Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0503106.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T22:01:31.903279Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T05:30:13.102649Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 c51c221b-e7d0-4b45-8f39-1cbfc2337323 · inbound
Generating Moving Field Initial Conditions with Spatially Varying Boost cites this paper.
Generating Moving Field Initial Conditions with Spatially Varying Boost Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:01:31.903279Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6b10d174-c008-4f55-9c10-74f4b24dfcd0 · inbound
$\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations cites this paper.
$\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T05:30:13.152973Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.