Research

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

This research line aims to use computational simulations of galaxy evolution (such as [Patricia’s simulation]

To understand the impact on phylogenetic trees regarding the role of the various chemicalelements, semi-analytical

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

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

Pristine Inner Galaxy Survey (PIGS) IX. The largest detailed chemical analysis of very metal-poor stars