Paper Citation Record · LEDGER

The importance of black hole repositioning for galaxy formation simulations

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2109.01489.

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

pith.paper-citation-record.v1
2109.01489 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:15:55.559533Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 81febc7e-6a44-4fcc-a0d5-a5d89694aa48 · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies The importance of black hole repositioning for galaxy formation simulations

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-06T18:15:55.559533Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a37c197b-d605-4b61-aa9a-4817bfb65ace · 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 importance of black hole repositioning for galaxy formation simulations

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-02T03:50:09.824188Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7cf1e54-2b66-46e7-ace1-1776b7eb8d33 · inbound

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations The importance of black hole repositioning for galaxy formation simulations

Reference 270

Resolution: unresolved; no resolver link, observed 2026-08-02T00:50:15.931264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 759f1e79-6ca7-414c-af9e-20fcbb5bc24a · inbound

Cosmological simulations of the high-redshift galaxy population adopting a variable stellar initial mass function cites this paper.

Cosmological simulations of the high-redshift galaxy population adopting a variable stellar initial mass function The importance of black hole repositioning for galaxy formation simulations

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T21:06:33.979649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.