activity
20012026
most citedThe Density Profiles of Massive, Relaxed Galaxy Clusters. I. The Total Density Over Three Decades in Radius

281 citations · 3.9k across the 104 of their papers we have counts for

collaborators

106 papers

astro-ph.GA2026

Euclid Quick Data Release (Q1). Exploring the complexity of quenching processes across time, environment, and mass through recently quenched galaxies

Euclid Collaboration, Z. Mao, L. Pozzetti +308

Recently quenched galaxies (RQGs) provide insights into galaxy quenching. We present a photometric and spectroscopic analysis of RQGs using the first Euclid Quick Data Release (Q1)…

astro-ph.CO2026

Monitoring the power spectrum of magnetic field fluctuations across the simulated intracluster medium

T. Bartalesi, F. Vazza, S. Ettori +2

Thanks to the current and forthcoming radio interferometers, Faraday rotation measure maps extend out to the outskirts of galaxy clusters. Interpreted through models of the magneti…

astro-ph.GA2025

The collar of early-type galaxies -- probing evolution by focusing on the inner stellar density profile

Rongfu Liu, Alessandro Sonnenfeld, Carlo Nipoti +1

Aims: In this work we aim to investigate the late evolution of ETGs, both observationally and theoretically, by focusing on the stellar mass density profile inside a fixed aperture…

astro-ph.GA2025

TDCOSMO XXI. Accurate stellar velocity dispersions of the SL2S lens sample and the fundamental plane of the lensing mass

Pritom Mozumdar, Shawn Knabel, Tommaso Treu +4

We reanalyzed spectra that were taken as part of the SL2S lens galaxy survey with the goal to obtain the stellar velocity dispersion with a precision and accuracy sufficient for ti…

astro-ph.CO2025★ 2 cited

Searching for rotation in X-COP galaxy clusters

Tommaso Bartalesi, Stefano Ettori, Carlo Nipoti

We search for evidence of rotational support by analyzing the thermodynamic profiles of the intracluster medium (ICM) in a sample of nearby, massive galaxy clusters. For each objec…

astro-ph.CO2023★ 2 cited

Gas rotation and dark matter halo shape in cool-core clusters of galaxies

Tommaso Bartalesi, Stefano Ettori, Carlo Nipoti

Aims. We study the possibility that the gas in cool-core clusters of galaxies has non-negligible rotation support, the impact of gas rotation on mass estimates from current X-ray o…