Formation of Supermassive Black Holes. One of the most remarkable discoveries in astronomy is the observation that supermassive black holes, weighing as much as a billion suns, are found in the centers of galaxies, including our own Milky Way. Astronomers do not understand how these black holes came to be, or their role in the evolution of galaxies. This Discovery Project will address these issues by analysing data on supermassive black holes from the local and early universes. Black holes fasci ....Formation of Supermassive Black Holes. One of the most remarkable discoveries in astronomy is the observation that supermassive black holes, weighing as much as a billion suns, are found in the centers of galaxies, including our own Milky Way. Astronomers do not understand how these black holes came to be, or their role in the evolution of galaxies. This Discovery Project will address these issues by analysing data on supermassive black holes from the local and early universes. Black holes fascinate students both young and old. This Discovery Project will train a new generation of young Australian astronomers at the leading edge of astrophysics.
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“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EA ....“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EAGLE-XL. MAGPI will deliver exquisite kinematics for hundreds of galaxies in the middle ages of the Universe, providing a view to the effect of dark matter on galaxies at this critical time, while EAGLE-XL represents the technological frontier in simulations and provides the best interpretative framework for MAGPI.Read moreRead less
From Nanosecond Timing to Nanohertz Gravitational Wave Detection. Radio pulsars are the collapsed cores of once-massive stars that are renowned for their exceptional rotational stability. Ever since their discovery Australia has played a prominent role in the discovery and monitoring of these enigmatic sources. The timing and discovery of millisecond pulsars is an area where Australia is a world leader. This programme will use a powerful new instrument on the Parkes radio telescope to search for ....From Nanosecond Timing to Nanohertz Gravitational Wave Detection. Radio pulsars are the collapsed cores of once-massive stars that are renowned for their exceptional rotational stability. Ever since their discovery Australia has played a prominent role in the discovery and monitoring of these enigmatic sources. The timing and discovery of millisecond pulsars is an area where Australia is a world leader. This programme will use a powerful new instrument on the Parkes radio telescope to search for the minute influence of gravitational waves from supermassive black hole binaries on the millisecond pulsars.Read moreRead less
Smart searches for continuous gravitational waves with advanced LIGO. This project aims to detect continuous gravitational waves from neutron stars, by using smart signal processing methods developed for engineering applications like mobile telephony. The first direct detection of Einstein's gravitational waves from two merging black holes by the Laser Interferometer Gravitational Wave Observatory in 2015 began a new era of human discovery. This project is expected to progress gravitational wave ....Smart searches for continuous gravitational waves with advanced LIGO. This project aims to detect continuous gravitational waves from neutron stars, by using smart signal processing methods developed for engineering applications like mobile telephony. The first direct detection of Einstein's gravitational waves from two merging black holes by the Laser Interferometer Gravitational Wave Observatory in 2015 began a new era of human discovery. This project is expected to progress gravitational wave science and Australia's role in it, and generate insights about the origin of neutron stars and the physics of bulk nuclear matter under extremes of gravity, density and magnetisation which cannot be replicated on Earth.Read moreRead less
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
Weighing the Giants: Using Galaxy Clusters to understand Dark Energy. This project seeks to reveal the nature of dark energy and thereby explain what is causing expansion of the Universe to accelerate. The project will develop new deep machine learning techniques to weigh galaxy clusters, and apply them to data from the SPT-3G experiment at the South Pole. By comparing theoretical predictions to the observed numbers and masses of galaxy clusters, the project will help determine whether the accel ....Weighing the Giants: Using Galaxy Clusters to understand Dark Energy. This project seeks to reveal the nature of dark energy and thereby explain what is causing expansion of the Universe to accelerate. The project will develop new deep machine learning techniques to weigh galaxy clusters, and apply them to data from the SPT-3G experiment at the South Pole. By comparing theoretical predictions to the observed numbers and masses of galaxy clusters, the project will help determine whether the acceleration is due to dark energy or a breakdown in general relativity. The data science training received by students and researchers on the project will also contribute to a highly skilled STEM workforce for Australia.
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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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0561136
Funder
Australian Research Council
Funding Amount
$376,352.00
Summary
36-megapixel CCD camera for wide-field astronomy. This project aims to design and build a state-of-the-art 36-megapixel charge-coupled device (CCD) camera for wide-field imaging on a robotic telescope at Siding Spring Observatory. The camera will employ a mosaic of two 18-megapixel CCDs, which are amongst the largest ever fabricated. This new facility will have an unprecedented ability to obtain precision photometry over a wide field, and will enable breakthroughs in research into areas as diver ....36-megapixel CCD camera for wide-field astronomy. This project aims to design and build a state-of-the-art 36-megapixel charge-coupled device (CCD) camera for wide-field imaging on a robotic telescope at Siding Spring Observatory. The camera will employ a mosaic of two 18-megapixel CCDs, which are amongst the largest ever fabricated. This new facility will have an unprecedented ability to obtain precision photometry over a wide field, and will enable breakthroughs in research into areas as diverse as detection of extra-solar planets and nearby supernovae. The camera will also lead to collaborative research with ANU's newly-funded Skymapper telescope, as well as the Anglo-Australian Observatory's 6dF and 2dF instruments.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100198
Funder
Australian Research Council
Funding Amount
$315,000.00
Summary
The SAMI facility: a revolutionary multi-object hexabundle spectrograph. SAMI is a new Australian instrument concept that uses fibre bundles to obtain detailed spectroscopic data at many positions across the face of numerous galaxies at a time. Now that the technology has been shown to work, with spectacular results, the project aims to turn this concept into a general-user facility at the Anglo-Australian Telescope.
Numerical modelling of the solar atmosphere. This project will develop a complete and realistic model of the magnetic solar activity using computer simulations of the interconnected solar interior and atmosphere. The results of this project will provide a deeper insight into the physical processes behind solar activity phenomena and will help in the development of methods of solar activity prediction.