<p>During my MSc by research at the University of Warwick, I developed the Transit Investigation and Recoverability Application (TIaRA). TIaRA is a tool which can measure the sensitivity of photometric data to exoplanets of different radii and orbital period. We can then combine this sensitivity information with calculated occurrence rates to estimate yields of planet discoveries. I have already led one study using TIaRA to predict yields for the TESS mission <a href="https://ui.adsabs.harvard.edu/abs/2024MNRAS.529..715R/abstract">(Rodel et al., 2024)</a> with plans for followup studies both using additional TESS data and applying TIaRA to other surveys. TIaRA was also used to determine detection sensitivities of known multiplanet host stars in both TESS and PLATO by <a href="https://ui.adsabs.harvard.edu/abs/2024MNRAS.535.1778E/abstract">Eschen et al., (2024)</a>.</p>
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