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Paper Citation Record · LEDGER

Models of binary neutron star remnants with tabulated equations of state

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2104.13672.

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

pith.paper-citation-record.v1
2104.13672 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T00:07:29.675638Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T21:58:59.601845Z

Reference resolution

0 of 0 outbound references displayed

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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 52a0a28b-b6e9-4f5b-b016-92c1fa990802 · 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 Models of binary neutron star remnants with tabulated equations of state

Reference 69

Resolution
verified exact
arxiv_id, observed 2026-05-09T04:41:37.842941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-23T20:56:06.983493Z digest=sha256:9e7cb9055749e6f1e99032c23b2ade0421f30954ac7b396a04aca5f1040eb8d6

Observation eb2e1576-68fa-4517-8dbb-a2d3f389f25b · inbound

Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory cites this paper.

Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory Models of binary neutron star remnants with tabulated equations of state

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-09T00:07:29.675638Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T00:07:29.675638Z digest=sha256:e05fb43b9c792f7479e7443c961c9b967f4b3308acac41e24a9717e573796326

Observation 523e2769-75ec-4407-b654-13973ae6b40c · 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 Models of binary neutron star remnants with tabulated equations of state

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-04T18:11:12.479782Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:11:12.479782Z digest=sha256:b708491600d4c642eb11b9f1382d0944ed94a3f82b46f95c6228a6c450fca472

Observation 968ccab2-3893-4e96-a335-fabb3dec065a · inbound

Hybrid Stars with Post-Merger Rotation Profiles cites this paper.

Hybrid Stars with Post-Merger Rotation Profiles Models of binary neutron star remnants with tabulated equations of state

Reference 82

Resolution
verified exact
arxiv_id, observed 2026-07-03T21:58:59.603389Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-26T23:50:12.361235Z digest=sha256:1124c91b615005617b658dcc0d4cddd9e9806749a38d26fd2763c99a25643a60