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: LE200100096
Funder
Australian Research Council
Funding Amount
$1,150,000.00
Summary
A next-generation receiver for Radio Astronomy. This project will provide a next-generation radio astronomy receiver to be used on the Parkes radio telescope. This facility will provide a major increase in performance, particularly in sensitivity and survey speed. The science goals are to better understand the ionized and neutral components of the cosmic web, and their evolution, through observations of Fast Radio Bursts and neutral hydrogen. Advances in the understanding of pulsars, molecules, ....A next-generation receiver for Radio Astronomy. This project will provide a next-generation radio astronomy receiver to be used on the Parkes radio telescope. This facility will provide a major increase in performance, particularly in sensitivity and survey speed. The science goals are to better understand the ionized and neutral components of the cosmic web, and their evolution, through observations of Fast Radio Bursts and neutral hydrogen. Advances in the understanding of pulsars, molecules, radio galaxies and cosmic rays will also be achieved with this facility. The technology is based on cryogenic cooling of a large phased array feed. This receiver is a major advance over existing receivers on the Parkes and Australian SKA Pathfinder (ASKAP) telescopes.Read moreRead less
Noise-free Cryogenic Wavefront Sensing. This project aims to optimise the prototype adaptive optics technology for the Giant Magellan Telescope (GMT) by leveraging past investment in adaptive optics instrumentation and shortwave infrared detector systems. This project expects to generate significant improvements in GMT performance, with ten times greater image resolution than the Hubble Space Telescope and current estimates of >90% sky coverage, compared with ~50% coverage for current technology ....Noise-free Cryogenic Wavefront Sensing. This project aims to optimise the prototype adaptive optics technology for the Giant Magellan Telescope (GMT) by leveraging past investment in adaptive optics instrumentation and shortwave infrared detector systems. This project expects to generate significant improvements in GMT performance, with ten times greater image resolution than the Hubble Space Telescope and current estimates of >90% sky coverage, compared with ~50% coverage for current technology. Expected outcomes of this project include the development of a highly trained workforce and continued international collaboration in the field of high-technology sensor systems. This contribution to the GMT will provide significant benefits—it will change the way we view the Universe.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100165
Funder
Australian Research Council
Funding Amount
$792,859.00
Summary
Veloce Verde+Azzuro - Tripling the Power of Australia's Planet Foundry. This project aims to better understand humanity’s place in the Universe, including questions such as whether we are alone or if our home in the Solar System is unique or common. This project will enable new observations using a revolutionary Australian facility, Veloce Verde+Azzuro. Moving beyond discovering habitable planets around dim red stars, it will enable science on the properties and system architectures of planets o ....Veloce Verde+Azzuro - Tripling the Power of Australia's Planet Foundry. This project aims to better understand humanity’s place in the Universe, including questions such as whether we are alone or if our home in the Solar System is unique or common. This project will enable new observations using a revolutionary Australian facility, Veloce Verde+Azzuro. Moving beyond discovering habitable planets around dim red stars, it will enable science on the properties and system architectures of planets orbiting stars like the Sun. It will deliver a ten-fold increase in collecting power for Sun-like stars, providing understanding of how exoplanetary systems, and our Solar System, were formed.Read moreRead less
Galactic seismology: a new window on Milky Way's evolution. This project aims to investigate how the Milky Way responds to the passage of a small dwarf galaxy through its plane. This is motivated by the observational discovery of largescale waves crossing the Milky Way disc, and by new related supercomputer simulations. The project expects to generate new knowledge in this field, based on further supercomputer simulations and comparison of the predictions with new data from the Gaia space missio ....Galactic seismology: a new window on Milky Way's evolution. This project aims to investigate how the Milky Way responds to the passage of a small dwarf galaxy through its plane. This is motivated by the observational discovery of largescale waves crossing the Milky Way disc, and by new related supercomputer simulations. The project expects to generate new knowledge in this field, based on further supercomputer simulations and comparison of the predictions with new data from the Gaia space mission. Expected outcomes of the project include a demonstration of the diagnostic power of this new seismological approach to galaxy evolution. The project promises significant benefits in the form of establishing Australia as a leader in Galactic seismology, as it is in the field of Galactic archaeology.
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