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Integrity report for The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars

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

arXiv:1808.07616 · pith:2018:MPCKTLTA6VXBGJ3YPADSBEKJ4O

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Paper page arXiv integrity.json bundle.json

Detector runs

Findings

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Signed record

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