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: LE150100070
Funder
Australian Research Council
Funding Amount
$270,000.00
Summary
The Cherenkov Telescope Array. The Cherenkov Telescope Array: The Cherenkov Telescope Array (CTA) is a major advance in very high energy gamma-ray astronomy. It will be ten times more sensitive than current instruments and will transform many topics in high energy astrophysics concerning extreme particle acceleration, and in astro-particle physics such as dark matter. Over 1000 scientists from over 25 countries are involved and prototype telescopes are under construction. This project will enabl ....The Cherenkov Telescope Array. The Cherenkov Telescope Array: The Cherenkov Telescope Array (CTA) is a major advance in very high energy gamma-ray astronomy. It will be ten times more sensitive than current instruments and will transform many topics in high energy astrophysics concerning extreme particle acceleration, and in astro-particle physics such as dark matter. Over 1000 scientists from over 25 countries are involved and prototype telescopes are under construction. This project will enable a hardware contribution to the pre-production array of telescopes, bringing with it full membership, plus access to all data and core science programmes of CTA. Australian astronomers can then influence astrophysics goals of CTA, and add new scientific value to Australia's radio astronomical facilities.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: LE120100158
Funder
Australian Research Council
Funding Amount
$750,000.00
Summary
The Nanten2 sub-millimetre telescope. The millimetre-wavelength sky holds the key for understanding how stars form in the coldest regions of interstellar space: the molecular clouds of our Galaxy. A new frontline facility in Chile will be used in an international research endeavour to map their structures, in order to find out how they form and what causes stars to be born inside them.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100038
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
The NANTEN2 Observatory sub-millimetre wave telescope. The millimetre-wavelength sky holds the key to understanding how stars form in the coldest regions of interstellar space: the molecular clouds of our Galaxy. This new frontline facility in Chile will be used in an international research endeavour to map these cold regions and the stars they contain in order to find out how they form and what causes stars to be born within them.
Australian Laureate Fellowships - Grant ID: FL140100278
Funder
Australian Research Council
Funding Amount
$2,513,348.00
Summary
Hector: a revolutionary survey machine to discover how galaxies formed. Hector: a revolutionary survey machine to discover how galaxies formed. The formation of the Milky Way, is one of the most important questions in cosmology today. One of the key unknowns is how the gas, which forms the stars, gets into dark matter halos to make galaxies and why these galaxies spin. This project aims to assemble a first-rate instrument team to build Hector, the first automated hexabundle spectrograph; to ass ....Hector: a revolutionary survey machine to discover how galaxies formed. Hector: a revolutionary survey machine to discover how galaxies formed. The formation of the Milky Way, is one of the most important questions in cosmology today. One of the key unknowns is how the gas, which forms the stars, gets into dark matter halos to make galaxies and why these galaxies spin. This project aims to assemble a first-rate instrument team to build Hector, the first automated hexabundle spectrograph; to assemble a large team to combine Hector's spectral imaging of 100,000 galaxies with new Australian radio observations; and to extend this technology for the Giant Magellan Telescope. This will help to ensure Australia's leadership in observational cosmology and instrumentation through this decade and into the era of extremely large telescopes.Read moreRead less
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
Development and study of a new theory of gravity. Gravity is thought to be an understood physical phenomena. But recently dramatic discoveries have revealed that major aspects of this phenomenon have been completely missed. This research project will develop and explore implications of these discoveries. At one level this project is about major breakthroughs in fundamental science, but discoveries are revealing space to be a complex dynamic system, and new technologies to detect and exp ....Development and study of a new theory of gravity. Gravity is thought to be an understood physical phenomena. But recently dramatic discoveries have revealed that major aspects of this phenomenon have been completely missed. This research project will develop and explore implications of these discoveries. At one level this project is about major breakthroughs in fundamental science, but discoveries are revealing space to be a complex dynamic system, and new technologies to detect and exploit this are foreseen. There is some evidence that space is a self-organising information system of a totally new kind, and this will also have applications. At a scientific level these developments will attract considerable international attention and will enthuse younger researchersRead moreRead less
Ultra High Energy Cosmic Ray and Neutrino Astronomy using Radio Telescopes. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discover the first UHE neutrino - this wo ....Ultra High Energy Cosmic Ray and Neutrino Astronomy using Radio Telescopes. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discover the first UHE neutrino - this would have huge impact and prestige for Australia. The technology developed resulting from this project will contribute to Australia's IT base. Read moreRead less
LUNASKA, a theoretical and experimental project for UHE neutrino astrophysics using a giant radio observatory. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discov ....LUNASKA, a theoretical and experimental project for UHE neutrino astrophysics using a giant radio observatory. There will be an increase in Australian visibility in the high energy astrophysics community and stronger links between and within the fields of radio astronomy and high energy astrophysics in Australia, and internationally. This project will enhance Australian participation in the international Square Kilometre Array. By making observations using the Australia Telescope we may discover the first UHE neutrino - this would have huge impact and prestige for Australia. The technology developed resulting from this project will contribute to Australia's IT base. Hosting an international workshop will benefit national prestige and economy. Read moreRead less