Degree-scale galactic radio emission at 122 MHz around the North Celestial Pole with LOFAR-AARTFAAC

Open Access

Fig. 9.

Angular power spectra () of the diffuse emission (grey curve, same as the grey curve in Fig. 8), CLEAN residual after subtraction of the CLEAN diffuse model (blue curve), and shapelet residual after subtraction of the shapelet diffuse model (orange curve) shown in Fig. 7.

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