We have recently demonstrated a novel technique to recover sub-dwarf M stars from the combination of VISTA infra-red and SkyMapper photometry.

Using ANU's SkyMapper Telescope we follow up on gravitational-wave events from LIGO/Virgo to characterise the ejecta from neutron-star collisions.

Using ANU's SkyMapper Telescope we follow up on gravitational-wave events from LIGO/Virgo to characterise the ejecta from neutron-star collisions.

The successful applicant will work on one of several software related projects for the DREAMS infrared surveyor

The successful applicant will work on one of several software related projects for the DREAMS infrared surveyor

This short project will using existing data for a sample of red giant stars from the OGLE II and III, and MACHO surveys.

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.

In this project, we have worked on developing and comparing empirical pressure-temperature (P-T) phase diagrams of water, Earth, and terrestrial life, to quantify the terrestrial limits on the habitability of water and help identify the factors that cause some terrestrial water to be uninhabited. 

In this project, we have worked on developing and comparing empirical pressure-temperature (P-T) phase diagrams of water, Earth, and terrestrial life, to quantify the terrestrial limits on the habitability of water and help identify the factors that cause some terrestrial water to be uninhabited. 

In this project we will be able to investigate the environmental effect on star formation and galaxy evolution in individual galaxies falling into the cluster through radio observations of active galactic nuclei (AGN).

This project will study red spirals in detail, and aim to understand what levels of star formation persist and for how long. We will use optical and infrared data to measure current rates of star formation and find out what we have been missing due to dust extinction.

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