Integrity report for Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations

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

arXiv:2606.05808 · pith:2026:2SAB6GYQJ5WC2M56R7NZUG7LC3

0Critical

0Advisory

4Detectors run

2026-06-05Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

citation_quote_validity skipped v0.1.0 · findings 0 · 2026-06-05 17:51:16.759245+00:00

cited_work_retraction completed v1.0.0 · findings 0 · 2026-06-05 12:27:48.676950+00:00

ai_meta_artifact skipped v1.0.0 · findings 0 · 2026-06-05 02:35:49.689972+00:00

claim_evidence completed v1.0.0 · findings 0 · 2026-06-05 02:29:13.645810+00:00

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/2SAB6GYQ/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.