Our group investigates the role that environment plays in galaxy evolution. We study the observed properties of galaxies in the nearby universe and correlate them with properties of their environment, including the mass of the dark matter halo they reside in, their position within their halo, the dynamical state of their environment, as well as the properties of the hot gas that surrounds them, as traced by X-ray emission.
Our goal is to understand the physical mechanisms responsible for transforming galaxies in dense regions of the universe.
Ian D. Roberts, Laura C. Parker, Toby Brown Gandhali D. Joshi, Julie Hlavacek-Larrondo, James Wadsley
Gandhali D. Joshi, Laura C. Parker, James Wadsley, Benjamin W. Keller
Fraser A. Evans, Laura C. Parker, Ian D. Roberts
Ryan Chown, Cheng Li, E. Athanassoula, Niu Li, Christine D. Wilson,
Lin Lin, Houjun Mo, Laura C. Parker, Ting Xiao
THE PARKER GROUP
Grad Student Alumni:
Melanie Demers (MSc)
Gandhali Joshi (PhD)
Fraser Evans (MSc)
Ian Roberts (MSc)
Annie Hou (PhD)
Marie-Pier Neault (MSc)
Adam Royle (MSc)
Robbie Henderson (MSc)
Blair Cardigan-Smith (MSc)
Rachel Anderson (MSc)
Jennifer Golding (MSc)
Annie Hou (MSc)
Survey course on the big questions in the physical sciences (astronomy, cosmology, quantum and nuclear physics) requiring no pre-requisite knowledge, and using no equations. Lectures are complemented with weekly tutorials.
ASTRONOMY 3X03 - GALAXIES AND COSMOLOGY
Third year astrophysics course that starts 'locally' with a look at the stars and interstellar medium of the Milky Way and nearby galaxies. We then move outwards and discuss the formation and evolution of galaxies and large scale structure, concluding the course with topics in observational and theoretical cosmology.
One term project-based course covering the basics of modern observational astronomy techniques. Students complete a series of projects in data analysis covering topics such as the fundamentals of image analysis, photometry, spectroscopy, and time series data.
Intro Astro II (galaxies and cosmology), observational cosmology, and a new course in galaxy evolution.