Containerised applications can improve modularity when interfacing hardware from different vendors across a variety of machines.

Containerised applications can improve modularity when interfacing hardware from different vendors across a variety of machines.

The aim of this research is to determine the correlation of the tip-tilt to confirm that the downlink can be used as a reliable reference source for adaptive optics applied to the uplink signal.

Magnetic fields are present throughout the universe on all scales: from planets and stars, star-forming clusters and spiral arms, entire galaxies, to galaxy clusters and cosmic filaments.

This project aims to conceptualize a UV astronomical space mission to explore the interstellar medium (ISM) in the Milky Way and nearby Local Group Galaxies. Utilizing recent UV coating and detector advancements, the proposed mission involves high-throughput, compact UV spectroscopic instruments.

This project aims to conceptualize a UV astronomical space mission to explore the interstellar medium (ISM) in the Milky Way and nearby Local Group Galaxies. Utilizing recent UV coating and detector advancements, the proposed mission involves high-throughput, compact UV spectroscopic instruments.

Ultraviolet photometry has revealed that young open clusters in the Milky Way display extended main sequence turn-off in the colour magnitude diagram.

In this project you will develop use and further develop the Chronostar tool to identify thousands of previously unknown young stars near the sun - ideal targets for future exoplanet detection campaigns.

In this project you will develop use and further develop the Chronostar tool to identify thousands of previously unknown young stars near the sun - ideal targets for future exoplanet detection campaigns.

The ANU Research School of Astronomy and Astrophysics (RSAA) is collaborating with the National Astronomical Observatory Japan to develop a next-generation Ground Layer Adaptive Optics (GLAO) system for installation on the 8-meter optical-infrared Subaru telescope at the summit of Maunakea, Hawaii.

The ANU Research School of Astronomy and Astrophysics (RSAA) is collaborating with the National Astronomical Observatory Japan to develop a next-generation Ground Layer Adaptive Optics (GLAO) system for installation on the 8-meter optical-infrared Subaru telescope at the summit of Maunakea, Hawaii.

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.

Using both the Wide-Field Spectrograph (WiFeS) on the ANU 2.3m telescope and the 1.4 GHz radio band on the Australia Telescope Compact Array (ATCA), the student will address how the radio jets from the supermassive black hole interact with the Seyfert host galaxy to affect the evolution of the galaxy.