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Integrity report for The rate of cooling of the pulsating white dwarf star G117-B15A: a new asteroseismological inference of the axion mass

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

arXiv:1205.6180 · pith:2012:NRFQGXEQJHSCW6CRSMWV756SOG

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