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Fig. 13

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Confirmed exoplanets on the NEA database with radii up to 2.5 RJup (open grey circles) and the seven exoplanet candidates identified in this work (black circles) plotted against their host star radii. The minimum detectable planet radii derived from the Q4 light curves (red circles and line) and from the Q2–Q16 light curves (blue circles and line) given in Table 1 are also shown.

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