Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1908.11418.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-30T14:53:42.242560Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T14:54:45.296655Z
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 1ef32caa-acba-4dc9-acd0-500a77f5ba10 · inbound
Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter cites this paper.
Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter
Reference 99
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T03:47:01.846512Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation e8d293b7-72b9-4bb6-b7fe-4e351badf856 · inbound
Inferring Neutron-Star Properties from Post-merger Gravitational-wave Spectra with Neural Networks cites this paper.
Inferring Neutron-Star Properties from Post-merger Gravitational-wave Spectra with Neural Networks kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter
Reference 65
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T14:54:45.297928Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.