Linkage Infrastructure, Equipment And Facilities - Grant ID: LE140100013
Funder
Australian Research Council
Funding Amount
$300,000.00
Summary
A sensitive tip-tilt wave-front sensor for the multi-conjugate adaptive-optics system on the Gemini south telescope. A sensitive tip-tilt wavefront sensor for the multi-conjugate adaptive-optics system on the Gemini South telescope: This project will construct a sensitive tip-tilt wavefront sensor for GeMS, the multi-conjugate adaptive-optics system on the Gemini South telescope in Chile. GeMS is a unique and revolutionary new system that delivers near-infrared images at similar resolution to th ....A sensitive tip-tilt wave-front sensor for the multi-conjugate adaptive-optics system on the Gemini south telescope. A sensitive tip-tilt wavefront sensor for the multi-conjugate adaptive-optics system on the Gemini South telescope: This project will construct a sensitive tip-tilt wavefront sensor for GeMS, the multi-conjugate adaptive-optics system on the Gemini South telescope in Chile. GeMS is a unique and revolutionary new system that delivers near-infrared images at similar resolution to the Hubble Space Telescope at optical wavelengths over wide fields. With this improvement in technology it will be possible to do this on much fainter objects than is currently possible using this new wave-front sensor. This will allow GeMS to routinely study the morphologies of external galaxies at high angular resolution - greatly extending its science scope. Sharper images will also be obtained for all objects that are currently accessible, leading to higher quality science data.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100087
Funder
Australian Research Council
Funding Amount
$760,000.00
Summary
Veloce - Australia's Next-Generation Planet Foundry. Veloce - Australia's next-generation planet foundry: This project will deliver to Australian astronomers a high-resolution, ultra-stabilised, red-wavelength-optimised spectrograph capable of delivering high-precision doppler velocities for the transiting exoplanet host-stars being discovered now by southern hemisphere transit-planet searches, and for the coming wave of discoveries to be made by NASA's Transiting Exoplanet Survey Satellite (TES ....Veloce - Australia's Next-Generation Planet Foundry. Veloce - Australia's next-generation planet foundry: This project will deliver to Australian astronomers a high-resolution, ultra-stabilised, red-wavelength-optimised spectrograph capable of delivering high-precision doppler velocities for the transiting exoplanet host-stars being discovered now by southern hemisphere transit-planet searches, and for the coming wave of discoveries to be made by NASA's Transiting Exoplanet Survey Satellite (TESS). In addition it will enable a vast suite of new research programs in exoplanetary science and galactic archaeology, as well as providing a sound base of ultra-stable infrastructure enabling future expansion to cover the full optical wavelength range at minimal cost.Read moreRead less
The Galaxy Genome Project 2. The Galaxy Genome Project builds on the Anglo-Australian Observatory's (AAO) major investments and world-leading strengths in wide-field survey astronomy and multi-object spectrographs. Combining the AAO's ongoing and planned survey programs with data from other new Australian facilities, such as SkyMapper and Australian Square Kilometre Array Pathfinder, will increase the scientific productivity and impact of all of these major Australian investments and leverage ac ....The Galaxy Genome Project 2. The Galaxy Genome Project builds on the Anglo-Australian Observatory's (AAO) major investments and world-leading strengths in wide-field survey astronomy and multi-object spectrographs. Combining the AAO's ongoing and planned survey programs with data from other new Australian facilities, such as SkyMapper and Australian Square Kilometre Array Pathfinder, will increase the scientific productivity and impact of all of these major Australian investments and leverage access for Australian researchers in other leading international astronomical surveys and facilities. The project will also increase the international profile of Australian astronomy and enhance the prospects of Australian scientific and technical involvement in next-generation astronomical facilities such as Square Kilometre Array and Giant Magellan Telescope.Read moreRead less
The Galaxy Genome Project 1. The Galaxy Genome Project builds on the Anglo-Australian Observatory's (AAO) major investments and world-leading strengths in wide-field survey astronomy and multi-object spectrographs. Combining the AAO's ongoing and planned survey programs with data from other new Australian facilities, such as SkyMapper and Australian Square Kilometre Array Pathfinder, this project will increase the scientific productivity and impact of all of these major Australian investments an ....The Galaxy Genome Project 1. The Galaxy Genome Project builds on the Anglo-Australian Observatory's (AAO) major investments and world-leading strengths in wide-field survey astronomy and multi-object spectrographs. Combining the AAO's ongoing and planned survey programs with data from other new Australian facilities, such as SkyMapper and Australian Square Kilometre Array Pathfinder, this project will increase the scientific productivity and impact of all of these major Australian investments and leverage access for Australian researchers in other leading international astronomical surveys and facilities. The project will also increase the international profile of Australian astronomy and enhance the prospects of Australian scientific and technical involvement in next-generation astronomical facilities such as Square Kilometre Array and Giant Magellan Telescope.Read moreRead less
