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
The worlds next door: terrestrial exoplanets with the TOLIMAN space mission. This project aims to to explore our nearest neighbour star system, Alpha Centauri, for the first time probing for exoplanets with physical characteristics that resemble those of Earth. The finding of any such world, with the potential to support a biosphere like our own and lying only 4 light-years away, would profoundly alter our view of our place in the universe. The primary outcome of this project will be the design, ....The worlds next door: terrestrial exoplanets with the TOLIMAN space mission. This project aims to to explore our nearest neighbour star system, Alpha Centauri, for the first time probing for exoplanets with physical characteristics that resemble those of Earth. The finding of any such world, with the potential to support a biosphere like our own and lying only 4 light-years away, would profoundly alter our view of our place in the universe. The primary outcome of this project will be the design, construction, launch and operation of a novel and innovative space telescope: the TOLIMAN mission. This profoundly benefits the Australian space and university sectors, partnering them with international agencies to deliver marquee science with global impact: the search for our first stepping stone to interstellar space.Read moreRead less
Utilising artificial intelligence to elucidate the physics of galaxies. For decades astronomers have puzzled over the connection between the structure and evolution of galaxies and the role played by host environments. This project aims to resolve this problem by combining multi-wavelength observations, multi-component simulations, and pioneering data analysis using artificial intelligence. In particular, we target the nearby Fornax galaxy cluster as a laboratory for studying galaxy formation in ....Utilising artificial intelligence to elucidate the physics of galaxies. For decades astronomers have puzzled over the connection between the structure and evolution of galaxies and the role played by host environments. This project aims to resolve this problem by combining multi-wavelength observations, multi-component simulations, and pioneering data analysis using artificial intelligence. In particular, we target the nearby Fornax galaxy cluster as a laboratory for studying galaxy formation in dense environments. Using our novel machine learning techniques, we will elucidate the physical mechanisms that drive the rapid evolution of star formation, galactic nuclei, and gas and dust content within Fornax. Our predictions will benefit ongoing and future surveys at the national and international level. Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE220100003
Funder
Australian Research Council
Funding Amount
$450,675.00
Summary
Understanding diversity: chemical and kinematic tracers of galaxy evolution. Understanding how galaxies form and evolve throughout the Universe is one of the biggest outstanding challenges in astrophysics. The project aims to develop an innovative method for understanding the fundamental properties of angular momentum and chemical content of all kinds of galaxies. This project expects to generate new knowledge in the field of galaxy evolution, for the first time enabling astronomers to robustly ....Understanding diversity: chemical and kinematic tracers of galaxy evolution. Understanding how galaxies form and evolve throughout the Universe is one of the biggest outstanding challenges in astrophysics. The project aims to develop an innovative method for understanding the fundamental properties of angular momentum and chemical content of all kinds of galaxies. This project expects to generate new knowledge in the field of galaxy evolution, for the first time enabling astronomers to robustly compare distant, long-ago galaxies with those in the nearby, present-day Universe. Expected outcomes include a novel framework for determining galaxy morphology, based on fundamental physics. The framework will be highly beneficial to understanding the evolution of diverse types of galaxies, including our own Milky Way.Read moreRead less
Catch me if you can: The race to rescue the smallest planets. This project will upgrade a unique Australian observatory to study the smallest planets around other stars, using an innovative new technique to provide high precision measurements capturing the tiny shadow of planets as they cross in front of their stars. The project aims to generate new knowledge on potentially Earth-like planets and contribute to the legacy of current and next-generation space telescopes. Expected outcomes include ....Catch me if you can: The race to rescue the smallest planets. This project will upgrade a unique Australian observatory to study the smallest planets around other stars, using an innovative new technique to provide high precision measurements capturing the tiny shadow of planets as they cross in front of their stars. The project aims to generate new knowledge on potentially Earth-like planets and contribute to the legacy of current and next-generation space telescopes. Expected outcomes include preserving a list of best planets for in-depth characterisations, and the first Australian facility to match the capability of space observatories: detecting planets as small as Earth. This project will benefit the international community by optimising the effort of future space telescopes.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE210101893
Funder
Australian Research Council
Funding Amount
$425,489.00
Summary
The Origins and Evolution of the Most Abundant Planets in our Galaxy. The majority of planetary systems around other stars are not like our Solar System. We now know that the most common types of exoplanets are super-Earths and Neptunes, planets with sizes ranging from Earth to Neptune, residing close to their parent stars. This project aims to characterise these planets at various stages of their evolution. This project will utilise Australian facilities to characterise new planets from the TES ....The Origins and Evolution of the Most Abundant Planets in our Galaxy. The majority of planetary systems around other stars are not like our Solar System. We now know that the most common types of exoplanets are super-Earths and Neptunes, planets with sizes ranging from Earth to Neptune, residing close to their parent stars. This project aims to characterise these planets at various stages of their evolution. This project will utilise Australian facilities to characterise new planets from the TESS space telescope, and is expected to probe the dynamical and physical properties of super-Earths and Neptunes as a function of age. Important benefits from this project include directly answering the origins of this dominant class of planets, and developing the techniques for the next decade of exoplanetary research.Read moreRead less