Integrity report for A Weak Fe Kβ Emission Line in the Broad-Line Radio Galaxy 3C 111 Observed with XRISM: An Ionized Wind Absorption Feature?

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

arXiv:2605.22388 · pith:2026:3YUV34WQGPKYB6AMNJBNVQZSWO

0Critical

0Advisory

7Detectors run

2026-05-25Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

doi_compliance completed v1.0.0 · findings 0 · 2026-05-25 04:21:31.262519+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-25 04:02:39.592823+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-25 01:43:39.105081+00:00

citation_quote_validity completed v0.1.0 · findings 0 · 2026-05-24 15:50:53.540754+00:00

shingle_duplication completed v0.1.0 · findings 0 · 2026-05-23 09:51:03.825164+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-22 08:24:37.394609+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-22 01:33:42.666357+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/3YUV34WQ/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.