Cubesat Technologies for High Spatial Resolution Astrophysics. This project aims to combine cubesat and hybrid cubesat/micro-satellite concepts studied in Australia and Japan, prototyping and space-qualifying the most custom components, enabling a future affordable launch. High angular resolution is critical for studying processes of star formation, black holes, and exoplanets. An array of small satellites can greatly exceed the angular resolution of a single telescope, or the sensitivity of atm ....Cubesat Technologies for High Spatial Resolution Astrophysics. This project aims to combine cubesat and hybrid cubesat/micro-satellite concepts studied in Australia and Japan, prototyping and space-qualifying the most custom components, enabling a future affordable launch. High angular resolution is critical for studying processes of star formation, black holes, and exoplanets. An array of small satellites can greatly exceed the angular resolution of a single telescope, or the sensitivity of atmosphere-limited ground-based interferometers. Space qualifying the key inter-spacecraft metrology and fibre injection technologies will not only enable a future Australian satellite astrophysical interferometer, but is also relevant for optical communications links and earth observations. Read moreRead less
Noise-free Cryogenic Wavefront Sensing. This project aims to optimise the prototype adaptive optics technology for the Giant Magellan Telescope (GMT) by leveraging past investment in adaptive optics instrumentation and shortwave infrared detector systems. This project expects to generate significant improvements in GMT performance, with ten times greater image resolution than the Hubble Space Telescope and current estimates of >90% sky coverage, compared with ~50% coverage for current technology ....Noise-free Cryogenic Wavefront Sensing. This project aims to optimise the prototype adaptive optics technology for the Giant Magellan Telescope (GMT) by leveraging past investment in adaptive optics instrumentation and shortwave infrared detector systems. This project expects to generate significant improvements in GMT performance, with ten times greater image resolution than the Hubble Space Telescope and current estimates of >90% sky coverage, compared with ~50% coverage for current technology. Expected outcomes of this project include the development of a highly trained workforce and continued international collaboration in the field of high-technology sensor systems. This contribution to the GMT will provide significant benefits—it will change the way we view the Universe.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100201
Funder
Australian Research Council
Funding Amount
$530,000.00
Summary
A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will ....A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will enable it to make detailed observations of initial discoveries made with the Australian Square Kilometre Array Pathfinder and other Australian telescopes. In short, it will enable Australian researchers to do more ambitious research, and make more discoveries, across broad areas of astrophysics.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100096
Funder
Australian Research Council
Funding Amount
$1,150,000.00
Summary
A next-generation receiver for Radio Astronomy. This project will provide a next-generation radio astronomy receiver to be used on the Parkes radio telescope. This facility will provide a major increase in performance, particularly in sensitivity and survey speed. The science goals are to better understand the ionized and neutral components of the cosmic web, and their evolution, through observations of Fast Radio Bursts and neutral hydrogen. Advances in the understanding of pulsars, molecules, ....A next-generation receiver for Radio Astronomy. This project will provide a next-generation radio astronomy receiver to be used on the Parkes radio telescope. This facility will provide a major increase in performance, particularly in sensitivity and survey speed. The science goals are to better understand the ionized and neutral components of the cosmic web, and their evolution, through observations of Fast Radio Bursts and neutral hydrogen. Advances in the understanding of pulsars, molecules, radio galaxies and cosmic rays will also be achieved with this facility. The technology is based on cryogenic cooling of a large phased array feed. This receiver is a major advance over existing receivers on the Parkes and Australian SKA Pathfinder (ASKAP) telescopes.Read moreRead less
A miniaturised laser manipulator for ultra-precise and pain-free dentistry. This project aims to develop a miniaturized high-precision laser robotic device that can fit comfortably in the mouth to perform pain-free, vibration-free dental operations by utilising silicon-carbide on silicon technology to create a millimetre-sized two-axis controllable, highly-reflective mirror robust to high-power ultra-short laser pulses. This project expects to generate new knowledge in micro-mirror control using ....A miniaturised laser manipulator for ultra-precise and pain-free dentistry. This project aims to develop a miniaturized high-precision laser robotic device that can fit comfortably in the mouth to perform pain-free, vibration-free dental operations by utilising silicon-carbide on silicon technology to create a millimetre-sized two-axis controllable, highly-reflective mirror robust to high-power ultra-short laser pulses. This project expects to generate new knowledge in micro-mirror control using optically excited piezo-resistive sensors, and cold femtosecond laser ablation of hard dental tissue. Expected outcomes include a working prototype for laser removal of tooth materials at speeds exceeding dental drills, providing benefits in miniaturized laser devices and ultimately removing pain from dental procedures. Read moreRead less
Better end-of-life care through an optimal, holistic regulatory framework. This project aims to enhance end-of-life care through better regulation. Current regulation does not work as intended and is complex and fragmented. This harms patients, families and health professionals, and wastes health resources across the 100,000 medical end-of-life decisions in Australia annually. Expected outcomes are: (1) the first study internationally to establish in practice how the interaction of conflicting l ....Better end-of-life care through an optimal, holistic regulatory framework. This project aims to enhance end-of-life care through better regulation. Current regulation does not work as intended and is complex and fragmented. This harms patients, families and health professionals, and wastes health resources across the 100,000 medical end-of-life decisions in Australia annually. Expected outcomes are: (1) the first study internationally to establish in practice how the interaction of conflicting law, policies, ethics and training affects the end-of-life care patients receive; and (2) a new holistic regulatory framework to enhance the quality of end-of-life care. Expected benefits are better palliative care, more patient involvement in decisions, reduced patient-doctor conflict and a more efficient health system.Read moreRead less