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An improved approach to measuringH0using X-ray and SZ observations of galaxy clusters

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XMM-Newtonobservation of the relaxed cluster A478: Gas and dark matter distribution from 0.01R$_\mathsf{200}$ to 0.5R$\mathsf{_{200}}$

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Models of the Intracluster Medium with Heating and Cooling: Explaining the Global and Structural X‐Ray Properties of Clusters

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A Systematic Study of Radio‐induced X‐Ray Cavities in Clusters, Groups, and Galaxies

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