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Australian State/Territory : WA
Research Topic : Instrumentation
Field of Research : Signal Processing
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  • Funded Activity

    Discovery Projects - Grant ID: DP0877550

    Funder
    Australian Research Council
    Funding Amount
    $508,000.00
    Summary
    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.
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    Funded Activity

    Discovery Early Career Researcher Award - Grant ID: DE140100316

    Funder
    Australian Research Council
    Funding Amount
    $325,515.00
    Summary
    Seeing in the dark: measuring the signature of the early Universe with low-frequency radio telescopes. This project will detect and measure the signature of the first ionising sources in the early Universe. It uses a unique intersection of information theory and analysis methodology to design and implement a method of extracting the faint neutral hydrogen signal of reionisation from complex datasets. The hydrogen structure around these first light sources will be measured using data from the Mur .... Seeing in the dark: measuring the signature of the early Universe with low-frequency radio telescopes. This project will detect and measure the signature of the first ionising sources in the early Universe. It uses a unique intersection of information theory and analysis methodology to design and implement a method of extracting the faint neutral hydrogen signal of reionisation from complex datasets. The hydrogen structure around these first light sources will be measured using data from the Murchison Widefield Array telescope in Western Australia, revealing the signature of reionisation for the first time. Measurement of this signal constrains our understanding of the large-scale evolution of the Universe, defines properties of the first generation of stars and galaxies, and expands our understanding of the full history of the Universe.
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    Funded Activity

    Discovery Early Career Researcher Award - Grant ID: DE160100849

    Funder
    Australian Research Council
    Funding Amount
    $326,637.00
    Summary
    Measuring the Universe’s early evolution using lunar occultations. This project seeks to measure a radio signal for the first time, using the Murchison Widefield Array telescope and a novel technique involving the Moon, to learn what luminous objects dominated the early Universe. There is an entire period in the early Universe that remains unobserved because familiar objects such as stars and galaxies have yet to form. One of the few observables from this period, and the time directly following .... Measuring the Universe’s early evolution using lunar occultations. This project seeks to measure a radio signal for the first time, using the Murchison Widefield Array telescope and a novel technique involving the Moon, to learn what luminous objects dominated the early Universe. There is an entire period in the early Universe that remains unobserved because familiar objects such as stars and galaxies have yet to form. One of the few observables from this period, and the time directly following it, is the radio signal emitted by neutral hydrogen atoms. Innovative analysis techniques may be developed and new training pathways for astronomers should be initiated. The Project aims to raise Australia’s scientific profile and engage the public, promoting astronomy by making results accessible and using the Moon as a familiar foundation.
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