Fig. 11

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Detection limits from RV (HARPS) + DI (SPHERE-IRDIS and SPHERE-IFS) + astrometric (Gaia and HIPPARCOS) data for the whole survey. Already known planets are overplotted in a filled orange (gray) circle if confirmed (unconfirmed). Although some planets seem beyond the reach of RV data, they were all detected with RV data (except the brown dwarf GJ 229 B) by using different RV instruments, whereas the limits plotted here only considered HARPS measurements.
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