Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100201
Funder
Australian Research Council
Funding Amount
$530,000.00
Summary
A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will ....A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will enable it to make detailed observations of initial discoveries made with the Australian Square Kilometre Array Pathfinder and other Australian telescopes. In short, it will enable Australian researchers to do more ambitious research, and make more discoveries, across broad areas of astrophysics.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100094
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
The Mopra Radio Telescope. The Mopra Radio Telescope:
This project aims to use Australia’s Mopra Radio Telescope – the largest millimetre-wave dish in the southern hemisphere – to complete a survey of the distribution of molecular gas across the southern Milky Way. The millimetre-wavelength sky holds the key for understanding molecular clouds in which stars are born, and the Mopra Telescope is the world’s most capable facility for imaging these clouds. The expected outcome is an order of magnit ....The Mopra Radio Telescope. The Mopra Radio Telescope:
This project aims to use Australia’s Mopra Radio Telescope – the largest millimetre-wave dish in the southern hemisphere – to complete a survey of the distribution of molecular gas across the southern Milky Way. The millimetre-wavelength sky holds the key for understanding molecular clouds in which stars are born, and the Mopra Telescope is the world’s most capable facility for imaging these clouds. The expected outcome is an order of magnitude improvement in the clarity of our view of this central component of the Galaxy. The project also aims to enable Mopra to serve as a key element in the Australian Long Baseline Array. The project aims to ensure Australian involvement in three grand design international endeavours.Read moreRead less
Radio Interferometer Studies of Compact Astronomical Sources. The giant black holes in the centres of distant galaxies that are the topic of this study are used to set the reference frame for geodesy on the earth. Remote and exotic as they are, they have real-world applications such as improving the positions available from GPS receivers and measuring continental drift. The signal processing equipment being developed for this new telescope is based on FPGA (field programmable gate array) chips ....Radio Interferometer Studies of Compact Astronomical Sources. The giant black holes in the centres of distant galaxies that are the topic of this study are used to set the reference frame for geodesy on the earth. Remote and exotic as they are, they have real-world applications such as improving the positions available from GPS receivers and measuring continental drift. The signal processing equipment being developed for this new telescope is based on FPGA (field programmable gate array) chips, that promise to revolutionize the data processing industry, from radar to cellular telephones to computer networks. The young scientists who are working on this project will go on to lead the commercial and industrial applications of this new technology.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100055
Funder
Australian Research Council
Funding Amount
$275,000.00
Summary
Hidden Earths and distant Suns: a new optical astronomy observatory in Tasmania. This facility at the University of Tasmania will be a remotely operable 1.3 metre optical telescope with a suite of powerful scientific cameras. It will be used to hunt for Earth-like planets around other stars and to study the variability of stars like the Sun, helping to answer fundamental questions about the Universe and our place in it.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100105
Funder
Australian Research Council
Funding Amount
$570,000.00
Summary
Broadband receivers for AuScope geodetic and astronomical applications . Broadband receivers for AuScope geodetic and astronomical applications: This project aims to develop an innovative broadband receiver system which will be deployed on the AuScope array of radio telescopes. This will enable the telescopes to play a key role in improving precision navigation both in Australia and throughout the Southern Hemisphere. The new receiver systems will significantly improve the capability of these fa ....Broadband receivers for AuScope geodetic and astronomical applications . Broadband receivers for AuScope geodetic and astronomical applications: This project aims to develop an innovative broadband receiver system which will be deployed on the AuScope array of radio telescopes. This will enable the telescopes to play a key role in improving precision navigation both in Australia and throughout the Southern Hemisphere. The new receiver systems will significantly improve the capability of these facilities for both geodetic and astronomical investigations. Improvements to the accuracy of the terrestrial reference frame in Australia will allow more accurate measurements of changes in sea level, while high precision astrometric observations undertaken with the new receivers will be used to determine the structure of our Milky Way Galaxy.Read moreRead less
New separation technologies for profiling metabolites in biological samples. Metabolomics is an important new field of science that is contributing to the understanding of life processes at the molecular level. But a widely acknowledged major limitation of current metabolomics technologies is the inability to accurately identify high numbers of detected metabolites in the biological extracts being studied. This project will develop cutting-edge separation science approaches to address this exist ....New separation technologies for profiling metabolites in biological samples. Metabolomics is an important new field of science that is contributing to the understanding of life processes at the molecular level. But a widely acknowledged major limitation of current metabolomics technologies is the inability to accurately identify high numbers of detected metabolites in the biological extracts being studied. This project will develop cutting-edge separation science approaches to address this existing problem in metabolomics analysis. In doing so it will provide enormous benefit to Australian biotechnology and biomedical research and play a major role in transferring capabilities to laboratories and research institutes that are involved in research aimed at elucidating biological pathways and networks.Read moreRead less
Creating a national time and frequency network for Australia. This project will develop the means to distribute accurate time and frequency across the Australian continent via an optical fibre network. This network will meet the needs of future telecommunications, science and astronomy projects including the Australian bid for the Square Kilometre Array radio-astronomy project.
Masers: high resolution probes of star formation. The largest stars in the Galaxy play a vital role in the formation of
the atoms which make life on Earth possible. The birth of these stars
is shrouded in gas and dust through which only radiowaves penetrate.
In this project we will make observations of interstellar masers from
the hydroxyl and methanol molecules and through mathematical modelling
of molecular excitation and radiative transfer probe the physical,
chemical and evolution ....Masers: high resolution probes of star formation. The largest stars in the Galaxy play a vital role in the formation of
the atoms which make life on Earth possible. The birth of these stars
is shrouded in gas and dust through which only radiowaves penetrate.
In this project we will make observations of interstellar masers from
the hydroxyl and methanol molecules and through mathematical modelling
of molecular excitation and radiative transfer probe the physical,
chemical and evolutionary status of the high-mass stars associated
with the masers.Read moreRead less
The scale and structure of the Milky Way. This project aims to use new Australian infrastructure to make the most accurate distance measurements to date in the southern Milky Way, completing the three-dimensional picture of our Galaxy. Australia's international standing in astronomy has led to it being one of the host countries for the square kilometre array project, which will bring significant economic and technological benefits to the country. This project builds upon Australia's astronomical ....The scale and structure of the Milky Way. This project aims to use new Australian infrastructure to make the most accurate distance measurements to date in the southern Milky Way, completing the three-dimensional picture of our Galaxy. Australia's international standing in astronomy has led to it being one of the host countries for the square kilometre array project, which will bring significant economic and technological benefits to the country. This project builds upon Australia's astronomical expertise and will provide the most accurate picture to date of the Milky Way. Astronomy provides unique opportunities for engaging the community in discussions of science and society and inspires students to study STEM subjects.Read moreRead less
A survey of the interstellar medium in the Milky Way and Magellanic Clouds using the Australian Square Kilometre Array Pathfinder. Between the stars in the Milky Way there are clouds of gas and dust; old stars eject heavy elements into this interstellar medium, and new stars form when interstellar clouds collapse under their own gravity. This survey is making maps of the interstellar gas using spectral lines at radio wavelengths to trace the cycle of star formation.