Mass profiles of Galaxy Clusters from X-ray analysis
S. Ettori, A. Donnarumma, E. Pointecouteau, T.H. Reiprich, S. Giodini,, L. Lovisari, R.W. Schmidt
TL;DR
This paper reviews methods for determining galaxy cluster mass profiles using X-ray data, discussing their limitations, biases, and applications in cosmology.
Contribution
It provides a comprehensive overview of X-ray based mass profile reconstruction techniques and their potential as cosmological tools.
Findings
Identification of key biases in X-ray mass measurements
Discussion of limitations affecting mass profile accuracy
Insights into using mass profiles as cosmological proxies
Abstract
We review the methods adopted to reconstruct the mass profiles in X-ray luminous galaxy clusters. We discuss the limitations and the biases affecting these measurements and how these mass profiles can be used as cosmological proxies.
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