Paper Citation Record · LEDGER

Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1401.4308.

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

pith.paper-citation-record.v1
1401.4308 v2

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:05:12.296640Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-25T05:40:25.247621Z

Reference resolution

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External citation measurements

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Outbound references

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Pith citing papers

Observation 71281088-bbba-4557-86ea-2629d7f4d2fd · inbound

Rotating neutron stars with non-barotropic thermal profile cites this paper.

Rotating neutron stars with non-barotropic thermal profile Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-14T10:30:45.015921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9789cf4-dac2-4ab2-a720-d8af45cd05ac · 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 Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-09T04:41:38.107468Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation a69b1aeb-3a95-4284-98cc-3c9ec0c27db1 · inbound

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta cites this paper.

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-05T15:52:56.437203Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5d63dcd-2081-4b0a-8d64-17687fcba319 · 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 Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-04T18:11:07.251539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 812a3f5f-521d-4ade-9c00-1c3377b3604f · inbound

Spin effects in superfluidity, neutron matter and neutron stars cites this paper.

Spin effects in superfluidity, neutron matter and neutron stars Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-13T18:43:07.390591Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 58d9240c-52f5-4ab5-8196-a5c41f4855ec · inbound

Anisotropic hybrid stars: Interplay of superconductivity and magnetic field leading to gravitational waves cites this paper.

Anisotropic hybrid stars: Interplay of superconductivity and magnetic field leading to gravitational waves Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-10T23:45:49.920402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 1c728f73-ef53-426b-b89b-896cd1431556 · inbound

Magnetized neutron stars: perturbative versus fully-numerical approaches cites this paper.

Magnetized neutron stars: perturbative versus fully-numerical approaches Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-05-20T04:23:03.451044Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation e42da6c4-2e86-4691-84f0-37bd3c5d6895 · inbound

Magnetic field dynamics in isolated neutron stars with an external dipole field cites this paper.

Magnetic field dynamics in isolated neutron stars with an external dipole field Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-05-25T05:40:25.250258Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation a275d0aa-7fac-40e9-8629-c9f177e28eef · inbound

Magnetic field dynamics in isolated neutron stars with an external dipole field cites this paper.

Magnetic field dynamics in isolated neutron stars with an external dipole field Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 47

Resolution: unresolved; no resolver link, observed 2026-07-12T16:13:25.334553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53bc420e-ac9a-4f8d-9df9-9b9f847a8dde · inbound

Structural quasi-universality in highly magnetized differentially rotating neutron stars cites this paper.

Structural quasi-universality in highly magnetized differentially rotating neutron stars Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-15T15:05:12.296640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.