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
Ultra-faint signatures of galaxy growth seen through the cosmic haze. This project aims to uncover the cosmic cannibalism of galaxy mergers, by using innovative new instrumentation to detect some of the faintest structures ever seen by astronomers. The project will provide a comprehensive measurement of the mass growth experienced by large galaxies consuming their smaller siblings, which will provide a critical test of our understanding of dark matter. The project will also conduct ultra-high-se ....Ultra-faint signatures of galaxy growth seen through the cosmic haze. This project aims to uncover the cosmic cannibalism of galaxy mergers, by using innovative new instrumentation to detect some of the faintest structures ever seen by astronomers. The project will provide a comprehensive measurement of the mass growth experienced by large galaxies consuming their smaller siblings, which will provide a critical test of our understanding of dark matter. The project will also conduct ultra-high-sensitivity measurements of the foreground haze from nearby interstellar clouds, a crucial step towards mitigating its impact on billion-dollar projects such as the Euclid space telescope. The statistics of spatial structures in these clouds will help us to understand how new stars are born in our own Milky Way.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE140100052
Funder
Australian Research Council
Funding Amount
$350,000.00
Summary
TAIPAN - a spectrograph to survey the southern sky. TAIPAN - a spectrograph to survey the southern sky: The TAIPAN spectroscopic survey of the southern sky aims to quadruple the number of nearby galaxies with measured redshifts, distances and velocities. Science goals include measuring the expansion rate of the universe to 1 per cent precision, and combining optical spectroscopy and radio data for each galaxy to measure the rate at which gas is being converted into stars in the local universe. T ....TAIPAN - a spectrograph to survey the southern sky. TAIPAN - a spectrograph to survey the southern sky: The TAIPAN spectroscopic survey of the southern sky aims to quadruple the number of nearby galaxies with measured redshifts, distances and velocities. Science goals include measuring the expansion rate of the universe to 1 per cent precision, and combining optical spectroscopy and radio data for each galaxy to measure the rate at which gas is being converted into stars in the local universe. This project supports construction of the TAIPAN high-performance spectrograph that will be used to carry out the survey on the UK Schmidt Telescope (UKST). The results of the survey will be made freely available to all Australian astronomers.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100104
Funder
Australian Research Council
Funding Amount
$740,000.00
Summary
Mapping the universe with the Panoramic Survey Telescope and Rapid Response System (PanSTARRS). This project plans to build a powerful new observatory, Panoramic Survey Telescope and Rapid Response System (PanSTARRS-2), to be located in Hawaii. PanSTARRS-2 will have an enormous fish-eye-lens view of the northern stars, which we will combine with Australian telescopes to give a unique view of the entire sky. Australian scientists will use this data to solve fundamental problems in astrophysics an ....Mapping the universe with the Panoramic Survey Telescope and Rapid Response System (PanSTARRS). This project plans to build a powerful new observatory, Panoramic Survey Telescope and Rapid Response System (PanSTARRS-2), to be located in Hawaii. PanSTARRS-2 will have an enormous fish-eye-lens view of the northern stars, which we will combine with Australian telescopes to give a unique view of the entire sky. Australian scientists will use this data to solve fundamental problems in astrophysics and cosmology.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100024
Funder
Australian Research Council
Funding Amount
$760,000.00
Summary
Kunlun Infrared Sky Survey. Kunlun Infrared Sky Survey (KISS): KISS is the first exploration of the time varying Universe in the infrared. The location at Kunlun station offers the advantage of the whole sky being available for study for the duration of the Antarctic winter every year. The primary scientific targets are the physics of active galactic nuclei, supersupernovae (Gamma Ray Bursters), the terminal phases of red giants (Miras) and initial phases of protostars. The project also aims to ....Kunlun Infrared Sky Survey. Kunlun Infrared Sky Survey (KISS): KISS is the first exploration of the time varying Universe in the infrared. The location at Kunlun station offers the advantage of the whole sky being available for study for the duration of the Antarctic winter every year. The primary scientific targets are the physics of active galactic nuclei, supersupernovae (Gamma Ray Bursters), the terminal phases of red giants (Miras) and initial phases of protostars. The project also aims to find exoplanets and to measure the cosmic infrared background and its angular fluctuations using the low background advantage of the Antarctic. KISS is complementary to SkyMapper in that it is infrared, and complementary to 2MASS in that it is time sensitive.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100012
Funder
Australian Research Council
Funding Amount
$632,000.00
Summary
Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telesco ....Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telescope will help answer questions that are both practical and profound. DREAMS is an important component of a longer-term international strategy that will reinforce Australia’s global leadership in the realm of Infrared Transient Astronomy.Read moreRead less
Advancing and applying stellar nucleosynthesis: using stars to probe galaxies. The project will determine how the lives of stars produce the elements that make up our world, and use this knowledge to look into how our galaxy formed. The project will use the latest results from super-computer studies as well as new instruments being built for Australia's largest optical telescope.
Space Science and Astronomy: Dissecting the Galaxy with High Resolution Multi-Object Echelle Spectrograph (HERMES) II: Decisive Observations. Australia has long been a world leader in wide-field astronomical surveys, and the new High Resolution Multi-Object Echelle Spectrograph (HERMES) being built for the Anglo-Australian Telescope (AAT) will enhance that leadership position. Through a combination of Australian technological and scientific advances, the surveys we conduct with HERMES will allow ....Space Science and Astronomy: Dissecting the Galaxy with High Resolution Multi-Object Echelle Spectrograph (HERMES) II: Decisive Observations. Australia has long been a world leader in wide-field astronomical surveys, and the new High Resolution Multi-Object Echelle Spectrograph (HERMES) being built for the Anglo-Australian Telescope (AAT) will enhance that leadership position. Through a combination of Australian technological and scientific advances, the surveys we conduct with HERMES will allow us to study galaxy formation and stellar astrophysics in unprecedented detail. There are powerful synergies between HERMES and Skymapper, another Australian astronomical survey, as well as with Gaia, the billion-dollar European space mission for studying the Galaxy; HERMES will thus promote both national and international research collaboration. In this proposal we lay the observational groundwork for maximising the scientific return from HERMES.Read moreRead less
Mapping the nearest habitable planetary systems with FunnelWeb and Veloce. This project aims to address questions of whether Earth is a uniquely habitable environment in the Universe. Within just a few years, we will discover the best planets to target in humanity's search for life outside our Solar System. Likely to be found orbiting low-mass M-dwarf stars, these planets will be the focus of bio-signature space missions for decades. Understanding how common these habitable M-dwarf planets are r ....Mapping the nearest habitable planetary systems with FunnelWeb and Veloce. This project aims to address questions of whether Earth is a uniquely habitable environment in the Universe. Within just a few years, we will discover the best planets to target in humanity's search for life outside our Solar System. Likely to be found orbiting low-mass M-dwarf stars, these planets will be the focus of bio-signature space missions for decades. Understanding how common these habitable M-dwarf planets are requires a comprehensive model for how the whole population of M-dwarf planets formed and evolved. This project will use new Australian facilities, FunnelWeb and Veloce, to map that broader landscape for M-dwarfs and their planets, and so deliver the critical context needed to interpret the coming wave of habitable planet discoveries.Read moreRead less