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Fig. 1


Distribution of planet mass vs. orbital separation of known exoplanets and candidates as listed on (Schneider et al. 2011). The main detection methods are marked by different colours. Solar system planets are marked by red letters. The dashed horizontal line marks the approximate deuterium burning mass limit. The grey-shaded area marks the parameter space probed by our NACO-ISPY survey (10% detection probability, cf. Fig. 10).

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