Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
GRMHD Simulations of Accreting Neutron Stars with Non-Dipole Fields
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2204.00249.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.168256Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T13:26:03.706770Z
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 099f57ed-8e24-49ad-9037-23959dee6fd2 · inbound
The swept-back multipolar magnetic field of neutron stars: Application to NICER MSP J0030+0451 cites this paper.
The swept-back multipolar magnetic field of neutron stars: Application to NICER MSP J0030+0451 GRMHD Simulations of Accreting Neutron Stars with Non-Dipole Fields
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T13:26:03.710646Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation b01aee57-3abe-472f-8148-7ec21491ee09 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry GRMHD Simulations of Accreting Neutron Stars with Non-Dipole Fields
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.168256Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.