Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The role of currents distribution in general relativistic equilibria of magnetized neutron stars
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1412.5347.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T11:12:36.339622Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-09T04:41:38.110925Z
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 8d246b00-95e7-4022-9a71-a8bd9853969e · inbound
General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars cites this paper.
General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars The role of currents distribution in general relativistic equilibria of magnetized neutron stars
Reference 25
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T20:21:07.840025Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 26b466bb-7112-4edf-8be7-49f214290e34 · inbound
Rotating neutron stars: anisotropy model comparison cites this paper.
Rotating neutron stars: anisotropy model comparison The role of currents distribution in general relativistic equilibria of magnetized neutron stars
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T11:12:36.339622Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.