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Integrity report for Boltzmann-Poisson-like approach to simulating the galactic halo response to satellite accretion Dependence on the halo density profile

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

arXiv:2205.11386 · pith:2022:RMBV2LNVGLD76FMHA7SNFRKJ6E

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Paper page arXiv integrity.json bundle.json

Detector runs

Findings

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Signed record

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