Physical limits on planetary mass companions derived as described in Sect. 5.1. The IFS mass limits are slightly better than the IRDIS ones. The shadowed area reflects the large uncertainty on the age of the plausible companions, ranging from 5 to 12 Myr. There are no warm start models for planets with masses above 10 M_Jup. The “hump” in sensitivity at ~ 60 au is due to disk emission. Mass limits from 115 to 130 au correspond to IRDIS K1-band observations using the same methodology as for the IFS.