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“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EA ....“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EAGLE-XL. MAGPI will deliver exquisite kinematics for hundreds of galaxies in the middle ages of the Universe, providing a view to the effect of dark matter on galaxies at this critical time, while EAGLE-XL represents the technological frontier in simulations and provides the best interpretative framework for MAGPI.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100015
Funder
Australian Research Council
Funding Amount
$1,680,000.00
Summary
The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021 ....The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021. This project will ensure Australia's contribution to complete the facility, leading into its operations phase (starting in 2027). It will also fund unique optical astronomy hardware that will enable Australian scientific leadership in supporting some of the Cherenkov Telescope Array's Key Science Projects.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100165
Funder
Australian Research Council
Funding Amount
$792,859.00
Summary
Veloce Verde+Azzuro - Tripling the Power of Australia's Planet Foundry. This project aims to better understand humanity’s place in the Universe, including questions such as whether we are alone or if our home in the Solar System is unique or common. This project will enable new observations using a revolutionary Australian facility, Veloce Verde+Azzuro. Moving beyond discovering habitable planets around dim red stars, it will enable science on the properties and system architectures of planets o ....Veloce Verde+Azzuro - Tripling the Power of Australia's Planet Foundry. This project aims to better understand humanity’s place in the Universe, including questions such as whether we are alone or if our home in the Solar System is unique or common. This project will enable new observations using a revolutionary Australian facility, Veloce Verde+Azzuro. Moving beyond discovering habitable planets around dim red stars, it will enable science on the properties and system architectures of planets orbiting stars like the Sun. It will deliver a ten-fold increase in collecting power for Sun-like stars, providing understanding of how exoplanetary systems, and our Solar System, were formed.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
ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions. This Centre aims to answer fundamental questions in astrophysics including the origin of matter and the periodic table of elements, and the origin of ionisation in the Universe. It intends to use Australian three-dimensional technology to transform our understanding of the Universe. It will unify world-leading Australian optical and radio surveys with theoretical simulations and new e-Science techniques for Peta-scale data sets. ....ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions. This Centre aims to answer fundamental questions in astrophysics including the origin of matter and the periodic table of elements, and the origin of ionisation in the Universe. It intends to use Australian three-dimensional technology to transform our understanding of the Universe. It will unify world-leading Australian optical and radio surveys with theoretical simulations and new e-Science techniques for Peta-scale data sets. The Centre will also nurture young scientific leaders and make high-school students interested in STEM sciences through education and outreach programmes. It is expected the research will propel Australia to the forefront of astronomical research for the coming decade while capitalising on innovative instrumentation.Read moreRead less
ARC Centre of Excellence for Gravitational Wave Discovery. This Centre aims to explore the historic first detections of gravitational waves to understand the extreme physics of black holes and warped spacetime, and inspire the next generation of Australian scientists and engineers. The next-generation gravity wave detectors will enable a thousand-fold increase in detection volume and result in the new gravitational wave discoveries, triggering a new era of gravitational wave astrophysics. Buil ....ARC Centre of Excellence for Gravitational Wave Discovery. This Centre aims to explore the historic first detections of gravitational waves to understand the extreme physics of black holes and warped spacetime, and inspire the next generation of Australian scientists and engineers. The next-generation gravity wave detectors will enable a thousand-fold increase in detection volume and result in the new gravitational wave discoveries, triggering a new era of gravitational wave astrophysics. Building on decades of Australian investment in gravitational wave and pulsar science, this Centre will coalesce research activities into a focussed national programme whose discoveries are intended to experimentally validate Einstein’s General Theory of Relativity and educate the public about the wonders of Einstein's Universe.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100104
Funder
Australian Research Council
Funding Amount
$1,390,000.00
Summary
The Cherenkov Telescope Array - Production phase. This project aims to ensure Australia’s contribution to the five-year production phase of the Cherenkov Telescope Array (CTA), a very high energy gamma-ray astronomy instrument that is expected to transform both high energy astrophysics and astro-particle physics. Gamma-ray astronomy probes extreme processes in the Universe such as exploding stars, black holes, and mysterious dark matter. The project will maintain Australian access to all data an ....The Cherenkov Telescope Array - Production phase. This project aims to ensure Australia’s contribution to the five-year production phase of the Cherenkov Telescope Array (CTA), a very high energy gamma-ray astronomy instrument that is expected to transform both high energy astrophysics and astro-particle physics. Gamma-ray astronomy probes extreme processes in the Universe such as exploding stars, black holes, and mysterious dark matter. The project will maintain Australian access to all data and key science programmes of the CTA. Australian astronomers will be able to directly influence the major astrophysics goals of CTA, and link in with Australia's flagship astronomical infrastructure. This is expected to benefit astrophysics, big data processing, electronics, atmospheric physics and optics.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