Probing the Tasmanian Devil Serum Proteome for Preclinical Diagnosis of Devil Facial Tumour Disease. The Tasmanian Devil (Sarcophilus harrisii) is a carnivorous marsupial endemic to the island state of Tasmania, and is found all over the state. Over the past decade, a dramatic decline has occurred in the Devil population in association with the emergence of Devil Facial Tumour Disease (DFTD). This project aims to develop a preclinical diagnostic test for DFTD that will provide vital information ....Probing the Tasmanian Devil Serum Proteome for Preclinical Diagnosis of Devil Facial Tumour Disease. The Tasmanian Devil (Sarcophilus harrisii) is a carnivorous marsupial endemic to the island state of Tasmania, and is found all over the state. Over the past decade, a dramatic decline has occurred in the Devil population in association with the emergence of Devil Facial Tumour Disease (DFTD). This project aims to develop a preclinical diagnostic test for DFTD that will provide vital information for use in developing management strategies to ensure the ongoing survival of the Tasmanian Devil. The benefit to Australia in performing this research rests in the new technology that will be developed and the application of this technology to key areas of national and international significance.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
Improving Signal Detection Range of Active Seismic Monitoring in Mines. This project will develop a new generation of sensors that will process incoming seismic waves from an active source to accurately estimate the properties of underground rock mass in real time. This will lead to safer mining operations that will decrease the number of injuries and deaths. A probability graph model will be used to fuse measurements from different sensors to produce more accurate estimates of the rock mass. A ....Improving Signal Detection Range of Active Seismic Monitoring in Mines. This project will develop a new generation of sensors that will process incoming seismic waves from an active source to accurately estimate the properties of underground rock mass in real time. This will lead to safer mining operations that will decrease the number of injuries and deaths. A probability graph model will be used to fuse measurements from different sensors to produce more accurate estimates of the rock mass. A new low-cost seismic source will excite large areas of rock mass for continuous monitoring of the changes in stress and fracture density caused by mining. This will lead to methodologies that will significantly improve mining operations and increase Australia’s productivity in the mining sector.Read moreRead less