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You will first implement new reliable and quantitative diffusion-ordered optical spectroscopy that will permit rapid and automated determination of fundamental photochemical parameters, such as optical spectra, quenching, or quantum yields. This will aid
The project aims to use radio emission from nearby stars and exoplanetary systems to understand stellar space weather, magnetic activity and star–planet interactions, ultimately helping determine the environments experienced by nearby exoplanets.
Conducting independent research in exoplanet science, resulting in academic publications in peer-reviewed international journals; Building and leading a research group, in the spirit of team science; Actively contributing to the development of national