Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Fully Relativistic Simulations
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:astro-ph/0205091.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T05:33:08.024639Z
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 6b8ad74e-1285-42f9-a05f-f0b299bb8748 · inbound
SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement cites this paper.
SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Fully Relativistic Simulations
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T05:33:08.024639Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.