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Fig. 26.


Integrated flux density ratios of the disk and halo at different frequencies for the three CHANG-ES galaxies NGC 4217 (this work), NGC 4013, and NGC 4666 from Stein et al. (2019b). The green data points are from LOFAR, the blue data points are from the CHANG-ES frequencies; slope_CL is the slope between the flux density ratios of the disk and halo at the two CHANG-ES frequencies.

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