Paper Integrity Record · LEDGER
Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:0910.4529. No listed check completed, so this record makes no findings claim.
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Coverage vector
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Listed checks
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Observations
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Methods and limits
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