PhD position: Galactic archeology through stellar spectroscopy

The PhD project focuses on so-called Galactic archaeology, where high-resolution stellar spectroscopy is the primary method. This means, in general terms, that spectroscopic data from individual stars, collected using large international telescopes, are used to investigate how specific parts of our galaxy, the Milky Way, have formed and evolved.

The project offers some flexibility depending on your previous experience but is expected to focus mainly on the local Galactic disk and/or globular clusters. The thesis will be built around one or more "medium-sized" sub-projects, where the research is niched by using rigorous, classical analysis methods to study thousands of stars - a methodology that is relatively uncommon. You will work together with your supervisor and colleagues to carry out both the practical analysis of stellar spectra, where elemental abundances of the stars are determined, as well as the scientific interpretation of the results: what do the measured elemental abundances reveal about the evolution of the stellar population and, in a broader perspective, the Galaxy?

The research environment is highly international, with members who have broad experience in both small-scale, classical projects and large-scale surveys. As a natural consequence of the international character of the work, you will be expected to actively participate in international conferences and workshops, conduct observations at world-leading telescopes, and, if interested and possible, participate in shorter international research exchanges.

Read more about the project, included benefits, and salary by following the link to the online application system below.