Detection limits for the companion mass in IRDIS and IFS datasets post-processed with TLOCI and PCA (10 modes). The red dots indicate the mass and semimajor axis of planets in the tested three planet configuration. The red vertical lines show the radial location of the inner and outer planetesimal belts, and the red shaded areas show their approximate extents. For comparison, the blue dots indicate the mass and semimajor axis of the Jovian planets, and the blue shaded areas show the extents of the main asteroid belt (between 2.5 and 3.5 au; Wyatt 2008) and the Edgeworth–Kuiper belt (between 30 and 50 au; Stern & Colwell 1997) in the Solar System. The gray shaded region shows the IWA of the coronagraph.