The successful applicant will join the ANU team and will assist with the development of instrumentation for the optical communication team

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

The Giant Magellan Telescope (GMT) is being designed and built by an international consortium of institutions and will be the largest optical telescope in the world when it is completed around 2020.

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.

This project requires significant data analysis efforts and some observational and theoretical efforts.

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.

Mapping azimuthal variations in metals across cosmic time

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.

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.