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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE100100111
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
A database for Australian optical astronomy. We will build an astronomy data facility to provide database facilities to analyse data from three major Australian optical astronomy projects, SkyMapper, WiggleZ and GAMA. The facility will provide efficient analysis tools not only for the researchers immediately involved with the projects, but, for the entire national and international astronomical community when the data become public. Long-term maintenance of the facility is vital, so the facilit ....A database for Australian optical astronomy. We will build an astronomy data facility to provide database facilities to analyse data from three major Australian optical astronomy projects, SkyMapper, WiggleZ and GAMA. The facility will provide efficient analysis tools not only for the researchers immediately involved with the projects, but, for the entire national and international astronomical community when the data become public. Long-term maintenance of the facility is vital, so the facility will be standards-compliant and stable to facilitate long-term support. For this reason the facility will be based at the ANU Supercomputer Facility (ANUSF) to leverage substantial expertise in this area and to provide long-term operations support.Read moreRead less
Early Evolution of the Solar System: A Planetary Perspective. A geochemical study of early solar system materials will be conducted to investigate physical conditions leading to assembly of the terrestrial planets, and the chronology of early geological events that shaped the Earth and Moon. Objects from the solar nebula and samples from the Earth, Moon, Mars, and differentiated asteroids will be studied. This research will contribute toward understanding the astrophysical environment of the inn ....Early Evolution of the Solar System: A Planetary Perspective. A geochemical study of early solar system materials will be conducted to investigate physical conditions leading to assembly of the terrestrial planets, and the chronology of early geological events that shaped the Earth and Moon. Objects from the solar nebula and samples from the Earth, Moon, Mars, and differentiated asteroids will be studied. This research will contribute toward understanding the astrophysical environment of the inner solar system, establish a high-resolution absolute timescale for early geological events, and Identify the population of solid bodies present during the initial stages of planetary development.Read moreRead less
Lithic Astronomy: The age and origin of the elements and their incorporation in the solar nebula. All heavy elements are produced in stars. The signature of nucleosynthesis is the isotopic composition of the elements and thus measurement of isotopic compositions allows nuclear astrophysics to be elucidated in the laboratory. This project will examine the linkages between stellar sites and the material in our solar system through measurement of interstellar grains and other primitive material ob ....Lithic Astronomy: The age and origin of the elements and their incorporation in the solar nebula. All heavy elements are produced in stars. The signature of nucleosynthesis is the isotopic composition of the elements and thus measurement of isotopic compositions allows nuclear astrophysics to be elucidated in the laboratory. This project will examine the linkages between stellar sites and the material in our solar system through measurement of interstellar grains and other primitive material obtained from meteorites. A chronology of processes affecting the solar nebula will be determined through measurement of radionuclides. Th/U measurements in presolar grains could allow a view of galactic chemical evolution billions of years prior to the solar nebula.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100031
Funder
Australian Research Council
Funding Amount
$1,000,000.00
Summary
Expanding our view of the Universe with the Murchison Widefield Array. Expanding our view of the Universe with the Murchison Widefield Array:
This project aims to build a Phase 2 Murchison Widefield Array (MWA) to boost the capabilities of the Phase 1 MWA by an order of magnitude. The Epoch of Reionisation (EoR), when the first stars and galaxies lit up the universe, is the last unstudied phase of cosmic evolution. The MWA is at the frontier of EoR research and all-sky survey astrophysics, is t ....Expanding our view of the Universe with the Murchison Widefield Array. Expanding our view of the Universe with the Murchison Widefield Array:
This project aims to build a Phase 2 Murchison Widefield Array (MWA) to boost the capabilities of the Phase 1 MWA by an order of magnitude. The Epoch of Reionisation (EoR), when the first stars and galaxies lit up the universe, is the last unstudied phase of cosmic evolution. The MWA is at the frontier of EoR research and all-sky survey astrophysics, is the only low frequency precursor for the Square Kilometre Array (SKA), and is the only SKA precursor delivering science quality data. This project to construct a Phase 2 MWA would double the number of antennas in the array, double the maximum baseline length, and boost our all-sky survey and EoR capabilities. Read moreRead less
Probing the Universe with gravitational waves: from cutting-edge technology to astronomy. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in ....Probing the Universe with gravitational waves: from cutting-edge technology to astronomy. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in areas of national priority, including frontier technologies such as photonics and smart information use through GRID computing. Developing ways to build instruments of almost unimaginable sensitivity fosters innovation leading to spin-offs into other areas of optical sensing - fundamental research resulting in economic benefit.Read moreRead less
The origin of the elements heavier than iron. This research investigates the cosmic origin of the elements heavier than iron, as they are produced by nuclear reactions inside stars. The study of these elements in stars and meteorites will help us to understand the origin and history of the Solar System, of old stars and of stellar clusters and galaxies.
Pushing the frontiers of gravitational wave science: from technology to astrophysics. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in ar ....Pushing the frontiers of gravitational wave science: from technology to astrophysics. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in areas of national priority, including frontier technologies such as photonics and smart information use through GRID computing. Developing ways to build instruments of almost unimaginable sensitivity fosters innovation leading to spin-offs into other areas of optical sensing - fundamental research resulting in economic benefit.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989093
Funder
Australian Research Council
Funding Amount
$1,800,000.00
Summary
Australian Partnership in Advanced LIGO. Advanced Interferometer Gravitational-Wave Observatory (LIGO) (AdvLIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. The development of instruments capable of doing this is driving technology in fields such as lasers , optics, photonics and data analysis. By playing a key role in this facility, Australia will reap the scienti ....Australian Partnership in Advanced LIGO. Advanced Interferometer Gravitational-Wave Observatory (LIGO) (AdvLIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. The development of instruments capable of doing this is driving technology in fields such as lasers , optics, photonics and data analysis. By playing a key role in this facility, Australia will reap the scientific and technical rewards of being part of the most exciting frontier of physics in the 21st Century whilst training scientists and technologists for tomorrow.Read moreRead less
Photochemistry of the Middle Atmospheres of Venus and the Earth. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand the processes that control atmospheric chemistry. The proposed research will improve the fidelity of photochemical models, provide additional insight into the recent evolution of the Venus atmosphere, and examine how atmospheric chemistry and climate change interact(ed) on Venus. This research will improve our understanding of l ....Photochemistry of the Middle Atmospheres of Venus and the Earth. Ongoing changes in the Earth's atmosphere, such as ozone depletion, demonstrate the need to understand the processes that control atmospheric chemistry. The proposed research will improve the fidelity of photochemical models, provide additional insight into the recent evolution of the Venus atmosphere, and examine how atmospheric chemistry and climate change interact(ed) on Venus. This research will improve our understanding of long-standing issues, such as how much water might have been present on Venus in the recent past. The research program will provide an opportunity for Australian science to participate in at least one spacecraft mission to Venus. Read moreRead less