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Paper Citation Record · LEDGER

Relativistic stars with purely toroidal magnetic fields with realistic equations of state

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0904.2044.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
0904.2044 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T18:11:05.237462Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-09T04:41:38.074155Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 1e8bb544-0062-47de-ae81-d6c4fd16413f · 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 with realistic equations of state

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-07-04T18:11:36.376019Z

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.

source=pdf_text observed=2026-05-23T20:56:06.983493Z digest=sha256:d932aa8dba13b91e45967abfab1ad30e9ade14e7052aafba494a41bd55e5b729

Observation 6fa37775-3d55-4256-9785-187f4b3d992f · 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 with realistic equations of state

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-04T18:11:05.237462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:11:05.237462Z digest=sha256:6b954c69ce89d74de0e4277b4b3f8fcb2ed42e0a57bf683f0928e8901284ca92