Integrity report for Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Paβ narrow-band imaging

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

arXiv:2605.20590 · pith:2026:3V6PSKKR7F4J6PJBKKR543QN2D

0Critical

0Advisory

6Detectors run

2026-05-31Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-31 17:04:34.282573+00:00

ai_meta_artifact completed v1.0.0 · findings 0 · 2026-05-28 05:38:32.735086+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-26 14:24:09.583488+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-05-26 07:35:10.106346+00:00

citation_quote_validity completed v0.1.0 · findings 0 · 2026-05-21 23:50:07.049213+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-21 16:00:56.418604+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/3V6PSKKR7F4J6PJBKKR543QN2D/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.