Large-scale maps of the universe: Enabling wide-field science with the Australian Square Kilometre Array Pathfinder and the Square Kilometre Array. Observational capabilities in astronomy continue to make great advances across the electromagnetic spectrum. The first truly global facility for radio astronomy will be the Square Kilometre Array (SKA), an international $2.5 billion project scheduled for deployment between 2015 and 2020, for which the proposed Australian site has been short-listed. T ....Large-scale maps of the universe: Enabling wide-field science with the Australian Square Kilometre Array Pathfinder and the Square Kilometre Array. Observational capabilities in astronomy continue to make great advances across the electromagnetic spectrum. The first truly global facility for radio astronomy will be the Square Kilometre Array (SKA), an international $2.5 billion project scheduled for deployment between 2015 and 2020, for which the proposed Australian site has been short-listed. The Australian SKA Pathfinder (ASKAP) is a next generation radio telescope that is on the strategic pathway towards the staged development and deployment of the SKA. By refining the ASKAP technology and enabling its scientific success we address the national strategic goal of ensuring Australia's technological and scientific readiness for the SKA.Read moreRead less
Peering through the Dark Ages with the Murchison Widefield Array. There is one large gap in our understanding of the early evolution of the universe, namely, when did the first sources of light appear? Resolution of this puzzle requires new observational and technical strategies, both in terms of telescopes and the analysis of observations. The Murchison Widefield Array, a major new radio telescope in Western Australia, is an international initiative under construction to tackle the problem. Thi ....Peering through the Dark Ages with the Murchison Widefield Array. There is one large gap in our understanding of the early evolution of the universe, namely, when did the first sources of light appear? Resolution of this puzzle requires new observational and technical strategies, both in terms of telescopes and the analysis of observations. The Murchison Widefield Array, a major new radio telescope in Western Australia, is an international initiative under construction to tackle the problem. This program will provide a significant Australian contribution at the forefront of modern cosmology.Read moreRead less
The morphological evolution of galaxies over cosmic time. Present-day galaxies look either red and round or blue and disc-like; this project will study galaxies that existed when the universe was one quarter its present age to understand how these different structures came about. To do this, the project will use a new high resolution near-infrared camera built at The Australian National University.
Interstellar Physics at the Epoch of Galaxy Formation. With large telescopes and major space observatories, we can finally reach back in time and see how galaxies were assembled in the first few billion years of our Universe. We need to determine how gas forms into stars, how massive black holes feed on and interact with their nascent galaxies, how heavy elements are produced, and how dust obscuration or re-radiation affects observations. This proposal brings a world-class team together to devel ....Interstellar Physics at the Epoch of Galaxy Formation. With large telescopes and major space observatories, we can finally reach back in time and see how galaxies were assembled in the first few billion years of our Universe. We need to determine how gas forms into stars, how massive black holes feed on and interact with their nascent galaxies, how heavy elements are produced, and how dust obscuration or re-radiation affects observations. This proposal brings a world-class team together to develop and apply new and unique pan-spectral tools based on physical models of the interstellar plasma and conceived to determine fundamental parameters of collapsing galaxies.Read moreRead less
The First Deep Infrared Study of the Nearby Galaxy Population. We will conduct two major near-infrared (IR) surveys: The Southern Galactic Cap near-IR survey, and the Local Sphere of Influence survey. These surveys will capitalise on the innovative and award winning Australian IRIS2 facility. The two surveys push the observational frontier by orders of magnitude. They will be used to explore the close connection between the near-IR global properties of a galaxy and its underlying physics and pro ....The First Deep Infrared Study of the Nearby Galaxy Population. We will conduct two major near-infrared (IR) surveys: The Southern Galactic Cap near-IR survey, and the Local Sphere of Influence survey. These surveys will capitalise on the innovative and award winning Australian IRIS2 facility. The two surveys push the observational frontier by orders of magnitude. They will be used to explore the close connection between the near-IR global properties of a galaxy and its underlying physics and provide a generic local reference for the upcoming next generation infrared space-telescope missions.
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Particle astrophysics with the Pierre Auger observatory. Australia's scientific reputation is enhanced through participation in international collaborations that aim to solve long-standing mysteries in science. The Pierre Auger Observatory covers a huge 3000 square km in western Argentina, where we are attempting to solve one of the biggest puzzles in modern astrophysics - the origin of the highest energy cosmic rays, particles 100 million times more energetic than we can produce on Earth. Ade ....Particle astrophysics with the Pierre Auger observatory. Australia's scientific reputation is enhanced through participation in international collaborations that aim to solve long-standing mysteries in science. The Pierre Auger Observatory covers a huge 3000 square km in western Argentina, where we are attempting to solve one of the biggest puzzles in modern astrophysics - the origin of the highest energy cosmic rays, particles 100 million times more energetic than we can produce on Earth. Adelaide scientists were founding members of the Auger project, and now have leading roles within the experiment. This is providing our students with access to world-class facilities and researchers in a field which has moved to the mainstream of astrophysics research.Read moreRead less