Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1905.01372.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T23:51:27.617375Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T09:39:46.334083Z
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 b672430c-7374-4c07-ae1d-b05521dc6045 · inbound
Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements cites this paper.
Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T23:51:27.617375Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9811742a-b2a9-4980-8fe9-44a07e8cb1ce · inbound
Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales cites this paper.
Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T09:39:46.335531Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.