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
Cosmic powerhouses: The birth, death, and legacy of black hole jets. This project targets relativistic jets powered by supermassive black holes - the most powerful systems in the Universe. Theoretically, the enormous energies released have a profound influence on how galaxies evolve; empirically, observations reveal signatures of their impact across cosmic time. However, fundamental questions remain about how these jets are triggered and what impact they have on galaxies. The project will addres ....Cosmic powerhouses: The birth, death, and legacy of black hole jets. This project targets relativistic jets powered by supermassive black holes - the most powerful systems in the Universe. Theoretically, the enormous energies released have a profound influence on how galaxies evolve; empirically, observations reveal signatures of their impact across cosmic time. However, fundamental questions remain about how these jets are triggered and what impact they have on galaxies. The project will address these questions using novel supercomputer models of black hole jets in realistic cosmological environments, then confront these predictions with new data from Square Kilometre Array (SKA) pathfinding radio telescopes. This will substantially enhance Australia’s leadership capacity in a strategically important area.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
Galaxy evolution in high definition with the world's largest telescopes. This project aims to determine where, when, and how galaxies formed their stars in the key epoch spanning the first four billion years of the Universe’s history. Astronomy has entered a new era with the Atacama Large Millimetre Array (ALMA) and James Webb Space Telescope (JWST), the most powerful telescopes ever built. Together, they provide the sharpest and most complete view of distant, young galaxies ever achieved. This ....Galaxy evolution in high definition with the world's largest telescopes. This project aims to determine where, when, and how galaxies formed their stars in the key epoch spanning the first four billion years of the Universe’s history. Astronomy has entered a new era with the Atacama Large Millimetre Array (ALMA) and James Webb Space Telescope (JWST), the most powerful telescopes ever built. Together, they provide the sharpest and most complete view of distant, young galaxies ever achieved. This project will use cutting-edge ALMA and JWST observations to produce high-definition maps of the physical parameters of young galaxies through innovative analysis techniques. The project will enhance Australia's standing in astrophysical research, while inspiring the next generation of STEM students and workers.Read moreRead less
Expanding the Foundation of Planetary Science. Our understanding of the Solar System is based on a foundation of meteorite analyses. Knowing their orbital origin provides a critical spatial context, but we have this data for <0.1% of samples. This project aims to address this issue. There are 66 meteorite falls across Australia with orbits determined by the Desert Fireball Network that await recovery - more than the current global dataset. This project expects to generate new knowledge by applyi ....Expanding the Foundation of Planetary Science. Our understanding of the Solar System is based on a foundation of meteorite analyses. Knowing their orbital origin provides a critical spatial context, but we have this data for <0.1% of samples. This project aims to address this issue. There are 66 meteorite falls across Australia with orbits determined by the Desert Fireball Network that await recovery - more than the current global dataset. This project expects to generate new knowledge by applying an innovative search methodology using drones and machine learning. Expected outcomes include dramatically increasing the number of orbital meteorites. This should provide significant benefits. By linking meteorites to their parent asteroids every rock becomes a small sample-return mission.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
Discovery Early Career Researcher Award - Grant ID: DE240101377
Funder
Australian Research Council
Funding Amount
$381,237.00
Summary
Measuring the glow from our Cosmic Dawn. The Cosmic Dawn is one of the last unexplored periods of the history of the Universe. The faint glow of intergalactic hydrogen during the birth of the first galaxies can shed light on the formation of structure in the Universe. Many are seeking the first detection, notably teams in Australia, the USA, and the Netherlands. This project proposes to synthesise the knowledge across these communities for the first time, resulting in a new, cross-validated anal ....Measuring the glow from our Cosmic Dawn. The Cosmic Dawn is one of the last unexplored periods of the history of the Universe. The faint glow of intergalactic hydrogen during the birth of the first galaxies can shed light on the formation of structure in the Universe. Many are seeking the first detection, notably teams in Australia, the USA, and the Netherlands. This project proposes to synthesise the knowledge across these communities for the first time, resulting in a new, cross-validated analysis utilising worldwide expertise, for the benefit of Australia's Murchison Widefield Array. This collaborative approach will discover the best methods for precision analysis of the early Universe, and definitively embed Australia as the global leader in the search for our Cosmic Dawn.Read moreRead less