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Paper Citation Record · LEDGER

Non Gaussian extrema counts for CMB maps

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1107.1863.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1107.1863 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:12:54.365680Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-04T09:39:46.351000Z

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 89b8f068-ccd7-4b2b-9c3e-b1d16b9c3cb5 · inbound

Stochastic Homology of Gaussian vs. non-Gaussian Random Fields: Graphs towards Betti Numbers and Persistence Diagrams cites this paper.

Stochastic Homology of Gaussian vs. non-Gaussian Random Fields: Graphs towards Betti Numbers and Persistence Diagrams Non Gaussian extrema counts for CMB maps

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-14T15:12:54.365680Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T15:12:54.365680Z digest=sha256:6647caedf2fb95dfba9647b641dccf9b33791c2944d2f40e79aae25a8df4d1c2

Observation 82920e69-b1f3-47f2-b247-32f1d9047006 · 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 extrema counts for CMB maps

Reference 35

Resolution
verified exact
local_arxiv, observed 2026-07-04T09:39:46.352438Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-26T09:46:24.839336Z digest=sha256:0b7c30dc3f6b367d225a5bdc3832ec6fb2e1a56e4f23c2be088ee2cf28395c0c