International collaboration in gravitational wave data analysis, simulations and third generation detectors. The project brings together seven outstanding international researchers into close collaboration with an Australian team to develop new techniques for finding gravitational wave signals in the vast archive of data they have helped to collect, as well as developing and testing theory for improved detectors that operate with sensitivity beyond the limits set by classical physics. The projec ....International collaboration in gravitational wave data analysis, simulations and third generation detectors. The project brings together seven outstanding international researchers into close collaboration with an Australian team to develop new techniques for finding gravitational wave signals in the vast archive of data they have helped to collect, as well as developing and testing theory for improved detectors that operate with sensitivity beyond the limits set by classical physics. The project will utilize a state of the art supercomputer and the superb national facility for high power laser interferometry at Gingin, Western Australia. 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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Real-Time Searches for Gravitational Waves and Identification of Their Radio and Optical Counterparts. The proposed project will directly address the national research priority in development of frontier technologies, directly involve Australians in frontier work in gravitational wave astronomy that will result in break-through sciences and improve the chance of the international Square-Kilometer-Array project being sited at Australia. In addition, it will foster a close collaboration of top int ....Real-Time Searches for Gravitational Waves and Identification of Their Radio and Optical Counterparts. The proposed project will directly address the national research priority in development of frontier technologies, directly involve Australians in frontier work in gravitational wave astronomy that will result in break-through sciences and improve the chance of the international Square-Kilometer-Array project being sited at Australia. In addition, it will foster a close collaboration of top international researchers with an Australian team. The research at The University of Western Australia will attract students from around the world and serve to educate and inspire young people in Australia.Read moreRead less
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
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
Precision Pulsar Timing and its Applications. The rapidly rotating pulsars known as millisecond pulsars have period stabilities which rival that of the best terrestrial clocks. Observations of many millisecond pulsars spread across the sky should allow detection of the gravitational-wave background - likely to be the first direct detection of gravity waves. It will also enable establishment of a long-term time standard which is independent of and probably superior to that derived from terrestria ....Precision Pulsar Timing and its Applications. The rapidly rotating pulsars known as millisecond pulsars have period stabilities which rival that of the best terrestrial clocks. Observations of many millisecond pulsars spread across the sky should allow detection of the gravitational-wave background - likely to be the first direct detection of gravity waves. It will also enable establishment of a long-term time standard which is independent of and probably superior to that derived from terrestrial clocks. New analysis techniques and establishment of an international observing network will be required. Investigation and application of techniques for overcoming radio interference will be an important part of the project.Read moreRead less
Defeating Radio Frequency Interference. The radio spectrum is a valuable resource. Development of techniques which minimize the impact of various users on one another, allowing this resource to be shared, will benefit the entire community. For astronomy in particular, shared use is essential because of the very wide bandwidths needed to obtain sufficient sensitivity. Usage of the radio spectrum is increasing rapidly and radio telescopes are becoming more and more sensitive, compounding the probl ....Defeating Radio Frequency Interference. The radio spectrum is a valuable resource. Development of techniques which minimize the impact of various users on one another, allowing this resource to be shared, will benefit the entire community. For astronomy in particular, shared use is essential because of the very wide bandwidths needed to obtain sufficient sensitivity. Usage of the radio spectrum is increasing rapidly and radio telescopes are becoming more and more sensitive, compounding the problems. The digital signal processing techniques developed under this project will be widely applicable, not only to future radio astronomy facilities such as the Square Kilometer Array, but also to the communications industry generally.Read moreRead less