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Integrity report for The relation between accretion rates and the initial mass function in hydrodynamical simulations of star formation

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

arXiv:1312.3330 · pith:2013:HAGSC2JHOUZXHOXQG34XYB3A3R

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Paper page arXiv integrity.json bundle.json

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Signed record

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