Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star
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/9704023.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T13:02:27.219999Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-20T08:53:09.623957Z
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 46492e47-bf5c-46bb-b668-64f18aa85573 · inbound
Perturbations of relativistic dissipative stars cites this paper.
Perturbations of relativistic dissipative stars Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:02:27.219999Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5d179eb5-6165-4fc7-905b-b2d3e002277b · inbound
Ringdown Signatures of Dehnen Dark Matter Halos: Fluid Modes and Detectability with Space-Based Detectors cites this paper.
Ringdown Signatures of Dehnen Dark Matter Halos: Fluid Modes and Detectability with Space-Based Detectors Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star
Reference 66
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:53:09.625540Z
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.
Observation 021d9955-2e66-4189-9f1d-f1cca065cdef · inbound
Quasi-Normal Modes of Stars and Black Holes cites this paper.
Quasi-Normal Modes of Stars and Black Holes Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star
Reference 5
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T02:26:20.342613Z
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.