Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational waves and pulsating stars: What can we learn from future observations?
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:gr-qc/9610035.
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 2026-08-11T14:29:01.316802Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-25T01:55:12.336442Z
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 33cd9358-43f9-4e0c-a527-00540d5188d8 · inbound
Phase transitions in neutron stars and their links to gravitational waves cites this paper.
Phase transitions in neutron stars and their links to gravitational waves Gravitational waves and pulsating stars: What can we learn from future observations?
Reference 250
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T01:55:12.339076Z
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 06e08b79-fffd-4a67-bbad-a1ff60d05555 · inbound
Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons cites this paper.
Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons Gravitational waves and pulsating stars: What can we learn from future observations?
Reference 108
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T14:29:01.316802Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 290cb1d8-30ef-4204-8864-f9d8a2642ebd · inbound
Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model cites this paper.
Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model Gravitational waves and pulsating stars: What can we learn from future observations?
Reference 131
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T11:42:10.949799Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0a0fc47d-2589-4105-bc89-18da4155a7e9 · 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 and pulsating stars: What can we learn from future observations?
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:53:09.602150Z
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 ac18eb3b-9c16-4c19-b7e1-fe6da7dd577b · inbound
Quasi-Normal Modes of Stars and Black Holes cites this paper.
Quasi-Normal Modes of Stars and Black Holes Gravitational waves and pulsating stars: What can we learn from future observations?
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T02:26:20.173507Z
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.