Integrity report for COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12

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

arXiv:2605.19661 · pith:2026:A2MODIRDIMZHVXCCN52JJOCLWN

2Critical

0Advisory

10Detectors run

2026-05-28Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

ai_meta_artifact completed v1.0.0 · findings 0 · 2026-05-28 14:36:18.396532+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-28 01:03:24.874823+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-05-26 02:39:16.393744+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-26 00:43:56.998274+00:00

citation_quote_validity completed v0.1.0 · findings 0 · 2026-05-20 13:50:11.049001+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-20 09:53:55.600958+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-05-20 04:07:54.782303+00:00

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-20 04:01:21.964684+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-20 01:41:59.486900+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-20 01:33:29.538052+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/A2MODIRDIMZHVXCCN52JJOCLWN/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.