collaborators

10 papers

physics.soc-ph2026

Beyond persuasion: Mobile electoral interfaces in polarized societies

Nuno Crokidakis, Celia Anteneodo

Many traditional models of electoral dynamics emphasize opinion change, social influence and persuasion mechanisms. In contrast, contemporary polarized societies often exhibit rela…

astro-ph.CO2026

Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches

Théo Lebeau, Nabila Aghanim, Jenny Sorce +1

An accurate estimation of the mass of galaxy clusters is key to precisely and unbiasedly constraining cosmological parameters through their number count. The hydrostatic mass, esti…

astro-ph.CO2026

Gas motion in the intracluster medium of the Virgo cluster replica

Théo Lebeau, Stefano Ettori, Jenny G. Sorce +2

Within the deep gravitational potential of galaxy clusters lies the intracluster medium (ICM). At the first order, it is considered to be at hydrostatic equilibrium within the pote…

astro-ph.CO2026

Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation

Jade Pasté, Céline Gouin, Nabila Aghanim +1

Galaxy clusters grow through the matter accretion from the cosmic web, mainly along filaments. We aim to characterize the gas accretion onto clusters, focusing on the role of filam…

astro-ph.GA2026

Euclid preparation. Far-infrared predictions for Euclid galaxy catalogues: cluster, protocluster, and field

Euclid Collaboration, A. Parmar, D. L. Clements +297

The MAMBO mock galaxy catalogue, based on the Millennium Simulation with empirically assigned galaxy properties, provides predictions of FIR fluxes and physical parameters of Eucli…

astro-ph.CO2026

A high-dynamic-range view of the growth of structure and the warm/hot Universe

Luca Di Mascolo, Tony Mroczkowski, Joshiwa van Marrewijk +23

Baryons heat to temperatures above as they accrete onto massive overdensities -- galaxies, groups, clusters, and filaments -- where they ionize and become o…