Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1509.06975.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T16:33:19.844614Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T15:07:19.539771Z
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 2565f0e0-2f87-4eb6-b47d-3b2108097e8b · 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 Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T16:33:19.844614Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 23262401-c3cb-444b-918e-f7a0131c7f24 · inbound
Love numbers of black holes and compact objects cites this paper.
Love numbers of black holes and compact objects Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars
Reference 96
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T20:53:26.410752Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 331664e0-c73a-4e4f-ad68-e2f58f514744 · 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 Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T15:07:19.540988Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.