Open Access

Fig. B.1


Depth of search of the SHINE survey for the 150 stars in the sample computed using detection limits converted into mass using three different sets of evolutionary models (left: BEX-COND-warm; center: BEX-COND-hot; right: COND-2003) and for different stellar ages (top: minimum; middle: nominal; bottom: maximum). Each plot gives the numbers of stars around which the survey is sensitive for substellar companions as a function of mass and semimajor axis.

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