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Integrity report for X-ray Emission Line Profile Modeling of O stars: Fitting a Spherically-Symmetric Analytic Wind-Shock Model to the Chandra Spectrum of zeta Puppis

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

arXiv:astro-ph/0211550 · pith:2002:5NZC7F4TRQKSJDZ7MGK6M6DJ2H

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Paper page arXiv integrity.json bundle.json

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Signed record

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