Open Access

Fig. 20.

image

Baryonic Tully–Fisher relation for disc galaxies in NEWHORIZON at different redshifts as labelled in the panel with the raw data points overplotted as crosses for redshift z = 0.25 (purple plus signs), compared to the two best fits from McGaugh & Schombert (2015; dashed black and dot-dashed black) and the best fit from Ponomareva et al. (2018; solid black; in thick their fit over the range of their data points, while the thin part is the extrapolated part). The fit to the NEWHORIZON data at z = 0.25 (thick dotted purple line) shows a better level of agreement with the data from Ponomareva et al. (2018; with a slope of one-third) over those of McGaugh & Schombert (2015; slope of one-fourth).

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