GJ 536 b and c in context. The upper panel shows the masses of known planets, for masses below 100 M_⊕, and periods shorter than 1000 days, with the planets of the system of GJ 536 highlighted, and the solar system planets as reference. The middle panel shows the same, but as a function of insolation. The lower panel shows the contrast in reflected light of low-mass planets orbiting bright stars (my < 12), compared to their angular separation to their parent star. The dotted vertical lines indicate the limits in which ANDES will be able to observe (Palle et al. 2025). The red symbols for the planets of GJ 536 show the potential range of contrasts. The green squares show the position of the ANDES golden sample.