Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Flux eruption events drive angular momentum transport in magnetically arrested accretion flows
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2210.08045.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:15:05.015008Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T17:13:13.539838Z
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 a59835c7-780c-41a7-9332-4da0479f55c2 · inbound
$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer cites this paper.
$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer Flux eruption events drive angular momentum transport in magnetically arrested accretion flows
Reference 123
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T17:13:13.545376Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 6febb46c-fbff-44d3-ac7a-4d97107f624f · inbound
The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 cites this paper.
The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Flux eruption events drive angular momentum transport in magnetically arrested accretion flows
Reference 105
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:15:05.015008Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.