Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational waves from f-modes excited by the inspiral of highly eccentric neutron star binaries
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1612.07097.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T11:52:48.381305Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T16:33:20.839264Z
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 81c23edd-2597-4d64-b61b-8550b5304e31 · inbound
CP violation in cold dense quark matter and axion effects on the non-radial oscillations of neutron stars cites this paper.
CP violation in cold dense quark matter and axion effects on the non-radial oscillations of neutron stars Gravitational waves from f-modes excited by the inspiral of highly eccentric neutron star binaries
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T11:52:48.381305Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d39140a2-f9d9-4dac-8b98-9b7ffd75ea7e · 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 Gravitational waves from f-modes excited by the inspiral of highly eccentric neutron star binaries
Reference 117
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T16:33:20.846031Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.