Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100217
Funder
Australian Research Council
Funding Amount
$850,000.00
Summary
Australian Partnership in Advanced LIGO+. This project aims to improve the sensitivity of the Advanced Laser Interferometer Gravitational wave Observatory (aLIGO). aLIGO’s detection of gravitational waves proved general relativity in the strong field limit and the existence of black hole binary systems. The increased sensitivity will enable daily detections and new classes of events, opening the field of gravitational wave astronomy. Since telescopes can detect only 5% of the stuff in the univer ....Australian Partnership in Advanced LIGO+. This project aims to improve the sensitivity of the Advanced Laser Interferometer Gravitational wave Observatory (aLIGO). aLIGO’s detection of gravitational waves proved general relativity in the strong field limit and the existence of black hole binary systems. The increased sensitivity will enable daily detections and new classes of events, opening the field of gravitational wave astronomy. Since telescopes can detect only 5% of the stuff in the universe, this is expected to greatly improve understanding of the universe. This Australian partnership will put its physicists and astronomers at the vanguard of this field and inspire the next generation to study the physical sciences.Read moreRead less
Linear Formation Interferometry for Astrophysics and New Space Technologies. This project will prototype a new type of visible and infrared light interferometry: telescopes freely moving in a line 10s of metres in length and directing their light towards a central beam combiner. This is particularly well suited to sparse aperture optical interferometry from space, which can be used to resolve angular scales much finer than the world's largest monolithic telescopes. The ground based prototype wil ....Linear Formation Interferometry for Astrophysics and New Space Technologies. This project will prototype a new type of visible and infrared light interferometry: telescopes freely moving in a line 10s of metres in length and directing their light towards a central beam combiner. This is particularly well suited to sparse aperture optical interferometry from space, which can be used to resolve angular scales much finer than the world's largest monolithic telescopes. The ground based prototype will also be able to make a several key astrophysical observations of benchmark stars and stellar systems, including making precise polarimetric measurements of dust shells around bright stars.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE210100953
Funder
Australian Research Council
Funding Amount
$405,000.00
Summary
Directly imaging exoplanets with astrophotonic innovation. Understanding our place in the universe and the possibility of life are profound questions. This project aims to develop innovative astro-photonic technologies to enable imaging of Earth-like planets beyond our solar system, and to perform unprecedented observations. The project expects to generate new knowledge and innovation in exoplanet science and photonics. Expected outcomes include the first glimpse of the most Earth-like planet to ....Directly imaging exoplanets with astrophotonic innovation. Understanding our place in the universe and the possibility of life are profound questions. This project aims to develop innovative astro-photonic technologies to enable imaging of Earth-like planets beyond our solar system, and to perform unprecedented observations. The project expects to generate new knowledge and innovation in exoplanet science and photonics. Expected outcomes include the first glimpse of the most Earth-like planet to date, and the development of ground-breaking technology. Benefits include technological innovation — benefiting fields such as remote-sensing, space-communications, life-science imaging, as well as astronomy — and revealing key insights into our planet’s history and the potential for life in the universe.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: 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: LE130100198
Funder
Australian Research Council
Funding Amount
$315,000.00
Summary
The SAMI facility: a revolutionary multi-object hexabundle spectrograph. SAMI is a new Australian instrument concept that uses fibre bundles to obtain detailed spectroscopic data at many positions across the face of numerous galaxies at a time. Now that the technology has been shown to work, with spectacular results, the project aims to turn this concept into a general-user facility at the Anglo-Australian Telescope.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100009
Funder
Australian Research Council
Funding Amount
$340,160.00
Summary
Doubling the power of a unique astronomical survey facility. This project aims to double the number of fibres in the spectrograph on the UK Schmidt Telescope and so double the number of stars and galaxies that it can observe simultaneously. This would allow rapid and timely completion of two major projects: the Taipan galaxy survey would be first to test a potential discrepancy in the expansion rate of the universe that may signal new physics, while the FunnelWeb stellar survey would (in tandem ....Doubling the power of a unique astronomical survey facility. This project aims to double the number of fibres in the spectrograph on the UK Schmidt Telescope and so double the number of stars and galaxies that it can observe simultaneously. This would allow rapid and timely completion of two major projects: the Taipan galaxy survey would be first to test a potential discrepancy in the expansion rate of the universe that may signal new physics, while the FunnelWeb stellar survey would (in tandem with two space missions) identify potential nearby exoplanets and trace the history of the Milky Way. The benefits include high scientific impact for the two surveys, international showcasing of the Australian Starbug technology, and a national astronomical survey facility for the next decade.Read moreRead less
How do galaxies get their gas? This project aims to build new understanding about the fundamental physics behind how galaxies get their gas. The way gas is accreted in galaxies affects how stars are made and what galaxies look like, including our own milky way. This project expects to build a new robotic instrument for three dimensional spectroscopy of galaxies, called Hector-I, to establish and run the Hector Galaxy Survey, the largest of its kind ever conducted. This survey data set will under ....How do galaxies get their gas? This project aims to build new understanding about the fundamental physics behind how galaxies get their gas. The way gas is accreted in galaxies affects how stars are made and what galaxies look like, including our own milky way. This project expects to build a new robotic instrument for three dimensional spectroscopy of galaxies, called Hector-I, to establish and run the Hector Galaxy Survey, the largest of its kind ever conducted. This survey data set will underpin broad investigations of gas accretion and the impact on the physical properties of galaxies. The project will clarify why our own galaxy looks so different to others, demonstrate Australian technologies for future commercialisation on international facilities, and train students for a high quality workforce.Read moreRead less