Fig. 1
Map of residuals at 28.4 GHz after subtracting off synchrotron, free-free, thermal dust, and CMB components (see text), in mK (R-J) units. A 5°-smoothed version of the map is subtracted to remove extended diffuse emission to more easily identify bright, relatively compact sources. This map is shown in the Mollweide projection, with l = 0° in the centre and increasing to the left.
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