Fig. 15.
Normalised scale heights 
at 6 GHz vs. mass surface densities for the CHANG-ES galaxy sample of Krause et al. (2018), as well as the CHANG-ES galaxies NGC 891, 4565 (both this work), 4631 (Mora-Partiarroyo et al. 2019), and 4666 (Stein et al. 2019). The weighted linear fit to the data (excluding NGC 4565 and UGC 10288) has a slope of 0.18 ± 0.02 (reduced χ2 = 0.38).
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