Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Why is the Galactic disk so cool?
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2411.08944.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T11:45:12.685568Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 56024316-251b-404f-8a35-944cf4b8c698 · inbound
Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar cites this paper.
Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar Why is the Galactic disk so cool?
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T11:45:12.685568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8e16285b-1202-4396-a3de-499f1b2d5766 · inbound
Nexae in caverna: the secular evolution of disks via collectively excited, transient spiral structure cites this paper.
Nexae in caverna: the secular evolution of disks via collectively excited, transient spiral structure Why is the Galactic disk so cool?
Reference 28
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-10T23:05:48.411813Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 61f6f296-1411-47e0-a4d6-02af6876a8b2 · inbound
Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration cites this paper.
Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration Why is the Galactic disk so cool?
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T09:36:20.804103Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.