activity
20242026
collaborators

5 papers

astro-ph.GA2026

FASTAR -- II. Semi-resolved evolutionary stellar population models

Ignacio Martín-Navarro, Alexandre Vazdekis, Luis Peralta de Arriba +12

Standard evolutionary synthesis models rely on the assumption of a fully sampled stellar initial mass function (IMF). Under this assumption, the age, chemical composition, and IMF…

astro-ph.GA2026

FASTAR -- I. Continuous and differentiable evolutionary stellar population models

Ignacio Martín-Navarro, Alexandre Vazdekis, Luis Peralta de Arriba +11

The development of evolutionary stellar population models is central to interpreting observations of galaxies in terms of astrophysical quantities. Stellar population models must t…

astro-ph.CO2025

The origin of the intra-cluster light in The Three Hundred simulations

A. Contreras-Santos, A. Knebe, W. Cui +9

We investigate the origin and formation mechanisms of the intra-cluster light (ICL) in The Three Hundred simulations, a set of 324 hydrodynamically resimulated massive galaxy clust…

astro-ph.GA2025

The intracluster light as an estimator of the cluster mass profile

Isaac Alonso Asensio, Ana Contreras-Santos

Context. The intracluster light (ICL) comprises stars that are not bound to individual galaxies within a galaxy cluster, and it provides insights into the cluster mass distribution…

astro-ph.GA2024

On the detection of stellar wakes in the Milky Way: a deep learning approach

Sven Põder, Joosep Pata, María Benito +2

Due to poor observational constraints on the low-mass end of the subhalo mass function, the detection of dark matter (DM) subhalos on sub-galactic scales would provide valuable inf…