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New Dimensions in Radio Astronomy: Mining Sparse Datasets with the Australian Square Kilometre Array Pathfinder. Radio astronomy is entering a new era, driven by technological advances that make rapid surveys of the sky possible. As leaders of three major surveys for the Australian Square Kilometre Array Pathfinder (ASKAP) telescope, we will explore three new dimensions of astronomy: searching for transient sources, detecting faint galaxies and investigating cosmic magnetism. The project will pu ....New Dimensions in Radio Astronomy: Mining Sparse Datasets with the Australian Square Kilometre Array Pathfinder. Radio astronomy is entering a new era, driven by technological advances that make rapid surveys of the sky possible. As leaders of three major surveys for the Australian Square Kilometre Array Pathfinder (ASKAP) telescope, we will explore three new dimensions of astronomy: searching for transient sources, detecting faint galaxies and investigating cosmic magnetism. The project will put Australian astronomers at the forefront of international research. In addition to novel scientific results we will produce data resources and software that will be critical for future Square Kilometre Array projects. These will be available online to amateur astronomers and the general public. We will train the next generation of astronomers with the skills required to make breakthrough discoveries.Read moreRead less
Caught in the act by PAndAS: An unparalleled view of galaxy evolution. How do galaxies, like our own Milky Way, form? Using a new survey of the nearby cosmos, we will search for the signatures of galactic cannibalism, the disrupted bodies of smaller galaxies, and use this archaeology to piece together the formation history. We will also reveal the presence of local dark matter, whose action has shaped our own galaxy's formation.
The Great Escape: The Gaseous Outflow from the Centre of the Milky Way. This project aims to increase our understanding of the workings of the central regions of galaxies. The nuclei of galaxies are galactic-scale powerhouses driven by fast-moving winds launched by either the active bursts of star formation in the galaxy’s core or the accretion of gas onto a central black hole more than a million times the mass of the Sun. In 2010, the Fermi space telescope discovered enormous bubbles filled wit ....The Great Escape: The Gaseous Outflow from the Centre of the Milky Way. This project aims to increase our understanding of the workings of the central regions of galaxies. The nuclei of galaxies are galactic-scale powerhouses driven by fast-moving winds launched by either the active bursts of star formation in the galaxy’s core or the accretion of gas onto a central black hole more than a million times the mass of the Sun. In 2010, the Fermi space telescope discovered enormous bubbles filled with hot gas emanating from the centre of the Milky Way, proof of a Galactic wind. Our Galaxy's wind offers the best laboratory in the universe for understanding what drives the powerhouses at the nuclei of normal galaxies. This project aims to determine whether the Milky Way’s nuclear wind and the Fermi bubbles were formed from a starburst wind or gas accretion onto the central black hole.Read moreRead less
Disentangling the origin and evolution of the tangled magellanic stream. This project aims to reveal the process of gaseous accretion in interacting galaxies by elucidating the origin and evolution of the Magellanic Stream. The Magellanic Stream is an enormous tail of hydrogen gas extending from the Magellanic Clouds almost fully around the Milky Way. Through unravelling the Magellanic Stream and revealing how it will impact the Milky Way, this project will help understand how galaxies receive n ....Disentangling the origin and evolution of the tangled magellanic stream. This project aims to reveal the process of gaseous accretion in interacting galaxies by elucidating the origin and evolution of the Magellanic Stream. The Magellanic Stream is an enormous tail of hydrogen gas extending from the Magellanic Clouds almost fully around the Milky Way. Through unravelling the Magellanic Stream and revealing how it will impact the Milky Way, this project will help understand how galaxies receive new gas to continue their star formation and very existence. The project will use the newly constructed Australian Square Kilometre Array Pathfinder to shed light on the question of how galaxies evolve, one of the highest priority questions in Australian Astrophysics as defined by the Australian Astronomy Decadal Plan.Read moreRead less
Australian Laureate Fellowships - Grant ID: FL100100114
Funder
Australian Research Council
Funding Amount
$2,784,765.00
Summary
A Survey of the Universe's Magnetism. This project will significantly advance our understanding of the structure and evolution of the Universe and will maintain our nation's outstanding track record of astronomical discovery by delivering ground-breaking world-class scientific discoveries, produced by Australian astronomers using an Australian telescope. The project will help demonstrate the viability of the technology that Australia is advocating for the design of the Square Kilometre Array by ....A Survey of the Universe's Magnetism. This project will significantly advance our understanding of the structure and evolution of the Universe and will maintain our nation's outstanding track record of astronomical discovery by delivering ground-breaking world-class scientific discoveries, produced by Australian astronomers using an Australian telescope. The project will help demonstrate the viability of the technology that Australia is advocating for the design of the Square Kilometre Array by carrying out innovative experiments with powerful new instrumentation. Finally, the project will provide new capacity for research and innovation by training the next generation of scientists and by providing them with unique skills and expertise.Read moreRead less
