Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The stability of tidally deformed neutron stars to three- and four-mode coupling
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1307.2890.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:33:19.832270Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T15:07:19.537375Z
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 e463da04-b041-4fae-968b-43e8e5a64169 · inbound
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides cites this paper.
Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides The stability of tidally deformed neutron stars to three- and four-mode coupling
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:33:19.832270Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ff605523-4093-4c74-a83a-fb678980d230 · inbound
Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions cites this paper.
Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions The stability of tidally deformed neutron stars to three- and four-mode coupling
Reference 54
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T15:07:19.538581Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.