Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Minkowski Functionals of CMB polarisation intensity with Pynkowski: theory and application to Planck and future data
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2211.07562.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-26T09:46:24.839336Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T09:39:46.315339Z
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 ade840d6-80e2-41d8-b5c0-3be853cbb2e5 · inbound
BROOM: a python package for model-independent analysis of microwave astronomical data cites this paper.
BROOM: a python package for model-independent analysis of microwave astronomical data Minkowski Functionals of CMB polarisation intensity with Pynkowski: theory and application to Planck and future data
Reference 83
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T11:51:02.175688Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation d6ee9353-25c0-4a85-96b8-e18d3a700621 · 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 Minkowski Functionals of CMB polarisation intensity with Pynkowski: theory and application to Planck and future data
Reference 42
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T09:39:46.316739Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.