Insensitivity of the survey distribution on telescope and coronagraph parameters. Each of these scenarios take the baseline case of the survey distribution shown in Figure 2 with D = 8 m and ﹩{\mathrm{log}}\,{C}_{\min }=-10.6﹩, varying either the diameter or minimum achievable contrast. Despite second-order differences between these scenarios, they largely have the same overall shape of their survey distribution.