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Paper Citation Record · LEDGER

A NEW NUMERICAL APPROACH TO THE OSCILLATION MODES OF RELATIVISTIC STARS

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:gr-qc/9503014.

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

pith.paper-citation-record.v1
gr-qc/9503014 v1

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 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T12:14:18.710525Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-16T08:17:36.418932Z

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 1c04fe5a-209d-4106-abaa-75c3cc7e97c5 · inbound

Combining simulation-based inference and universal relations for precise and accurate neutron star science cites this paper.

Combining simulation-based inference and universal relations for precise and accurate neutron star science A NEW NUMERICAL APPROACH TO THE OSCILLATION MODES OF RELATIVISTIC STARS

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-03T12:14:18.710525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T12:14:18.710525Z digest=sha256:0735b7d255cf4ca0db6c5b359bf1c8886e261ab92ad5fd865af1b26045996df9

Observation 68c297a4-159c-4104-974d-f070cb49631b · inbound

Radial Oscillations of Neutron Stars with Vector-Induced Scalar Hair cites this paper.

Radial Oscillations of Neutron Stars with Vector-Induced Scalar Hair A NEW NUMERICAL APPROACH TO THE OSCILLATION MODES OF RELATIVISTIC STARS

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-05-16T08:17:36.420759Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-16T08:15:27.979441Z digest=sha256:aad1dd10bcfd20dff34dea44f10fec6eefa750cd7f4c45ba4f6895969e167328

Observation 441c1cfc-b6ca-4fa8-b017-5698b4311c2b · inbound

Quasi-Normal Modes of Stars and Black Holes cites this paper.

Quasi-Normal Modes of Stars and Black Holes A NEW NUMERICAL APPROACH TO THE OSCILLATION MODES OF RELATIVISTIC STARS

Reference 21

Resolution
verified exact
arxiv_id, observed 2026-05-13T02:26:20.236998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-13T02:26:20.097934Z digest=sha256:b86510ca3d89edcd18c7613292769c0b7c73ab0db6cdc5e81c1f5509ad68a1c0