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
Closing the Solar Cycle. This project aims to decisively settle the debate about the mechanism driving magnetic activity on the surface of the Sun. By drawing on extensive, big-data analysis of solar observations the project intends to use the technique of helioseismology to reveal differences in the statistical evolution of magnetic regions. Expected outcomes of this project will powerfully refine our models of the interaction between convective flows and magnetic fields in the Sun, resulting i ....Closing the Solar Cycle. This project aims to decisively settle the debate about the mechanism driving magnetic activity on the surface of the Sun. By drawing on extensive, big-data analysis of solar observations the project intends to use the technique of helioseismology to reveal differences in the statistical evolution of magnetic regions. Expected outcomes of this project will powerfully refine our models of the interaction between convective flows and magnetic fields in the Sun, resulting in a leap forward in solar dynamo theory, one of the fundamental problems in astrophysics. The anticipated benefits include moving from nowcasting to forecasting space weather, mitigating the billion dollar economic effects of geomagnetic storms.Read moreRead less
Space RAdiation Monitoring System (SRAMS) for safe space missions. The goal of the project is to develop a comprehensive space radiation monitoring system (SRAMS) that can evaluate: i) the radiation related hazards for astronauts, ii) the radiation damage in electronics during space missions and iii) the ground radiation facility environment used in radiation hardness assurance tests. SRAMS will also address important issue in space by minimizing manned or satellite space mission aborts due to s ....Space RAdiation Monitoring System (SRAMS) for safe space missions. The goal of the project is to develop a comprehensive space radiation monitoring system (SRAMS) that can evaluate: i) the radiation related hazards for astronauts, ii) the radiation damage in electronics during space missions and iii) the ground radiation facility environment used in radiation hardness assurance tests. SRAMS will also address important issue in space by minimizing manned or satellite space mission aborts due to space radiation adverse effects on astronaut’s health and electronics failure, and translates into an enormous economic value proposition. SRAMS will be paramount for leveraging the quantifiable standards of the space-radiation qualification facilities that are important for boosting the Australian Space industry. Read moreRead less
Mid-infrared quantum dots for room temperature photodetectors and emitters. This project aims to develop new technologies for mid-wave infrared (MWIR) cameras based on quantum dots (QDs). These will include MWIR photodetectors based on QD-sensitised photodetectors and MWIR emitters based on QD electroluminescence devices.
This project expects to generate new knowledge in MWIR QDs and in devices that sense and emit infrared light.
Expected outcomes of the project include MWIR cameras that are ....Mid-infrared quantum dots for room temperature photodetectors and emitters. This project aims to develop new technologies for mid-wave infrared (MWIR) cameras based on quantum dots (QDs). These will include MWIR photodetectors based on QD-sensitised photodetectors and MWIR emitters based on QD electroluminescence devices.
This project expects to generate new knowledge in MWIR QDs and in devices that sense and emit infrared light.
Expected outcomes of the project include MWIR cameras that are smaller, lighter, lower in power consumption and cheaper than existing technologies.
This project is expected to provide significant benefits, such as dramatic reductions in the cost of infrared cameras and sensors. The high cost of infrared cameras currently limits their use in Australia largely to defence.
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ARC Centre of Excellence for Gravitational Wave Discovery. ARC Centre of Excellence for Gravitational Wave Discovery. The mission of our Centre is to use gravitational waves to investigate the fundamental nature of relativistic gravity, ultra-dense matter, and cosmology. This will generate critical discoveries that cement Australia's leadership role in the gravitational wave mega-science instruments of the 2030s and 2040s. By bringing together a world-class team with broad and complementary expe ....ARC Centre of Excellence for Gravitational Wave Discovery. ARC Centre of Excellence for Gravitational Wave Discovery. The mission of our Centre is to use gravitational waves to investigate the fundamental nature of relativistic gravity, ultra-dense matter, and cosmology. This will generate critical discoveries that cement Australia's leadership role in the gravitational wave mega-science instruments of the 2030s and 2040s. By bringing together a world-class team with broad and complementary expertise we will develop core technologies for future detectors, discover new sources of gravitational waves, probe fundamental physics, and lay the foundations for an Australian gravitational wave observatory. Our discoveries will inspire Australia's youth to pursue high tech careers and position our staff and students to become leaders in both industry and academia.Read moreRead less
Australian Laureate Fellowships - Grant ID: FL220100020
Funder
Australian Research Council
Funding Amount
$2,647,737.00
Summary
