Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
How black holes shape globular clusters: Modeling NGC 3201
As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1802.09553.
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 2026-07-20T06:30:07.809122+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T06:51:42.465920Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-11T06:57:50.587913Z
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 173e6849-6360-4c8c-9390-f76f4b8e8813 · inbound
Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.
Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins How black holes shape globular clusters: Modeling NGC 3201
Reference 59
- Resolution
- verified exact
- local_arxiv, observed 2026-07-11T06:57:50.589968Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-20T06:30:07.809122+00:00.