On the dynamical and morphological state of the CHEX-MATE clusters

Abstract

The CHEX-MATE sample was built to provide an overview of the statistical properties of the underlying cluster population and to set the stage for future X-ray missions. In this work, we perform a morphological analysis of the 118 clusters included in the sample with the aim to provide a classification of their dynamical state which will be useful for future studies of the collaboration.

To appear in the Proceedings of the International Conference entitled 'mm Universe @ NIKA2', Rome (Italy), June 2021, EPJ Web of conferences

References in corpus (3)

• On the connection between giant radio halos and cluster mergers
• The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
• Searching for Cool Core Clusters at High redshift