Dark gas and the formation of molecular clouds. Using frontline radio telescopes in Australia, Chile and Antarctica the project aims to understand how molecular clouds are formed in space, a part of the life cycle of our galaxy, and the role of hard-to-detect 'dark gas' in this process. Australia's Mopra telescope plays a central role in this international endeavour.
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.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0238884
Funder
Australian Research Council
Funding Amount
$220,000.00
Summary
Development of the CANGAROO III Very High Energy Gamma-ray telescope. This international project will explore the only part of the electromagnetic spectrum yet to be subjected to detailed astronomical study. CANGAROO III will span the energy range from ~100GeV to >10TeV, expanding upwards the range of satellite observations, and downwards the range accessible from previous ground-based systems. Gamma-ray observations have opened a new window on the universe and it is clear that there is much to ....Development of the CANGAROO III Very High Energy Gamma-ray telescope. This international project will explore the only part of the electromagnetic spectrum yet to be subjected to detailed astronomical study. CANGAROO III will span the energy range from ~100GeV to >10TeV, expanding upwards the range of satellite observations, and downwards the range accessible from previous ground-based systems. Gamma-ray observations have opened a new window on the universe and it is clear that there is much to be discovered with this new instrument. This project will provide an Australian infrastructure contribution to support the multi-million dollar contribution of our Japanese partners, and thus provide Australian access to a key astrophysical field at very modest cost.Read moreRead less
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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE120100181
Funder
Australian Research Council
Funding Amount
$650,000.00
Summary
Strengthening merit-based access and support at the new National Computing Infrastructure petascale supercomputing facility. World-leading high-performance computing is fundamental to Australia's international research success. This facility will provide access to the new National Computational Infrastructure facility by world-leading researchers from six research universities, and sustain ground-breaking work in an increasingly competitive environment.