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Fig. 1


Modified CMB spectrum emerging from the DA and EoR, in units of brightness temperature relative to the CMB (Evoli, priv. comm.): a fiducial model without DM (solid line; this is our benchmark model), an extreme model without DM (dashed line), a fiducial model with DM with Mmin = 10-3M (dot-dashed line), where Mmin is the mass of the smallest DM subhalo, and a fiducial model with DM with Mmin = 10-6M (three dots-dashed line).

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