This project aims to demonstrate the advantages of LGS-AO for deep space optical communications.

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.

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 honours research developed numerical models of the inner radio structure of Centaurus A using the FLASH relativistic hydrodynamics code, and compared the predictions with observations of the galaxy.

Modelling the oscillations of Red Clump stars using stellar evolution codes to study their internal structure.

Modelling the oscillations of Red Clump stars using stellar evolution codes to study their internal structure.

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

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

This Honours project was designed to complement the High Efficiency and Resolution Multi-Element Spectroscopy (HERMES) project being undertake at the AAT.