Integrity report for How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function

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

arXiv:2605.26209 · pith:2026:HIZHYPMRW3FASTWE7BRXUUFEHC

0Critical

0Advisory

3Detectors run

2026-05-27Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-27 00:34:11.433698+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-27 00:24:17.535905+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-27 00:23:35.616794+00:00

Findings

No public integrity findings for this paper.

Signed record

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