Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2408.04132.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T11:29:09.014284Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T18:16:22.223912Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 6a548d43-0e49-4d30-8c52-0317221b0412 · inbound
A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability
Reference 17
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 062937f1-615b-47d3-9089-7000b59949a8 · inbound
Polarimetric Signatures of Bulk Comptonization from within the Plunging Region of Accreting Black Holes The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability
Reference 6
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4578377b-9b48-4c58-8afd-22d260ae7041 · inbound
The Impact of Plasma Angular Momentum on Magnetically Arrested Flows and Relativistic Jets in Hot Accretion Flows Around Black Holes The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability
Reference 3
Source-reported events for the cited work
Unavailable: canonical work link unavailable.