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Fig. D.3.

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Heat map of the relative difference in the completeness for four non-LAHs on the diagram of Ih and rs, h of halo models. The relative difference in completeness is defined as ()/, where and are the completeness for halo and continuum-like model, and that for halo only model, respectively. The heat map gets white when the relative difference is not available () or . Black stars and asterisks on the map indicate the halo parameter sets that have completeness values for halo models from 45% to 54% and those from 54% to 70%, respectively, while gray large, middle-size, and small circles represent the parameter sets whose Lyα fluxes of the halo models are from 1 × 10−18 erg s−1 cm−2 to 2 × 10−18 erg s−1 cm−2, those from 4 × 10−18 erg s−1 cm−2 to 6 × 10−18 erg s−1 cm−2, and those from 1 × 10−17 erg s−1 cm−2 to 2 × 10−17 erg s−1 cm−2, respectively.

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