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Integrity report for A New Method for the Assessment of Age and Age-Spread of Pre-Main Sequence Stars in Young Stellar Associations of the Magellanic Clouds

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

arXiv:1009.0006 · pith:2010:TE4LLVU72RI4PEYXNELB2CB26X

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Paper page arXiv integrity.json bundle.json

Detector runs

Findings

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Signed record

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