Same as Fig. 8, but for different mission and astrophysical parameters. The mirror size is kept constant at 2 m. The top three panels show the predicted yield as a function of the total throughput T from 1% to 19% in steps of 2%. The middle three panels show the predicted planet yield as a function of the exozodiacal dust level z from 1 zodi to 1000 zodi in logarithmic steps of log₁₀(∆z) ~ 0.3. The bottom three panels show the predicted planet yield for different wavelength ranges. In the latter case, the overlaid power laws are functions of the width W of the wavelength range, and the x-axes do not scale linearly with W.