Ambitious students will investigate optimal ways to measure the stellar properties (eg Teff, age, mass) and chemical composition of this immense amount of data.

In this project you will use existing and new data to understand the nature of filamentary structure in galaxies and how they relate to magnetic fields.

In the spectra of distant stars, we can often find a series of absorption features, such as Diffuse Interstellar Bands (DIBs) or those of neutral atomic potassium, K I. Although the exact carriers of DIBs are still a matter of debate, various candidates have been proposed over the years.

Dust in the Milky Way affects astronomical observations. Here we try too improve our knowledge of its distribution.

Magnetic fields are present throughout the universe on all scales: from planets and stars, star-forming clusters and spiral arms, entire galaxies, to galaxy clusters and cosmic filaments.

Ultraviolet photometry has revealed that young open clusters in the Milky Way display extended main sequence turn-off in the colour magnitude diagram.

The goal of the project would be to analyse the spectra and determine the underlying reason for the different spectra of the two orbit families.

Accreted stellar populations are comprised of the remnants of destroyed galaxies, and often dominate the 'stellar haloes' of galaxies such as the Milky Way.

You will model stellar spectra with spots to improve the spectrum analysis for some of the active stars observed by the million-star spectroscopic GALAH Survey.

You will model stellar spectra with spots to improve the spectrum analysis for some of the active stars observed by the million-star spectroscopic GALAH Survey.

This has wide potential applications to chemical and dynamical studies of galaxies from two-dimensional  integral field unit (IFU) spectroscopy.

In this project, the student would study both the spectral and structural properties of the thermal electron density and magnetic fields in the ionised gas phase of the Milky Way.

In this project, the student would study both the spectral and structural properties of the thermal electron density and magnetic fields in the ionised gas phase of the Milky Way.

Our team is looking for enthusiastic Honours, Masters and PhD students with a strong background in Maths, Physics, or Computer Science who want to work on some of the most important questions currently discussed in near-field cosmology community.

This project will simulate observations of the magnetic fields of a Milky Way-like galaxy from a recent, high-resolution simulation. The goal is to identify effective ways to reconstruct the 3D magnetic field geometry of this simulated galaxy using observables projected onto the 2D sky.