Same as Fig. B.6, but now referring to the low-kurtosis subsample of α.btfr galaxies. The thick dashed line is the no-scatter fit to the subsample, and is the same as the thick dashed line in Fig. 6. The intrinsic scatter bands correspond to the best fit value of the parameter for the subsample, σ⊥ ,intr = 0.041 dex.
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