Integrity report for The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback

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

arXiv:2605.28777 · pith:2026:HCGR5KWNPT645C4GYBLWHFRXPO

0Critical

0Advisory

6Detectors run

2026-05-29Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

claim_evidence completed v1.0.0 · findings 0 · 2026-05-29 03:25:06.675532+00:00

external_links completed v1.0.0 · findings 0 · 2026-05-28 17:31:44.793681+00:00

shingle_duplication skipped v0.1.0 · findings 0 · 2026-05-28 05:49:59.600404+00:00

citation_quote_validity skipped v0.1.0 · findings 0 · 2026-05-28 03:50:24.325323+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-28 02:53:49.394801+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-28 02:34:18.900778+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/HCGR5KWN/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.