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Integrity report for Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties

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

arXiv:2605.18062 · pith:2026:HRGBTORPPV6AMMKYE56EDLVR2N

0Critical
0Advisory
9Detectors run
2026-06-02Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

ai_meta_artifact completed v1.0.0 · findings 0 · 2026-06-02 00:43:03.260741+00:00
doi_compliance completed v1.0.0 · findings 0 · 2026-05-26 01:38:37.219972+00:00
doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-26 01:32:51.836822+00:00
claim_evidence completed v1.0.0 · findings 0 · 2026-05-25 23:03:56.576055+00:00
cited_work_retraction completed v1.0.0 · findings 0 · 2026-05-23 03:24:08.805371+00:00
doi_compliance completed v1.0.0 · findings 0 · 2026-05-20 01:04:37.346227+00:00
doi_title_agreement completed v1.0.0 · findings 0 · 2026-05-20 01:01:20.731345+00:00
claim_evidence completed v1.0.0 · findings 0 · 2026-05-19 23:41:59.265935+00:00
ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-05-19 23:33:35.473183+00:00

Findings

No public integrity findings for this paper.

Signed record

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