Integrity report for Heavy element enrichment of gas in surface-accretion disks: A possible origin of the mass-metallicity anti-correlation in exoplanets

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

arXiv:2605.27289 · pith:2026:OCPCTYBHRLIFOX2C5H4UXKO2MH

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 05:45:10.070675+00:00

external_links completed v1.0.0 · findings 0 · 2026-05-27 17:31:50.591814+00:00

shingle_duplication skipped v0.1.0 · findings 0 · 2026-05-27 09:49:58.915548+00:00

citation_quote_validity skipped v0.1.0 · findings 0 · 2026-05-27 05:50:19.415558+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-27 03:23:36.267288+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-27 02:34:12.074615+00:00

Findings

No public integrity findings for this paper.

Signed record

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