collaborators

5 papers

astro-ph.CO2026

CHEX-MATE: Relationship between X-ray and millimetre inferences of galaxy cluster temperature profiles

F. De Luca, H. Bourdin, P. Mazzotta +25

Thermodynamic profiles from X-ray and millimetre observations of galaxy clusters are often compared under the simplifying assumptions of smooth, spherically symmetric intracluster…

astro-ph.CO2025

CHEX-MATE: towards a consistent universal pressure profile and cluster mass reconstruction

M. Muñoz-Echeverría, E. Pointecouteau, G. W. Pratt +31

In a self-similar paradigm of structure formation, the thermal pressure of the hot intra-cluster gas follows a universal distribution once the profile of each cluster is normalised…

astro-ph.CO2025

CHEX-MATE: exploring the kinematical properties of Planck galaxy clusters

Lorenzo Pizzuti, Rafael Barrena, Mauro Sereno +19

We analyse the kinematical properties of the CHEX-MATE (Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation) galaxy c…

astro-ph.CO2025

CHEX-MATE: Multi-probe analysis of Abell 1689

L. Chappuis, D. Eckert, M. Sereno +25

The nature of the elusive dark matter can be probed by comparing the predictions of the cold dark matter framework with the gravitational field of massive galaxy clusters. However,…

astro-ph.CO2025

CHEX-MATE: Scaling relations of radio halo profiles for clusters in the LoTSS DR2 area

M. Balboni, S. Ettori, F. Gastaldello +21

The thermal and non-thermal components in galaxy clusters have properties that, although shaped from different physical phenomena, can share some similarities, mainly driven by the…