Paper Citation Record · LEDGER

The optimal gravitational softening length for cosmological N-body simulations

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1810.07055.

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

pith.paper-citation-record.v1
1810.07055 v2

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 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:10:44.019889Z

measured 1 of 1 external citation measurements

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

Source: openalex, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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malformed identifier0
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External citation measurements

28
openalex, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4386462e-c5fd-43a6-8166-76a952b84379 · inbound

Darkness Visible: N-Body Simulations of Dark Matter Spikes in Hernquist Haloes cites this paper.

Darkness Visible: N-Body Simulations of Dark Matter Spikes in Hernquist Haloes The optimal gravitational softening length for cosmological N-body simulations

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T18:10:44.019889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0de289cb-d9f2-4104-8092-f24fe320ae53 · inbound

An essential building block for cosmological zoom-in perturbation theory cites this paper.

An essential building block for cosmological zoom-in perturbation theory The optimal gravitational softening length for cosmological N-body simulations

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-05-16T10:50:51.696415Z

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.

Observation de5feda0-e9a6-40c6-8998-d613b8fab281 · inbound

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization The optimal gravitational softening length for cosmological N-body simulations

Reference 220

Resolution: verified exact; local_arxiv, observed 2026-05-19T16:17:38.921437Z

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.

Observation 3546b134-19d4-4a2d-bacf-7f847518eac2 · inbound

Constructing a Mock Galaxy Catalog for the All-sky SPECtroscopic Survey of Nearby Galaxies (A-SPEC) Using the Machine-assisted Semi-Simulation Model cites this paper.

Constructing a Mock Galaxy Catalog for the All-sky SPECtroscopic Survey of Nearby Galaxies (A-SPEC) Using the Machine-assisted Semi-Simulation Model The optimal gravitational softening length for cosmological N-body simulations

Reference 134

Resolution: metadata mismatch; doi, observed 2026-07-09T22:56:37.412253Z

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.