Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Minimally modeled characterization method of postmerger gravitational wave emission from binary neutron star coalescences
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2304.12831.
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 2026-08-04T06:34:03.388597+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 2026-06-30T14:54:45.290000Z
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 64f08d4a-6400-44f0-9fc3-2fe5ab777752 · inbound
Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors cites this paper.
Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors Minimally modeled characterization method of postmerger gravitational wave emission from binary neutron star coalescences
Reference 76
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T05:56:01.550519Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 8620fd4e-efc2-472a-83bd-44549e709bcd · 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 Minimally modeled characterization method of postmerger gravitational wave emission from binary neutron star coalescences
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T14:54:45.291199Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.