Fig. 8

21 cm temperature power spectrum for a few Lyman alpha emission models and simulations S1 and S2. Top black solid lines correspond to ⟨ xα ⟩ = 0.4 while bottom dashed/dotted curves to ⟨ xα ⟩ = 0.1 (all at z ~ 20.25). The green dot-dashed line uses halos down to 106 M⊙ and a Pop III type emission spectra. The error bars in blue corresponds to the full SKA while the ones in red to 10% of the collecting area.
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