You will model stellar spectra with spots to improve the spectrum analysis for some of the active stars observed by the million-star spectroscopic GALAH Survey.

This has wide potential applications to chemical and dynamical studies of galaxies from two-dimensional  integral field unit (IFU) spectroscopy.

We have recently demonstrated a novel technique to recover sub-dwarf M stars from the combination of VISTA infra-red and SkyMapper photometry.

This Honours project was designed to complement the High Efficiency and Resolution Multi-Element Spectroscopy (HERMES) project being undertake at the AAT.

The successful applicant will work on one of several software related projects for the DREAMS infrared surveyor

The successful applicant will work on one of several software related projects for the DREAMS infrared surveyor

This short project will using existing data for a sample of red giant stars from the OGLE II and III, and MACHO surveys.

This project aims to research and potentially develop the design of calibration light sources for use in the MAVIS instrument (currently being designed for the ESO VLT).

This project aims to research and potentially develop the design of calibration light sources for use in the MAVIS instrument (currently being designed for the ESO VLT).

In this project, the student would study both the spectral and structural properties of the thermal electron density and magnetic fields in the ionised gas phase of the Milky Way.

In this project, the student would study both the spectral and structural properties of the thermal electron density and magnetic fields in the ionised gas phase of the Milky Way.

In this project, we have worked on developing and comparing empirical pressure-temperature (P-T) phase diagrams of water, Earth, and terrestrial life, to quantify the terrestrial limits on the habitability of water and help identify the factors that cause some terrestrial water to be uninhabited. 

In this project, we have worked on developing and comparing empirical pressure-temperature (P-T) phase diagrams of water, Earth, and terrestrial life, to quantify the terrestrial limits on the habitability of water and help identify the factors that cause some terrestrial water to be uninhabited. 

The Giant Magellan Telescope (GMT) requires real-time phasing of its primary mirror segments. Each instrument of GMT is required to provide phasing telemetry from guide-star images.