Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Star Clusters, Self-Interacting Dark Matter Halos and Black Hole Cusps: The Fluid Conduction Model and its Extension to General Relativity
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1809.02618.
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 2026-08-07T14:41:49.515187Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-16T11:37:48.822145Z
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 d4fdf9c1-debe-4b5c-9ed4-0583cf0131c2 · inbound
Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations cites this paper.
Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations Star Clusters, Self-Interacting Dark Matter Halos and Black Hole Cusps: The Fluid Conduction Model and its Extension to General Relativity
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:41:49.515187Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1096e802-e960-4b7d-8e5d-0926fbec3e75 · inbound
Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass cites this paper.
Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass Star Clusters, Self-Interacting Dark Matter Halos and Black Hole Cusps: The Fluid Conduction Model and its Extension to General Relativity
Reference 112
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T11:37:48.823904Z
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.