Fig. C.1.
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Different components of the CMB B-mode maps for SAT configuration and sky coverage. All the maps only includes multipoles in the range 30 ≤ ℓ ≤ 300. Observed B-mode map in top-left panel includes residue after component separation noise and foreground for the d10s5 model. The remaining maps are noise-free and foreground-free.
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