Fig. 7.
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Map containing the sum of all foregrounds described in Sect. 3.1 (top) and their respective residuals after GNILC (bottom) at 1115 MHz in the MD30 configuration (see Table 1). The maps are in celestial coordinates and are covered with the apodized Galactic mask defined in Sect. 3.2. We note the region of extreme declination where the signal is attenuated by the apodized mask.
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