Exploiting SkyMapper for Galactic Astrophysics. The SkyMapper telescope will commence a digital imaging survey of the entire southern hemisphere sky in the second quarter of 2014. This project aims to exploit the SkyMapper survey data to discover and characterise the oldest and most metal-poor stars in our Galaxy, constraining both the origin of the chemical elements and the star formation processes that occurred during the initial stages of our Galaxy's formation. At the same time the project w ....Exploiting SkyMapper for Galactic Astrophysics. The SkyMapper telescope will commence a digital imaging survey of the entire southern hemisphere sky in the second quarter of 2014. This project aims to exploit the SkyMapper survey data to discover and characterise the oldest and most metal-poor stars in our Galaxy, constraining both the origin of the chemical elements and the star formation processes that occurred during the initial stages of our Galaxy's formation. At the same time the project will use SkyMapper and other imaging data to increase understanding of the formation of the Galactic halo and of our nearest galaxy neighbours, the Magellanic Clouds.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE190100375
Funder
Australian Research Council
Funding Amount
$315,000.00
Summary
Extragalactic archaeology: our galaxy as a rosetta stone of galaxy evolution. This project aims to measure the stellar populations of nearby galaxies that are apparently similar to the Milky Way. The stellar population of a galaxy provides a fossil record of its entire history and is a key window into galaxy evolution. The project will use the well-studied stellar population of our own galaxy as a galactic Rosetta Stone to interpret the light from nearby galaxies, revealing their chemical compos ....Extragalactic archaeology: our galaxy as a rosetta stone of galaxy evolution. This project aims to measure the stellar populations of nearby galaxies that are apparently similar to the Milky Way. The stellar population of a galaxy provides a fossil record of its entire history and is a key window into galaxy evolution. The project will use the well-studied stellar population of our own galaxy as a galactic Rosetta Stone to interpret the light from nearby galaxies, revealing their chemical compositions and star formation histories. This project will advance understanding of galaxy evolution and reveal the evolutionary history of galaxies that are similar to our own Milky Way. The highly novel approach used will enable Australia to capitalise on its investment in optical astronomy, provide training and inspiration for the next generation of scientists, and maintain Australia’s international reputation for cutting-edge optical astronomy research.Read moreRead less
Discovery and characterisation of Milky Way satellite galaxies. Cold dark matter simulations, known to accurately describe the large-scale cosmic web of the Universe, predict hundreds of dark matter subhalos orbiting the Milky Way. Our hemispheric survey aims at finding and systematically acquiring information about their optical counterparts, the ultra-faint galaxies, the most extreme class of stellar systems.
Exploiting the discovery of ultra-faint dwarf galaxies in the southern hemisphere sky. The scientific exploitation of newly discovered southern hemisphere ultra-faint Milky Way satellite galaxies will make Australia a leader in this rapidly developing research field. It will be enabled by access to national and international telescope facilities such as the Anglo- Australian Telescope (AAT), Gemini and Magellan, and by access to national computing resources for theoretical simulations. National ....Exploiting the discovery of ultra-faint dwarf galaxies in the southern hemisphere sky. The scientific exploitation of newly discovered southern hemisphere ultra-faint Milky Way satellite galaxies will make Australia a leader in this rapidly developing research field. It will be enabled by access to national and international telescope facilities such as the Anglo- Australian Telescope (AAT), Gemini and Magellan, and by access to national computing resources for theoretical simulations. National benefit will also flow from collaborations between the team and its Super Science Fellows and researchers at overseas institutions. Results from the project will motivate research programs for the coming era of extremely large telescopes and will position the Fellows as potential future leaders in the exploiting the scientific potential of those facilities.Read moreRead less
Caught in the act: an unparalleled view of galaxy evolution. How do galaxies, like our own Milky Way, form? Using a new survey of the nearby cosmos, this project will search for the signatures of galactic cannibalism, the disrupted bodies of smaller galaxies, and use this archaeology to piece together the formation history. This project will also reveal the presence of local dark matter, whose action has shaped our own formation.