This project aims to utilize LLMs (Large Language Models) to enhance the usability of systems engineering documentation, including system requirement documents and flowdowns, interface documents, design documents, and reliability assessments.

This project aims to utilize LLMs (Large Language Models) to enhance the usability of systems engineering documentation, including system requirement documents and flowdowns, interface documents, design documents, and reliability assessments.

The Milky Way's magnetic field is critical for shaping the structure and evolution of the galaxy, regulating star formation, and transporting cosmic rays. Understanding the interaction between the magnetic field and atomic HI gas is key to unraveling the galaxy's dynamics and evolution.

With this project we will be using the newly automated ANU 2.3m telescope and the powerful WiFeS optical spectrograph to perform a time-series measurement of luminous active galaxies (AGN) using the technique of Quasar Reverberation Mapping.

A student undertaking this project will investigate the potential customisations of lenslet arrays afforded by optical meta-surfaces, and propose designs to be fabricated in the Research School of Physics at ANU.

A student undertaking this project will investigate the potential customisations of lenslet arrays afforded by optical meta-surfaces, and propose designs to be fabricated in the Research School of Physics at ANU.

A student undertaking this project will investigate the potential customisations of lenslet arrays afforded by optical meta-surfaces, and propose designs to be fabricated in the Research School of Physics at ANU.

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

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.

This project aims to research and potentially develop the design of calibration light sources for use in the MAVIS instrument (currently being designed for the ESO VLT).

This project aims to research and potentially develop the design of calibration light sources for use in the MAVIS instrument (currently being designed for the ESO VLT).

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.