Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Evolution of neutron stars with toroidal magnetic fields: Axisymmetric simulation in full general relativity
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:0805.2712.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-05-23T20:56:06.983493Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-09T04:41:38.139615Z
Reference resolution
0 of 0 outbound references displayed
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- verified fuzzy0
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- 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 a6fe9a28-f91a-4470-9576-7ba6b2199a6f · 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 Evolution of neutron stars with toroidal magnetic fields: Axisymmetric simulation in full general relativity
Reference 30
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T15:34:07.498953Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.