Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The early evolution of young massive clusters: The kinematic history of NGC6611 / M16
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2207.08452.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.088428Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
20
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation d7fcb785-5b17-47af-9aeb-8830d1bd1ffa · inbound
Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors cites this paper.
Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors The early evolution of young massive clusters: The kinematic history of NGC6611 / M16
Reference 91
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T20:56:34.085018Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 0e00e7d7-fad5-4eab-85b1-c41bd8957642 · inbound
Runaway OB stars within 1 kpc of the Sun cites this paper.
Runaway OB stars within 1 kpc of the Sun The early evolution of young massive clusters: The kinematic history of NGC6611 / M16
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:38:04.066654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8149fdc5-9b07-483f-8f0b-068281a9ab27 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry The early evolution of young massive clusters: The kinematic history of NGC6611 / M16
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.088428Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.