Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Necessary Condition for Individual Time-Steps in SPH Simulations
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0808.0773.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:40.435004Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 f5b01af4-2c18-4fae-9107-d92ff7586b05 · inbound
Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds cites this paper.
Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds A Necessary Condition for Individual Time-Steps in SPH Simulations
Reference 223
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:21:15.541076Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c67a461f-7075-4fe4-b400-2fc5b015018f · 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 A Necessary Condition for Individual Time-Steps in SPH Simulations
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T03:50:02.982790Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b3d9bf18-93ad-465d-b8e4-149e8a3b2cc3 · inbound
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation A Necessary Condition for Individual Time-Steps in SPH Simulations
Reference 176
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T17:19:40.435004Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.