Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Relativistic stars with purely toroidal magnetic fields
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0802.2983.
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 2026-08-04T18:11:05.129343Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-20T04:23:03.392291Z
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 0408d6a0-959a-4bf9-ada3-2d9ee66de730 · 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 Relativistic stars with purely toroidal magnetic fields
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T04:41:38.072379Z
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.
Observation 188cec01-69a2-4be6-a725-c539c52afb7c · inbound
Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field cites this paper.
Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field Relativistic stars with purely toroidal magnetic fields
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T18:11:05.129343Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d73b90aa-0483-4214-9218-926f2dd0e39e · inbound
Magnetized neutron stars: perturbative versus fully-numerical approaches cites this paper.
Magnetized neutron stars: perturbative versus fully-numerical approaches Relativistic stars with purely toroidal magnetic fields
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T04:23:03.396199Z
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.