Integrity report for Inferring stellar metallicity and elemental abundances from kinematic and spectroscopic data using machine learning -- Implications for exoplanet host stars

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

arXiv:2605.18131 · pith:2026:AI7UTK4DSW4WWDO5NY5I6YC2Q5

0Critical

0Advisory

4Detectors run

2026-05-20Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-20 01:01:20.654884+00:00

doi_compliance completed v1.0.0 · findings 0 · 2026-05-20 00:44:02.438106+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-05-19 23:41:59.126349+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-19 23:33:35.392406+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/AI7UTK4D/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.