Transmission spectrum models for the hazy 100 × solar atmospheres calculated with ﹩\dot{M}﹩_exp (yellow line) and ﹩\dot{M}﹩ (thick red line; same as the thick red line in Figure 9) and 1000 × solar atmospheres calculated with ﹩{\dot{M}}_{\exp }﹩ (light-blue line) and ﹩\dot{M}﹩ (thick purple line; same as the thick purple line in Figure 9) . See the text for the definition of each quantity. The transmission spectrum for the 100 × solar and 1000 × solar atmospheres without haze is also plotted as the thin red line (same as the thin red line in Figure 9) and thin purple line (same as the thin purple line in Figure 9), respectively. Note that the transmission spectrum models are smoothed for clarity.