Integrity report for Star formation at very low metallicity. II: On the insignificance of metal-line cooling during the early stages of gravitational collapse
A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.
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Paper page arXiv integrity.json
Detector runs
Findings
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Signed record
The machine-readable record for this paper lives at /pith/astro-ph/0511400/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.