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Integrity report for Studies of the Origin of High-Frequency Quasi-Periodic Oscillations of Mass Accreting Black Holes in X-ray Binaries with Next-Generation X-ray Telescopes

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

arXiv:1605.09756 · pith:2016:KA7B7UWLKQRY4N3OTPGDR6Q762

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Paper page arXiv integrity.json bundle.json

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Signed record

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