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Integrity report for New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars

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

arXiv:1807.09365 · pith:2018:LYPNJ3ZTNTQJXVGT43CCKPITAK

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Paper page arXiv integrity.json bundle.json

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Signed record

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