Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Cosmological SPH simulations: A hybrid multi-phase model for star formation
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0206393.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T15:44:29.364916Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T15:44:32.943239Z
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 038aa66b-45b6-4245-b055-a83480c2bc26 · inbound
3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum cites this paper.
3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Cosmological SPH simulations: A hybrid multi-phase model for star formation
Reference 22
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T15:44:33.119284Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation b11752f2-7063-44f5-9b4e-c6ebddaa2025 · inbound
CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.
CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Cosmological SPH simulations: A hybrid multi-phase model for star formation
Reference 134
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:26:46.955787Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.