Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Cosmic Web Dynamics: Forces and Strains
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.16489.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T22:04:38.344013Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 9318d6cb-be4d-40aa-8864-eed6504d955b · inbound
Observed Anti-parallel Correlation Between Spiral Galaxy and Cosmic Filament Spins cites this paper.
Observed Anti-parallel Correlation Between Spiral Galaxy and Cosmic Filament Spins Cosmic Web Dynamics: Forces and Strains
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:04:38.344013Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d3322bf-4a7e-4c76-8f91-45f9f1aa894b · inbound
The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection cites this paper.
The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Cosmic Web Dynamics: Forces and Strains
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:03:34.113495Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 321fdca9-4ff7-419c-a4b3-2a73db3fe728 · inbound
The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos cites this paper.
The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos Cosmic Web Dynamics: Forces and Strains
Reference 26
- Resolution
- verified exact
- arxiv_id, observed 2026-06-26T19:49:51.019479Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.