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Paper Citation Record · LEDGER

Statistical properties of Galactic synchrotron temperature and polarization maps -- a multi-frequency comparison

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2212.06076.

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

pith.paper-citation-record.v1
2212.06076 v3

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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:49:47.311282Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T09:39:46.237621Z

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 99339b5f-749a-4b48-a69b-8ccb72cf2c75 · inbound

On the statistical nature of Betti numbers and Euler characteristic of smooth random fields cites this paper.

On the statistical nature of Betti numbers and Euler characteristic of smooth random fields Statistical properties of Galactic synchrotron temperature and polarization maps -- a multi-frequency comparison

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-06T19:49:47.311282Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T19:49:47.311282Z digest=sha256:aa0de4398a4cc84b930e8e650428ad9ed3ef1d7782eaf7c13d83f3e01e5299f3

Observation 6e56784f-3b53-4b05-af9c-e811c6d38933 · 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 Statistical properties of Galactic synchrotron temperature and polarization maps -- a multi-frequency comparison

Reference 51

Resolution
verified exact
arxiv_id, observed 2026-07-04T09:39:46.239197Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-26T09:46:24.839336Z digest=sha256:021fb4543faf0e9e6505af435d6e5c11bbd1f137ead3e39dd0956c5af430e798