Illuminating the cosmic web with Fast Radio Bursts. This project aims to establish the use of millisecond-duration Fast Radio Bursts as a wholly new means to map out the distribution of matter in the Universe. This project expects to localise 100s of bursts using novel infrastructure deployed on Australia's largest radio telescopes. Expected outcomes include an understanding of the processes that shape both the large-scale structures of the Universe, and the extreme conditions that exist at the ....Illuminating the cosmic web with Fast Radio Bursts. This project aims to establish the use of millisecond-duration Fast Radio Bursts as a wholly new means to map out the distribution of matter in the Universe. This project expects to localise 100s of bursts using novel infrastructure deployed on Australia's largest radio telescopes. Expected outcomes include an understanding of the processes that shape both the large-scale structures of the Universe, and the extreme conditions that exist at the sites of Fast Radio Bursts. This should provide significant benefits to our fundamental knowledge of the Universe, inspire students into careers in science, technology, engineering and mathematics, and develop signal processing techniques of application to both the Square Kilometre Array and industry.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100107
Funder
Australian Research Council
Funding Amount
$672,000.00
Summary
The next generation fast radio burst detector for Australia. This project intends to provide a next-generation fast radio burst detector for the Australian Square Kilometre Array Pathfinder. The project expects to both transform our understanding of fast radio bursts, enigmatic flashes of radio waves of unknown origin, but also use the bursts as tools to study the cosmic web of matter that resides in intergalactic space. To do so, the project aims to deliver a more sensitive detection system ca ....The next generation fast radio burst detector for Australia. This project intends to provide a next-generation fast radio burst detector for the Australian Square Kilometre Array Pathfinder. The project expects to both transform our understanding of fast radio bursts, enigmatic flashes of radio waves of unknown origin, but also use the bursts as tools to study the cosmic web of matter that resides in intergalactic space. To do so, the project aims to deliver a more sensitive detection system capable of localising a large sample of fast radio bursts to greater distances, found commensal to other observations. This should provide significant benefit, including the resolutions to key open astrophysical questions and improved scientific outcomes for transient searches with the Square Kilometre Array.Read moreRead less
New multi-scale seed dispersal models for improved regional weed management. This project will exploit recent advances in ecological and atmospheric modelling with the aim to build improved models of seed dispersal across landscapes to anticipate weed spread. Damaging invasive plants are rapidly transforming landscapes and altering ecosystem function worldwide. The speed and direction of weed spread determines the success or failure of costly containment and control actions, however we lack the ....New multi-scale seed dispersal models for improved regional weed management. This project will exploit recent advances in ecological and atmospheric modelling with the aim to build improved models of seed dispersal across landscapes to anticipate weed spread. Damaging invasive plants are rapidly transforming landscapes and altering ecosystem function worldwide. The speed and direction of weed spread determines the success or failure of costly containment and control actions, however we lack the ability to adequately predict spread. New models that combine micrometeorological measurements, within-canopy turbulence and topographic variation in wind flows will be designed to better predict where dispersal will occur. In this project, these improved predictions are planned to be combined with decision models to direct the management of invasive species across entire landscapes.Read moreRead less
Understanding snow gum dieback for effective and integrated management. The project leverages recent research and infrastructure investments and our determined and collaborative team as it aims to: 1) assess the future geography of snow gum dieback in the high country and identify priority locations for pro-active management, 2) quantify the impact of snow gums on high country water and carbon budgets and thus the socio- economic and biodiversity values, and 3) determine options for mitigation. ....Understanding snow gum dieback for effective and integrated management. The project leverages recent research and infrastructure investments and our determined and collaborative team as it aims to: 1) assess the future geography of snow gum dieback in the high country and identify priority locations for pro-active management, 2) quantify the impact of snow gums on high country water and carbon budgets and thus the socio- economic and biodiversity values, and 3) determine options for mitigation. Dieback of our iconic snow gum forests is diminishing the ecological, hydrological and cultural values of the Australian Alps and will impact state and national water-supply and power-generation systems. Our research will inform Alps-wide management efforts designed for long-term success.Read moreRead less
Galactic Archaeology: A Radial Velocity Experiment to Unveil the History of the Milky Way. The ambitious RAdial Velocity Experiment (RAVE) will measure velocities and chemical properties of 50 million stars in the period 2006-2010 - 2000 times the number measured throughout history. RAVE will use a new-technology Australian fiber spectrometer at the Siding Spring UK Schmidt Telescope. A key demonstrator for RAVE is our proposed pilot survey using existing instruments to measure 100,000 stars - a ....Galactic Archaeology: A Radial Velocity Experiment to Unveil the History of the Milky Way. The ambitious RAdial Velocity Experiment (RAVE) will measure velocities and chemical properties of 50 million stars in the period 2006-2010 - 2000 times the number measured throughout history. RAVE will use a new-technology Australian fiber spectrometer at the Siding Spring UK Schmidt Telescope. A key demonstrator for RAVE is our proposed pilot survey using existing instruments to measure 100,000 stars - already 20 times larger than any previous survey - providing unique chemical and kinematical fingerprints of our Galaxy's formation. This is critical for determining the optimum observing strategy, data management, and software pipeline, before embarking on the full survey in 2006.Read moreRead less
