Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2001.11470.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:58:53.845940Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-15T15:58:54.510062Z
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 4dc8d8e7-46ac-4992-8a02-67f91e42c1fa · inbound
Testing the nature of compact objects in the lower mass gap using gravitational wave observations cites this paper.
Testing the nature of compact objects in the lower mass gap using gravitational wave observations Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
Reference 88
- Resolution
- verified exact
- local_arxiv, observed 2026-08-15T15:58:54.533777Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.