conclusion on light and universe
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The study of galaxy evolution is central to our understanding of the composition and evolution of the universe.
However, linking observations to theory is significantly impeded by many uncertainties, both observational and theoretical.
Three issues have been addressed in this thesis: the accuracy and interpretation of measurements of the sizes of high-redshift galaxies; the more general determination of galaxy structure and the discrepancy between light distributions and stellar
mass distributions; and the interpretation of observed evolutionary trends in the context of galaxy formation models.
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