

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9606182.

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

pith.paper-citation-record.v1
astro-ph/9606182 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T03:50:00.616835Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T13:26:07.766988Z

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 f462fae1-9212-4954-9c17-bbc8139c594a · inbound

Merger rate of initially clustered primordial black holes for the two-body channel cites this paper.

Merger rate of initially clustered primordial black holes for the two-body channel The time-scale for core collapse in spherical star clusters

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:00:10.507800Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-10T01:37:57.266623Z digest=sha256:ba03a8e18abc1ad89f98cfadf45bd4c1c392a40bc32c249cecae3edde9b9c078

Observation 0e927896-ad98-4c7e-b977-052eb0df9a0f · inbound

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime The time-scale for core collapse in spherical star clusters

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-02T03:50:00.616835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:50:00.616835Z digest=sha256:cd899cce04e34adcea9ad13383d9bab22b9e3302db2902ee4208dbc802cf5128