Fig. A.1.
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The Tully-Fisher relation obtained by using the maximum rotational velocity, Vmax, for the CIELO galaxies, coloured by B/T. Observations by McQuinn et al. (2022, downwards-pointing black triangles) and Lelli et al. (2019, black triangles) are displayed from comparison. The best-fitting regression for the data of Lapi et al. (2018) is also shown (black, dashed line). The shaded region is defined by 1σ.
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