Fig. A.1.
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Thermal emission at 1.5 GHz (CHANG-ES L band) (left column) and thermal fraction maps of the L-band data (right column) of NGC 891 (top row), NGC 3432 (middle row), and NGC 4013 (bottom row). Thermal emission maps use a power law scaling with a power law index of 0.5. Thermal fraction maps are clipped below 3σ above the background noise. The beam is displayed in the bottom-right corner of each map as a white (thermal emission maps) or red (thermal fraction maps) circle.
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