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Integrity report for On the dust abundance gradients in late-type galaxies: II. Analytical models as evidence for massive interstellar dust growth in SINGS galaxies

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

arXiv:1201.3374 · pith:2012:7LFIMHN7PH7YIW2VRZCMO3IHRP

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