Predicted masses from the de Juan Ovelar et al. (2013) prescription (black) using SPHERE scattered-light images and ALMA millimetre peak emission. Arrows are used when the estimated mass limit is either lower than 1 M_Jup or higher than 15 M_Jup (i.e. outside the regime of Eq. (5)). ANDROMEDA/IRDIS detection limits with AMES-DUSTY, BEX-HOT, and BEX-WARM initial starts are shown as red, orange, and blue bars, respectively. The dashed lines correspond to ASDI/IFS AMES-DUSTY detection limits.