Paper Citation Record · LEDGER

Gravitational waves from axisymmetrically oscillating neutron stars in general relativistic simulations

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0402184.

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

pith.paper-citation-record.v1
astro-ph/0402184 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 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T05:33:07.933338Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-09T00:07:30.044223Z

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 6566b515-a840-436b-94df-58a311b3b79d · inbound

SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement cites this paper.

SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement Gravitational waves from axisymmetrically oscillating neutron stars in general relativistic simulations

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-09T05:33:07.933338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1bd28a8f-1cf3-461b-802c-94903a0e89d6 · 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 Gravitational waves from axisymmetrically oscillating neutron stars in general relativistic simulations

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-08-09T00:07:30.049459Z

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.