Unveiling the Winds of Star-Forming Galaxies. This project seeks to resolve an outstanding problem in the formation of cosmic structure: what is the nature of galactic winds, and what physical mechanisms are responsible for driving them? Answering these questions requires computer simulations of greater resolution than have previously been possible, coupled to next-generation telescopic observations. This research aims to develop novel methods to enable the required simulations, leveraging new h ....Unveiling the Winds of Star-Forming Galaxies. This project seeks to resolve an outstanding problem in the formation of cosmic structure: what is the nature of galactic winds, and what physical mechanisms are responsible for driving them? Answering these questions requires computer simulations of greater resolution than have previously been possible, coupled to next-generation telescopic observations. This research aims to develop novel methods to enable the required simulations, leveraging new hardware architectures at Australian supercomputer facilities, and to use these approaches to solve a major open problem in astrophysics, open new frontiers in simulation, and multiply the return on Australia's investment in both computer facilities and telescopes that will study galactic winds.Read moreRead less
The Dark-side of the Milky Way. Astronomers have long sought to determine the 3-dimensional structure of our Galaxy, the Milky Way, with limited success owing to its immense size and obscuration by dust at optical wavelengths. We know more about structure of tens of thousands of other galaxies than we do about the structure of the Milky Way on the far-side of the Galactic Centre. This program will use Australian infrastructure to make the most accurate distance measurements to date of the far-si ....The Dark-side of the Milky Way. Astronomers have long sought to determine the 3-dimensional structure of our Galaxy, the Milky Way, with limited success owing to its immense size and obscuration by dust at optical wavelengths. We know more about structure of tens of thousands of other galaxies than we do about the structure of the Milky Way on the far-side of the Galactic Centre. This program will use Australian infrastructure to make the most accurate distance measurements to date of the far-side of the Milky Way visible from the Southern hemisphere, completing the 3-dimensional picture of our Galaxy. These results will be leveraged to yield accurate distances, providing fundamental information on the stellar masses, luminosities, and ages.Read moreRead less
Exploiting James Webb Space Telescope Observations of the First Galaxies. This Discovery Project aims exploit the next generation spectroscopy with the James Webb Space Telescope, combined with Australian supercomputing expertise to make fundamental new measurements of the formation of stars in the first galaxies. The results will be used to make predictions for key experiments that will be conducted with the Square Kilometer Array. The research outcomes aim to benefit astronomy by generating ne ....Exploiting James Webb Space Telescope Observations of the First Galaxies. This Discovery Project aims exploit the next generation spectroscopy with the James Webb Space Telescope, combined with Australian supercomputing expertise to make fundamental new measurements of the formation of stars in the first galaxies. The results will be used to make predictions for key experiments that will be conducted with the Square Kilometer Array. The research outcomes aim to benefit astronomy by generating new knowledge of high redshift galaxies and provide new spectral star-formation diagnostics which will be made available to the general astronomical community. The project also aims to provide cultural benefit through effective public and education as well training of future leaders for astronomy and industry research.Read moreRead less
Australian Laureate Fellowships - Grant ID: FL220100191
Funder
Australian Research Council
Funding Amount
$2,609,122.00
Summary
Unveiling the mass of the Universe: stars, gas, plasma and dark matter. Using unique Australian-built fibre-positioning technologies, the Fellowship will measure the distances to 2 million galaxies, transforming our understanding of dark matter on the scales of galaxies, galaxy groups, and filaments – the largest structures that exist. There are two specific goals: (i) to test precise predictions of the leading cold dark matter model by constructing dark-matter halo catalogues based on the motio ....Unveiling the mass of the Universe: stars, gas, plasma and dark matter. Using unique Australian-built fibre-positioning technologies, the Fellowship will measure the distances to 2 million galaxies, transforming our understanding of dark matter on the scales of galaxies, galaxy groups, and filaments – the largest structures that exist. There are two specific goals: (i) to test precise predictions of the leading cold dark matter model by constructing dark-matter halo catalogues based on the motions of galaxies measured to unprecedented accuracy; and (ii) to solve the long-standing "missing mass" problem by measuring the extent of the plasma, neutral gas, and stellar contents within these halos. Both programs will capitalise on our strategic engagement with the European Southern Observatory.Read moreRead less
Uncovering the First Stars and Galaxies with the James Webb Space Telescope. This project aims to find "First Light": the first stars and galaxies that formed after the Big Bang. Understanding the astrophysics of the first galaxies, their explosive growth, and how they set ablaze the remaining gas in the Universe have long been among the most important unsolved mysteries of astronomy. Decades in the making, the launch of the James Webb Space Telescope in December 2021 marks a watershed moment. T ....Uncovering the First Stars and Galaxies with the James Webb Space Telescope. This project aims to find "First Light": the first stars and galaxies that formed after the Big Bang. Understanding the astrophysics of the first galaxies, their explosive growth, and how they set ablaze the remaining gas in the Universe have long been among the most important unsolved mysteries of astronomy. Decades in the making, the launch of the James Webb Space Telescope in December 2021 marks a watershed moment. This project uses privileged access to the revolutionary space telescope to find "First Light" and contribute to rewriting the first chapter of our cosmic history. The project is expected to significantly enhance Australia's international standing through leadership in use of the world's flagship scientific facility.Read moreRead less