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Fig. 9.

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Modeling of reionization history x ¯ HI ( z ) $ \overline{x}_{\mathrm{HI}}(z) $ using Eq. (6). The top panel shows the evolution of the neutral fraction as a function of redshift for different reionization scenarios generated using GRIZZLY code. The bold black curve corresponds to our GRIZZLY fiducial reionization scenario. The bottom panel shows fitting error Δ x ¯ HI = x ¯ HI x ¯ HI , f $ \Delta\overline{x}_{\mathrm{HI}}=\overline{x}_{\mathrm{HI}}-\overline{x}_{\mathrm{HI,f}} $ on the redshift evolution of x ¯ HI $ \overline{x}_{\mathrm{HI}} $. We have used an asymmetric tanh function (see Eq. (6)) to model the redshift evolution of x ¯ HI $ \overline{x}_{\mathrm{HI}} $.

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