Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T18:10:44.019889Z
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
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+00:00.