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Paper Citation Record · LEDGER

The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2409.18096.

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

pith.paper-citation-record.v1
2409.18096 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T19:45:42.540266Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T09:21:21.261575Z

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 0ce19d33-8e16-4174-ac8a-2bf23050f699 · inbound

The GHOSDT Simulations (Galaxy Hydrodynamical Simulations with Supernova-Driven Turbulence) -- I. Magnetic Support in Gas Rich Disks cites this paper.

The GHOSDT Simulations (Galaxy Hydrodynamical Simulations with Supernova-Driven Turbulence) -- I. Magnetic Support in Gas Rich Disks The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-12T19:45:42.540266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T19:45:42.540266Z digest=sha256:924a92b62ee31a25deb1f65fd09164dbd6846391a3c45207019c286fd395820e

Observation 3662f620-0909-486c-b9fa-3961e793cf3c · inbound

Supermassive black hole growth in hierarchically merging nuclear star clusters cites this paper.

Supermassive black hole growth in hierarchically merging nuclear star clusters The importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-11T11:36:57.031972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T11:36:57.031972Z digest=sha256:696223ce4885122ee06511841a062dec43feb217b040ff63e26145fb7582b6c1

Observation 9afa93b0-4339-43e7-ac60-dd9bd19ad501 · 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 importance of nuclear star clusters for massive black hole growth and nuclear star formation in simulated low-mass galaxies

Reference 58

Resolution
verified exact
arxiv_id, observed 2026-05-22T09:21:21.263960Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-22T09:20:09.976842Z digest=sha256:6d4abb1a1a4f49810f3dc44fac0ea9889b15887e85129a05b2e8df8de19f96b2