Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1909.01934.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T00:25:52.772479Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T00:25:56.003187Z
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 110b5e14-b0f0-4432-90f9-0285e438f1bb · inbound
Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge cites this paper.
Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T00:25:56.049619Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.