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Fig. A.4.
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HILC-cleaned CMB maps (upper row) and foreground residual maps (lower row) for SAT configuration and sky coverage for the Galactic foreground models d1s1 (left), (b) d10s5 (middle) and d12s7 (right). These cleaned maps (upper row) includes residual HILC noise and foreground defined by Eq. (A.6).
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