activity
19952026
most citedGone with the wind: the origin of S0 galaxies in clusters

636 citations · 3.2k across the 60 of their papers we have counts for

collaborators

60 papers

astro-ph.GA2026

The impact of relativistic AGN jets on realistic galaxy cluster environments

K. Hervella-Seoane, M. Perucho, S. Planelles +2

Context. Low-power FRI-like radio jets dominate the AGN population, yet the main mechanism of heating the intracluster medium (ICM) and its efficiency remain a matter of debate. Ai…

astro-ph.IM2026

cosmokdtree: a flexible OpenMP-parallelized k-d tree for computational astrophysics applications

Óscar Monllor-Berbegal, David Vallés-Pérez, Susana Planelles +1

Modern numerical astrophysics applications present a common demand for efficient spatial querying techniques, such as neighbor searches or density estimations over billions of reso…

astro-ph.CO2025

The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM

David Vallés-Pérez, Susana Planelles, Vicent Quilis

Context. The internal structure of the intracluster medium (ICM) is tightly linked to the assembly history and physical processes in groups and clusters, but the role of recent acc…

astro-ph.CO2025

The signature of major mergers on the hydrostatic mass bias of galaxy clusters

Isac Barranco-Llorca, David Vallés-Pérez, Susana Planelles +1

While galaxy cluster masses are fundamental cosmological observables, estimates based on intra-cluster medium observations rely on hydrostatic equilibrium, introducing a systematic…

astro-ph.CO2025★ 1 cited

AVISM: Algorithm for Void Identification in coSMology

Óscar Monllor-Berbegal, David Vallés-Pérez, Susana Planelles +1

Cosmic voids are key elements in our understanding of the large-scale structure of the Universe. They are crucial to constrain cosmological parameters, understand the structure for…

astro-ph.CO2025★ 4 cited

The eventful life journey of galaxy clusters. I. Impact of DM halo and ICM properties on their full assembly histories

David Vallés-Pérez, Susana Planelles, Vicent Quilis

Context. Galaxy clusters assemble over gigayears in a very anisotropic environment, which causes a remarkable diversity in their mass assembly histories (MAH). Aims. In this work,…