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Paper Citation Record · LEDGER

Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0511394.

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

pith.paper-citation-record.v1
astro-ph/0511394 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:05:12.285490Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T04:16:49.417973Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • 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 1e90d72e-0e56-4ba5-8e6d-a5f6269fda57 · 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 Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-04T18:11:08.583058Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:11:08.583058Z digest=sha256:8853d08ff117e034430d7ff602c11ae98942f7bf47c5c694d5e468a0ae481ba6

Observation 6454e543-c18d-43f1-a7d9-4485b577bc80 · inbound

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

Structural quasi-universality in highly magnetized differentially rotating neutron stars Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-15T15:05:12.285490Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T15:05:12.285490Z digest=sha256:bf0230de379382f560c8ba4facfbf2b082fdd518d7a18a8fa50c1facc0860e43

Observation 79808bbf-294b-442e-b369-a78115d7b0c5 · inbound

On the nature of oscillating modes of proto-neutron stars cites this paper.

On the nature of oscillating modes of proto-neutron stars Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation

Reference 35

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:16:49.424285Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:16:46.506991Z digest=sha256:dfccdce57a6b6197bf29df2d15ee63f4a658aacea38b2b36f1badc17a2e82842