Collaborative Research: The Circumgalactic Dictionary: An Interpretation Guide For Circumgalactic Medium Observations

University Of Alabama Tuscaloosa, Tuscaloosa AL

Investigators

Abstract

The history of the formation of a galaxy like our own Milky Way is recorded in the properties of gas between the visible stars in the galaxy. The gas is in low density clouds and is difficult to study. This surrounding gas is usually detected by observing its silhouette in the light of background quasars, known as “quasar absorption lines”. The investigators will develop tools to help astronomers to better interpret the chemical history of this gas. They will develop tools to use quasar absorption lines to determine the gas composition, temperature and density. These tools will better determine where the gas clouds are in these galaxies and how clouds of gas are moving. By comparing the properties of these clouds of gas, they seek to understand the history of galaxy’s transformation of hydrogen and helium into more complex atoms. During this study, the investigators will train graduate and undergraduate students in a variety of astronomical and machine learning techniques. The investigators will reach out to K-12 students and the community at large. The investigators will generate synthetic quasar absorption spectra from galaxy formation simulations for a range of galaxy masses and properties. They will analyze these simulated spectra in the same manner as astronomical observations. By correlating observed spectra with synthetic absorption systems, they will determine the conditions responsible for the absorption. In the simulations the particles will be tagged by their physical properties (phase, chemical composition, 3D location, kinematics) and history (e.g. from a galactic outflow or part of pristine in-fall). Using state-of-the-art algorithms including a machine learning approach, they will provide a probabilistic mapping between the observables and the true physical properties and history of the gas. The resulting mapping code will be tested on real observations and provided to the astronomical community to enable them to interpret current and future observations. This project will combine expertise in galaxy simulations, observational quasar spectroscopy, and machine learning, and provide new research and outreach opportunities in a geographical region underrepresented in astrophysics. This project is jointly funded by the Astronomy Division and the Established Program to Stimulate Competitive Research (EPSCoR). This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.