Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The black hole low mass X-ray binary V404 Cygni is part of a wide hierarchical triple, and formed without a kick
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2404.03719.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T14:12:23.717848Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T18:16:22.223912Z
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 0fdaa0a0-cb71-4641-8af3-f658283842ed · inbound
Triple Evolution Pathways to Black Hole Low-Mass X-ray Binaries: Insights from V404 Cygni cites this paper.
Triple Evolution Pathways to Black Hole Low-Mass X-ray Binaries: Insights from V404 Cygni The black hole low mass X-ray binary V404 Cygni is part of a wide hierarchical triple, and formed without a kick
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:12:23.717848Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a182c9ef-2460-48e1-923b-2d923950c9e1 · inbound
Mixed origins: strong natal kicks for some black holes and none for others cites this paper.
Mixed origins: strong natal kicks for some black holes and none for others The black hole low mass X-ray binary V404 Cygni is part of a wide hierarchical triple, and formed without a kick
Reference 14
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-12T13:03:37.891732Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation fe3390e0-536e-4e48-8ff2-1fb263a0a6ca · inbound
A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters cites this paper.
A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters The black hole low mass X-ray binary V404 Cygni is part of a wide hierarchical triple, and formed without a kick
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T13:41:03.177542Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.