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Fig. D.1.

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Heat map of the simulated completeness on the diagram of Ih and rs, h of halo models for the first two non-LAH sources (RID = 5479 and 22230). Left and right panels show completeness maps for halo only models and those for halo and continuum-like components models. Black stars and asterisks on the map indicate the halo parameter sets that have completeness values from 45% to 54% and those from 54% to 70%, respectively, while white 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. (a) and (b): RID = 5479. The flux of the continuum-like component is f(Lyα) = 1.5 × 10−17 erg s−1 cm−2.

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