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Paper Citation Record · LEDGER

Quasi-normal modes of rotating relativistic stars - neutral modes for realistic equations of state

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/9806008.

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

pith.paper-citation-record.v1
gr-qc/9806008 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:36:55.303200Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T18:36:55.818155Z

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 a094dc9f-e070-497f-b18c-f6e971a72a56 · inbound

Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? cites this paper.

Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? Quasi-normal modes of rotating relativistic stars - neutral modes for realistic equations of state

Reference 99

Resolution
verified exact
local_arxiv, observed 2026-08-11T18:36:55.822293Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-11T18:36:55.303200Z digest=sha256:700928b6c9ddded71c2a2703c0ccbc57d55cc856528a62381c6ad5086905d764

Observation 9e45c7eb-9fdf-4c16-8f57-604bb0ef4c56 · inbound

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement cites this paper.

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement Quasi-normal modes of rotating relativistic stars - neutral modes for realistic equations of state

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-03T17:54:37.597728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:54:37.597728Z digest=sha256:d7a46a7b782e0c358df52130dfd4ad733031df7cb617d859f76a588f7f668506