The Gaia mission has revolutionised our understanding of the Milky Way halo, but the biggest discoveries, which rely on individual abundances, are yet to be made. Using new and novel methods that this project will develop, we will be able to determine the distribution of progenitor systems that have built the Milky Way, thereby reconstructing its merger history.  

Publication: The Homogeneity of the Star-forming Environment of the Milky Way Disk over Time