Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Numerical Simulations of Optically Thick Accretion onto a Black Hole - II. Rotating Flow
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1408.4460.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T17:12:21.132204Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-15T03:08:58.530567Z
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 068a68c1-229a-4a03-9bdf-a7de9651d532 · inbound
Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter cites this paper.
Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter Numerical Simulations of Optically Thick Accretion onto a Black Hole - II. Rotating Flow
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:12:21.132204Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 65251a11-2b27-436a-8d0b-9628fd469deb · inbound
Dispersion relations of relativistic radiation hydrodynamics cites this paper.
Dispersion relations of relativistic radiation hydrodynamics Numerical Simulations of Optically Thick Accretion onto a Black Hole - II. Rotating Flow
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T05:39:24.974460Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation af11ce0c-0075-4f5f-b73e-c6c84daf15aa · inbound
Polarization Signatures from GRMHD Simulations of Black Hole Accretion cites this paper.
Polarization Signatures from GRMHD Simulations of Black Hole Accretion Numerical Simulations of Optically Thick Accretion onto a Black Hole - II. Rotating Flow
Reference 99
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T03:08:58.533741Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.