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Integrity report for Star Formation in the First Galaxies - II: Clustered Star Formation and the Influence of Metal Line Cooling

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

arXiv:1307.1982 · pith:2013:QMPY7RR23AC6BV2K3ROUAZGJQ6

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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/QMPY7RR2/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.