Do you enjoy working with instrumentation? Are you interested in using data to inform real-world decisions? Are you an independent thinker who loves to solve problems? If so, we’d love to hear from you.

Or team is working with major national and international detector vendors to develop novel new sensor systems that solve tricky problems not only for astronomy but also for more down-to-Earth issues such as Bushfire Hazard management from Low Earth Orbit remote sensing.

CSIRO has a cold spray research group which is developing cold sprayed Invar. This project will be developing an optical metrology setup to measure the creep of the cold sprayed Invar in collaboration with CSIRO Lab22 in Clayton, Victoria.

This project aims to address the potential of Spatial Light Modulators (SLMs) as highly nonlinear optical elements, including their potential use in pyramid wavefront sensing.

This project aims to address the potential of Spatial Light Modulators (SLMs) as highly nonlinear optical elements, including their potential use in pyramid wavefront sensing.

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

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.

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.

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.