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Integrity report for Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

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/0406247 · pith:2004:C34XEIRNHWC7Q5FDXMUEA55DTC

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Paper page arXiv integrity.json bundle.json

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Signed record

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