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From the 2 of 5 linked papers with an AI index.

activity
20242026
collaborators

5 papers

astro-ph.GA2026

The Three Hundred project: Low Gas Fraction Galaxy Clusters properties and their environment

Francesco Guidi, Marco De Petris, Sara Santoni +7

Galaxy cluster samples based on X-ray and Sunyaev-Zel'dovich (SZ) observations are affected by selection biases. These catalogs preferentially include systems with high gas content…

astro-ph.CO2026

Here, There and Everywhere: How AGN jets affect galaxy cluster environments

Isaac Rosenberg, Martine Lokken, Renée Hložek +3

The paper uses zoom‑in hydrodynamic simulations of galaxy clusters to test how AGN jet properties (velocity, orientation, coupling) affect the thermal state of surrounding gas and…

astro-ph.CO2026

The Three Hundred project: cosmic web identification from 2D gas and Compton- maps of galaxy clusters outskirts

Sara Santoni, Marco De Petris, Gustavo Yepes +4

Galaxy clusters are located at the nodes of the filamentary network known as the cosmic web. A more comprehensive understanding of galaxy clusters can be achieved by considering th…

astro-ph.CO2025

The Atacama Cosmology Telescope: A census of bridges between galaxy clusters

G. Isopi, V. Capalbo, A. D. Hincks +27

According to CMB measurements, baryonic matter constitutes about of the mass-energy density of the universe. A significant population of these baryons, for a long time referr…

astro-ph.CO2024

The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters

Sara Santoni, Marco De Petris, Gustavo Yepes +7

Galaxy clusters are located in the densest areas of the universe and are intricately connected to larger structures through the filamentary network of the Cosmic Web. In this scena…