This project is intended to search for the magnetic field signature of the Magellanic halo.

The goal of this project is to build a software pipeline that can take simulations of galactic winds, such as the one shown in the figure, and make simulated observational images from them that can be compared directly to telescopic data.

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.

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.

In order to further the MAVIS design, an image simulator was built in Python, allowing star catalogs to be fed in, which are used to generate realistic MAVIS images. MAVIS now requires an IFU simulator to be developed, providing realistic IFU images from star catalogs.

In order to further the MAVIS design, an image simulator was built in Python, allowing star catalogs to be fed in, which are used to generate realistic MAVIS images. MAVIS now requires an IFU simulator to be developed, providing realistic IFU images from star catalogs.

This project will build on work within the Dark-ages, Reionization And Galaxy-formation Observables Numerical Simulation project (DRAGONS).

This project will build on work within the Dark-ages, Reionization And Galaxy-formation Observables Numerical Simulation project (DRAGONS).

Star Clusters as Engines of Ionisation and their HII Regions in NGC 7793

We will use simulations of the Milky Way to make predictions for SKA.

We will use simulations of the Milky Way to make predictions for SKA.

We aim to build an innovative framework to leverage future 21-cm experiments to observe cosmic dawn, and to forecast the optimal constraints on dark matter.

You will use new data from the Australian SKA Pathfinder survey, GASKAP-HI to help take the temperature of the Milky Way and Magellanic Clouds. PhD & Masters students on this project will have the opportunity to be among the first users of ASKAP.  

We have a variety of projects that will use the new GASKAP-HI data to study the structure and temperature of hydrogen in the Magellanic System.