Exoplanets and asteroseismology with TESS.

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This project will make use of novel data from the NASA Transiting Exoplanet Survey Satellite (TESS). TESS is the first space mission to provide nearly all-sky photometry, covering an area 400 times larger than that of the previous NASA planet finding-mission, called Kepler (Borucki et al. 2010). During this PhD project we will use these state-of-the-art observations to understand not only exoplanets, but also their host stars. The latter will consist of an investigation of stellar oscillations, a technique known as asteroseismology. Employing asteroseismology, we will seek to gain a detailed insight into the properties of exoplanet host stars, and link these findings to the properties of their exoplanets. In this way, we will curate a gold sample of exoplanet systems that are known in exquisite detail, and use this sample to learn about the formation of exoplanet systems as well as our own solar system.