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The White Dwarf Luminosity Function and the History of Star Formation in the Galaxy. The numbers of white dwarfs at different brightnesses and colours maps out a continuous record of the star formation history of the Milky Way. Our program seeks to unravel that history using white dwarfs discovered with the SkyMapper Survey and thereby understand how our Milky Way galaxy and other galaxies evolved the form and mixture of sub-structures that we see today. These results will be widely disseminated ....The White Dwarf Luminosity Function and the History of Star Formation in the Galaxy. The numbers of white dwarfs at different brightnesses and colours maps out a continuous record of the star formation history of the Milky Way. Our program seeks to unravel that history using white dwarfs discovered with the SkyMapper Survey and thereby understand how our Milky Way galaxy and other galaxies evolved the form and mixture of sub-structures that we see today. These results will be widely disseminated stimulating interest in the natural sciences amongst the general public and the nation's youth. We will train young researchers in cutting edge science, enhancing skills in data analysis, stellar atmosphere and interior computations and problem solving. Read moreRead less
The Early Epochs of the Milky Way Galaxy. By determining the chemical compositions and space velocities of the oldest stars in our Milky Way Galaxy, our program seeks to understand the first objects in the Universe and the manner in which the Galaxy formed. Our team will utilize a program that is observing 250,000 Milky Way stars and seek access to the world's largest telescopes to a monetary value of several million dollars - stimulating interest in the natural sciences among the general public ....The Early Epochs of the Milky Way Galaxy. By determining the chemical compositions and space velocities of the oldest stars in our Milky Way Galaxy, our program seeks to understand the first objects in the Universe and the manner in which the Galaxy formed. Our team will utilize a program that is observing 250,000 Milky Way stars and seek access to the world's largest telescopes to a monetary value of several million dollars - stimulating interest in the natural sciences among the general public and the nation's youth. It will train young researchers in cutting-edge science, enhancing skills in data analysis, problem solving, project management, and effective communications.Read moreRead less
Discovering the First Generation of Stars in the Galaxy - The Most Metal-Poor Stars. The most metal-poor stars carry a fossil record of the early chemical and dynamical evolution of the Galaxy. The most interesting objects are those with the lowest metal abundances representing the earliest generation of stars in the Galaxy. The aim of the present project is to extend the mining of the HES objective spectra to identify extremely metal-deficient giants, which together with the already identified ....Discovering the First Generation of Stars in the Galaxy - The Most Metal-Poor Stars. The most metal-poor stars carry a fossil record of the early chemical and dynamical evolution of the Galaxy. The most interesting objects are those with the lowest metal abundances representing the earliest generation of stars in the Galaxy. The aim of the present project is to extend the mining of the HES objective spectra to identify extremely metal-deficient giants, which together with the already identified dwarfs will be further distilled using 6dF and the DBS. We anticipate trebling the total number of the most metal deficient stars known and targeting these for observations with 8m telescopes.Read moreRead less
Illuminating the Universe with Exploding Stars. We are using Exploding Stars (Supernovae and Gamma Ray Bursts) to measure fundamental properties of the Universe. We use Type Ia Supernovaeto trace the Expansion History of the Universe and learn about the nature of the Dark Energy which currently dominates the Universe. We use Gamma Ray Bursts to illuminate the gas in and around galaxies to measure the chemical composition and structure of the Early Universe.