Figure 4
Thomson scattering optical depth of the microwave background versus limiting UV magnitude. The colours represent our three different galaxy UV LF parametrizations: FIT (blue), MIN (cyan) and MAX (magenta). The solid line corresponds to the FID (ζion= 1) Lν model and the shaded regions are bounded by the SOFT (ζion= 0.5) and HARD (ζion= 2) models. The WMAP-7 τe= 0.088 ± 0.015 (Komatsu et al. 2011) is indicated with a grey band. The top panel is for fesc= 20 per cent, the bottom left for fesc= 5 per cent and the bottom right for fesc= 50 per cent. Mlim, ζion and fesc are assumed constant in these calculations, and we used a clumping factor of .

Thomson scattering optical depth of the microwave background versus limiting UV magnitude. The colours represent our three different galaxy UV LF parametrizations: FIT (blue), MIN (cyan) and MAX (magenta). The solid line corresponds to the FID (ζion= 1) Lν model and the shaded regions are bounded by the SOFT (ζion= 0.5) and HARD (ζion= 2) models. The WMAP-7 τe= 0.088 ± 0.015 (Komatsu et al. 2011) is indicated with a grey band. The top panel is for fesc= 20 per cent, the bottom left for fesc= 5 per cent and the bottom right for fesc= 50 per cent. Mlim, ζion and fesc are assumed constant in these calculations, and we used a clumping factor of formula.

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