Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dynamical properties of magnetized low angular momentum accretion flow around a Kerr black hole
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2403.18359.
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 2026-08-07T11:45:03.769217Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T11:46:57.945898Z
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 1c37c631-2897-44f3-9938-df9b684786e1 · inbound
A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes cites this paper.
A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes Dynamical properties of magnetized low angular momentum accretion flow around a Kerr black hole
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T11:46:57.970880Z
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.
Observation daa60124-5c5c-4e31-859f-9cb935cc93d7 · inbound
Hamiltonian variational reconstruction of the 3D magnetic geometry of relativistic jets: accuracy across GRMHD models and the fundamental sign degeneracy cites this paper.
Hamiltonian variational reconstruction of the 3D magnetic geometry of relativistic jets: accuracy across GRMHD models and the fundamental sign degeneracy Dynamical properties of magnetized low angular momentum accretion flow around a Kerr black hole
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T02:05:12.200287Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.