activity
20202025
most citedCHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles

27 citations · 50 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2025★ 1 cited

CHEX-MATE: Cluster Multi-Probes in Three Dimensions (CLUMP-3D) II. Combined Gas and Dark Matter Analysis from X-ray, SZE, and WL

Adriana Gavidia, Junhan Kim, Jack Sayers +15

Under the standard model of hierarchical structure formation, the overall geometry of galaxy clusters is better described by a triaxial ellipse than a sphere. As a result, applying…

astro-ph.CO2025★ 4 cited

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.IM2025★ 1 cited

Euclid Quick Data Release (Q1): From images to multiwavelength catalogues: the Euclid MERge Processing Function

Euclid Collaboration, E. Romelli, M. Kümmel +345

The Euclid satellite is an ESA mission that was launched in July 2023. \Euclid is working in its regular observing mode with the target of observing an area of $14\,000~\text{deg}^…

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…

astro-ph.CO2025★ 3 cited

Radio emission from a massive node of the cosmic web. A discovery powered by machine learning

C. Stuardi, A. Botteon, M. Sereno +4

Aims. We aim to understand the nature of the diffuse radio emission surrounding the massive galaxy cluster PSZ2 G083.29-31.03, at z=0.412, already known to host a radio halo. Our i…

astro-ph.CO2024★ 7 cited

CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime

G. Riva, G. W. Pratt, M. Rossetti +26

We characterise the entropy profiles of 32 very high mass () galaxy clusters (HIGHMz), selected from the CHEX-MATE sample, to study the intracl…

astro-ph.CO2023★ 7 cited

CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles

A. Iqbal, G. W. Pratt, J. Bobin +21

Temperature profiles of the hot galaxy cluster intracluster medium (ICM) have a complex non-linear structure that traditional parametric modelling may fail to fully approximate. Fo…

astro-ph.CO2023★ 27 cited

CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles

I. Bartalucci, S. Molendi, E. Rasia +25

We investigate the statistical properties and the origin of the scatter within the spatially resolved surface brightness profiles of the CHEX-MATE sample, formed by 118 galaxy clus…

astro-ph.CO2020

The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview

MATE Collaboration, M. Arnaud, S. Ettori +66

The Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a three mega-second Multi-Year Heritage Progra…