Integrity report for Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN

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

arXiv:1211.1021 · pith:2012:XM5HWAYH6X7WQJ43LRRJS3RGBK

0Critical

0Advisory

0Detectors run

—Last checked

Paper page arXiv integrity.json bundle.json

Detector runs

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/XM5HWAYH6X7WQJ43LRRJS3RGBK/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.