Fig. 4

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Overview of retrieved median planetary radii and their 1σ-confidence intervals as a function of the stellar magnitude and impact parameter (colour-coded) for different baseline models. Each point represents a distribution of 88 planetary radii, with each radius being retrieved from one of the 88 one-day light curves containing a single transit event. The grey vertical lines represent the injected signal. In the case of a flat baseline (FB) and stellar magnitude 12.5 the results could not be visualised because the majority of solutions are at the upper boundary of the parameter space.
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