Speaker
Description
The Cluster HEritage project with XMM-Newton – Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) provides a comprehensive dataset of 118 galaxy clusters, offering insights into their morphology within a volume-limited and mass-limited sample of the universe. In this work, we introduce a three-dimensional modeling framework CLUMP-3D that integrates multiwavelength observations to analyze the matter distribution in CHEX-MATE clusters. We focus on a triaxial analysis of the intracluster medium by combining X-ray observations, Planck-derived Sunyaev–Zel’dovich effect data, and complementary ground-based measurements. We apply our method to the CHEX-MATE DR1 sample as an initial step toward a full survey analysis, examining the distribution of geometric parameters such as gas axial ratios and elongation. A companion study that incorporates lensing data to characterize the dark matter distribution will be presented by Gavidia at this conference.
| Would you be interested in presenting a poster if the conference is oversubcribed? | Yes |
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