The Last 8 Billion Years of Cosmic Evolution. A key factor in Australia's international prominence in astronomy has been the development and use of innovative instrumentation on its telescopes to undertake major leading-edge surveys. This project will enhance this reputation by using the new AAOmega facility on the 3.9m Anglo-Australian Telescope to make the largest ever survey of galaxies in the distant universe. This will allow us to address the two most important issues in cosmology today - ....The Last 8 Billion Years of Cosmic Evolution. A key factor in Australia's international prominence in astronomy has been the development and use of innovative instrumentation on its telescopes to undertake major leading-edge surveys. This project will enhance this reputation by using the new AAOmega facility on the 3.9m Anglo-Australian Telescope to make the largest ever survey of galaxies in the distant universe. This will allow us to address the two most important issues in cosmology today - the nature of the "dark energy" that is causing the universe's expansion to accelerate, and the detailed role of dark matter in galaxy formation and evolution. Read moreRead less
The fundamental physics governing the formation of cosmic structure. This project will investigate the physics that underlie three of the most fundamental processes within the universe - its accelerated expansion, the formation of cosmic structure, and galaxy formation - thereby contributing to the Priority Goal of Breakthrough Science under National Research Priority 3. It will involve world-leading research in these areas, enabled by innovative instrumentation on Australia's national telescope ....The fundamental physics governing the formation of cosmic structure. This project will investigate the physics that underlie three of the most fundamental processes within the universe - its accelerated expansion, the formation of cosmic structure, and galaxy formation - thereby contributing to the Priority Goal of Breakthrough Science under National Research Priority 3. It will involve world-leading research in these areas, enabled by innovative instrumentation on Australia's national telescope facilities. National benefit will also come via the collaborations it will involve with prestigious North American institutions. These collaborations will lead to new research capability being built within Australia, through knowledge and expertise being vested in young postgraduate and postdoctoral researchers.Read moreRead less
Building resilient alpine environments with less snow. In this project, we aim to build resilience into alpine National Parks and Alpine Resorts to counter the effects of ongoing declines in snow. Alpine environments depend on snow to regulate water flows, insulate vegetation, control soil erosion and promote proper ecosystem functioning. How these processes will operate in a snow-free future is unknown. We will determine how and where snow characteristics drive soil water availability for plant ....Building resilient alpine environments with less snow. In this project, we aim to build resilience into alpine National Parks and Alpine Resorts to counter the effects of ongoing declines in snow. Alpine environments depend on snow to regulate water flows, insulate vegetation, control soil erosion and promote proper ecosystem functioning. How these processes will operate in a snow-free future is unknown. We will determine how and where snow characteristics drive soil water availability for plants and which plant species have the best adaptation and regeneration potential under extreme conditions such as heat, frost and drought. Benefits of the project include innovative land management and rehabilitation solutions, to safeguard Australia's alpine areas under changing environmental conditions.Read moreRead less
The Evolution of Gas in Galaxy Groups. The evolution of gas in galaxy groups is poorly understood, but is crucial to understanding galaxy evolution. This project provides a training opportunity for a talented postdoc to conduct the first `multiwavelength census' of southern galaxy groups, perform simulations and make predictions of group properties at early times. We will better understand the evolutionary processes in groups and provide a `local anchor' for future surveys. The knowledge gained ....The Evolution of Gas in Galaxy Groups. The evolution of gas in galaxy groups is poorly understood, but is crucial to understanding galaxy evolution. This project provides a training opportunity for a talented postdoc to conduct the first `multiwavelength census' of southern galaxy groups, perform simulations and make predictions of group properties at early times. We will better understand the evolutionary processes in groups and provide a `local anchor' for future surveys. The knowledge gained will feed directly into the design of the future Square Kilometre Array, and raise Australia's profile in this $1B project. We exploit Australia's best astronomical facilities, and establish a new University-CSIRO collaboration.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0236657
Funder
Australian Research Council
Funding Amount
$210,000.00
Summary
Renewed Great Melbourne Telescope: Opening a Window on the Universe. We propose to refurbish the Great Melbourne Telescope (GMT) located at Mount Stromlo Observatory with a new state-of-the-art imager. This instrument will be available to the entire Australian Astronomical community, and will allow Australian researchers to undertake cutting edge research with this world leading two colour wide field imager. A fully automated observing and data reduction pipeline, a world first for a telescope o ....Renewed Great Melbourne Telescope: Opening a Window on the Universe. We propose to refurbish the Great Melbourne Telescope (GMT) located at Mount Stromlo Observatory with a new state-of-the-art imager. This instrument will be available to the entire Australian Astronomical community, and will allow Australian researchers to undertake cutting edge research with this world leading two colour wide field imager. A fully automated observing and data reduction pipeline, a world first for a telescope of this size, means astronomers can work on their data, analyzing everything from the Solar System, to the most distant objects in the Universe, rather than spending night after night at the telescope.Read moreRead less