Expected number of detectable exoplanets binned in the radius-equilibrium temperature plane (like in Fig. 2) for a large aperture, space-based optical/NIR telescope assuming the instrument parameters presented in Table 5 observing in the V band (top), J band (middle) and H band (bottom). The geometric albedos of our planet population are now distributed uniformly between 0 and 0.6 and the x-axis is shifted by 100 K toward cooler equilibrium temperatures.