Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Non-Gaussian modelling and statistical denoising of Planck dust polarization full-sky maps using scattering transforms
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2207.12527.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T23:51:27.713520Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T09:39:46.312844Z
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 ab9cc4b0-090c-4843-b7a7-93c29f109a88 · inbound
Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements cites this paper.
Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements Non-Gaussian modelling and statistical denoising of Planck dust polarization full-sky maps using scattering transforms
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T23:51:27.713520Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 71abfea6-4875-413a-8b45-65a8238a172d · 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 Non-Gaussian modelling and statistical denoising of Planck dust polarization full-sky maps using scattering transforms
Reference 25
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T09:39:46.314181Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.