Expected number of one-year detectable subhaloes per mass decade at |b| ≥ 20°. The subhaloes′ mass and spatial distributions were adopted from Aquarius (Appendix C) while the SHM concentration was used. M_min = 10^-6   M_⊙. The number corresponding to the WIMP model is shown in the left (right) panel. The mass assigned to each bar denotes the geometric mean of the interval. Red and red-patterned bars show the number considering observational constraints on  ⟨ σv ⟩ _eff by Abazajian et al. (2010) and Papucci & Strumia (2010), respectively.