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Integrity report for Dynamical Mass Constraints on Low-Mass Pre-Main-Sequence Stellar Evolutionary Tracks: An Eclipsing Binary in Orion with a 1.0 Msun Primary and an 0.7 Msun Secondary

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/0312575

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Paper page arXiv integrity.json

Detector runs

Findings

No public integrity findings for this paper.

Signed record

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