Simulating the Magellanic system using new special-purpose computers for gravitational dynamics. Australia is renowned for its significant contribution to great progress in observational studies of the Large and the Small Magellanic Clouds. The proposed state-of-the-art computer simulations will provide new and better understanding of the Magellanic Clouds and thus stimulate public interest, in particular, the next generation of Australian scientists. The extensive comparison between results fro ....Simulating the Magellanic system using new special-purpose computers for gravitational dynamics. Australia is renowned for its significant contribution to great progress in observational studies of the Large and the Small Magellanic Clouds. The proposed state-of-the-art computer simulations will provide new and better understanding of the Magellanic Clouds and thus stimulate public interest, in particular, the next generation of Australian scientists. The extensive comparison between results from fastest computers and world-class telescopes will make important breakthroughs in the areas of computational astrophysics and extragalactic astronomy and thus inspire many scientists and engineers in other fields.Read moreRead less
International partnership in robotic astronomy and gravitational wave data analysis using a supercomputer. The project is aimed at providing student participation in frontier research using robotic astronomy and novel data analysis methods. It will focus on the study of the most violent explosions in the Universe - cosmological gamma ray bursts. These cataclysmic events possibly herald the formation of the most exotic objects in the Universe - black holes. It provides an exciting opportunity for ....International partnership in robotic astronomy and gravitational wave data analysis using a supercomputer. The project is aimed at providing student participation in frontier research using robotic astronomy and novel data analysis methods. It will focus on the study of the most violent explosions in the Universe - cosmological gamma ray bursts. These cataclysmic events possibly herald the formation of the most exotic objects in the Universe - black holes. It provides an exciting opportunity for students to be trained in robotic astronomy, supercomputing, image analysis and signal processing.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0775621
Funder
Australian Research Council
Funding Amount
$494,000.00
Summary
Mileura Widefield Array: A New Low Frequency Telescope. A new radio-quiet site for international radio astronomy is being developed at Mileura in Western Australia. We have constructed a low frequency test array on the site, and established that the site is excellent for radio astronomy. We plan to build a telescope which will observe the early universe, when stars and galaxies where first born. This will be the first telescope capable of this type of measurement of the early universe. In addi ....Mileura Widefield Array: A New Low Frequency Telescope. A new radio-quiet site for international radio astronomy is being developed at Mileura in Western Australia. We have constructed a low frequency test array on the site, and established that the site is excellent for radio astronomy. We plan to build a telescope which will observe the early universe, when stars and galaxies where first born. This will be the first telescope capable of this type of measurement of the early universe. In addition, the telescope will measure the solar wind, and its potential interactions with the earth.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0882938
Funder
Australian Research Council
Funding Amount
$1,430,000.00
Summary
MIRA Widefield Array: a new low frequency telescope. A new radio-quiet site for international radio astronomy is being developed at Boolardy in Western Australia. We have constructed a low frequency test array on the site, and established that the site is excellent for radio astronomy. We plan to build a telescope which will observe the early universe, when stars and galaxies where first born. This will be the first telescope capable of this type of measurement of the early universe. In additi ....MIRA Widefield Array: a new low frequency telescope. A new radio-quiet site for international radio astronomy is being developed at Boolardy in Western Australia. We have constructed a low frequency test array on the site, and established that the site is excellent for radio astronomy. We plan to build a telescope which will observe the early universe, when stars and galaxies where first born. This will be the first telescope capable of this type of measurement of the early universe. In addition, the telescope will measure the solar wind, and its potential interactions with the Earth. Read moreRead less
The astrophysical stochastic background of gravitational waves and detection by advanced high optical power interferometers: an Australia-US collaboration. The proposed project is designed to enable one of the most exciting and least studied components of the gravitational wave spectrum, the Astrophysical Gravitational wave Background (AGB), to be detected by Advanced LIGO. It will extend the Australia-US collaboration in Advanced LIGO to include modeling, simulation and detection methods of the ....The astrophysical stochastic background of gravitational waves and detection by advanced high optical power interferometers: an Australia-US collaboration. The proposed project is designed to enable one of the most exciting and least studied components of the gravitational wave spectrum, the Astrophysical Gravitational wave Background (AGB), to be detected by Advanced LIGO. It will extend the Australia-US collaboration in Advanced LIGO to include modeling, simulation and detection methods of the AGB and the study of the optical noise in LIGO and Advanced LIGO type systems. In particular we plan to search for anomalous noise sources and, especially those arising in high optical power cavities that could limit detection of the AGB.Read moreRead less
A deep survey for compact structure in the nearby universe: key science for the upgraded Australian Long Baseline Array. This project uses advances in ICT to build a national and international network of facilities that includes existing telescopes primarily on the east coast of Australia, as well as planned facilities in Western Australia and New Zealand. One of these facilities, the New Technology Demonstrator, is a crucial part of Australia's roadmap to the Square Kilometre Array. The SKA-r ....A deep survey for compact structure in the nearby universe: key science for the upgraded Australian Long Baseline Array. This project uses advances in ICT to build a national and international network of facilities that includes existing telescopes primarily on the east coast of Australia, as well as planned facilities in Western Australia and New Zealand. One of these facilities, the New Technology Demonstrator, is a crucial part of Australia's roadmap to the Square Kilometre Array. The SKA-related science and technology demonstrations we will undertake as part of this project will contribute to Australia's bid to host this $US1b instrument. This project cements a significant Trans-Tasman collaboration and brings together researchers in astrophysics and ICT to give Australia a leading position in the field of eVLBI.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0561104
Funder
Australian Research Council
Funding Amount
$402,128.00
Summary
A 10 Gbit/s Fibre Optic link to the Mt Pleasant and Mt Canopus Observatories. A 10 gigabit per second fibre optic link to the Mt Pleasant and Mt Canopus observatories will enable a wide range of new and exciting research opportunities. Very long baseline interferometry (VLBI) allows imaging of distant astronomical objects with much higher resolution than any other technique. The proposed fibre optic link will revolutionise Australia's VLBI capability, giving it the world's most sensitive array, ....A 10 Gbit/s Fibre Optic link to the Mt Pleasant and Mt Canopus Observatories. A 10 gigabit per second fibre optic link to the Mt Pleasant and Mt Canopus observatories will enable a wide range of new and exciting research opportunities. Very long baseline interferometry (VLBI) allows imaging of distant astronomical objects with much higher resolution than any other technique. The proposed fibre optic link will revolutionise Australia's VLBI capability, giving it the world's most sensitive array, with enhanced reliability and faster access to results for researchers. This project will greatly facilitate studies of astrophysical processes in Galactic and extra-galactic environments as well as precision measurements of the Earth's crustal dynamics.Read moreRead less