Research

We developed methods to determine chemical composition in stars. ERIS attributes the chemical abundances imprinted

This research line aimed to use computational simulations of galaxy evolution (such as CIELO and L-Galaxies)

To understand the impact on phylogenetic trees regarding the role of the various chemical elements,

This line aims at merging the astronomical lines on chemical abundance determination and galaxy evolution

There is still no model to infer phylogeny of galaxy evolution. We are developing such

Unveiling the formation channels of stellar halos through their chemical fingerprints Stellar halos around galaxies