Integrity report for A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz

A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.

arXiv:2605.23489 · pith:2026:H7KGWRJ5NYOWJUUGAWROR4TZUC

0Critical

0Advisory

5Detectors run

2026-05-25Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-25 08:55:18.641582+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-05-25 04:07:25.030340+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-25 04:02:39.056397+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-25 02:43:39.906662+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-25 02:35:19.322427+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/H7KGWRJ5/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.